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2022-12-14: How Can Matter Be BOTH Liquid AND Gas?

  • 17:05: Amorphant points out that we didn’t mention magnetic monopoles as an example of quasiparticles.
  • 17:18: Actual magnetic monopoles, if they really exist, would be elementary particles, and we’ve done an episode on these before.
  • 17:24: ... be created as quasiparticles by separating the poles of a regular dipole magnetic field, for example by careful manipulation of spins in a crystal ...
  • 17:05: Amorphant points out that we didn’t mention magnetic monopoles as an example of quasiparticles.
  • 17:18: Actual magnetic monopoles, if they really exist, would be elementary particles, and we’ve done an episode on these before.

2022-11-23: How To See Black Holes By Catching Neutrinos

  • 01:03: They report seeing neutrinos produced in the colossal magnetic fields surrounding a black hole with the mass of 10 million Suns.
  • 09:26: ... know that AGNs have powerful magnetic fields because in many of them we see jets of high energy particles ...
  • 01:03: They report seeing neutrinos produced in the colossal magnetic fields surrounding a black hole with the mass of 10 million Suns.
  • 09:26: ... know that AGNs have powerful magnetic fields because in many of them we see jets of high energy particles blasted out ...
  • 01:03: They report seeing neutrinos produced in the colossal magnetic fields surrounding a black hole with the mass of 10 million Suns.
  • 10:10: Now a blazar is an AGN where a magnetically-channeled jet happens to be pointing more or less directly at us.
  • 09:47: And collisions of magnetic-field-accelerated particles is exactly how we make neutrinos in our experiments.

2022-09-28: Why Is 1/137 One of the Greatest Unsolved Problems In Physics?

  • 02:36: ... spins are separated slightly by their interaction with their own orbital magnetic ...

2022-09-14: Could the Higgs Boson Lead Us to Dark Matter?

  • 04:06: ... gamma ray photons, which could be picked up by telescopes like the Alpha Magnetic ...

2022-08-24: What Makes The Strong Force Strong?

  • 11:32: That means photons can interact with objects without affecting their electric charge, and thus neutral objects can interact with magnetic fields.

2022-06-30: Could We Decode Alien Physics?

  • 07:38: ... define this rule. Say you have an electron moving   through a magnetic field. That field is going to apply a force in some direction to ...
  • 16:39: ... light  sails that decelerate in the light and wind   and magnetic field of the destination star,  or Bussard ramjets - vast scoops ...
  • 07:38: ... define this rule. Say you have an electron moving   through a magnetic field. That field is going to apply a force in some direction to that ...
  • 16:39: ... light  sails that decelerate in the light and wind   and magnetic field of the destination star,  or Bussard ramjets - vast scoops that ...
  • 07:38: ... the cross product. Force equals   charge times velocity cross magnetic field.  This is a type of vector multiplication where   the direction ...
  • 16:39: ... your magnetic shield,   or for generating a hot plasma in that magnetic field to vaporize particles. There are lots of   novel shielding ...
  • 07:38: ... using the left-hand rule by placing a minus sign in front of your magnetic force equation.   Well that minus sign can equally be ...
  • 16:39: ... an electromagnetic shield would be sufficient. Well actually a magnetic shield may be   enough to block many charged particles, but  ...

2022-06-22: Is Interstellar Travel Impossible?

  • 10:38: There are more advanced options for the latter - for example, deflection of grains by magnetic fields or a shielding mass moving in front of the ship.
  • 12:29: These things are accelerated in the monstrous magnetic fields of black holes and supernovae and of the galaxy itself.
  • 10:38: There are more advanced options for the latter - for example, deflection of grains by magnetic fields or a shielding mass moving in front of the ship.
  • 12:29: These things are accelerated in the monstrous magnetic fields of black holes and supernovae and of the galaxy itself.

2022-06-01: What If Physics IS NOT Describing Reality?

  • 04:56: ... ask this question with a Stern   Gerlach apparatus, where the magnetic moment  of the particles interact with a magnetic field   ...

2022-05-04: Space DOES NOT Expand Everywhere

  • 13:50: ... is created in a particle collider it travels through the powerful magnetic fields of the detector. The amount by which its path is deflected by ...

2022-04-27: How the Higgs Mechanism Give Things Mass

  • 05:38: ... this random thermal motion gets overpowered by the   magnetic interaction and they end up all aligning.  The equations of ...

2022-03-08: Is the Proxima System Our Best Hope For Another Earth?

  • 11:22: ... convection through the star’s body generates crazy magnetic storms, which can cause the star to have powerful outbursts - flares - ...
  • 11:43: ... sufficiently thick atmosphere and strong planetary magnetic field could in principle protect any surface dwellers, who would then ...
  • 11:22: ... convection through the star’s body generates crazy magnetic storms, which can cause the star to have powerful outbursts - flares - that ...

2022-02-23: Are Cosmic Strings Cracks in the Universe?

  • 04:51: ... pulling them towards the same value, just   like how the magnetic dipoles in a ferromagnet  drag each other into alignment. So, when ...
  • 07:33: ... a zero-dimensional, point-like  topological defect would be a magnetic monopoles,   which we talked about recently. There are ...
  • 04:51: ... pulling them towards the same value, just   like how the magnetic dipoles in a ferromagnet  drag each other into alignment. So, when ...
  • 07:33: ... a zero-dimensional, point-like  topological defect would be a magnetic monopoles,   which we talked about recently. There are also  ways to produce 2-D ...

2022-01-19: How To Build The Universe in a Computer

  • 09:34: ... don’t get me started about the complexity  of including magnetic fields, or of Einstein’s general relativity when the gravitational field ...

2021-10-13: New Results in Quantum Tunneling vs. The Speed of Light

  • 10:48: ... phenomenon is called Larmor precession, in which a particle’s dipole magnetic field, which is defined by its spin axis, precesses like a top in an ...
  • 11:20: ... those ones, their spins were altered by the magnetic field of the laser, and the longer they spent inside the barrier, the ...
  • 14:15: In the last episode we talked about why physicists believe magnetic monopoles.
  • 14:19: ... - the radiating knots in the Higgs field that might lead to magnetic ...
  • 15:23: Erik says that if magnetic monopoles are massive enough to collapse the early univeres, wouldn’t we only find them inside black holes?
  • 15:36: ... certainly possible that magnetic monopoles to end up inside black holes, in fact some recent work ...
  • 15:48: ... would still behave like a monopole in that the black hole would radiate magnetic field ...
  • 16:08: As it is, the magnetic fields we observe around black holes seem more consistent with regular dipole fields, with both north and south poles.
  • 16:23: ... Magnetic monopoles aside, why did Moody arrange for the whole Goblet of Fire ...
  • 10:48: ... phenomenon is called Larmor precession, in which a particle’s dipole magnetic field, which is defined by its spin axis, precesses like a top in an external ...
  • 11:20: ... those ones, their spins were altered by the magnetic field of the laser, and the longer they spent inside the barrier, the more ...
  • 15:48: ... would still behave like a monopole in that the black hole would radiate magnetic field ...
  • 16:08: As it is, the magnetic fields we observe around black holes seem more consistent with regular dipole fields, with both north and south poles.
  • 15:36: ... inside black holes, in fact some recent work suggests that an individual magnetic monopole would manifest as a black hole - in that it would have an event ...
  • 14:15: In the last episode we talked about why physicists believe magnetic monopoles.
  • 14:19: ... - the radiating knots in the Higgs field that might lead to magnetic monopoles. ...
  • 15:23: Erik says that if magnetic monopoles are massive enough to collapse the early univeres, wouldn’t we only find them inside black holes?
  • 15:36: ... certainly possible that magnetic monopoles to end up inside black holes, in fact some recent work suggests that an ...
  • 16:23: ... Magnetic monopoles aside, why did Moody arrange for the whole Goblet of Fire thing when he ...

2021-10-05: Why Magnetic Monopoles SHOULD Exist

  • 00:08: It’s the magnetic monopole - and of all the fantastical beasts of particle physics, this is perhaps the most likely to actually exist.
  • 00:50: You get a dipole magnetic field that’s very similar to the dipole electric field.
  • 00:55: So if we cut this bar in half surely we get a pair of magnetic charges similar to our electric charges, right?
  • 01:11: ... doesn’t matter how many times you slice it - you’ll never get isolated magnetic charges - what we call magnetic ...
  • 01:51: ... other popular way to make a dipole magnetic field is the electromagnet - where were push electrons around in a ...
  • 02:06: And according to classical electrodynamics, moving electric charge is the source of the magnetic field.
  • 02:12: If that’s true then, why should we even expect there to be isolated magnetic charges - magnetic monopoles?
  • 02:22: The non-existence of magnetic monopoles is codified in the mathematics of electrodynamics.
  • 02:32: It states that the divergence of a magnetic field is zero.
  • 02:51: Magnetic field lines can form loops or head out toward infinity, but they never end.
  • 02:57: According to this law there are no magnetic monopoles.
  • 03:23: This is them without any charges - electric or magnetic.
  • 03:26: E is the electric field and B is the magnetic field.
  • 03:40: You could also have symmetry between these equations if there was such a thing as magnetic charge.
  • 03:46: If you add magnetic charges to these equations then you get a magnetic force that looks exactly like the electrostatic force.
  • 04:05: ... nothing in Maxwell’s equations that really says magnetic monopoles can’t exist except for the fact that James Clark Maxwell set ...
  • 04:18: But in principle it could exist, and so could magnetic monopoles.
  • 04:54: ... require this - but in that version of electromagnetism, the electric and magnetic fields are VERY different from each other, and not at all ...
  • 05:09: ... particular, the magnetic field emerging from the quantum theory must have zero divergence - its ...
  • 05:22: So perhaps here we have our reason for the apparent non-existence of magnetic monopoles.
  • 05:49: But then in 1931, just before his antimatter thing was verified, Dirac made another prediction - of the existence of magnetic monopoles.
  • 06:00: ... you start with a dipole magnetic field, you can approximate a monopole by moving the ends far enough ...
  • 06:23: So make the width of the coil much smaller than the length, and it looks like two isolated magnetic charges.
  • 06:30: ... the string part of the Dirac string is fundamentally undetectable, then magnetic monopoles can ...
  • 06:49: So magnetic fields affect charged particles.
  • 07:09: ... presence of the string, with its magnetic fields, should introduce different phase shifts depending on which side ...
  • 08:13: ... charge - electric charge has to be discrete if there’s even a single magnetic monopole in the entire ...
  • 08:34: ... this as a prediction of charge quantization, you can also flip it: magnetic monopoles are possible if electric charge is ...
  • 09:19: Well it turns out that magnetic monopoles are inevitable in all “GUTs”.
  • 10:55: And it turns out these knots in the Higgs field in GUT theories behave as massive particles with magnetic charge - magnetic monopoles.
  • 11:12: ... turns out that GUT theories generically predict these magnetic monopoles, and that they should be A) very massive, and B) should form ...
  • 11:29: The fact that magnetic monopoles should exist in these theories was both exciting and problematic.
  • 12:16: ... should have happened after the production of magnetic monopoles, and so should have thrown these things far apart that there ...
  • 12:36: ... you have one of these magnetic monopoles in your lab it wouldn’t be too hard to spot - for example a ...
  • 13:24: ... also look for magnetic monopoles coming from space - typically using cosmic ray observatories - ...
  • 13:37: We have been hunting for magnetic monopoles for longer than just about any particle.
  • 14:18: Kyle, we are taught by Paul Dirac that if there's even a single magnetic monopole in the entire universe then electric charge must be quantized.
  • 14:28: We don't know where that single magnetic monopole would be, but it's rare and special and so we decided to name it after you.
  • 14:36: ... now Kyle, the magnetic monopole Kyle - is doubly important - sure, it ensures the quantization ...
  • 03:40: You could also have symmetry between these equations if there was such a thing as magnetic charge.
  • 04:05: ... can’t exist except for the fact that James Clark Maxwell set the magnetic charge to zero because he didn’t believe it ...
  • 10:55: And it turns out these knots in the Higgs field in GUT theories behave as massive particles with magnetic charge - magnetic monopoles.
  • 00:55: So if we cut this bar in half surely we get a pair of magnetic charges similar to our electric charges, right?
  • 01:11: ... doesn’t matter how many times you slice it - you’ll never get isolated magnetic charges - what we call magnetic ...
  • 02:12: If that’s true then, why should we even expect there to be isolated magnetic charges - magnetic monopoles?
  • 03:46: If you add magnetic charges to these equations then you get a magnetic force that looks exactly like the electrostatic force.
  • 06:23: So make the width of the coil much smaller than the length, and it looks like two isolated magnetic charges.
  • 01:11: ... doesn’t matter how many times you slice it - you’ll never get isolated magnetic charges - what we call magnetic ...
  • 02:12: If that’s true then, why should we even expect there to be isolated magnetic charges - magnetic monopoles?
  • 00:50: You get a dipole magnetic field that’s very similar to the dipole electric field.
  • 01:51: ... other popular way to make a dipole magnetic field is the electromagnet - where were push electrons around in a circle In ...
  • 02:06: And according to classical electrodynamics, moving electric charge is the source of the magnetic field.
  • 02:32: It states that the divergence of a magnetic field is zero.
  • 02:51: Magnetic field lines can form loops or head out toward infinity, but they never end.
  • 03:26: E is the electric field and B is the magnetic field.
  • 05:09: ... particular, the magnetic field emerging from the quantum theory must have zero divergence - its field ...
  • 06:00: ... you start with a dipole magnetic field, you can approximate a monopole by moving the ends far enough apart and ...
  • 13:24: ... using cosmic ray observatories - or contributing to the Earth’s magnetic field - and in a number of other ...
  • 05:09: ... particular, the magnetic field emerging from the quantum theory must have zero divergence - its field lines can ...
  • 02:51: Magnetic field lines can form loops or head out toward infinity, but they never end.
  • 04:54: ... require this - but in that version of electromagnetism, the electric and magnetic fields are VERY different from each other, and not at all interchangeable as ...
  • 06:49: So magnetic fields affect charged particles.
  • 07:09: ... presence of the string, with its magnetic fields, should introduce different phase shifts depending on which side of the ...
  • 06:49: So magnetic fields affect charged particles.
  • 03:46: If you add magnetic charges to these equations then you get a magnetic force that looks exactly like the electrostatic force.
  • 00:08: It’s the magnetic monopole - and of all the fantastical beasts of particle physics, this is perhaps the most likely to actually exist.
  • 08:13: ... charge - electric charge has to be discrete if there’s even a single magnetic monopole in the entire ...
  • 14:18: Kyle, we are taught by Paul Dirac that if there's even a single magnetic monopole in the entire universe then electric charge must be quantized.
  • 14:28: We don't know where that single magnetic monopole would be, but it's rare and special and so we decided to name it after you.
  • 14:36: ... now Kyle, the magnetic monopole Kyle - is doubly important - sure, it ensures the quantization of all ...
  • 00:08: It’s the magnetic monopole - and of all the fantastical beasts of particle physics, this is perhaps the most likely to actually exist.
  • 14:36: ... now Kyle, the magnetic monopole Kyle - is doubly important - sure, it ensures the quantization of all charge, ...
  • 01:11: ... you slice it - you’ll never get isolated magnetic charges - what we call magnetic monopoles. ...
  • 02:12: If that’s true then, why should we even expect there to be isolated magnetic charges - magnetic monopoles?
  • 02:22: The non-existence of magnetic monopoles is codified in the mathematics of electrodynamics.
  • 02:57: According to this law there are no magnetic monopoles.
  • 04:05: ... nothing in Maxwell’s equations that really says magnetic monopoles can’t exist except for the fact that James Clark Maxwell set the ...
  • 04:18: But in principle it could exist, and so could magnetic monopoles.
  • 05:22: So perhaps here we have our reason for the apparent non-existence of magnetic monopoles.
  • 05:49: But then in 1931, just before his antimatter thing was verified, Dirac made another prediction - of the existence of magnetic monopoles.
  • 06:30: ... the string part of the Dirac string is fundamentally undetectable, then magnetic monopoles can ...
  • 08:34: ... this as a prediction of charge quantization, you can also flip it: magnetic monopoles are possible if electric charge is ...
  • 09:19: Well it turns out that magnetic monopoles are inevitable in all “GUTs”.
  • 10:55: And it turns out these knots in the Higgs field in GUT theories behave as massive particles with magnetic charge - magnetic monopoles.
  • 11:12: ... turns out that GUT theories generically predict these magnetic monopoles, and that they should be A) very massive, and B) should form ...
  • 11:29: The fact that magnetic monopoles should exist in these theories was both exciting and problematic.
  • 12:16: ... should have happened after the production of magnetic monopoles, and so should have thrown these things far apart that there may be very ...
  • 12:36: ... you have one of these magnetic monopoles in your lab it wouldn’t be too hard to spot - for example a monopole ...
  • 13:24: ... also look for magnetic monopoles coming from space - typically using cosmic ray observatories - or ...
  • 13:37: We have been hunting for magnetic monopoles for longer than just about any particle.
  • 13:24: ... also look for magnetic monopoles coming from space - typically using cosmic ray observatories - or contributing ...

2021-09-15: Neutron Stars: The Most Extreme Objects in the Universe

  • 01:42: ... we encounter is its magnetosphere. This is the strongest magnetic field in the universe. Even   the weakest neutron star fields ...
  • 02:00: ... pairs are created out of the extreme  energy photons in the magnetic field.   That field then becomes a particle ...
  • 11:29: ... an essential part of maintaining the neutron star’s enormous magnetic ...
  • 01:42: ... we encounter is its magnetosphere. This is the strongest magnetic field in the universe. Even   the weakest neutron star fields are a ...
  • 11:29: ... an essential part of maintaining the neutron star’s enormous magnetic field. ...
  • 02:00: ... pairs are created out of the extreme  energy photons in the magnetic field.   That field then becomes a particle accelerator, with electron ...

2021-09-07: First Detection of Light from Behind a Black Hole

  • 01:21: And the more recent version of this in polarized light shows the grain of the magnetic field right near the black hole’s edge.
  • 03:48: They sputter and flare with violent events, for example as dense clumps of gas hitting the center, or magnetic instabilities shaking things up.
  • 01:21: And the more recent version of this in polarized light shows the grain of the magnetic field right near the black hole’s edge.
  • 03:48: They sputter and flare with violent events, for example as dense clumps of gas hitting the center, or magnetic instabilities shaking things up.

2021-08-18: How Vacuum Decay Would Destroy The Universe

  • 02:52: ... example, for an electromagnetic wave  - a photon - the electric and magnetic   fields rise and fall between positive and  negative values, but the ...

2021-08-10: How to Communicate Across the Quantum Multiverse

  • 16:27: ... Persona asks what happens to the star’s magnetic fields after it goes supernova. And then guesses the correct answer - it ...
  • 16:58: ... by watching the radio light emitted by electrons spiraling in that magnetic field - what we call synchrotron radiation. Galactic magnetic fields ...
  • 16:27: ... reach the earth. The magnetic fields then go on to add to the galaxy’s magnetic field. ...
  • 16:58: ... by watching the radio light emitted by electrons spiraling in that magnetic field - what we call synchrotron radiation. Galactic magnetic fields have very ...
  • 16:27: ... Persona asks what happens to the star’s magnetic fields after it goes supernova. And then guesses the correct answer - it ...
  • 16:58: ... in that magnetic field - what we call synchrotron radiation. Galactic magnetic fields have very clear bubble-like structures that come from past ...

2021-08-03: How An Extreme New Star Could Change All Cosmology

  • 03:19: ... all over the place in a way that suggests the presence of gigantic magnetic fields. Fields around a billion times stronger than the earth or sun’s ...
  • 08:48: ... part is that it’s rotating extremely quickly and has a crazy strong magnetic field. We just don’t see these extreme properties in the white dwarfs ...
  • 09:51: ... the orbits of the parent stars. This process also explains the intense magnetic fields. Magnetic fields in stars and planets are generated by dynamos - ...
  • 14:52: ... your praises, Charlie, and extend their white dwarf blessings: may your magnetic fields stay untangled, your electrons be ever degenerate, and may your ...
  • 15:05: ... last time we took a magnetic tour of the universe, exploring how magnetism shapes our cosmos from the ...
  • 15:55: ... asks whether magnetic fields have any measurable effect on the orbits of stars around the ...
  • 16:19: So the locations that stars formed may be influenced by magnetic fields, which in turn affects their orbits. So the answer is yes, sort of.
  • 16:29: ... Charlton and Brandon Munshaw ask whether magnetic field lines are really “lines” versus some sort of continuous thing. ...
  • 17:08: ... number of you ask questions about the potential role of magnetic fields in the universe that all have the answer I just gave - can ...
  • 15:05: ... shapes our cosmos from the scale of planets up to entire galaxies. That magnetic episode .. attracted many ...
  • 03:19: ... fields. Fields around a billion times stronger than the earth or sun’s magnetic field. That’s at the top tier of the most magnetic white ...
  • 08:48: ... part is that it’s rotating extremely quickly and has a crazy strong magnetic field. We just don’t see these extreme properties in the white dwarfs produced ...
  • 09:51: ... motion to jump start a dynamo powerful enough to produce the observed magnetic field. ...
  • 15:55: ... on the orbits of stars around the galaxy. Not directly. The galactic magnetic field is very weak compared to the magnetic fields of stars, or even planets. ...
  • 16:29: ... Charlton and Brandon Munshaw ask whether magnetic field lines are really “lines” versus some sort of continuous thing. Well it's ...
  • 15:55: ... respond to that field directly. However gas does respond to the galactic magnetic field - it can definitely move gas around and even trigger gas to collapse into ...
  • 16:29: ... Charlton and Brandon Munshaw ask whether magnetic field lines are really “lines” versus some sort of continuous thing. Well it's ...
  • 03:19: ... all over the place in a way that suggests the presence of gigantic magnetic fields. Fields around a billion times stronger than the earth or sun’s magnetic ...
  • 09:51: ... the orbits of the parent stars. This process also explains the intense magnetic fields. Magnetic fields in stars and planets are generated by dynamos - ...
  • 14:52: ... your praises, Charlie, and extend their white dwarf blessings: may your magnetic fields stay untangled, your electrons be ever degenerate, and may your mass ...
  • 15:55: ... asks whether magnetic fields have any measurable effect on the orbits of stars around the galaxy. Not ...
  • 16:19: So the locations that stars formed may be influenced by magnetic fields, which in turn affects their orbits. So the answer is yes, sort of.
  • 17:08: ... number of you ask questions about the potential role of magnetic fields in the universe that all have the answer I just gave - can magnetic ...
  • 03:19: ... all over the place in a way that suggests the presence of gigantic magnetic fields. Fields around a billion times stronger than the earth or sun’s magnetic field. ...
  • 09:51: ... the orbits of the parent stars. This process also explains the intense magnetic fields. Magnetic fields in stars and planets are generated by dynamos - self-sustaining ...
  • 14:52: ... your praises, Charlie, and extend their white dwarf blessings: may your magnetic fields stay untangled, your electrons be ever degenerate, and may your mass remain ...
  • 15:05: ... last time we took a magnetic tour of the universe, exploring how magnetism shapes our cosmos from the ...
  • 03:19: ... the earth or sun’s magnetic field. That’s at the top tier of the most magnetic white ...

2021-07-21: How Magnetism Shapes The Universe

  • 00:02: As far as the north magnetic pole, where the needle starts spinning wildly?
  • 00:07: Compass needles align with magnetic field lines, and on the precise spot of magnetic north, those field lines are vertical.
  • 01:12: Personally, I’d rather be able to see magnetic fields.
  • 01:43: Even if the substance is electrically neutral you’ll still get a magnetic field as long as the charges are moving in opposite directions.
  • 01:51: That means magnetic fields can add up - and magnetism adds up to having enormous influence on the development of structure in our universe.
  • 02:01: Understanding magnetic fields is of fundamental importance to astrophysicists.
  • 02:12: Magnetic field lines form in concentric circles around moving charges.
  • 02:26: So those are magnetic field lines - but what do they do?
  • 02:30: ... the net result of that is that charged particles tend to spiral around magnetic field ...
  • 02:43: ... spins in a ferromagnet, then that current will want to loop around the magnetic ...
  • 03:17: As with the gravitational field, in a sense there’s only one universal magnetic field.
  • 03:23: ... field loops back - but some of those field lines connect to this greater magnetic field of the solar system - and even of the ...
  • 03:38: Now I don’t want to spend too much time in the solar system - greater magnetic wonders lie beyond.
  • 04:16: Magnetic field lines cross each other, and enormous magnetic energy densities pile up.
  • 04:29: ... these field lines snap and then reconnect, and in the process spray that magnetic field out into the solar system - carrying high energy particles with ...
  • 04:43: Follow one of these magnetic blasts and you’ll spiral through the solar system on a giangantic magnetic tornado.
  • 04:49: This is still the Sun’s magnetic field, which connects here and there to the piddling little fields of the planets.
  • 04:55: About 4x the distance to Pluto, the Sun’s magnetic field connects to the field of the galaxy itself.
  • 05:46: Beyond the heliosphere, seeing magnetic fields gets trickier.
  • 06:08: These specks tend to align with the local magnetic field of the Galaxy in exactly the same way as our iron filings align around a bar magnet.
  • 06:29: The light gets polarized - which means the direction of its electric and magnetic fields pick up a preferred direction rather than being random.
  • 06:37: By measuring this polarization we can map the direction of these tiny compass needles, and so map the magnetic field of the Milky Way.
  • 07:01: KInda makes me wonder if van Gogh could see magnetic fields.
  • 07:05: Actually there’s a more traditional way to map the magnetic fields of galaxies.
  • 07:35: If the electric and magnetic fields of a collection of photons all tend to point in the same direction, we say the light is linearly polarized.
  • 07:55: The electrons in their magnetic fields tend to slow one circular polarization direction more than the other.
  • 08:12: So by measuring the Faraday rotation of distant radio sources we can also map magnetic fields.
  • 08:21: We even have clear views of magnetic fields in many distant spiral galaxies.
  • 08:30: These are the densest regions of those galactic disks - places where magnetic fields have confined the charged particles of the interstellar plasma.
  • 08:39: And that plasma in turn drags the magnetic fields in orbit around the galaxy.
  • 08:44: OK, so galaxies have magnetic fields.
  • 08:47: But where do those magnetic fields come from?
  • 08:51: Large-scale magnetic fields can grow and reinforce themselves in very particular configurations called dynamos.
  • 09:38: Those supernovae may also give us the seeds of magnetic fields that can then be amplified by the galactic dynamo.
  • 09:45: However it got there, the Milky Way has built itself a substantial magnetic field.
  • 09:53: Magnetic fields generated by collapsing gas clouds help to slow the rotation of those clouds - expel angular momentum.
  • 10:05: And magnetic fields also facilitate star formation after stars die.
  • 10:09: ... Magnetic blasts accompany every supernova explosion, and these help to compress ...
  • 10:27: But the galactic magnetic field constrains that flow, funneling some of it into vast galactic fountains erupting from the poles.
  • 10:34: That’s right - if you follow a magnetic field line too far, you may accidentally leave the galaxy.
  • 10:53: The other cool thing that galactic magnetic fields do is that they act as colossal particle accelerators.
  • 11:08: Electrons and atomic nuclei can be accelerated in this magnetic field to high energies - into what we call cosmic rays.
  • 11:15: These can also be accelerated in the magnetic shock-fronts of supernova explosions.
  • 11:20: But the most energetic cosmic rays are accelerated by the strongest magnetic fields.
  • 11:40: Intense magnetic fields live just above the event horizon of some of thses black hole, and thread the infalling disk.
  • 11:54: ... even taken our first picture of the such a magnetic field - in the polarized light surrounding the M81 supermassive black ...
  • 12:05: But there’s an even more spectacular result of these magnetic fields.
  • 12:23: ... jets carry magnetic fields out into the cosmos, and we see them through the radio light ...
  • 12:32: OK, we’ve ridden our magnetic field lines pretty far and into some strange places.
  • 12:38: To summarize what we’ve learned: magnetic fields are ubiquitous, powerful, and extremely complicated.
  • 12:53: But it turns out that without cosmic-scale magnetic fields we probably wouldn’t be here today.
  • 12:59: ... are spending more and more time learning how to map and to model magnetic fields, to better understand the mysteries of this magnetic space ...
  • 04:43: Follow one of these magnetic blasts and you’ll spiral through the solar system on a giangantic magnetic tornado.
  • 10:09: ... Magnetic blasts accompany every supernova explosion, and these help to compress gas in ...
  • 04:16: Magnetic field lines cross each other, and enormous magnetic energy densities pile up.
  • 00:07: Compass needles align with magnetic field lines, and on the precise spot of magnetic north, those field lines are vertical.
  • 01:43: Even if the substance is electrically neutral you’ll still get a magnetic field as long as the charges are moving in opposite directions.
  • 02:12: Magnetic field lines form in concentric circles around moving charges.
  • 02:26: So those are magnetic field lines - but what do they do?
  • 02:30: ... the net result of that is that charged particles tend to spiral around magnetic field ...
  • 02:43: ... spins in a ferromagnet, then that current will want to loop around the magnetic field. ...
  • 03:17: As with the gravitational field, in a sense there’s only one universal magnetic field.
  • 03:23: ... field loops back - but some of those field lines connect to this greater magnetic field of the solar system - and even of the ...
  • 04:16: Magnetic field lines cross each other, and enormous magnetic energy densities pile up.
  • 04:29: ... these field lines snap and then reconnect, and in the process spray that magnetic field out into the solar system - carrying high energy particles with ...
  • 04:49: This is still the Sun’s magnetic field, which connects here and there to the piddling little fields of the planets.
  • 04:55: About 4x the distance to Pluto, the Sun’s magnetic field connects to the field of the galaxy itself.
  • 06:08: These specks tend to align with the local magnetic field of the Galaxy in exactly the same way as our iron filings align around a bar magnet.
  • 06:37: By measuring this polarization we can map the direction of these tiny compass needles, and so map the magnetic field of the Milky Way.
  • 09:45: However it got there, the Milky Way has built itself a substantial magnetic field.
  • 10:27: But the galactic magnetic field constrains that flow, funneling some of it into vast galactic fountains erupting from the poles.
  • 10:34: That’s right - if you follow a magnetic field line too far, you may accidentally leave the galaxy.
  • 11:08: Electrons and atomic nuclei can be accelerated in this magnetic field to high energies - into what we call cosmic rays.
  • 11:54: ... even taken our first picture of the such a magnetic field - in the polarized light surrounding the M81 supermassive black hole ...
  • 12:32: OK, we’ve ridden our magnetic field lines pretty far and into some strange places.
  • 11:54: ... even taken our first picture of the such a magnetic field - in the polarized light surrounding the M81 supermassive black hole ...
  • 04:55: About 4x the distance to Pluto, the Sun’s magnetic field connects to the field of the galaxy itself.
  • 10:27: But the galactic magnetic field constrains that flow, funneling some of it into vast galactic fountains erupting from the poles.
  • 00:07: Compass needles align with magnetic field lines, and on the precise spot of magnetic north, those field lines are vertical.
  • 02:12: Magnetic field lines form in concentric circles around moving charges.
  • 02:26: So those are magnetic field lines - but what do they do?
  • 02:30: ... the net result of that is that charged particles tend to spiral around magnetic field lines. ...
  • 04:16: Magnetic field lines cross each other, and enormous magnetic energy densities pile up.
  • 12:32: OK, we’ve ridden our magnetic field lines pretty far and into some strange places.
  • 01:12: Personally, I’d rather be able to see magnetic fields.
  • 01:51: That means magnetic fields can add up - and magnetism adds up to having enormous influence on the development of structure in our universe.
  • 02:01: Understanding magnetic fields is of fundamental importance to astrophysicists.
  • 05:46: Beyond the heliosphere, seeing magnetic fields gets trickier.
  • 06:29: The light gets polarized - which means the direction of its electric and magnetic fields pick up a preferred direction rather than being random.
  • 07:01: KInda makes me wonder if van Gogh could see magnetic fields.
  • 07:05: Actually there’s a more traditional way to map the magnetic fields of galaxies.
  • 07:35: If the electric and magnetic fields of a collection of photons all tend to point in the same direction, we say the light is linearly polarized.
  • 07:55: The electrons in their magnetic fields tend to slow one circular polarization direction more than the other.
  • 08:12: So by measuring the Faraday rotation of distant radio sources we can also map magnetic fields.
  • 08:21: We even have clear views of magnetic fields in many distant spiral galaxies.
  • 08:30: These are the densest regions of those galactic disks - places where magnetic fields have confined the charged particles of the interstellar plasma.
  • 08:39: And that plasma in turn drags the magnetic fields in orbit around the galaxy.
  • 08:44: OK, so galaxies have magnetic fields.
  • 08:47: But where do those magnetic fields come from?
  • 08:51: Large-scale magnetic fields can grow and reinforce themselves in very particular configurations called dynamos.
  • 09:38: Those supernovae may also give us the seeds of magnetic fields that can then be amplified by the galactic dynamo.
  • 09:53: Magnetic fields generated by collapsing gas clouds help to slow the rotation of those clouds - expel angular momentum.
  • 10:05: And magnetic fields also facilitate star formation after stars die.
  • 10:53: The other cool thing that galactic magnetic fields do is that they act as colossal particle accelerators.
  • 11:20: But the most energetic cosmic rays are accelerated by the strongest magnetic fields.
  • 11:40: Intense magnetic fields live just above the event horizon of some of thses black hole, and thread the infalling disk.
  • 12:05: But there’s an even more spectacular result of these magnetic fields.
  • 12:23: ... jets carry magnetic fields out into the cosmos, and we see them through the radio light emitted by ...
  • 12:38: To summarize what we’ve learned: magnetic fields are ubiquitous, powerful, and extremely complicated.
  • 12:53: But it turns out that without cosmic-scale magnetic fields we probably wouldn’t be here today.
  • 12:59: ... are spending more and more time learning how to map and to model magnetic fields, to better understand the mysteries of this magnetic space ...
  • 09:53: Magnetic fields generated by collapsing gas clouds help to slow the rotation of those clouds - expel angular momentum.
  • 11:40: Intense magnetic fields live just above the event horizon of some of thses black hole, and thread the infalling disk.
  • 06:29: The light gets polarized - which means the direction of its electric and magnetic fields pick up a preferred direction rather than being random.
  • 07:55: The electrons in their magnetic fields tend to slow one circular polarization direction more than the other.
  • 00:07: Compass needles align with magnetic field lines, and on the precise spot of magnetic north, those field lines are vertical.
  • 00:02: As far as the north magnetic pole, where the needle starts spinning wildly?
  • 11:15: These can also be accelerated in the magnetic shock-fronts of supernova explosions.
  • 12:59: ... and to model magnetic fields, to better understand the mysteries of this magnetic space ...
  • 04:43: Follow one of these magnetic blasts and you’ll spiral through the solar system on a giangantic magnetic tornado.
  • 03:38: Now I don’t want to spend too much time in the solar system - greater magnetic wonders lie beyond.
  • 03:50: This is a violent place, magnetically speaking.

2021-07-07: Electrons DO NOT Spin

  • 00:47: ... - suspend a cylinder of iron from a thread and switch on a vertical magnetic field. The cylinder immediately starts rotating with a constant speed. ...
  • 02:25: ... that these energy levels tend to split when atoms are put in an external magnetic field.  This Zeeman effect was explained by Lorentz himself with ...
  • 03:20: ... But then came the anomalous  Zeeman effect. In some cases, the magnetic field causes energy levels to split even further  - for reasons ...
  • 03:48: ... that has huge problems. For example, in order to produce the observed magnetic moment they’d need to be spinning  faster than the speed of light. ...
  • 04:40: ... like  in the Einstein de-Haas effect, and it also gives electrons a magnetic field. An electron’s  spin is an entirely quantum mechanical ...
  • 05:15: ... by Walther Gerlach a year later. In it silver atoms are fired through a magnetic field with a gradient - in this example stronger towards the north  ...
  • 05:31: A lone electron in the outer shell of the silver atoms grants the atom a magnetic moment.
  • 05:37: ... means the external magnetic field induces a  force on the atoms that depends on the direction ...
  • 07:02: ... the direction  of a rotation axis, or the north-south pole of the magnetic ...
  • 11:34: ... derive the right values of the  electron spin angular momentum and magnetic moment by looking at the energy and charge  currents in the so ...
  • 07:02: ... the direction  of a rotation axis, or the north-south pole of the magnetic dipole. ...
  • 00:47: ... - suspend a cylinder of iron from a thread and switch on a vertical magnetic field. The cylinder immediately starts rotating with a constant speed. At first ...
  • 02:25: ... around the atom, that motion  leads to a magnetic moment - a dipole magnetic field like a tiny bar magnet. The different alignments of that orbital ...
  • 03:20: ... But then came the anomalous  Zeeman effect. In some cases, the magnetic field causes energy levels to split even further  - for reasons that ...
  • 04:40: ... like  in the Einstein de-Haas effect, and it also gives electrons a magnetic field. An electron’s  spin is an entirely quantum mechanical property, and ...
  • 05:15: ... by Walther Gerlach a year later. In it silver atoms are fired through a magnetic field with a gradient - in this example stronger towards the north  pole ...
  • 05:37: ... means the external magnetic field induces a  force on the atoms that depends on the direction that ...
  • 02:25: ... field like a tiny bar magnet. The different alignments of that orbital magnetic field relative to the external field turns one energy level into ...
  • 00:47: ... with. Except there was - or at least there sort of was. The external magnetic field  magnetized the iron, causing the electrons in the iron’s outer shells to ...
  • 02:25: ... that these energy levels tend to split when atoms are put in an external magnetic field.  This Zeeman effect was explained by Lorentz himself with the ideas of ...
  • 00:47: ... with. Except there was - or at least there sort of was. The external magnetic field  magnetized the iron, causing the electrons in the iron’s outer shells to align ...
  • 02:25: ... charge moving in circles around the atom, that motion  leads to a magnetic moment - a dipole magnetic field like a tiny bar magnet. The different ...
  • 03:20: ... that sort of works is  to say that each electron has its own magnetic moment - by itself it acts like a tiny bar magnet. So you have the alignment of ...
  • 03:48: ... that has huge problems. For example, in order to produce the observed magnetic moment they’d need to be spinning  faster than the speed of light. This ...
  • 05:31: A lone electron in the outer shell of the silver atoms grants the atom a magnetic moment.
  • 11:34: ... derive the right values of the  electron spin angular momentum and magnetic moment by looking at the energy and charge  currents in the so called ...
  • 02:25: ... charge moving in circles around the atom, that motion  leads to a magnetic moment - a dipole magnetic field like a tiny bar magnet. The different alignments ...
  • 03:20: ... that sort of works is  to say that each electron has its own magnetic moment - by itself it acts like a tiny bar magnet. So you have the alignment of ...
  • 05:37: ... force on the atoms that depends on the direction that these little magnetic moments are pointing  relative to that field. Those that are perfectly ...
  • 04:40: ... weirdness, let me give you one more  experiment that reveals the magnetic properties that result from ...
  • 05:37: ... be deflected by less. So a stream of silver atoms with randomly aligned magnetic  moments is sent through the magnetic ...
  • 07:02: ... not only do electrons have this magnetic  moment without rotation, but the direction of the underlying ...
  • 05:37: ... be deflected by less. So a stream of silver atoms with randomly aligned magnetic  moments is sent through the magnetic ...
  • 07:02: ... moment without rotation, but the direction of the underlying magnetic  momentum is fundamentally quantum.   The direction of this "spin" ...

2021-06-09: Are We Running Out of Space Above Earth?

  • 12:59: ... to fall faster, or even electromagnetic tethers which push on earth’s magnetic field to deorbit a ...

2021-04-21: The NEW Warp Drive Possibilities

  • 14:41: ... makes it pretty hard to watch tau particles precess in magnetic fields, and so far the g-factor for the tau hasn’t even been measured to ...
  • 17:54: ... If the Quantum Zeno Effect plays a role in birds' ability to see magnetic fields, then according to the Many-Worlds interpretation are there many, ...
  • 14:41: ... makes it pretty hard to watch tau particles precess in magnetic fields, and so far the g-factor for the tau hasn’t even been measured to 1 ...
  • 17:54: ... If the Quantum Zeno Effect plays a role in birds' ability to see magnetic fields, then according to the Many-Worlds interpretation are there many, many ...

2021-04-07: Why the Muon g-2 Results Are So Exciting!

  • 01:18: And that's the anomalous magnetic dipole moment of the muon.
  • 01:35: What's an anomalous magnetic dipole moment?
  • 01:41: We've actually talked at about the anomalous magnetic dipole moment before in terms of the electron.
  • 02:05: One of the interactions that QED describes is how a charge particle will tend to rotate to align with a magnetic field.
  • 03:15: ... particles with quantum spin do generate a magnetic field, same as if you send an electric charge around a looped wire, or ...
  • 03:25: The result is a dipole magnetic field with a North and a South pole.
  • 03:29: Place an object with such a field inside a second magnetic field, and the object will tend to rotate to align with that field.
  • 04:15: So the electron responds to a magnetic field twice as strongly compared to what you'd expect for an equivalent classical rotating charge.
  • 05:23: We can represent an electron interacting with a magnetic field, with the simplest possible Feynman diagram.
  • 05:48: ... is for the electron to emit a virtual photon just prior to absorbing the magnetic field photon, and then reabsorbing that virtual ...
  • 06:34: By the way, the anomalous in the anomalous magnetic dipole moment, refers to that little bit extra after the two.
  • 09:41: At the Fermilab experiment, physicists send muons flying at nearly the speed of light around a 50 foot diameter magnetic tube.
  • 09:49: The muons interact with the magnetic field and their own magnetic dipole axis, rotate like a top just before it falls.
  • 01:18: And that's the anomalous magnetic dipole moment of the muon.
  • 01:35: What's an anomalous magnetic dipole moment?
  • 01:41: We've actually talked at about the anomalous magnetic dipole moment before in terms of the electron.
  • 06:34: By the way, the anomalous in the anomalous magnetic dipole moment, refers to that little bit extra after the two.
  • 09:49: The muons interact with the magnetic field and their own magnetic dipole axis, rotate like a top just before it falls.
  • 01:18: And that's the anomalous magnetic dipole moment of the muon.
  • 01:35: What's an anomalous magnetic dipole moment?
  • 01:41: We've actually talked at about the anomalous magnetic dipole moment before in terms of the electron.
  • 06:34: By the way, the anomalous in the anomalous magnetic dipole moment, refers to that little bit extra after the two.
  • 02:05: One of the interactions that QED describes is how a charge particle will tend to rotate to align with a magnetic field.
  • 03:15: ... particles with quantum spin do generate a magnetic field, same as if you send an electric charge around a looped wire, or have ...
  • 03:25: The result is a dipole magnetic field with a North and a South pole.
  • 03:29: Place an object with such a field inside a second magnetic field, and the object will tend to rotate to align with that field.
  • 04:15: So the electron responds to a magnetic field twice as strongly compared to what you'd expect for an equivalent classical rotating charge.
  • 05:23: We can represent an electron interacting with a magnetic field, with the simplest possible Feynman diagram.
  • 05:48: ... is for the electron to emit a virtual photon just prior to absorbing the magnetic field photon, and then reabsorbing that virtual ...
  • 09:49: The muons interact with the magnetic field and their own magnetic dipole axis, rotate like a top just before it falls.
  • 05:48: ... is for the electron to emit a virtual photon just prior to absorbing the magnetic field photon, and then reabsorbing that virtual ...
  • 09:41: At the Fermilab experiment, physicists send muons flying at nearly the speed of light around a 50 foot diameter magnetic tube.

2021-03-23: Zeno's Paradox & The Quantum Zeno Effect

  • 08:02: ... role in the photochemical reactions that give birds their ability to see magnetic fields - something we’ve talked about ...

2021-02-17: Gravitational Wave Background Discovered?

  • 00:00: ... stars tend to channel jets of high energy particles due to their intense magnetic fields they also rotate rapidly with the rotational axis offset from the ...

2021-01-19: Can We Break the Universe?

  • 15:23: ... way that changed depending on the direction and strength of a very weak magnetic ...

2020-12-22: Navigating with Quantum Entanglement

  • 02:22: ... that birds have a “magnetoreception” that they navigate by the Earth’s magnetic field came from the Russian zoologist Alexander von Middendorf back in ...
  • 02:32: ... when German biologists Wolfgang Wiltschko and Friedrich Merkel applied magnetic fields to enclosures with European robins, preventing them from ...
  • 02:48: How exactly birds detect magnetic fields remains an open question.
  • 03:03: ... one: the idea that proposes birds can in a sense see the Earth’s magnetic field due to quantum weirdness happening inside their ...
  • 03:19: Before we get into all the cool quantum stuff, a quick review on Earth’s magnetic field is in order.
  • 04:12: This “declination” points towards the magnetic poles, which are offset from the true poles defined by Earth’s rotational axis.
  • 04:52: In principle it’s easy to come up with ways to sense a magnetic field.
  • 04:56: Magnetic fields exert a force on a moving or rotating charged particle.
  • 05:00: An electron, for example, can be thought of as a spinning charge, and magnetic fields can cause that spin to flip direction.
  • 05:08: ... like the one found in a compass needle aure ferromagnets, and their magnetic fields come from countless electrons with aligned ...
  • 05:17: External magnetic fields tug on those electrons resulting in a force that can swivel the compass needle.
  • 07:10: ... spin tends to stay fixed until disturbed by its environment. And Earth's magnetic field isn't strong enough to influence spin in that ...
  • 07:27: They do that evenly in the absence of a magnetic field - 75% of the time in the triplet state and 25% in the singlet.
  • 07:35: But even a weak magnetic field like the Earth's can affect the amount of time the radical pair spends in these states.
  • 07:53: ... does the entanglement need to last in order to be influenced by Earth's magnetic field, and how does the simple slipping of electron spins go on to give ...
  • 08:43: ... if the bird changes the orientation of its head relative to the Earth’s magnetic ...
  • 08:59: That could lead to a true visual sense of magnetic field orientation.
  • 09:15: ... have shown that it’s possible to affect cryptochromes with a weak magnetic field and get that characteristic change of rate of chemical ...
  • 10:12: ... chemical reactions remember the quantum state, and so remember the magnetic ...
  • 10:33: The team’s calculations showed that only a full quantum description of the process could produce the required sensitivity to magnetic fields.
  • 10:40: ... for example, the valence electrons were just interacting due to their magnetic fields - so-called spin-spin interactions - rather than true entangled ...
  • 02:22: ... that birds have a “magnetoreception” that they navigate by the Earth’s magnetic field came from the Russian zoologist Alexander von Middendorf back in ...
  • 03:03: ... one: the idea that proposes birds can in a sense see the Earth’s magnetic field due to quantum weirdness happening inside their ...
  • 03:19: Before we get into all the cool quantum stuff, a quick review on Earth’s magnetic field is in order.
  • 04:52: In principle it’s easy to come up with ways to sense a magnetic field.
  • 07:10: ... spin tends to stay fixed until disturbed by its environment. And Earth's magnetic field isn't strong enough to influence spin in that ...
  • 07:27: They do that evenly in the absence of a magnetic field - 75% of the time in the triplet state and 25% in the singlet.
  • 07:35: But even a weak magnetic field like the Earth's can affect the amount of time the radical pair spends in these states.
  • 07:53: ... does the entanglement need to last in order to be influenced by Earth's magnetic field, and how does the simple slipping of electron spins go on to give the ...
  • 08:43: ... if the bird changes the orientation of its head relative to the Earth’s magnetic field. ...
  • 08:59: That could lead to a true visual sense of magnetic field orientation.
  • 09:15: ... have shown that it’s possible to affect cryptochromes with a weak magnetic field and get that characteristic change of rate of chemical ...
  • 10:12: ... chemical reactions remember the quantum state, and so remember the magnetic field. ...
  • 07:27: They do that evenly in the absence of a magnetic field - 75% of the time in the triplet state and 25% in the singlet.
  • 07:10: ... spin tends to stay fixed until disturbed by its environment. And Earth's magnetic field isn't strong enough to influence spin in that ...
  • 08:59: That could lead to a true visual sense of magnetic field orientation.
  • 02:32: ... when German biologists Wolfgang Wiltschko and Friedrich Merkel applied magnetic fields to enclosures with European robins, preventing them from navigating ...
  • 02:48: How exactly birds detect magnetic fields remains an open question.
  • 04:56: Magnetic fields exert a force on a moving or rotating charged particle.
  • 05:00: An electron, for example, can be thought of as a spinning charge, and magnetic fields can cause that spin to flip direction.
  • 05:08: ... like the one found in a compass needle aure ferromagnets, and their magnetic fields come from countless electrons with aligned ...
  • 05:17: External magnetic fields tug on those electrons resulting in a force that can swivel the compass needle.
  • 10:33: The team’s calculations showed that only a full quantum description of the process could produce the required sensitivity to magnetic fields.
  • 10:40: ... for example, the valence electrons were just interacting due to their magnetic fields - so-called spin-spin interactions - rather than true entangled states - ...
  • 04:56: Magnetic fields exert a force on a moving or rotating charged particle.
  • 02:48: How exactly birds detect magnetic fields remains an open question.
  • 05:17: External magnetic fields tug on those electrons resulting in a force that can swivel the compass needle.
  • 04:12: This “declination” points towards the magnetic poles, which are offset from the true poles defined by Earth’s rotational axis.

2020-11-04: Electroweak Theory and the Origin of the Fundamental Forces

  • 09:35: Consider a magnetic material, made up of many little magnetic dipoles, like little bar magnets that can point in different directions.
  • 09:56: But the individual magnetic particles interact with each other, they want to align with their neighbours.
  • 10:13: However, if we cool the material down, the interactions between magnetic particles can start to come into play.
  • 11:06: Spinning vectors and magnetic materials.
  • 09:35: Consider a magnetic material, made up of many little magnetic dipoles, like little bar magnets that can point in different directions.
  • 11:06: Spinning vectors and magnetic materials.
  • 09:56: But the individual magnetic particles interact with each other, they want to align with their neighbours.
  • 10:13: However, if we cool the material down, the interactions between magnetic particles can start to come into play.
  • 09:56: But the individual magnetic particles interact with each other, they want to align with their neighbours.

2020-09-28: Solving Quantum Cryptography

  • 14:24: Last week we talked about a highly speculative idea - lifeforms inside stars, formed from cosmic strings and magnetic monopoles.
  • 14:52: ... inside a star than outside - cosmic necklaces can be locked into the magnetic fields within the solar plasma so they don’t fall apart ...
  • 15:28: John Momberg asks if this could all happen with electric monopoles, given that magnetic monopoles don’t exist.
  • 15:35: Well, first let me say that magnetic monopoles may well exist - in fact mainstream grand unified theory candidates routinely predict them.
  • 14:52: ... inside a star than outside - cosmic necklaces can be locked into the magnetic fields within the solar plasma so they don’t fall apart ...
  • 14:24: Last week we talked about a highly speculative idea - lifeforms inside stars, formed from cosmic strings and magnetic monopoles.
  • 15:28: John Momberg asks if this could all happen with electric monopoles, given that magnetic monopoles don’t exist.
  • 15:35: Well, first let me say that magnetic monopoles may well exist - in fact mainstream grand unified theory candidates routinely predict them.
  • 15:28: John Momberg asks if this could all happen with electric monopoles, given that magnetic monopoles don’t exist.

2020-09-21: Could Life Evolve Inside Stars?

  • 00:16: Oh, and here’s an extra crazy one - life composed of cosmic strings and magnetic monopoles, evolving in the hearts of stars.
  • 01:03: ... and defects in the fabric of the universe - cosmic strings beaded with magnetic monopoles - may evolve into complex structures, and even life, within ...
  • 01:28: What exactly are cosmic strings and magnetic monopoles?
  • 01:38: Cosmic strings and magnetic monopoles are what we call topological defects.
  • 02:31: ... can have exactly the same thing in magnetic materials, where the direction of the poles of the little magnetic ...
  • 03:44: ... go through the possibilities: a 0-dimensional topological defect is a magnetic monopole - like the north or south pole of a bar magnet that somehow ...
  • 05:44: With simple magnetic monopoles, the only possible necklace is an alternating series of north and south poles - or poles and anti-poles.
  • 07:18: ... plasma and magnetic fields may stretch and break necklaces, which could reconfigure them ...
  • 02:31: ... can have exactly the same thing in magnetic materials, where the direction of the poles of the little magnetic particles ...
  • 03:44: ... go through the possibilities: a 0-dimensional topological defect is a magnetic monopole - like the north or south pole of a bar magnet that somehow lost its ...
  • 00:16: Oh, and here’s an extra crazy one - life composed of cosmic strings and magnetic monopoles, evolving in the hearts of stars.
  • 01:03: ... and defects in the fabric of the universe - cosmic strings beaded with magnetic monopoles - may evolve into complex structures, and even life, within ...
  • 01:28: What exactly are cosmic strings and magnetic monopoles?
  • 01:38: Cosmic strings and magnetic monopoles are what we call topological defects.
  • 05:44: With simple magnetic monopoles, the only possible necklace is an alternating series of north and south poles - or poles and anti-poles.
  • 01:03: ... and defects in the fabric of the universe - cosmic strings beaded with magnetic monopoles - may evolve into complex structures, and even life, within ...
  • 00:16: Oh, and here’s an extra crazy one - life composed of cosmic strings and magnetic monopoles, evolving in the hearts of stars.
  • 02:31: ... in magnetic materials, where the direction of the poles of the little magnetic particles changes across the ...

2020-08-24: Can Future Colliders Break the Standard Model?

  • 01:22: ... charged particles in a straight line, while the beam is focused by magnetic ...
  • 01:32: ... particles are still accelerated by electric fields, but now a constant magnetic field causes the beam to spiral outwards from its central ...
  • 07:03: And there are other anomalies like the muon’s magnetic moment.
  • 07:25: ... particle accelerators like the sun or supernovae or quasars or galactic magnetic fields, which continuously spray the earth with particles at higher ...
  • 01:32: ... particles are still accelerated by electric fields, but now a constant magnetic field causes the beam to spiral outwards from its central ...
  • 01:22: ... charged particles in a straight line, while the beam is focused by magnetic fields. ...
  • 07:25: ... particle accelerators like the sun or supernovae or quasars or galactic magnetic fields, which continuously spray the earth with particles at higher energies ...
  • 07:03: And there are other anomalies like the muon’s magnetic moment.

2020-08-17: How Stars Destroy Each Other

  • 04:31: If the white dwarf has a strong magnetic field, the flow of gas from its companion is channeled by that field.
  • 04:38: ... charged particles spiral along the magnetic field lines they emit synchrotron radiation, and bright X-ray light is ...
  • 06:16: ... powerful magnetic field channels high energy particles into a jet that traces a circle ...
  • 04:31: If the white dwarf has a strong magnetic field, the flow of gas from its companion is channeled by that field.
  • 04:38: ... charged particles spiral along the magnetic field lines they emit synchrotron radiation, and bright X-ray light is emitted ...
  • 06:16: ... powerful magnetic field channels high energy particles into a jet that traces a circle across ...
  • 04:38: ... charged particles spiral along the magnetic field lines they emit synchrotron radiation, and bright X-ray light is emitted as ...

2020-07-08: Does Antimatter Explain Why There's Something Rather Than Nothing?

  • 06:00: ... electrically neutral and so are hard to even store using electric and magnetic ...
  • 08:00: ... anti-protons are trapped by a combination of electric and magnetic fields in a so-called Penning ...
  • 08:50: ... anti-hydrogen is electrically neutral, it does have a small magnetic moment - like a tiny bar magnet. ALPHA introduces a new magnetic field ...
  • 09:19: ... mass and charge of the particles, their orbital angular momentum, their magnetic and electric dipole moments, and even the strength of the coupling ...
  • 08:50: ... a small magnetic moment - like a tiny bar magnet. ALPHA introduces a new magnetic field that forces the anti-matter to the center of the chamber. In this way ...
  • 06:00: ... electrically neutral and so are hard to even store using electric and magnetic fields. ...
  • 08:00: ... anti-protons are trapped by a combination of electric and magnetic fields in a so-called Penning ...
  • 08:50: ... anti-hydrogen is electrically neutral, it does have a small magnetic moment - like a tiny bar magnet. ALPHA introduces a new magnetic field that ...

2020-06-08: Can Viruses Travel Between Planets?

  • 07:26: ... lifted to the very edge of an atmosphere with the help of the planet’s magnetic field and then swept into interplanetary or even interstellar space by ...

2020-05-27: Does Gravity Require Extra Dimensions?

  • 10:08: The experiment is now typically done in a vacuum, with precise temperature control and electrostatic and magnetic shielding.

2020-04-28: Space Time Livestream: Ask Matt Anything

  • 00:00: ... on the edge where your giant streamers of plasma are channeled by magnetic fields it's a cool cool toy now but what have I actually been doing ...

2020-04-14: Was the Milky Way a Quasar?

  • 11:16: ... by electrons, but in this case, the electrons are accelerated by magnetic fields and are emitting what’s known as synchrotron ...

2020-03-24: How Black Holes Spin Space Time

  • 10:51: ... universe. It’s the Blandford-Znajek process. In this case you have a magnetic field produced by the flow of material around the black hole in an ...

2020-03-16: How Do Quantum States Manifest In The Classical World?

  • 08:44: ... hasn't collapsed. Here’s more evidence, even with the vertically-aligned magnetic fields, which only affect the vertical component of the electron’s spin, ...
  • 11:48: ... some extent the way you set up the experiment - whether you align your magnetic field vertically or horizontally. But ultimately they are states that ...
  • 08:44: ... hasn't collapsed. Here’s more evidence, even with the vertically-aligned magnetic fields, which only affect the vertical component of the electron’s spin, we ...

2020-02-11: Are Axions Dark Matter?

  • 08:05: ... an axion turning into a photon - typically in the presence of a strong magnetic field. And photons can turn into axions in a similar ...
  • 08:23: ... opaque wall. It goes like this: a light is passed through a strong magnetic field and then blocked by a metal wall. But some photons get converted ...
  • 08:53: One issue may be that we just can’t make sufficiently strong artificial magnetic fields.
  • 08:58: ... axions. CAST forms the detector part of the apparatus and uses strong magnetic fields of its own to try to turn those axions back into detectable ...
  • 09:45: ... are other spacey tests for axions. Magnetars - highly magnetic pulsars - and quasars may convert some of their own gamma ray output ...
  • 08:05: ... an axion turning into a photon - typically in the presence of a strong magnetic field. And photons can turn into axions in a similar ...
  • 08:23: ... opaque wall. It goes like this: a light is passed through a strong magnetic field and then blocked by a metal wall. But some photons get converted to ...
  • 08:53: One issue may be that we just can’t make sufficiently strong artificial magnetic fields.
  • 08:58: ... axions. CAST forms the detector part of the apparatus and uses strong magnetic fields of its own to try to turn those axions back into detectable photons. No ...
  • 09:45: ... rays get converted back and forth between axions and photons by the magnetic fields of entire galaxies. That makes them invisible for part of their journey, ...

2020-01-06: How To Detect a Neutrino

  • 03:09: ♪ ♪ More magnetic fields are used to sort the positively charged pion particles from the debris ♪ ♪ and focus *them* into a beam.

2019-11-11: Does Life Need a Multiverse to Exist?

  • 13:28: ... in Earth's core, which may help explain the strength of our protective magnetic ...
  • 13:56: The result: more iron, less rock, more magnetic field.
  • 13:28: ... in Earth's core, which may help explain the strength of our protective magnetic field. ...
  • 13:56: The result: more iron, less rock, more magnetic field.

2019-11-04: Why We Might Be Alone in the Universe

  • 05:59: ... in a molten metal outer core, and this motion generates a powerful magnetic field that protects Earth from dangerous space radiation and solar ...

2019-09-23: Is Pluto a Planet?

  • 16:47: The magnetic field that it does have comes from the interaction of the solar wind with its super thick atmosphere.

2019-09-16: Could We Terraform Mars?

  • 03:39: ... than Earth’s core, solidifying long ago and shutting down its global magnetic ...
  • 03:49: Earth’s magnetic field protects us from the solar wind, as we saw in a recent episode.
  • 13:10: We canNOT restart Mars’ magnetic field – to do that we’d have to re-melt the entire core.
  • 13:16: But we can try to build an external magnetic shield.
  • 16:05: ... well as the episode on the exciting possibility that the North and South magnetic poles may be about to ...
  • 17:59: For now, let's move on to the possible flipping of Earth's North and South magnetic poles.
  • 18:06: ... points out that while Venus lacks an Earth-type intrinsic magnetic field, the solar wind striking its atmosphere creates an induced ...
  • 18:23: Electrical currents are induced and these produce a magnetic field that pushes back against the Sun's magnetic field.
  • 18:29: ... magnetic force-shield isn't nearly as strong as Earth's, however, so our Venusian ...
  • 18:38: ... many viewers noted, what we currently call the north magnetic pole is technically a south magnetic pole - as in, what we would call ...
  • 18:50: You know how the magnetic north pole of a bar magnet is attracted to the south pole of a second bar magnet?
  • 18:56: Well, your compass's north pole is attracted to geographic north - which means geographic north must correspond to a magnetic south pole.
  • 19:06: Nolan Westrich, while laughing in Australian, notes that with the flipping of the magnetic poles it will be America's turn to be upside down.
  • 19:15: ... given that the northern hemisphere is currently the magnetic south, I think that means that North America, Europe, and most of Asia ...
  • 18:38: ... a south magnetic pole - as in, what we would call the south pole of a magnetic dipole or a bar ...
  • 03:39: ... than Earth’s core, solidifying long ago and shutting down its global magnetic field. ...
  • 03:49: Earth’s magnetic field protects us from the solar wind, as we saw in a recent episode.
  • 13:10: We canNOT restart Mars’ magnetic field – to do that we’d have to re-melt the entire core.
  • 18:06: ... points out that while Venus lacks an Earth-type intrinsic magnetic field, the solar wind striking its atmosphere creates an induced magnetic field ...
  • 18:23: Electrical currents are induced and these produce a magnetic field that pushes back against the Sun's magnetic field.
  • 03:49: Earth’s magnetic field protects us from the solar wind, as we saw in a recent episode.
  • 18:29: ... magnetic force-shield isn't nearly as strong as Earth's, however, so our Venusian floating ...
  • 18:50: You know how the magnetic north pole of a bar magnet is attracted to the south pole of a second bar magnet?
  • 18:38: ... many viewers noted, what we currently call the north magnetic pole is technically a south magnetic pole - as in, what we would call the ...
  • 16:05: ... well as the episode on the exciting possibility that the North and South magnetic poles may be about to ...
  • 17:59: For now, let's move on to the possible flipping of Earth's North and South magnetic poles.
  • 19:06: Nolan Westrich, while laughing in Australian, notes that with the flipping of the magnetic poles it will be America's turn to be upside down.
  • 13:16: But we can try to build an external magnetic shield.
  • 18:56: Well, your compass's north pole is attracted to geographic north - which means geographic north must correspond to a magnetic south pole.
  • 19:15: ... given that the northern hemisphere is currently the magnetic south, I think that means that North America, Europe, and most of Asia have ...
  • 18:56: Well, your compass's north pole is attracted to geographic north - which means geographic north must correspond to a magnetic south pole.

2019-09-03: Is Earth's Magnetic Field Reversing?

  • 00:00: Earth’s magnetic field protects us from deadly space radiation.
  • 00:24: ... of magnetic force, forged by currents in the planet’s molten core, erupt from the ...
  • 00:38: Magnetic fields exert a force on moving charged particles, causing them to spiral around those force lines.
  • 00:55: Our magnetic field deflects the worst of these.
  • 01:21: The magnetic field is currently undergoing rapid changes, possibly signaling the imminent flipping of its polarity.
  • 01:56: Magnetic materials like iron often form with their natural fields aligned with Earth’s field.
  • 02:02: We can track the direction of Earth’s magnetic field in sedimentary layers and in old volcanic flows.
  • 02:42: Except for the fact that the magnetic field DOES seem to be acting strangely lately.
  • 02:54: And for that we need to understand the Earth’s magnetic field.
  • 02:58: ... we think of magnetic fields being generated in two way: In magnetic materials like iron, the ...
  • 03:15: Alternatively, flows of many charged particles like electrons – so electrical currents - can produce magnetic fields.
  • 03:26: But Earth’s interior is not intrinsically magnetic – its too hot for the iron atoms in the core to spontaneously align.
  • 03:41: How, then, does the Earth generate such a gigantic and well-organized dipole magnetic field?
  • 05:10: ... all of this motion that together produces Earth’s magnetic field through a process called the dynamo effect – or so most scientists ...
  • 05:42: ... key is that the dynamo effect doesn’t really create a magnetic field from scratch – instead it amplifies, organizes, and sustains an ...
  • 05:52: I’ll come back to where that initial magnetic field comes from.
  • 06:05: Conductors have this cool property that they drag magnetic fields with them.
  • 06:10: So if the entire core is rotating with the Earth then the magnetic field will also rotate.
  • 06:21: As a result, the starting magnetic field gets wound up into rings around the axis of rotation – into a torus shape.
  • 06:40: Those flows grab hold of our toroidal magnetic field and twist it up further - into many little loops.
  • 06:47: Those loops form magnetic tubes around Earth’s rotational axis.
  • 07:09: But where does that initial magnetic field come from in the first place.
  • 07:50: In fact Earth’s magnetic field is a highly dynamic beast.
  • 08:06: ... magnetic north pole is currently moving at around 60 km per year around 5 degrees ...
  • 08:27: OK, so what’s all this about the magnetic field flipping over?
  • 08:30: In fact, HOW can it flip? – surely the direction of the magnetic field depends on the direction Earth is spinning.
  • 08:37: ... electrical currents, which in turn depend on the direction of small magnetic loops generated by these helical convection ...
  • 08:50: ... fact, we expect that if the magnetic field were switched off entirely, it would reestablish itself randomly, ...
  • 09:12: Earth’s magnetic field isn’t necessarily switched off, but it’s scrambled in some way.
  • 09:51: ... in which the chaotic motion of outer-core fluid causes a tangling of magnetic field lines and a global drop in field ...
  • 10:57: ... international World Magnetic Model is a global maps of Earth’s magnetic field updated every 5 years – ...
  • 11:10: ... WMM scientists found the north magnetic pole was moving so quickly that they updated nearly a year early – at ...
  • 12:06: The field also becomes very messy – with mini north and south magnetic poles popping up across the surface of the planet.
  • 12:24: ... scientists have a pretty good idea, and think that Earth’s magnetic field is likely to hold out for our lifetimes – and those of some ...
  • 13:04: ... made of millions of refrigerator magnets to protect us once the Earth’s magnetic field ...
  • 00:00: Earth’s magnetic field protects us from deadly space radiation.
  • 00:55: Our magnetic field deflects the worst of these.
  • 01:21: The magnetic field is currently undergoing rapid changes, possibly signaling the imminent flipping of its polarity.
  • 02:02: We can track the direction of Earth’s magnetic field in sedimentary layers and in old volcanic flows.
  • 02:42: Except for the fact that the magnetic field DOES seem to be acting strangely lately.
  • 02:54: And for that we need to understand the Earth’s magnetic field.
  • 03:41: How, then, does the Earth generate such a gigantic and well-organized dipole magnetic field?
  • 05:10: ... all of this motion that together produces Earth’s magnetic field through a process called the dynamo effect – or so most scientists ...
  • 05:42: ... key is that the dynamo effect doesn’t really create a magnetic field from scratch – instead it amplifies, organizes, and sustains an existing ...
  • 05:52: I’ll come back to where that initial magnetic field comes from.
  • 06:10: So if the entire core is rotating with the Earth then the magnetic field will also rotate.
  • 06:21: As a result, the starting magnetic field gets wound up into rings around the axis of rotation – into a torus shape.
  • 06:40: Those flows grab hold of our toroidal magnetic field and twist it up further - into many little loops.
  • 07:09: But where does that initial magnetic field come from in the first place.
  • 07:50: In fact Earth’s magnetic field is a highly dynamic beast.
  • 08:27: OK, so what’s all this about the magnetic field flipping over?
  • 08:30: In fact, HOW can it flip? – surely the direction of the magnetic field depends on the direction Earth is spinning.
  • 08:50: ... fact, we expect that if the magnetic field were switched off entirely, it would reestablish itself randomly, with ...
  • 09:12: Earth’s magnetic field isn’t necessarily switched off, but it’s scrambled in some way.
  • 09:51: ... in which the chaotic motion of outer-core fluid causes a tangling of magnetic field lines and a global drop in field ...
  • 10:57: ... international World Magnetic Model is a global maps of Earth’s magnetic field updated every 5 years – in the past that’s been frequent enough to ...
  • 12:24: ... scientists have a pretty good idea, and think that Earth’s magnetic field is likely to hold out for our lifetimes – and those of some generations ...
  • 13:04: ... made of millions of refrigerator magnets to protect us once the Earth’s magnetic field ...
  • 00:55: Our magnetic field deflects the worst of these.
  • 08:30: In fact, HOW can it flip? – surely the direction of the magnetic field depends on the direction Earth is spinning.
  • 13:04: ... made of millions of refrigerator magnets to protect us once the Earth’s magnetic field fails. ...
  • 08:27: OK, so what’s all this about the magnetic field flipping over?
  • 09:12: Earth’s magnetic field isn’t necessarily switched off, but it’s scrambled in some way.
  • 09:51: ... in which the chaotic motion of outer-core fluid causes a tangling of magnetic field lines and a global drop in field ...
  • 00:00: Earth’s magnetic field protects us from deadly space radiation.
  • 10:57: ... international World Magnetic Model is a global maps of Earth’s magnetic field updated every 5 years – in the past that’s been frequent enough to account for ...
  • 00:38: Magnetic fields exert a force on moving charged particles, causing them to spiral around those force lines.
  • 02:58: ... we think of magnetic fields being generated in two way: In magnetic materials like iron, the sum ...
  • 03:15: Alternatively, flows of many charged particles like electrons – so electrical currents - can produce magnetic fields.
  • 06:05: Conductors have this cool property that they drag magnetic fields with them.
  • 00:38: Magnetic fields exert a force on moving charged particles, causing them to spiral around those force lines.
  • 00:24: ... of magnetic force, forged by currents in the planet’s molten core, erupt from the surface ...
  • 08:37: ... electrical currents, which in turn depend on the direction of small magnetic loops generated by these helical convection ...
  • 01:56: Magnetic materials like iron often form with their natural fields aligned with Earth’s field.
  • 02:58: ... we think of magnetic fields being generated in two way: In magnetic materials like iron, the sum total of the tiny magnetic fields of their ...
  • 10:57: ... international World Magnetic Model is a global maps of Earth’s magnetic field updated every 5 years – in ...
  • 08:06: ... magnetic north pole is currently moving at around 60 km per year around 5 degrees south ...
  • 11:10: ... WMM scientists found the north magnetic pole was moving so quickly that they updated nearly a year early – at the ...
  • 08:50: ... entirely, it would reestablish itself randomly, with the north and south magnetic poles aligned either one way or the ...
  • 12:06: The field also becomes very messy – with mini north and south magnetic poles popping up across the surface of the planet.
  • 08:50: ... entirely, it would reestablish itself randomly, with the north and south magnetic poles aligned either one way or the ...
  • 12:06: The field also becomes very messy – with mini north and south magnetic poles popping up across the surface of the planet.
  • 06:47: Those loops form magnetic tubes around Earth’s rotational axis.

2019-08-06: What Caused the Big Bang?

  • 01:04: Another problem fixed by inflation is the absence of magnetic monopoles.
  • 05:16: A familiar example is the magnetic field. The stronger the field, the more it pulls or pushes.
  • 05:45: ... all energy besides whatever is bound up in particles. For example, a magnetic field will quickly fade away if we take away the electric currents that ...
  • 05:16: A familiar example is the magnetic field. The stronger the field, the more it pulls or pushes.
  • 05:45: ... all energy besides whatever is bound up in particles. For example, a magnetic field will quickly fade away if we take away the electric currents that ...
  • 01:04: Another problem fixed by inflation is the absence of magnetic monopoles.

2019-06-17: How Black Holes Kill Galaxies

  • 06:33: ... through the surrounding galaxy or its channeled into jets by powerful magnetic ...

2019-05-09: Why Quantum Computing Requires Quantum Cryptography

  • 04:58: Polarization defines the direction that its electric and magnetic fields … wave.
  • 16:09: What was imaged was light escaping from the photon sphere that was produced a the magnetically driven jet.

2019-05-01: The Real Science of the EHT Black Hole

  • 05:39: It’s also blasting out a jet of energetic particles, channeled by the intense magnetic fields around the black hole.
  • 07:59: Synchrotron results from electrons spiraling in magnetic fields.
  • 08:55: ... simulation that weaves in all of the physics of fluid flow and magnetic fields, in this case with the addition of the warped spacetime of a ...
  • 05:39: It’s also blasting out a jet of energetic particles, channeled by the intense magnetic fields around the black hole.
  • 07:59: Synchrotron results from electrons spiraling in magnetic fields.
  • 08:55: ... simulation that weaves in all of the physics of fluid flow and magnetic fields, in this case with the addition of the warped spacetime of a black hole ...

2019-03-06: The Impossibility of Perpetual Motion Machines

  • 10:45: Alex Taylor has an especially cool dynamo device in which the masses are contained in a magnetic field.
  • 13:47: ... electrons either bumping into other charged particles or circling in magnetic fields Fortunately we can model that stuff pretty ...
  • 10:45: Alex Taylor has an especially cool dynamo device in which the masses are contained in a magnetic field.
  • 13:47: ... electrons either bumping into other charged particles or circling in magnetic fields Fortunately we can model that stuff pretty ...

2019-01-16: Our Antimatter, Mirrored, Time-Reversed Universe

  • 01:48: ... an array of cobalt-60 atoms in a magnetic field, the cobalt nuclei have angular momenta that will align with a ...
  • 03:02: ... atoms have negatively charged nuclei which means their nuclear magnetic fields point in the opposite direction to regular matter relative to ...
  • 01:48: ... an array of cobalt-60 atoms in a magnetic field, the cobalt nuclei have angular momenta that will align with a magnetic ...
  • 03:02: ... direction to regular matter relative to their angular momentum the magnetic field in our clock will align antimatter nuclei in the opposite direction to ...

2018-12-12: Quantum Physics in a Mirror Universe

  • 00:02: ... spin which means it's possible to align the spin of the nucleus using a magnetic field so Wuan team applied a magnetic field to our layer of cobalt-60 ...

2018-11-14: Supersymmetric Particle Found?

  • 03:52: ... explosions, gamma ray bursts, black hole magnetic fields are all expected to blast high energy particles like electrons ...

2018-11-07: Why String Theory is Right

  • 14:26: Uri Nation asks about the photons that mediate the magnetic field or the contact force between two bodies.

2018-08-23: How Will the Universe End?

  • 13:46: OK, onto your comments for last week's episode on the most accurate prediction in all of science, the anomalous magnetic moment of the electron.

2018-08-15: Quantum Theory's Most Incredible Prediction

  • 01:53: ... measuring the G factor, or in simple English, measuring the anomalous magnetic dipole moment of the ...
  • 02:10: What is the anomalous magnetic dipole moment?
  • 02:14: Well, it's just like the regular magnetic dipole moment but more anomalous.
  • 02:21: Let's break down these magnetic dipole moment thing.
  • 02:25: It has a dipole magnetic field, basically meaning it has a north and south pole.
  • 02:33: If we put a bar magnet in a second external magnetic field, it'll feel a torque, a force causing it to rotate to align with that field.
  • 02:42: The tendency of a dipole magnet to rotate in an external magnetic field is its magnetic dipole moment.
  • 02:50: ... with a dipole magnetic field has a magnetic dipole moment is basically a measure of how much it ...
  • 03:03: Magnetic fields are produced by moving electric charges.
  • 03:16: But in the case of a bar magnet, the source of its magnetic field is a bit weirder.
  • 03:21: It mostly comes from the summed dipole magnetic fields of individual electrons in the outer shells of its atoms.
  • 04:12: Despite not being the same as classical rotation, this quantum spin does grant electrons a dipole magnetic field.
  • 04:20: So electrons have a magnetic dipole moment, meaning they feel magnetic fields and act as little bar magnets.
  • 04:27: Electrons in atoms feel the magnetic fields produced by their own orbits around the atom.
  • 04:57: It also gives you completely the wrong answer if you try to calculate the electron's magnetic moment.
  • 05:09: ... fact, weirdly, if you measure the magnetic dipole moment of an electron, you get almost exactly twice the value ...
  • 05:23: This difference between the quantum versus classical magnetic moments for the electron is called the G factor.
  • 06:45: This messiness messes with the interaction of the electron and the magnetic field to shift the G factor slightly.
  • 07:02: And this is the anomalous magnetic dipole moment.
  • 08:36: An electron encounters a real photon that could represent an external magnetic field.
  • 09:04: ... say, the overall strength of an electron's interaction with the magnetic field when we calculate the electrons magnetic dipole moment and it's G ...
  • 10:45: One way to do it is to watch the way electrons process in the constant magnetic field of a cyclotron, a type of particle accelerator.
  • 10:54: Electron spin axes are always slightly misaligned with an external magnetic field, due to quantum uncertainty in the spin direction.
  • 11:41: So it's really the relationship between the electron magnetic moment and the fine structure constant that we're verifying.
  • 14:23: Andrea Smith asks whether the Suns million Kelvin corona temperature is caused by magnetic reconnection.
  • 14:48: It's pretty firmly established that energy must be pumped into the corona by magnetic fields.
  • 14:59: Magnetic fields can do the job in two ways.
  • 15:02: One is this magnetic reconnection thing.
  • 15:05: ... magnetic loops extending from the surface break and reconnect into different ...
  • 15:13: Another possible mechanism is through turbulence in waves generated by the rapid motion of magnetic fields.
  • 01:53: ... measuring the G factor, or in simple English, measuring the anomalous magnetic dipole moment of the ...
  • 02:10: What is the anomalous magnetic dipole moment?
  • 02:14: Well, it's just like the regular magnetic dipole moment but more anomalous.
  • 02:21: Let's break down these magnetic dipole moment thing.
  • 02:42: The tendency of a dipole magnet to rotate in an external magnetic field is its magnetic dipole moment.
  • 02:50: ... with a dipole magnetic field has a magnetic dipole moment is basically a measure of how much it would interact with an ...
  • 04:20: So electrons have a magnetic dipole moment, meaning they feel magnetic fields and act as little bar magnets.
  • 05:09: ... fact, weirdly, if you measure the magnetic dipole moment of an electron, you get almost exactly twice the value you'd ...
  • 07:02: And this is the anomalous magnetic dipole moment.
  • 09:04: ... interaction with the magnetic field when we calculate the electrons magnetic dipole moment and it's G ...
  • 01:53: ... measuring the G factor, or in simple English, measuring the anomalous magnetic dipole moment of the ...
  • 02:10: What is the anomalous magnetic dipole moment?
  • 02:14: Well, it's just like the regular magnetic dipole moment but more anomalous.
  • 02:21: Let's break down these magnetic dipole moment thing.
  • 02:42: The tendency of a dipole magnet to rotate in an external magnetic field is its magnetic dipole moment.
  • 02:50: ... with a dipole magnetic field has a magnetic dipole moment is basically a measure of how much it would interact with an external ...
  • 04:20: So electrons have a magnetic dipole moment, meaning they feel magnetic fields and act as little bar magnets.
  • 05:09: ... fact, weirdly, if you measure the magnetic dipole moment of an electron, you get almost exactly twice the value you'd expect for ...
  • 07:02: And this is the anomalous magnetic dipole moment.
  • 09:04: ... interaction with the magnetic field when we calculate the electrons magnetic dipole moment and it's G ...
  • 02:25: It has a dipole magnetic field, basically meaning it has a north and south pole.
  • 02:33: If we put a bar magnet in a second external magnetic field, it'll feel a torque, a force causing it to rotate to align with that field.
  • 02:42: The tendency of a dipole magnet to rotate in an external magnetic field is its magnetic dipole moment.
  • 02:50: ... with a dipole magnetic field has a magnetic dipole moment is basically a measure of how much it would ...
  • 03:16: But in the case of a bar magnet, the source of its magnetic field is a bit weirder.
  • 04:12: Despite not being the same as classical rotation, this quantum spin does grant electrons a dipole magnetic field.
  • 06:45: This messiness messes with the interaction of the electron and the magnetic field to shift the G factor slightly.
  • 08:36: An electron encounters a real photon that could represent an external magnetic field.
  • 09:04: ... say, the overall strength of an electron's interaction with the magnetic field when we calculate the electrons magnetic dipole moment and it's G ...
  • 10:45: One way to do it is to watch the way electrons process in the constant magnetic field of a cyclotron, a type of particle accelerator.
  • 10:54: Electron spin axes are always slightly misaligned with an external magnetic field, due to quantum uncertainty in the spin direction.
  • 02:25: It has a dipole magnetic field, basically meaning it has a north and south pole.
  • 02:33: If we put a bar magnet in a second external magnetic field, it'll feel a torque, a force causing it to rotate to align with that field.
  • 03:03: Magnetic fields are produced by moving electric charges.
  • 03:21: It mostly comes from the summed dipole magnetic fields of individual electrons in the outer shells of its atoms.
  • 04:20: So electrons have a magnetic dipole moment, meaning they feel magnetic fields and act as little bar magnets.
  • 04:27: Electrons in atoms feel the magnetic fields produced by their own orbits around the atom.
  • 14:48: It's pretty firmly established that energy must be pumped into the corona by magnetic fields.
  • 14:59: Magnetic fields can do the job in two ways.
  • 15:13: Another possible mechanism is through turbulence in waves generated by the rapid motion of magnetic fields.
  • 04:27: Electrons in atoms feel the magnetic fields produced by their own orbits around the atom.
  • 15:05: ... magnetic loops extending from the surface break and reconnect into different forms, ...
  • 04:57: It also gives you completely the wrong answer if you try to calculate the electron's magnetic moment.
  • 11:41: So it's really the relationship between the electron magnetic moment and the fine structure constant that we're verifying.
  • 05:23: This difference between the quantum versus classical magnetic moments for the electron is called the G factor.
  • 14:23: Andrea Smith asks whether the Suns million Kelvin corona temperature is caused by magnetic reconnection.
  • 15:02: One is this magnetic reconnection thing.

2018-08-01: How Close To The Sun Can Humanity Get?

  • 01:22: Magnetic storms driving a constant stream of energy and potentially, destructive particles.
  • 02:29: ... received electric shocks from currents induced by Earth's compressed magnetic ...
  • 03:51: It'll directly probe the sun's electromagnetic field and will connect the sun's magnetic activity with the sources of the solar wind.
  • 04:00: It will also measure the outward flow of the magnetic field through the pointing flux, as well as the plasma density and electron temperature.
  • 03:51: It'll directly probe the sun's electromagnetic field and will connect the sun's magnetic activity with the sources of the solar wind.
  • 02:29: ... received electric shocks from currents induced by Earth's compressed magnetic field. ...
  • 04:00: It will also measure the outward flow of the magnetic field through the pointing flux, as well as the plasma density and electron temperature.
  • 01:22: Magnetic storms driving a constant stream of energy and potentially, destructive particles.

2018-06-27: How Asteroid Mining Will Save Earth

  • 09:15: There are also proposals to scrape regolith, asteroid dust, from the surface, or to magnetically harvest loose surface metals.

2018-06-13: What Survives Inside A Black Hole?

  • 08:30: But what about the magnetic part of electromagnetism, and what about angular momentum?
  • 08:38: A changing electric field produces a magnetic field.
  • 08:40: And so if the black hole is spinning or racing past you, you'll see that magnetic field.
  • 08:38: A changing electric field produces a magnetic field.
  • 08:40: And so if the black hole is spinning or racing past you, you'll see that magnetic field.

2018-04-25: Black Hole Swarms

  • 06:25: One we expect to be common in the galactic core are magnetic cataclysmic variables, also called polars.
  • 06:32: Polars are a bit like X-ray binaries, except instead of a black hole or a neutron star, you have a white dwarf with a powerful magnetic field.
  • 06:39: ... magnetic fields act like a dam, allowing gas from the companion star to build up ...
  • 06:25: One we expect to be common in the galactic core are magnetic cataclysmic variables, also called polars.
  • 06:32: Polars are a bit like X-ray binaries, except instead of a black hole or a neutron star, you have a white dwarf with a powerful magnetic field.
  • 06:39: ... magnetic fields act like a dam, allowing gas from the companion star to build up and ...

2018-04-04: The Unruh Effect

  • 09:06: A charged particle accelerating in a magnetic field emits radiation, bremsstrahlung radiation.
  • 09:13: An inertial observer sees the charged particle itself radiating, its energy extracted from the magnetic field.
  • 09:06: A charged particle accelerating in a magnetic field emits radiation, bremsstrahlung radiation.
  • 09:13: An inertial observer sees the charged particle itself radiating, its energy extracted from the magnetic field.
  • 09:06: A charged particle accelerating in a magnetic field emits radiation, bremsstrahlung radiation.

2018-01-31: Kronos: Devourer Of Worlds

  • 08:08: ... but most ideas involve increasing the rate of the solar wind while also magnetically driving the outflow towards the poles so Earth doesn't get ...

2018-01-10: What Do Stars Sound Like?

  • 06:11: This differential rotation powers the sun's magnetic field and is also responsible for twisting that magnetic field to drive the sunspot cycle.
  • 12:26: Felix Schneider asks how electromagnetic radiation can be focused by a magnetic field.
  • 12:39: In fact, the magnetic field of a gamma ray burst focuses charged particles-- electrons and the nuclei of the exploding star.
  • 12:56: The charged particles spiral around the axial magnetic fields and emit photons as they do.
  • 06:11: This differential rotation powers the sun's magnetic field and is also responsible for twisting that magnetic field to drive the sunspot cycle.
  • 12:26: Felix Schneider asks how electromagnetic radiation can be focused by a magnetic field.
  • 12:39: In fact, the magnetic field of a gamma ray burst focuses charged particles-- electrons and the nuclei of the exploding star.
  • 12:56: The charged particles spiral around the axial magnetic fields and emit photons as they do.

2017-12-20: Extinction by Gamma-Ray Burst

  • 03:08: In that case, the powerful magnetic fields can channel the explosion into narrow jets that massively focus and amplify the blast.

2017-11-22: Suicide Space Robots

  • 08:44: ... system in 2012, it passed the heliopause-- the boundary where the sun's magnetic field and solar wind give way to the ambient environment of the Milky ...

2017-10-11: Absolute Cold

  • 01:00: Using lasers and magnetic fields, we've now managed to cool certain substances to less than a billionth of a Kelvin.

2017-10-04: When Quasars Collide STJC

  • 04:54: When a black hole feeds, the vortex of infalling plasma-- the accretion disk-- can produce a powerful magnetic field.
  • 05:08: Those jets can blast through the surrounding galaxy and beyond, carrying their magnetic fields with them.
  • 05:15: The radio light seen here is from electrons spiraling in those magnetic fields, so-called synchrotron radiation.
  • 04:54: When a black hole feeds, the vortex of infalling plasma-- the accretion disk-- can produce a powerful magnetic field.
  • 05:08: Those jets can blast through the surrounding galaxy and beyond, carrying their magnetic fields with them.
  • 05:15: The radio light seen here is from electrons spiraling in those magnetic fields, so-called synchrotron radiation.

2017-09-28: Are the Fundamental Constants Changing?

  • 05:17: Now, quantum spin gives electrons what we call a magnetic moment.
  • 05:22: They have magnetic fields, just like a little bar magnet, or electric currents rotating in a ring even though there is no actual rotation.
  • 05:31: These same electrons are also orbiting the atomic nucleus, and that motion generates its own magnetic field.
  • 05:38: ... magnetic fields produced by an electron's spin and by its orbital motion actually ...
  • 05:31: These same electrons are also orbiting the atomic nucleus, and that motion generates its own magnetic field.
  • 05:22: They have magnetic fields, just like a little bar magnet, or electric currents rotating in a ring even though there is no actual rotation.
  • 05:38: ... magnetic fields produced by an electron's spin and by its orbital motion actually ...
  • 05:17: Now, quantum spin gives electrons what we call a magnetic moment.

2017-09-13: Neutron Stars Collide in New LIGO Signal?

  • 02:39: ... stars can rotate up to thousands of times per second and have enormous magnetic fields that result in jets of near light speed particles that sweep ...

2017-08-16: Extraterrestrial Superstorms

  • 08:10: ... studying cloud chemistry, a magnetometer for measuring Jupiter's intense magnetic field, and a four-color wide-field ...

2017-06-28: The First Quantum Field Theory

  • 09:40: ... electron energy levels due to electron spins-- spins interacting with magnetic fields in the so-called hyperfine splitting or spins interacting with ...

2017-06-21: Anti-Matter and Quantum Relativity

  • 02:47: For example, an electron's spin causes them to align themselves with magnetic fields, just like a rotating electric charge would.
  • 04:26: But when a magnetic field is present, spin direction becomes very important.
  • 02:47: For example, an electron's spin causes them to align themselves with magnetic fields, just like a rotating electric charge would.

2017-05-17: Martian Evolution

  • 07:20: These bombard the surface due to the sparse atmosphere and the absence of a protective magnetic field.

2017-04-19: The Oh My God Particle

  • 06:00: We build artificial ones on Earth using giant rings and powerful magnetic fields.
  • 06:18: When a star explodes, the expanding shock wave carries a strong magnetic field.
  • 06:41: But they may come from magnetic acceleration in quasars, or perhaps they're blasted out in gamma ray bursts.
  • 08:29: Part of the challenge in understanding cosmic rays is that our atmosphere and magnetic field shield the surface of the earth so well.
  • 06:41: But they may come from magnetic acceleration in quasars, or perhaps they're blasted out in gamma ray bursts.
  • 06:18: When a star explodes, the expanding shock wave carries a strong magnetic field.
  • 08:29: Part of the challenge in understanding cosmic rays is that our atmosphere and magnetic field shield the surface of the earth so well.
  • 06:00: We build artificial ones on Earth using giant rings and powerful magnetic fields.

2017-03-15: Time Crystals!

  • 04:13: Spins in nearby atoms like to line up with each other due to interacting magnetic fields.
  • 04:25: This is the same effect that results in magnetic materials.
  • 04:13: Spins in nearby atoms like to line up with each other due to interacting magnetic fields.
  • 04:25: This is the same effect that results in magnetic materials.

2017-02-22: The Eye of Sauron Reveals a Forming Solar System!

  • 08:54: By the way, the third star in the system is a flare star, violently fluctuating due to magnetic storms on its surface.

2017-01-25: Why Quasars are so Awesome

  • 05:07: This may be due to the magnetic field of a rapidly rotating black hole, but the jury is still out.

2017-01-19: The Phantom Singularity

  • 16:22: ... what I'd expect when you generate temperature differentials and large magnetic fields around a very sensitive position measuring ...

2017-01-04: How to See Black Holes + Kugelblitz Challenge Answer

  • 03:29: This has enabled EHT to map the strange magnetic field structures around the Sag A star black hole.

2016-11-30: Pilot Wave Theory and Quantum Realism

  • 14:25: Sebastian Lopez asks how are the magnetic fields of neutron stars created.
  • 14:30: Well, to create and sustain a magnetic field, you need some charge that's moving or spinning in some way.
  • 15:06: With their extreme rotation rates, neutron stars support electric currents sufficient for magnetic fields of up to 100 million tesla.
  • 14:30: Well, to create and sustain a magnetic field, you need some charge that's moving or spinning in some way.
  • 14:25: Sebastian Lopez asks how are the magnetic fields of neutron stars created.
  • 15:06: With their extreme rotation rates, neutron stars support electric currents sufficient for magnetic fields of up to 100 million tesla.

2016-11-16: Strange Stars

  • 02:23: Its immense magnetic field drives jets of material at extreme speeds.

2016-11-02: Quantum Vortices and Superconductivity + Drake Equation Challenge Answers

  • 02:11: ... how differences in topology were the culprit behind a strange quantized magnetic field observed in the mysterious "quantum hole effect." These findings ...

2016-10-19: The First Humans on Mars

  • 03:13: Mars's thin atmosphere and lack of magnetic field make shielding critical, especially for a permanent settlement.
  • 06:32: ... we'll will build entire centrifuge cities levitating on superconducting magnetic rails and rotating once every few ...
  • 03:13: Mars's thin atmosphere and lack of magnetic field make shielding critical, especially for a permanent settlement.
  • 06:32: ... we'll will build entire centrifuge cities levitating on superconducting magnetic rails and rotating once every few ...

2016-09-29: Life on Europa?

  • 01:51: ... that produce those plumes and then discolored by Jupiter's intense magnetic ...
  • 07:50: ... imaging and infrared scans, probe the interior with radar and magnetic mapping, and use a variety of instruments to sniff out the chemical ...
  • 01:51: ... that produce those plumes and then discolored by Jupiter's intense magnetic field. ...
  • 07:50: ... imaging and infrared scans, probe the interior with radar and magnetic mapping, and use a variety of instruments to sniff out the chemical composition ...

2016-09-21: Quantum Entanglement and the Great Bohr-Einstein Debate

  • 08:05: Polarization is just the alignment of a photon's electric and magnetic fields.

2016-07-27: The Quantum Experiment that Broke Reality

  • 12:25: Juno will figure that out by carefully mapping Jupiter's gravitational and magnetic fields.

2016-07-06: Juno to Reveal Jupiter's Violent Past

  • 01:52: The conductivity of metallic hydrogen is thought to result in the enormous electric currents that produce Jupiter's prodigious magnetic field.

2016-03-23: How Cosmic Inflation Flattened the Universe

  • 13:00: Although the magnetic field of a spinning black hole can also play a part here.

2016-02-03: Will Mars or Venus Kill You First?

  • 01:23: ... its once spinning iron core to a halt and essentially turning off its magnetic ...
  • 04:35: Both thick atmosphere and strong magnetic field are excellent protection against this stuff.
  • 05:27: This is when a magnetic storm on the sun's surface sends out a blast of extremely high energy particles, most notably protons and electrons.
  • 08:00: Venus does not generate its own magnetic field.
  • 08:03: ... the interaction of the sun's magnetic field with Venus's think atmosphere actually induces something of a ...
  • 01:23: ... its once spinning iron core to a halt and essentially turning off its magnetic field. ...
  • 04:35: Both thick atmosphere and strong magnetic field are excellent protection against this stuff.
  • 08:00: Venus does not generate its own magnetic field.
  • 08:03: ... the interaction of the sun's magnetic field with Venus's think atmosphere actually induces something of a protective ...
  • 05:27: This is when a magnetic storm on the sun's surface sends out a blast of extremely high energy particles, most notably protons and electrons.

2015-10-22: Have Gravitational Waves Been Discovered?!?

  • 09:55: ... there are a number of ideas for protecting against this, including magnetic shielding and deploying layers of absorbing or deflecting material ahead ...
  • 10:30: ... the idea is, you have this gigantic physical or magnetic funnel ahead of your craft, which scoops up this interstellar hydrogen ...
  • 09:55: ... there are a number of ideas for protecting against this, including magnetic shielding and deploying layers of absorbing or deflecting material ahead of our ...

2015-10-15: 5 REAL Possibilities for Interstellar Travel

  • 05:34: Channeled with magnetic fields, these pions provide our thrust.

2015-10-07: The Speed of Light is NOT About Light

  • 03:03: So an electric skater monkey on a rollerblading pony generates a magnetic field, obviously.
  • 03:27: She sees the monkey moving at only monkey skate speed, and so gets a totally different magnetic field.
  • 03:37: We don't measure magnetic field.
  • 03:45: See, there's a velocity-dependent trade-off between the electric and magnetic fields.
  • 03:03: So an electric skater monkey on a rollerblading pony generates a magnetic field, obviously.
  • 03:27: She sees the monkey moving at only monkey skate speed, and so gets a totally different magnetic field.
  • 03:37: We don't measure magnetic field.
  • 03:45: See, there's a velocity-dependent trade-off between the electric and magnetic fields.

2015-07-02: Can a Circle Be a Straight Line?

  • 09:18: ... don't think the answer is well understood, but since magnetic pole reversal wouldn't affect Earth's orbit or the tilt, any effects on ...
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