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2022-10-26: Why Did Quantum Entanglement Win the Nobel Prize in Physics?

  • 01:24: You have two balls - one black, one white.
  • 01:38: While that box is closed, the ball on the moon has a 50-50 chance of being black or white.
  • 02:13: Each ball is in a superposition state of maybe black-maybe white until a measurement is made.

2022-09-21: Science of the James Webb Telescope Explained!

  • 09:28: Those white blobby things are massive elliptical galaxies of the cluster, several billion light years away.

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

  • 10:03: Your screen can’t make this color, or this one, or even this pure white.
  • 10:12: White is what you get when you combine the three in equal quantities - that’s your red + green + blue = 0.
  • 13:22: ... or as we know them better, cyan, yellow and magenta, and then black and white at the ...
  • 13:56: ... of three, and two of those combinations are neutral, like black and white for example, you get this mathematical ...

2022-04-20: Does the Universe Create Itself?

  • 17:08: ... physics. In a way that’s right. If the universe is a black or a white hole then it formed by a different process than the black holes that ...

2022-03-30: Could The Universe Be Inside A Black Hole?

  • 06:05: It’s a white hole, and it’s a valid a solution to the Einstein equations.
  • 06:13: ... past, space-like singularity of the white hole is surrounded by an event horizon that is the opposite to a black ...
  • 06:35: But there’s still an “outside” in which the white hole appears as a bright, localized point in space.
  • 06:48: On the other hand, anyone inside the white hole wouldn't know that.
  • 06:59: At first glance, despite the similarities the interior of the white hole looks nothing like our universe.
  • 07:06: Now the white hole was “discovered” by messing around with the coordinates of the OG black hole solution by Karl Schwarzschild.
  • 07:22: The interior of this type of white hole looks nothing like our universe.
  • 07:48: And the space-time curvature is nearly flat, so no crazy tidal forces like in a white or black hole.
  • 08:05: But there is actually a way to fit an FLRW metric inside a black or white hole so that those inside it couldn’t tell the difference.
  • 09:43: If it works for the black hole then it should work for the white hole.
  • 09:47: Just flip the timel axis and you have a white hole containing a bubble of expanding space that looks much like our universe.
  • 09:55: If such a white hole was big enough, it could look exactly like our universe.
  • 10:14: There’s also the idea that universes are born as white holes produced after the collapse of a black hole.
  • 10:27: ... rather bounce back outward to create a new spacetimes from the resulting white hole - which itself creates new black holes, ...
  • 10:48: ... from the cosmic microwave background - then the line between the white hole and black hole becomes ...
  • 11:08: ... you lump all of this together - a very specific construction for white holes to make them look like our universe from within, and Hawking’s ...
  • 11:27: Or a white hole?
  • 06:05: It’s a white hole, and it’s a valid a solution to the Einstein equations.
  • 06:13: ... past, space-like singularity of the white hole is surrounded by an event horizon that is the opposite to a black hole ...
  • 06:35: But there’s still an “outside” in which the white hole appears as a bright, localized point in space.
  • 06:48: On the other hand, anyone inside the white hole wouldn't know that.
  • 06:59: At first glance, despite the similarities the interior of the white hole looks nothing like our universe.
  • 07:06: Now the white hole was “discovered” by messing around with the coordinates of the OG black hole solution by Karl Schwarzschild.
  • 07:22: The interior of this type of white hole looks nothing like our universe.
  • 08:05: But there is actually a way to fit an FLRW metric inside a black or white hole so that those inside it couldn’t tell the difference.
  • 09:43: If it works for the black hole then it should work for the white hole.
  • 09:47: Just flip the timel axis and you have a white hole containing a bubble of expanding space that looks much like our universe.
  • 09:55: If such a white hole was big enough, it could look exactly like our universe.
  • 10:27: ... rather bounce back outward to create a new spacetimes from the resulting white hole - which itself creates new black holes, ...
  • 10:48: ... from the cosmic microwave background - then the line between the white hole and black hole becomes ...
  • 11:27: Or a white hole?
  • 10:27: ... rather bounce back outward to create a new spacetimes from the resulting white hole - which itself creates new black holes, ...
  • 06:35: But there’s still an “outside” in which the white hole appears as a bright, localized point in space.
  • 10:14: There’s also the idea that universes are born as white holes produced after the collapse of a black hole.
  • 11:08: ... you lump all of this together - a very specific construction for white holes to make them look like our universe from within, and Hawking’s argument ...
  • 10:14: There’s also the idea that universes are born as white holes produced after the collapse of a black hole.

2022-03-23: Where Is The Center of The Universe?

  • 10:53: We might ask whether the Big Bang is a reverse black hole - also called a white hole.

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

  • 14:45: Four lights are visible through the thick atmosphere - the gleaming white twins Tolimar and Rigel Kentaurus, the glowering red orb of Proxima herself.
  • 14:56: But there’s another white star on the horizon,  but it’s slowly slipping away on its own orbit around the Milky Way.
  • 14:45: Four lights are visible through the thick atmosphere - the gleaming white twins Tolimar and Rigel Kentaurus, the glowering red orb of Proxima herself.

2021-12-10: 2021 End of Year AMA!

  • 00:02: ... this is actually normally a luxurious brown i paint on these little white parts just to gain some amount of credibility in academia these are ...

2021-10-05: Why Magnetic Monopoles SHOULD Exist

  • 16:32: ... massive enough it smashes through the degeneracy pressure that supports white dwarf stars and instead produces a black hole or neutron ...

2021-09-21: How Electron Spin Makes Matter Possible

  • 16:27: ... were just discovered and there was speculation that they might be white holes. So I came along only a little after, I imagine those were giddy ...

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

  • 04:04: ... is   not all that different from the stuff inside  of a white dwarf - the dead core of a lower   mass star like our Sun. The ...

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

  • 14:02: ... episode we talked about this one very weird white dwarf star that scientists think may be the first observation of the ...
  • 14:53: ... by awuma to help answer this. Awuma tells us that such rapidly rotating white dwarfs are found in post-common envelope close binary systems - V471 ...
  • 15:35: ... this tells me that yes, you can greatly spin up a white dwarf by feeding it the envelope of its binary partner. But is there a ...
  • 15:46: ... goes on to explode as a supernova. But the mass transfer onto the white dwarf actually makes this less likely because losing mass reduces the ...
  • 14:02: ... episode we talked about this one very weird white dwarf star that scientists think may be the first observation of the result of ...
  • 14:53: ... that they share an envelope - you can also describe that as saying he white dwarf orbits inside the other star. Now V471 is a post-common-envelope system, ...
  • 15:35: ... this tells me that yes, you can greatly spin up a white dwarf by feeding it the envelope of its binary partner. But is there a way to ...
  • 15:46: ... goes on to explode as a supernova. But the mass transfer onto the white dwarf actually makes this less likely because losing mass reduces the internal ...
  • 14:02: ... from being the result of a merger, rather than being a more usual white dwarf accreting from a partner star before being ejected from that binary system. OK, so ...
  • 15:46: ... - but it seems these scientists think that, that's less likely that the white dwarf collision explanation, which at any rate we know must happen at least ...
  • 14:53: ... that they share an envelope - you can also describe that as saying he white dwarf orbits inside the other star. Now V471 is a post-common-envelope system, ...
  • 14:02: ... episode we talked about this one very weird white dwarf star that scientists think may be the first observation of the result of the ...
  • 14:53: ... by awuma to help answer this. Awuma tells us that such rapidly rotating white dwarfs are found in post-common envelope close binary systems - V471 Tauri with ...
  • 14:02: ... think may be the first observation of the result of the merger of two white dwarfs - and how this may have huge implications for all of cosmology. Let’s see ...

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

  • 00:21: ... particular “huh, that’s weird” takes the form of a white dwarf star that’s doing some stuff that no white dwarf should ever be ...
  • 00:47: ... objects that vary over time. Astronomers using the ZTF caught a white dwarf that, at first glance, looked suspicious - a bit too massive and ...
  • 01:31: ... Observations with the Hale Telescope confirmed that it’s 1) definitely a white dwarf, and 2) definitely spinning way too fast to make ...
  • 01:45: ... we get into why this is so weird, let’s review what we know about white dwarfs - or at least, what we thought we knew. When all but the most ...
  • 02:13: ... how we thought all white dwarfs were formed. But something is off with Zee - particularly with ...
  • 02:51: ... in the world. Keck was needed to do the spectroscopy - to break the white dwarf’s light up into component colours. Splitting the light this way ...
  • 03:19: ... or sun’s magnetic field. That’s at the top tier of the most magnetic white ...
  • 05:39: ... 2140 kilometers, plus or minus a few hundred. And that is tiny, even by white dwarf ...
  • 05:51: ... comparison, a white dwarf the mass of our sun would be around the size of the earth, this ...
  • 06:04: ... one reason that it’s good to know the size of a white dwarf is that it also tells you its mass. Here we need to learn ...
  • 06:17: That’s true of planets and regular stars, but it’s not true of white dwarfs.
  • 06:21: ... white dwarfs, matter is crushed so close together that the inward ...
  • 06:51: ... closer the electron is to escaping the atom. Electrons are bound to the white dwarf by gravity, but they still have discrete energy levels. A forming ...
  • 07:24: ... happens if you add more mass to a white dwarf? First let’s think about what happens when you add mass to less ...
  • 08:05: ... if Zee is the smallest known white dwarf it must also be the most massive. Doing a little quantum ...
  • 08:29: ... collapses into a neutron star or a black hole. But If you already have a white dwarf and then slowly add more mass it’ll explode as a type 1a ...
  • 08:48: ... fate very soon. OK, let’s review the evidence. We have one weird white dwarf - it’s extremely massive and compact - but that’s not so strange ...
  • 09:18: ... never seen conclusive evidence for it. Zee could be the result of a white dwarf collision. If two white dwarfs are orbiting each other, we expect ...
  • 09:51: ... a pair of white dwarfs merge, two things might happen - either their mass adds up to ...
  • 10:37: ... so we have a possible origin story for this white dwarf. Remember I said that we should assume typical until proven weird? ...
  • 11:20: ... don’t actually know - it could go either way. But if merging white dwarfs DO explode then it may well be that many of the type 1a ...
  • 11:52: ... out that a significant number of those supernovae came from merging white dwarfs rather than accreting white dwarfs then perhaps our calculations ...
  • 12:16: ... to a black dwarf over trillions of years? That’s the usual doom of a white dwarf. But Zee may get its explosive finale after all. A typical white ...
  • 12:50: ... a chain reaction of so-called electron capture which is how you turn a white dwarf into a neutron ...
  • 13:41: ... we have it- ZTF J1901+1458 - Zee - is a moon-sized, highly magnetized white dwarf probably formed when two low mass white dwarfs spiralled into each ...
  • 14:14: ... of space around us thrums with the infinitesimal vibrations of countless white dwarfs that have merged since the beginning of time. With the help of ...
  • 14:52: ... turns out that they sing your praises, Charlie, and extend their white dwarf blessings: may your magnetic fields stay untangled, your electrons ...
  • 00:21: ... particular “huh, that’s weird” takes the form of a white dwarf star that’s doing some stuff that no white dwarf should ever be able to ...
  • 00:47: ... objects that vary over time. Astronomers using the ZTF caught a white dwarf that, at first glance, looked suspicious - a bit too massive and ...
  • 01:31: ... Observations with the Hale Telescope confirmed that it’s 1) definitely a white dwarf, and 2) definitely spinning way too fast to make ...
  • 02:13: ... it’s hard to see how any star could be rotating fast enough to produce a white dwarf that spins every 7 ...
  • 05:39: ... 2140 kilometers, plus or minus a few hundred. And that is tiny, even by white dwarf ...
  • 05:51: ... comparison, a white dwarf the mass of our sun would be around the size of the earth, this new guy ...
  • 06:04: ... one reason that it’s good to know the size of a white dwarf is that it also tells you its mass. Here we need to learn something ...
  • 06:51: ... closer the electron is to escaping the atom. Electrons are bound to the white dwarf by gravity, but they still have discrete energy levels. A forming white ...
  • 07:24: ... happens if you add more mass to a white dwarf? First let’s think about what happens when you add mass to less weird ...
  • 08:05: ... if Zee is the smallest known white dwarf it must also be the most massive. Doing a little quantum mechanics, it ...
  • 08:29: ... collapses into a neutron star or a black hole. But If you already have a white dwarf and then slowly add more mass it’ll explode as a type 1a ...
  • 08:48: ... fate very soon. OK, let’s review the evidence. We have one weird white dwarf - it’s extremely massive and compact - but that’s not so strange in ...
  • 09:18: ... never seen conclusive evidence for it. Zee could be the result of a white dwarf collision. If two white dwarfs are orbiting each other, we expect them ...
  • 09:51: ... come back to. Or it adds up to less and we get a bigger, much weirder white dwarf. That star would be spinning really really fast because it doesn’t just ...
  • 10:37: ... so we have a possible origin story for this white dwarf. Remember I said that we should assume typical until proven weird? Well ...
  • 12:16: ... to a black dwarf over trillions of years? That’s the usual doom of a white dwarf. But Zee may get its explosive finale after all. A typical white dwarf is ...
  • 12:50: ... a chain reaction of so-called electron capture which is how you turn a white dwarf into a neutron ...
  • 13:41: ... we have it- ZTF J1901+1458 - Zee - is a moon-sized, highly magnetized white dwarf probably formed when two low mass white dwarfs spiralled into each ...
  • 14:52: ... turns out that they sing your praises, Charlie, and extend their white dwarf blessings: may your magnetic fields stay untangled, your electrons be ...
  • 08:48: ... fate very soon. OK, let’s review the evidence. We have one weird white dwarf - it’s extremely massive and compact - but that’s not so strange in ...
  • 14:52: ... turns out that they sing your praises, Charlie, and extend their white dwarf blessings: may your magnetic fields stay untangled, your electrons be ever ...
  • 09:18: ... never seen conclusive evidence for it. Zee could be the result of a white dwarf collision. If two white dwarfs are orbiting each other, we expect them to slowly ...
  • 10:37: ... assume typical until proven weird? Well that still applies. If this one white dwarf formed this way, that means others probably did also. And it means that white ...
  • 05:39: ... 2140 kilometers, plus or minus a few hundred. And that is tiny, even by white dwarf standards. ...
  • 00:21: ... particular “huh, that’s weird” takes the form of a white dwarf star that’s doing some stuff that no white dwarf should ever be able to do. ...
  • 08:05: ... weigh in at 1.32 times the Sun’s mass. And that’s a lot, at least for a white dwarf. We’ve known for some time that the absolute maximum mass for a white dwarf is ...
  • 00:21: ... that it almost certainly did NOT form in the way that we thought all white dwarfs formed. This one peculiar point of faint light may change our ...
  • 01:45: ... we get into why this is so weird, let’s review what we know about white dwarfs - or at least, what we thought we knew. When all but the most massive ...
  • 02:13: ... how we thought all white dwarfs were formed. But something is off with Zee - particularly with how fast ...
  • 02:51: ... in the world. Keck was needed to do the spectroscopy - to break the white dwarf’s light up into component colours. Splitting the light this way makes it ...
  • 03:19: ... or sun’s magnetic field. That’s at the top tier of the most magnetic white dwarfs. ...
  • 06:04: ... you its mass. Here we need to learn something that’s weird about all white dwarfs, not just Zee. We normally think about objects getting bigger the more ...
  • 06:17: That’s true of planets and regular stars, but it’s not true of white dwarfs.
  • 06:21: ... white dwarfs, matter is crushed so close together that the inward gravitational pull ...
  • 07:24: ... that adding matter usually causes an object to increase in size. But for white dwarfs it’s different - as you add mass, the white dwarf has to actually shrink ...
  • 08:48: ... strong magnetic field. We just don’t see these extreme properties in the white dwarfs produced as stars ...
  • 09:18: ... for it. Zee could be the result of a white dwarf collision. If two white dwarfs are orbiting each other, we expect them to slowly spiral together ...
  • 09:51: ... a pair of white dwarfs merge, two things might happen - either their mass adds up to more than ...
  • 10:37: ... collapse for massive stellar cores or absolute explosion for accreting white dwarfs. So what happens to merging white dwarfs that exceed this ...
  • 11:20: ... don’t actually know - it could go either way. But if merging white dwarfs DO explode then it may well be that many of the type 1a supernovae that ...
  • 11:52: ... out that a significant number of those supernovae came from merging white dwarfs rather than accreting white dwarfs then perhaps our calculations of the ...
  • 13:41: ... highly magnetized white dwarf probably formed when two low mass white dwarfs spiralled into each other. It teeters on the edge of explosion, and may ...
  • 14:14: ... of space around us thrums with the infinitesimal vibrations of countless white dwarfs that have merged since the beginning of time. With the help of your ...
  • 01:45: ... we get into why this is so weird, let’s review what we know about white dwarfs - or at least, what we thought we knew. When all but the most massive ...
  • 00:21: ... that it almost certainly did NOT form in the way that we thought all white dwarfs formed. This one peculiar point of faint light may change our understanding of ...
  • 02:51: ... in the world. Keck was needed to do the spectroscopy - to break the white dwarf’s light up into component colours. Splitting the light this way makes it even ...
  • 06:21: ... white dwarfs, matter is crushed so close together that the inward gravitational pull is ...
  • 09:51: ... a pair of white dwarfs merge, two things might happen - either their mass adds up to more than the ...
  • 08:48: ... strong magnetic field. We just don’t see these extreme properties in the white dwarfs produced as stars ...
  • 13:41: ... highly magnetized white dwarf probably formed when two low mass white dwarfs spiralled into each other. It teeters on the edge of explosion, and may force us ...

2021-04-13: What If Dark Matter Is Just Black Holes?

  • 06:48: For example, they’d puncture white dwarfs and neutron stars on a regular basis.
  • 06:53: ... primordial micro-black hole would pass right through a white dwarf, but it would deposit enough heat to allow the stars' ultra dense ...
  • 06:48: For example, they’d puncture white dwarfs and neutron stars on a regular basis.

2021-03-16: The NEW Crisis in Cosmology

  • 03:13: ... - the incredibly bright “type 1a” supernovae that result when a white dwarf   star explodes after cannibalizing its binary  ...

2020-12-22: Navigating with Quantum Entanglement

  • 13:47: ... - that’s a type 2 supernova - or the remnant of a lower mass star - a white dwarf - gains extra mass and explodes - that’s a type ...
  • 14:50: The Star may go through a phase as a white - or perhaps now black dwarf and will continue to evaporate due to proton decay.
  • 13:47: ... - that’s a type 2 supernova - or the remnant of a lower mass star - a white dwarf - gains extra mass and explodes - that’s a type ...
  • 03:31: This “geomagnetic” field is generated by the convective motion in Earth’s outer core - which is a churning liquid mass of white-hot nickel and iron.

2020-12-15: The Supernova At The End of Time

  • 04:18: A new type of star had been discovered - white dwarfs.
  • 04:58: Meanwhile the outer layers would have been ejected, leaving its exposed core as the white dwarf.
  • 05:05: Most eminent physicists of the era were coming to believe that the white dwarf should be the fate of all stars.
  • 05:37: And in the extreme density of a white dwarf, electrons would indeed be traveling fast enough for relativity to change the physics.
  • 06:24: ... on the SS Pilsner, Chandra just knew that no white dwarf could exist above that mass limit - what we now call the ...
  • 07:16: In a white dwarf, the nuclei can never recapture their electrons to become atoms again.
  • 07:35: ... all white dwarfs must cool to the temperature of the ambient space - now a frigid ...
  • 07:49: Eventually, all white dwarf must fade to near-invisible nuggets we call black dwarfs.
  • 09:02: ... protons can decay, then the entire white dwarf will vaporize into a subatomic mist in a mere 10^32 or so years, ...
  • 10:50: ... means that a white dwarf - or now iron black dwarf - that was initially stable with a mass ...
  • 04:58: Meanwhile the outer layers would have been ejected, leaving its exposed core as the white dwarf.
  • 05:05: Most eminent physicists of the era were coming to believe that the white dwarf should be the fate of all stars.
  • 05:37: And in the extreme density of a white dwarf, electrons would indeed be traveling fast enough for relativity to change the physics.
  • 06:24: ... on the SS Pilsner, Chandra just knew that no white dwarf could exist above that mass limit - what we now call the Chandrasekhar ...
  • 07:16: In a white dwarf, the nuclei can never recapture their electrons to become atoms again.
  • 07:49: Eventually, all white dwarf must fade to near-invisible nuggets we call black dwarfs.
  • 09:02: ... protons can decay, then the entire white dwarf will vaporize into a subatomic mist in a mere 10^32 or so years, long ...
  • 10:50: ... means that a white dwarf - or now iron black dwarf - that was initially stable with a mass below ...
  • 05:37: And in the extreme density of a white dwarf, electrons would indeed be traveling fast enough for relativity to change the physics.
  • 04:18: A new type of star had been discovered - white dwarfs.
  • 07:35: ... all white dwarfs must cool to the temperature of the ambient space - now a frigid 3 ...

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

  • 15:59: ... limit is 1.4 times the mass of the sun - it’s the maximum mass of a white dwarf before crushing gravitational pressure causes electrons to be ...
  • 16:19: But what about white dwarfs that gain more mass after they form? Or that collide to have above that mass?
  • 16:36: ... the white dwarf exceeds the limit by cannibalizing a companion star, and also ...
  • 16:46: Instead you’re most likely to just get an explosion as thermonuclear fusion rips through the white dwarfs carbon and oxygen interior.
  • 15:59: ... limit is 1.4 times the mass of the sun - it’s the maximum mass of a white dwarf before crushing gravitational pressure causes electrons to be pounded ...
  • 16:36: ... the white dwarf exceeds the limit by cannibalizing a companion star, and also presumably ...
  • 16:19: But what about white dwarfs that gain more mass after they form? Or that collide to have above that mass?
  • 16:46: Instead you’re most likely to just get an explosion as thermonuclear fusion rips through the white dwarfs carbon and oxygen interior.

2020-08-17: How Stars Destroy Each Other

  • 00:44: Ejecting its outer layers, it became a searing hot, planet-sized orb of incredible density - a white dwarf.
  • 01:11: There, in the extreme surface gravity of the ultradense white dwarf, a layer of hydrogen built up.
  • 01:22: ... storm of fusion ripped around the planet-sized white dwarf, spraying its atmosphere into space and for a couple of weeks ...
  • 02:16: ... we’re going to look at the worst of these - from the novae produced by white dwarfs, to X-ray binaries created by neutron stars and black holes - and ...
  • 03:07: ... finally identified a nearby flaring white dwarf binary - a so-called cataclysmic variable - and realized that it ...
  • 03:30: They result when denser streams of matter hit the white dwarf and flare due to heat, but do not produce the storm of fusion of the classical nova.
  • 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: ... bright X-ray light is emitted as the gas hits the polar regions of the white dwarf - like a particularly violent ...
  • 04:59: Just replace the white dwarf with a neutron star or black hole.
  • 09:38: The white dwarf in these systems builds up mass until releasing it as a nova.
  • 09:47: The rest stays with the white dwarf, which slowly grows in mass.
  • 09:51: Eventually, the core of the white dwarf reaches a temperature of hundred of millions of Kelvin, and the star’s carbon and oxygen can begin to fuse.
  • 00:44: Ejecting its outer layers, it became a searing hot, planet-sized orb of incredible density - a white dwarf.
  • 01:11: There, in the extreme surface gravity of the ultradense white dwarf, a layer of hydrogen built up.
  • 01:22: ... storm of fusion ripped around the planet-sized white dwarf, spraying its atmosphere into space and for a couple of weeks shining 10s ...
  • 03:07: ... finally identified a nearby flaring white dwarf binary - a so-called cataclysmic variable - and realized that it was the ...
  • 03:30: They result when denser streams of matter hit the white dwarf and flare due to heat, but do not produce the storm of fusion of the classical nova.
  • 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: ... bright X-ray light is emitted as the gas hits the polar regions of the white dwarf - like a particularly violent ...
  • 04:59: Just replace the white dwarf with a neutron star or black hole.
  • 09:38: The white dwarf in these systems builds up mass until releasing it as a nova.
  • 09:47: The rest stays with the white dwarf, which slowly grows in mass.
  • 09:51: Eventually, the core of the white dwarf reaches a temperature of hundred of millions of Kelvin, and the star’s carbon and oxygen can begin to fuse.
  • 04:38: ... bright X-ray light is emitted as the gas hits the polar regions of the white dwarf - like a particularly violent ...
  • 03:07: ... finally identified a nearby flaring white dwarf binary - a so-called cataclysmic variable - and realized that it was the same ...
  • 09:51: Eventually, the core of the white dwarf reaches a temperature of hundred of millions of Kelvin, and the star’s carbon and oxygen can begin to fuse.
  • 01:22: ... storm of fusion ripped around the planet-sized white dwarf, spraying its atmosphere into space and for a couple of weeks shining 10s of ...
  • 02:16: ... we’re going to look at the worst of these - from the novae produced by white dwarfs, to X-ray binaries created by neutron stars and black holes - and much ...

2020-06-22: Building Black Holes in a Lab

  • 05:01: ... is in the opposite direction to the waves this is actually an analog white hole. Other experiments use a carefully-shaped hole in a tank to create ...

2020-05-18: Mapping the Multiverse

  • 09:45: It leads to what looks like a white hole.
  • 09:49: Now we saw that in the Schwarzschild solution, a white hole exists in the past of a purely hypothetical eternal non-rotating black hole.
  • 10:00: The Kerr black hole also has a white hole in the past, but it has one in the future too.
  • 10:18: You caught a glimpse of the entire history of that universe the moment you crossed into the white hole.
  • 10:25: That white hole will eject you as forcibly as the black hole pulled you down.
  • 10:49: If you try to head back to the white hole, you won’t find it - you’ll only find a new black hole that lies in its future.
  • 09:45: It leads to what looks like a white hole.
  • 09:49: Now we saw that in the Schwarzschild solution, a white hole exists in the past of a purely hypothetical eternal non-rotating black hole.
  • 10:00: The Kerr black hole also has a white hole in the past, but it has one in the future too.
  • 10:18: You caught a glimpse of the entire history of that universe the moment you crossed into the white hole.
  • 10:25: That white hole will eject you as forcibly as the black hole pulled you down.
  • 10:49: If you try to head back to the white hole, you won’t find it - you’ll only find a new black hole that lies in its future.
  • 09:49: Now we saw that in the Schwarzschild solution, a white hole exists in the past of a purely hypothetical eternal non-rotating black hole.

2020-04-22: Will Wormholes Allow Fast Interstellar Travel?

  • 04:50: ... universe. The black hole also has a mirror reflection that we call the white ...
  • 05:17: ... you could potentially reach this strange point - the nexus between the white and black ...
  • 04:50: ... universe. The black hole also has a mirror reflection that we call the white hole. ...

2020-03-31: What’s On The Other Side Of A Black Hole?

  • 06:15: ... looks just like the black hole - but with time reversed. This is the white hole, and we’ve this before - but perhaps we’ll get a little more ...
  • 09:39: ... where opinion is divided. Some think that the parallel universe AND the white hole are just coordinate reflections of the regular universe and black ...
  • 09:55: ... depends on how that reflection works. Perhaps you emerge from the past “white hole” traveling forward in time, or from the future black hole but ...
  • 10:35: ... parallel universe and white hole are needed in the map of the eternal Schwarzschild black hole in ...
  • 06:15: ... looks just like the black hole - but with time reversed. This is the white hole, and we’ve this before - but perhaps we’ll get a little more insight into ...
  • 09:39: ... where opinion is divided. Some think that the parallel universe AND the white hole are just coordinate reflections of the regular universe and black hole - ...
  • 09:55: ... depends on how that reflection works. Perhaps you emerge from the past “white hole” traveling forward in time, or from the future black hole but traveling ...
  • 10:35: ... parallel universe and white hole are needed in the map of the eternal Schwarzschild black hole in order ...
  • 09:55: ... depends on how that reflection works. Perhaps you emerge from the past “white hole” traveling forward in time, or from the future black hole but traveling backwards ...

2020-02-24: How Decoherence Splits The Quantum Multiverse

  • 00:21: The Heisenberg cut - is it the share of proceeds you send to Walter White to avoid, well, getting cut?

2020-01-06: How To Detect a Neutrino

  • 09:42: ... Ansar" (bright teal heart symbol) ♥ (text) "KORNHABERBROWN" (image: white PBS logo on navy background) (white text - slides out from behind logo) ...

2019-04-24: No Dark Matter = Proof of Dark Matter?

  • 00:03: ... soldier of ministereth in the background there but wasn't he Gandalf the White not the gray by the time the fellowshipped reached the tower of watch oh ...

2019-03-20: Is Dark Energy Getting Stronger?

  • 04:02: Type-1a supernovae– which result from exploding white dwarf stars.
  • 16:37: IT's called launcherone, and it'll launch from WhiteKnightTwo - the same plane that carries spaceshiptwo.

2019-03-13: Will You Travel to Space?

  • 05:59: Unity is dropped at 15,000 meters by its carrier, White Night, after which it blasts it's rocket engine sending it into a sub-orbital flight.

2019-01-24: The Crisis in Cosmology

  • 04:41: These result when white dwarfs, ancient remnants of dead stars,...
  • 17:01: ...should transform it into a white hole.
  • 04:41: These result when white dwarfs, ancient remnants of dead stars,...
  • 17:01: ...should transform it into a white hole.

2018-08-30: Is There Life on Mars?

  • 02:06: ... surface, and so measure Mars's 24-hour rotation rate, as well as a white spot on its south ...
  • 02:45: The white spot was indeed a polar ice cap.
  • 02:06: ... surface, and so measure Mars's 24-hour rotation rate, as well as a white spot on its south ...
  • 02:45: The white spot was indeed a polar ice cap.

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

  • 00:27: ... expand, the final atoms of hydrogen fuel and settle quietly into a dim white dwarf before slowly fading to black as it radiates away its remaining ...
  • 02:32: ... stars and black holes from long-extinct massive stars, as well as the white dwarfs left from lower-mass stars, including the recently extinguished ...
  • 02:51: Those white dwarfs will fade to black in only several billion years, far shorter than the several trillion-year lives of those stars.
  • 04:05: But neutron stars and white-- or, by now, black-- dwarfs are made of degenerate matter.
  • 00:27: ... expand, the final atoms of hydrogen fuel and settle quietly into a dim white dwarf before slowly fading to black as it radiates away its remaining ...
  • 02:32: ... stars and black holes from long-extinct massive stars, as well as the white dwarfs left from lower-mass stars, including the recently extinguished red ...
  • 02:51: Those white dwarfs will fade to black in only several billion years, far shorter than the several trillion-year lives of those stars.
  • 02:32: ... stars and black holes from long-extinct massive stars, as well as the white dwarfs left from lower-mass stars, including the recently extinguished red ...

2018-06-20: The Black Hole Information Paradox

  • 02:40: Hawking radiation is like a cosmic whiteboard eraser.

2018-05-09: How Gaia Changed Astronomy Forever

  • 03:06: After which, lower mass stars will become red giants, before leaving behind white dwarf remnants.
  • 03:32: We also see the full sequence of faint white dwarfs, showing the paths they follow as they slowly fade into blackness.
  • 03:39: ... evolutionary paths that may reveal the composition and past life of the white ...
  • 03:51: We see hot, newly formed white dwarfs, some of which are still embedded in the nebula of gas injected in the death of their star.
  • 08:54: Selman123 asks about the difference between a white dwarf and a red dwarf.
  • 09:03: A white dwarf is the remnant core of a low to mid-mass star after it burns out and ejects its outer layers, leaving only the hot core.
  • 09:11: White dwarfs aren't necessarily white.
  • 09:13: They start out blue and are expected to eventually fade, through white to red to black, but we always call them, white dwarfs.
  • 09:26: And we expect them to pass through white, and some to blue, at the ends of their lives.
  • 09:33: Until they burn out, and then, they're white dwarfs.
  • 03:06: After which, lower mass stars will become red giants, before leaving behind white dwarf remnants.
  • 03:39: ... evolutionary paths that may reveal the composition and past life of the white dwarf. ...
  • 08:54: Selman123 asks about the difference between a white dwarf and a red dwarf.
  • 09:03: A white dwarf is the remnant core of a low to mid-mass star after it burns out and ejects its outer layers, leaving only the hot core.
  • 03:06: After which, lower mass stars will become red giants, before leaving behind white dwarf remnants.
  • 03:32: We also see the full sequence of faint white dwarfs, showing the paths they follow as they slowly fade into blackness.
  • 03:51: We see hot, newly formed white dwarfs, some of which are still embedded in the nebula of gas injected in the death of their star.
  • 09:11: White dwarfs aren't necessarily white.
  • 09:13: They start out blue and are expected to eventually fade, through white to red to black, but we always call them, white dwarfs.
  • 09:33: Until they burn out, and then, they're white dwarfs.
  • 03:32: We also see the full sequence of faint white dwarfs, showing the paths they follow as they slowly fade into blackness.

2018-05-02: The Star at the End of Time

  • 00:47: And finally, our heirs or successors find new homes among the stars after the Sun's final death and transformation into a dim white dwarf.
  • 05:46: First, they shine white as their black-body spectrum spans the visible range, just like our Sun.
  • 06:00: ... will become composed of helium and will quietly contract into a helium white dwarf, supported by quantum mechanical electron degeneracy ...
  • 06:33: ... billion years from now, but they will have expired, leaving their own white ...
  • 06:43: And those white dwarfs will have faded long before the first red dwarf passes away.
  • 07:03: Individual points of white light will appear in the night sky, shining for up to a few billion years before winking out.
  • 00:47: And finally, our heirs or successors find new homes among the stars after the Sun's final death and transformation into a dim white dwarf.
  • 06:00: ... will become composed of helium and will quietly contract into a helium white dwarf, supported by quantum mechanical electron degeneracy ...
  • 06:33: ... billion years from now, but they will have expired, leaving their own white dwarfs. ...
  • 06:43: And those white dwarfs will have faded long before the first red dwarf passes away.
  • 07:03: Individual points of white light will appear in the night sky, shining for up to a few billion years before winking out.

2018-04-25: Black Hole Swarms

  • 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: ... the companion star to build up and then, fall very suddenly onto the white dwarf, producing a burst of ...
  • 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: ... the companion star to build up and then, fall very suddenly onto the white dwarf, producing a burst of ...

2018-04-18: Using Stars to See Gravitational Waves

  • 04:34: ... black holes, as well as the faint hum of thousands of binary pairs of white dwarfs, neutron stars, and black holes long before they ...
  • 08:03: A similar effect may cause white dwarf stars in binary orbits to explode as they absorb gravitational radiation from their own orbits.
  • 04:34: ... black holes, as well as the faint hum of thousands of binary pairs of white dwarfs, neutron stars, and black holes long before they ...

2018-03-07: Should Space be Privatized?

  • 11:48: ... that point, the whole thing becomes a white dwarf, but without the dramatic cycle of shell burning and red giant ...

2018-02-21: The Death of the Sun

  • 07:18: The sun has become a white dwarf.
  • 07:46: It's also possible that the iron core survives and will continue to orbit the white dwarf sun until the end of everything.
  • 07:18: The sun has become a white dwarf.
  • 07:46: It's also possible that the iron core survives and will continue to orbit the white dwarf sun until the end of everything.

2017-11-22: Suicide Space Robots

  • 13:00: A few of you point out that the EM drive now has a peer reviewed paper coming from Harold white at NASA's Eagle Works Laboratories.
  • 13:26: And there was a long list of systematic errors that may have been to blame, which Harold White listed with admirable honesty.

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

  • 14:47: Regarding our episode on white holes, a few of you wanted some clarification of a point I made.
  • 14:53: I said that the Big Bang is mathematically similar to a white hole, except that it doesn't possess a singularity.
  • 15:13: Now, we can imagine both the white hole and the earliest instant of the Big Bang as possessing infinite or at least extremely high density.
  • 15:21: But for the Big Bang, that density is everywhere, not concentrated at a single point, as in the case of the white hole.
  • 14:53: I said that the Big Bang is mathematically similar to a white hole, except that it doesn't possess a singularity.
  • 15:13: Now, we can imagine both the white hole and the earliest instant of the Big Bang as possessing infinite or at least extremely high density.
  • 15:21: But for the Big Bang, that density is everywhere, not concentrated at a single point, as in the case of the white hole.
  • 14:47: Regarding our episode on white holes, a few of you wanted some clarification of a point I made.

2017-08-30: White Holes

  • 00:14: In fact, it's the black hole's mirror twin-- the white hole.
  • 01:18: One such entity is the white hole.
  • 01:21: A white hole is the opposite of a black hole in a very literal mathematical sense.
  • 01:41: That makes a white hole a region of outward flowing space time.
  • 01:51: Nothing outside a white hole can ever enter, and everything inside must be ejected.
  • 01:56: Not even light can leave a black hole, hence the whole black thing, but light can only leave a white hole.
  • 02:05: So these might be expected to radiate like crazy, and white would be an understatement.
  • 02:12: ... before everyone gets too excited, white holes are probably a figment of mathematical imagination, but they're a ...
  • 02:26: White holes first emerged in the very earliest mathematical description of black holes.
  • 07:51: So far, this region fits perfectly the description of a white hole.
  • 07:56: The eternal black hole of the past technically is a white hole.
  • 08:06: One, light rays exiting that past white hole can never reach us.
  • 08:34: Even though this type of white hole isn't observable, some physicists have taken the description very seriously.
  • 08:41: The math describing the white hole is a perfectly good use of the Schwarzschild metric.
  • 09:01: So can new white holes actually form?
  • 09:12: ... although it's possible to build a white hole in general relativity, there are other laws of physics that the ...
  • 09:46: ... rare entropy dip could lead to an effective reversal of time and a white hole could ...
  • 10:09: We actually did talk about a case where a random drop in entropy lead to something very much like a white hole in this episode.
  • 10:18: ... it happens, the Big Bang looks-- mathematically, at least-- much like a white ...
  • 10:43: The difference between the Big Bang and a white hole is that the former possesses no singularity.
  • 10:57: It's been proposed that, when a black hole forms, a white hole forms on the opposite side.
  • 11:04: Energy entering the black hole exits the white hole.
  • 11:08: ... Lee Smolin takes it a step further to suggest that the resulting white hole is the Big Bang of a new baby universe and that, in fact, our ...
  • 11:32: The past white hole was revealed when we traced the eternal black hole backwards in time.
  • 00:14: In fact, it's the black hole's mirror twin-- the white hole.
  • 01:18: One such entity is the white hole.
  • 01:21: A white hole is the opposite of a black hole in a very literal mathematical sense.
  • 01:41: That makes a white hole a region of outward flowing space time.
  • 01:51: Nothing outside a white hole can ever enter, and everything inside must be ejected.
  • 01:56: Not even light can leave a black hole, hence the whole black thing, but light can only leave a white hole.
  • 07:51: So far, this region fits perfectly the description of a white hole.
  • 07:56: The eternal black hole of the past technically is a white hole.
  • 08:06: One, light rays exiting that past white hole can never reach us.
  • 08:34: Even though this type of white hole isn't observable, some physicists have taken the description very seriously.
  • 08:41: The math describing the white hole is a perfectly good use of the Schwarzschild metric.
  • 09:12: ... although it's possible to build a white hole in general relativity, there are other laws of physics that the universe ...
  • 09:46: ... rare entropy dip could lead to an effective reversal of time and a white hole could ...
  • 10:09: We actually did talk about a case where a random drop in entropy lead to something very much like a white hole in this episode.
  • 10:18: ... it happens, the Big Bang looks-- mathematically, at least-- much like a white hole. ...
  • 10:43: The difference between the Big Bang and a white hole is that the former possesses no singularity.
  • 10:57: It's been proposed that, when a black hole forms, a white hole forms on the opposite side.
  • 11:04: Energy entering the black hole exits the white hole.
  • 11:08: ... Lee Smolin takes it a step further to suggest that the resulting white hole is the Big Bang of a new baby universe and that, in fact, our universe ...
  • 11:32: The past white hole was revealed when we traced the eternal black hole backwards in time.
  • 10:57: It's been proposed that, when a black hole forms, a white hole forms on the opposite side.
  • 08:34: Even though this type of white hole isn't observable, some physicists have taken the description very seriously.
  • 02:12: ... before everyone gets too excited, white holes are probably a figment of mathematical imagination, but they're a ...
  • 02:26: White holes first emerged in the very earliest mathematical description of black holes.
  • 09:01: So can new white holes actually form?

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

  • 01:31: To our eyes it twinkles bluish white on the night sky.

2017-01-19: The Phantom Singularity

  • 12:36: ... our Patreon Google Hangout where he pretty much obliterated the entire white hole hypothesis by correctly pointing out that if they existed in any ...
  • 12:53: ... week, we inaugurated the "Space Time" Journal Club by looking at Harold White et al's paper on an apparently positive vacuum test of the EM ...
  • 12:36: ... our Patreon Google Hangout where he pretty much obliterated the entire white hole hypothesis by correctly pointing out that if they existed in any great ...

2017-01-11: The EM Drive: Fact or Fantasy?

  • 01:23: ... one of the Space Time Journal Club, we're jumping into Harold "Sonny" White, et al., 2016 "Measurement of Impulsive Thrust from a Closed ...
  • 08:05: ... two separate papers, Harold White performs computer simulations, which he argues demonstrates that such a ...

2016-12-08: What Happens at the Event Horizon?

  • 11:04: And down here we have what we call a white hole.
  • 14:14: ... the recent paper out of Eagle Works Labs, Herald White and collaborators present some results on the thrust produced by their ...
  • 11:04: And down here we have what we call a white hole.

2016-11-09: Did Dark Energy Just Disappear?

  • 00:37: These exploding white dwarf stars have predictable brightnesses that allow astronomers to figure out how far away they are.
  • 02:52: However, in the 18 years since the first studies, we've observed a lot more of these exploding white dwarfs.
  • 00:37: These exploding white dwarf stars have predictable brightnesses that allow astronomers to figure out how far away they are.
  • 02:52: However, in the 18 years since the first studies, we've observed a lot more of these exploding white dwarfs.

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

  • 10:38: So many of you, including Neil deGrasse Tyson, point out that the sun is actually white and not yellow.
  • 10:46: ... the sun usually appears white to our eyes and so to our brains, and since the entire concept of color ...
  • 11:00: But this observed whiteness is a result of the fact that our color sensitivity is limited.
  • 11:25: Our eyes can't register the difference in brightness across the visible part of the spectrum, so we register the color as white.
  • 11:00: But this observed whiteness is a result of the fact that our color sensitivity is limited.

2016-05-25: Is an Ice Age Coming?

  • 07:12: You might be wondering, when are the glaciers going to rush down from the north, bringing polar bears, white walkers, Tontons?

2016-05-04: Will Starshot's Insterstellar Journey Succeed?

  • 11:03: ... need some sort of luminosity reference point before we can start using white dwarf supernovae or Type 1a supernovae, the standard ...
  • 11:25: We do that by finding independent distances to white dwarf supernovae in nearby galaxies.
  • 11:03: ... need some sort of luminosity reference point before we can start using white dwarf supernovae or Type 1a supernovae, the standard ...
  • 11:25: We do that by finding independent distances to white dwarf supernovae in nearby galaxies.
  • 11:03: ... need some sort of luminosity reference point before we can start using white dwarf supernovae or Type 1a supernovae, the standard ...
  • 11:25: We do that by finding independent distances to white dwarf supernovae in nearby galaxies.

2016-04-27: What Does Dark Energy Really Do?

  • 03:51: It's a type Ia or white dwarf supernova.
  • 03:55: Take a white dwarf, the leftover core of a dead, low-mass star like our sun, and let it cannibalize some of the material from a binary companion.
  • 04:24: When you catch a white dwarf supernova, you know its distance and redshift.
  • 06:03: ... separate teams of astronomers spent years catching white dwarf supernovae exploding in galaxies billions of light years away to ...
  • 09:19: That's what we see in our white dwarf supernova measurements.
  • 03:51: It's a type Ia or white dwarf supernova.
  • 03:55: Take a white dwarf, the leftover core of a dead, low-mass star like our sun, and let it cannibalize some of the material from a binary companion.
  • 04:24: When you catch a white dwarf supernova, you know its distance and redshift.
  • 06:03: ... separate teams of astronomers spent years catching white dwarf supernovae exploding in galaxies billions of light years away to measure ...
  • 09:19: That's what we see in our white dwarf supernova measurements.
  • 03:51: It's a type Ia or white dwarf supernova.
  • 04:24: When you catch a white dwarf supernova, you know its distance and redshift.
  • 09:19: That's what we see in our white dwarf supernova measurements.
  • 06:03: ... separate teams of astronomers spent years catching white dwarf supernovae exploding in galaxies billions of light years away to measure the past ...

2016-04-06: We Are Star Stuff

  • 05:24: And in most cases, remains locked forever inside the final white dwarf.
  • 08:47: ... a white dwarf, a remnant of a low mass star like the sun, has a binary partner ...
  • 05:24: And in most cases, remains locked forever inside the final white dwarf.
  • 08:47: ... a white dwarf, a remnant of a low mass star like the sun, has a binary partner star and ...

2016-02-11: LIGO's First Detection of Gravitational Waves!

  • 06:48: ... see the slow ringing of binary white dwarf stars in our own galaxy, as well as the final dance of pairs of ...

2015-11-18: 5 Ways to Stop a Killer Asteroid

  • 05:47: Seriously, arm a spacecraft with a cosmic-sized can of spray paint, and color one side of the asteroid white.

2015-08-27: Watch THIS! (New Host + Challenge Winners)

  • 03:19: ... with Andromeda doesn't disrupt our planetary system, it'll be a white dwarf remnant, and after the sun ejects its outer layers, there's a ...
  • 04:00: Let's go to the white board.
  • 03:19: ... with Andromeda doesn't disrupt our planetary system, it'll be a white dwarf remnant, and after the sun ejects its outer layers, there's a planetary ...

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

  • 08:12: ... of "Spacetime." Last week we asked whether Australia would ever get a White Christmas in order to discuss the calendar, the seasons, and their ...
  • 08:55: Australian white Christmas was just a motif for talking about reversal of the seasons relative to the calendar.
  • 09:00: ... and QuannanHade, namely that Santa's sleigh is already pulled by six white boomers, or older white furred ...
  • 08:12: ... of "Spacetime." Last week we asked whether Australia would ever get a White Christmas in order to discuss the calendar, the seasons, and their connection to ...
  • 08:55: Australian white Christmas was just a motif for talking about reversal of the seasons relative to the calendar.
  • 09:00: ... that Santa's sleigh is already pulled by six white boomers, or older white furred ...

2015-06-24: The Calendar, Australia & White Christmas

  • 02:01: ... change, wouldn't that mean Christmas on the beach for the north and white Christmas for the south after a few thousand years or so, depending on ...
  • 02:37: ... always remain close to the spring equinox, which prevents a southern white Christmas by ...
  • 04:14: Other factors could bring the south a white Christmas even sooner.
  • 02:01: ... change, wouldn't that mean Christmas on the beach for the north and white Christmas for the south after a few thousand years or so, depending on exactly ...
  • 02:37: ... always remain close to the spring equinox, which prevents a southern white Christmas by ...
  • 04:14: Other factors could bring the south a white Christmas even sooner.

2015-06-03: Is Gravity An Illusion?

  • 01:11: ... to pause me right now and go watch this super awesome 1960s black and white video from MIT all about frames of ...
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