Loading video...

Video Failed to Load

There was a problem loading this video. This could be due to a temporary network issue or the video might be unavailable.

A perfect water vortex folding inward, the same geometry that bends spacetime around a black hole

Amazing Physics

657,917 subscribers

43,619 views • 6 days ago •via X (Twitter)

Science & Technology

Anya Rossi• Live Now

Private livecam show

0 Comments

No comments available

Comments from the original post will appear here

Related Videos

White Holes Don’t Push You Way. Spacetime Refuses Your Future. A White Hole appears in the maximally extended Schwarzschild solution of General Relativity, the full mathematical extension of the Spacetime around an eternal, non-rotating Black Hole. The exterior geometry is the same Schwarzschild geometry ds² = −(1 − 2M/r)dt² + (1 − 2M/r)⁻¹dr² + r²dΩ² But the causal direction is reversed. For a Black Hole, future-directed paths can cross the horizon inward. For a White Hole, future-directed paths can emerge from the horizon, but outside particles cannot enter that region. The object has not been observed in nature. But inside the Mathematics of General Relativity, it is a real sector of the extended Schwarzschild Spacetime... the Black Hole’s time-reversed counterpart.

White Holes Don’t Push You Way. Spacetime Refuses Your Future. A White Hole appears in the maximally extended Schwarzschild solution of General Relativity, the full mathematical extension of the Spacetime around an eternal, non-rotating Black Hole. The exterior geometry is the same Schwarzschild geometry ds² = −(1 − 2M/r)dt² + (1 − 2M/r)⁻¹dr² + r²dΩ² But the causal direction is reversed. For a Black Hole, future-directed paths can cross the horizon inward. For a White Hole, future-directed paths can emerge from the horizon, but outside particles cannot enter that region. The object has not been observed in nature. But inside the Mathematics of General Relativity, it is a real sector of the extended Schwarzschild Spacetime... the Black Hole’s time-reversed counterpart.

Mathelirium

31,120 views • 3 months ago

A Black Hole Can Be Dragged Through Spacetime A Black Hole does not have to sit still. Einstein’s equations allow a stranger possibility... a Black Hole that accelerates. This is the C-metric, an exact solution of General Relativity describing an accelerating Black Hole. The Black Hole accelerates because the geometry of Spacetime says it must. The C-metric is one of those exact solutions that reminds us how wild General Relativity really is. Gravity is not just attraction, and Spacetime is not just a stage. Sometimes the stage itself contains the force. #Astrophysics #GeneralRelativity #Einstein #CMetric #BlackHole #CosmicStrings #Spacetime #Cosmology #Mathematics #Physics

A Black Hole Can Be Dragged Through Spacetime A Black Hole does not have to sit still. Einstein’s equations allow a stranger possibility... a Black Hole that accelerates. This is the C-metric, an exact solution of General Relativity describing an accelerating Black Hole. The Black Hole accelerates because the geometry of Spacetime says it must. The C-metric is one of those exact solutions that reminds us how wild General Relativity really is. Gravity is not just attraction, and Spacetime is not just a stage. Sometimes the stage itself contains the force. #Astrophysics #GeneralRelativity #Einstein #CMetric #BlackHole #CosmicStrings #Spacetime #Cosmology #Mathematics #Physics

Mathelirium

789,165 views • 1 month ago

What Happens When a Black Hole Does More Than Fall? In General Relativity, a rotating Black Hole is described by the Kerr Metric. Its spin does something strange to spacetime... it drags the geometry around with it. The horizon sits at r₊ = M + √(M² - a²) but outside it there is another surface, the Ergosphere, r_E(θ) = M + √(M² - a²cos²θ) Inside that region, Spacetime is being swept around so strongly that remaining still is no longer possible. Every particle, every light thread, every local observer is forced to rotate with the geometry. For this scene, the C-metric acceleration remains alive in the background and the Black Hole still moves through the fabric, pulled along an axial defect. But the main event is Kerr frame dragging. The fabric twists. The Ergosphere breathes. Light paths shear into spirals. Particles that try to cross the region get carried around before falling inward. #GeneralRelativity #BlackHole #KerrMetric #FrameDragging #Ergosphere #Spacetime #EinsteinEquations #Astrophysics #Physics

What Happens When a Black Hole Does More Than Fall? In General Relativity, a rotating Black Hole is described by the Kerr Metric. Its spin does something strange to spacetime... it drags the geometry around with it. The horizon sits at r₊ = M + √(M² - a²) but outside it there is another surface, the Ergosphere, r_E(θ) = M + √(M² - a²cos²θ) Inside that region, Spacetime is being swept around so strongly that remaining still is no longer possible. Every particle, every light thread, every local observer is forced to rotate with the geometry. For this scene, the C-metric acceleration remains alive in the background and the Black Hole still moves through the fabric, pulled along an axial defect. But the main event is Kerr frame dragging. The fabric twists. The Ergosphere breathes. Light paths shear into spirals. Particles that try to cross the region get carried around before falling inward. #GeneralRelativity #BlackHole #KerrMetric #FrameDragging #Ergosphere #Spacetime #EinsteinEquations #Astrophysics #Physics

Mathelirium

27,112 views • 1 month ago

When Light Becomes Heavy Enough to Trap Itself Can light collapse into a black hole? In General Relativity, light is not weightless in the geometric sense. It has energy, it carries momentum, and energy curves Spacetime. A Vaidya-type collapse describes a mass that grows because radiation is falling inward. The mathematics is the same brutal idea behind Einstein’s equation Gᵤᵥ = 8πTᵤᵥ If the stress-energy Tᵤᵥ is made from radiation, then light itself becomes a source of curvature. As more radiation falls inward, the mass aspect grows, the Spacetime fabric tightens, and a clean black horizon appears where escaping paths begin to fail. #GeneralRelativity #EinsteinEquations #BlackHole #Spacetime #Astrophysics #TheoreticalPhysics #Light #Mathematics #Science

When Light Becomes Heavy Enough to Trap Itself Can light collapse into a black hole? In General Relativity, light is not weightless in the geometric sense. It has energy, it carries momentum, and energy curves Spacetime. A Vaidya-type collapse describes a mass that grows because radiation is falling inward. The mathematics is the same brutal idea behind Einstein’s equation Gᵤᵥ = 8πTᵤᵥ If the stress-energy Tᵤᵥ is made from radiation, then light itself becomes a source of curvature. As more radiation falls inward, the mass aspect grows, the Spacetime fabric tightens, and a clean black horizon appears where escaping paths begin to fail. #GeneralRelativity #EinsteinEquations #BlackHole #Spacetime #Astrophysics #TheoreticalPhysics #Light #Mathematics #Science

Mathelirium

27,635 views • 1 month ago

A visualization of how wormholes are a manipulation of spacetime geometry.

A visualization of how wormholes are a manipulation of spacetime geometry.

Ashton Forbes

49,021 views • 2 months ago

String Theory makes an ambitious proposal: Quantum excitations and Spacetime geometry may arise from the same extended objects.

String Theory makes an ambitious proposal: Quantum excitations and Spacetime geometry may arise from the same extended objects.

Mathelirium

32,499 views • 1 month ago

Black Hole Can Ring Like a Bell A Black Hole can vibrate after it is disturbed. Instead of settling instantly, its horizon releases gravitational waves in fading tones called quasinormal modes. This is commonly known as Ringdown. Each tone carries information about the black hole’s final mass and spin, which is why physicists call this Black-Hole Spectroscopy. In a way, when Spacetime strikes a Black Hole, the Black Hole answers with its own gravitational sound. #BlackHole #GeneralRelativity #GravitationalWaves #Spacetime #Einstein #Astrophysics #Physics #Mathematics #Cosmology

Black Hole Can Ring Like a Bell A Black Hole can vibrate after it is disturbed. Instead of settling instantly, its horizon releases gravitational waves in fading tones called quasinormal modes. This is commonly known as Ringdown. Each tone carries information about the black hole’s final mass and spin, which is why physicists call this Black-Hole Spectroscopy. In a way, when Spacetime strikes a Black Hole, the Black Hole answers with its own gravitational sound. #BlackHole #GeneralRelativity #GravitationalWaves #Spacetime #Einstein #Astrophysics #Physics #Mathematics #Cosmology

Mathelirium

30,802 views • 1 month ago

What If a Black Hole Shredded Worlds Before They Fell In? Far away from a Black Hole, an object can orbit, drift past, or escape. But if its path carries it too close, the geometry decides its fate. The exterior geometry is Schwarzschild-like ds² = -(1 - 2M/r)dt² + (1 - 2M/r)⁻¹dr² + r²dΩ² The event horizon sits at rₛ = 2M The photon sphere sits at rₚₕ = 3M #Astrophysics #GeneralRelativity #Einstein #BlackHole #Spacetime #TidalForces #PhotonSphere #Cosmology #Mathematics

What If a Black Hole Shredded Worlds Before They Fell In? Far away from a Black Hole, an object can orbit, drift past, or escape. But if its path carries it too close, the geometry decides its fate. The exterior geometry is Schwarzschild-like ds² = -(1 - 2M/r)dt² + (1 - 2M/r)⁻¹dr² + r²dΩ² The event horizon sits at rₛ = 2M The photon sphere sits at rₚₕ = 3M #Astrophysics #GeneralRelativity #Einstein #BlackHole #Spacetime #TidalForces #PhotonSphere #Cosmology #Mathematics

Mathelirium

40,811 views • 1 month ago

A gravitational singularity is a point at the center of a black hole where spacetime curvature becomes infinite and the known laws of physics break down.

A gravitational singularity is a point at the center of a black hole where spacetime curvature becomes infinite and the known laws of physics break down.

Physics In History

80,212 views • 7 months ago

Geometry of the Universe ☄️ BLACK HOLE. Subscribe.

Geometry of the Universe ☄️ BLACK HOLE. Subscribe.

Black Hole

20,761 views • 6 months ago

A White Hole is a Black Hole Running Backward A Black Hole is famous because it lets things fall in, but never lets them come back out. A White Hole is the time-reversed version of that idea. In the full Schwarzschild solution of General Relativity, the Black-Hole region and the White-Hole region appear as two different causal parts of the same exact geometry. Outside the horizon, the metric is the usual Schwarzschild metric ds² = -(1 - 2M/r)dt² + (1 - 2M/r)⁻¹dr² + r²dΩ². The horizon sits at rₛ = 2M, using G = c = 1. For an ordinary Black Hope, future-directed paths can cross this surface inward. Once they do, they cannot return to the outside universe. For a White Hole, the arrow is reversed and particles and light can come out from the horizon, but outside observers cannot enter it. No one has observed a physical White Hole. It may be an ideal solution rather than an object that nature actually forms. But as Mathematics, it is one of the strangest lessons of General Relativity: The equations allow a horizon that throws the universe outward. #WhiteHoles #GeneralRelativity #Schwarzschild #Spacetime #BlackHoles #Cosmology #Physics #Mathematics #Astrophysics #Astronomy

A White Hole is a Black Hole Running Backward A Black Hole is famous because it lets things fall in, but never lets them come back out. A White Hole is the time-reversed version of that idea. In the full Schwarzschild solution of General Relativity, the Black-Hole region and the White-Hole region appear as two different causal parts of the same exact geometry. Outside the horizon, the metric is the usual Schwarzschild metric ds² = -(1 - 2M/r)dt² + (1 - 2M/r)⁻¹dr² + r²dΩ². The horizon sits at rₛ = 2M, using G = c = 1. For an ordinary Black Hope, future-directed paths can cross this surface inward. Once they do, they cannot return to the outside universe. For a White Hole, the arrow is reversed and particles and light can come out from the horizon, but outside observers cannot enter it. No one has observed a physical White Hole. It may be an ideal solution rather than an object that nature actually forms. But as Mathematics, it is one of the strangest lessons of General Relativity: The equations allow a horizon that throws the universe outward. #WhiteHoles #GeneralRelativity #Schwarzschild #Spacetime #BlackHoles #Cosmology #Physics #Mathematics #Astrophysics #Astronomy

Mathelirium

44,259 views • 1 month ago

White Hole - A Black Hole With Time Reversed A White Hole is the time-reversed shadow of a Black Hole. It appears in the maximally extended Schwarzschild solution of General Relativity. The exterior geometry is the same ds² = −(1 − 2M/r)dt² + (1 − 2M/r)⁻¹dr² + r²dΩ² The difference is causal. A Black Hole lets paths enter but not escape. A White Hole lets paths emerge but not enter. No White Hole has been observed. But inside the equations of GR, the question is real: What does a Black Hole look like when time runs the other way?

White Hole - A Black Hole With Time Reversed A White Hole is the time-reversed shadow of a Black Hole. It appears in the maximally extended Schwarzschild solution of General Relativity. The exterior geometry is the same ds² = −(1 − 2M/r)dt² + (1 − 2M/r)⁻¹dr² + r²dΩ² The difference is causal. A Black Hole lets paths enter but not escape. A White Hole lets paths emerge but not enter. No White Hole has been observed. But inside the equations of GR, the question is real: What does a Black Hole look like when time runs the other way?

Mathelirium

74,866 views • 3 months ago

A graphical representation showing the region around a black hole.

A graphical representation showing the region around a black hole.

Black Hole

39,690 views • 3 months ago

What you’re seeing is a Riemannian Manifold—the mathematical "skeleton" of our universe. While most see a grid, physicists see the secret language of gravity and curved space-time. The transformation you see at 0:32 is a total "glitch" in the logic of a flat world, but it’s exactly how the fabric of existence behaves when it meets mass. In our daily lives, we assume a straight line is the shortest distance between two points, but in a Riemannian world, "straight" is an illusion. This visual captures the moment where geometry transcends the 3rd dimension, twisting and folding back on itself in a way that would make Euclidean logic shatter. It is the same mind-bending curvature that governs everything from the orbit of planets to the way light bends around a black hole.

What you’re seeing is a Riemannian Manifold—the mathematical "skeleton" of our universe. While most see a grid, physicists see the secret language of gravity and curved space-time. The transformation you see at 0:32 is a total "glitch" in the logic of a flat world, but it’s exactly how the fabric of existence behaves when it meets mass. In our daily lives, we assume a straight line is the shortest distance between two points, but in a Riemannian world, "straight" is an illusion. This visual captures the moment where geometry transcends the 3rd dimension, twisting and folding back on itself in a way that would make Euclidean logic shatter. It is the same mind-bending curvature that governs everything from the orbit of planets to the way light bends around a black hole.

Mathematica

28,564 views • 4 months ago

Travis Taylor: "Our Universe lives inside a Black Hole" 😱 “The math keeps pointing to the same place. A black hole between 5 and 10 solar masses, with the best fit right around 7.2.” He arrived at the model by starting with something unexpected: the way video game world maps handle boundaries. That led him to event horizons, then to a Hawking radiation analogy that locked the numbers in place. The paper and the calculations line up on a stellar mass black hole as the container for everything we observe. If the model holds, the edge of our observable universe is not just a light-travel limit. It is the event horizon of a black hole whose mass sits in that narrow 5 to 10 solar mass window, peaking near 7.2. The same mathematics that describe the interior geometry of such a black hole also reproduce the expansion history and the cosmic horizon we measure. It is a clean, testable claim built from the paper’s equations rather than speculation. The numbers either fit or they do not. So far they do.

Travis Taylor: "Our Universe lives inside a Black Hole" 😱 “The math keeps pointing to the same place. A black hole between 5 and 10 solar masses, with the best fit right around 7.2.” He arrived at the model by starting with something unexpected: the way video game world maps handle boundaries. That led him to event horizons, then to a Hawking radiation analogy that locked the numbers in place. The paper and the calculations line up on a stellar mass black hole as the container for everything we observe. If the model holds, the edge of our observable universe is not just a light-travel limit. It is the event horizon of a black hole whose mass sits in that narrow 5 to 10 solar mass window, peaking near 7.2. The same mathematics that describe the interior geometry of such a black hole also reproduce the expansion history and the cosmic horizon we measure. It is a clean, testable claim built from the paper’s equations rather than speculation. The numbers either fit or they do not. So far they do.

Interstellar

73,244 views • 4 days ago

You're watching spacetime in motion...two spinning black holes orbit, twist, and merge, dragging the very geometry of the universe into a luminous storm. Their union births a single remnant that fires smoke-wreathed jet as gravitational waves ring the cosmic fabric itself. 🤩😍 #Math #Physics #Astrophysics #SciArt #MathArt

You're watching spacetime in motion...two spinning black holes orbit, twist, and merge, dragging the very geometry of the universe into a luminous storm. Their union births a single remnant that fires smoke-wreathed jet as gravitational waves ring the cosmic fabric itself. 🤩😍 #Math #Physics #Astrophysics #SciArt #MathArt

Mathelirium

42,531 views • 8 months ago

Stealing Energy from a Rotating Black Hole A rotating black hole doesn’t just pull things in. It drags spacetime itself into motion. In the spinning region just outside the horizon, nothing can remain still in any normal sense. That strange rule opens a loophole. One incoming body can split, with one piece swallowed while the other escapes with more energy than it came in with. A Penrose-style heist where the difference is paid for by the black hole’s rotation. The same idea shows up in wave form. A coherent packet can skim that region and return brighter, as if the geometry itself acted like an amplifier. Split near the ergosphere and you can steal spin. Skim it as a wave and you can come back louder.

Stealing Energy from a Rotating Black Hole A rotating black hole doesn’t just pull things in. It drags spacetime itself into motion. In the spinning region just outside the horizon, nothing can remain still in any normal sense. That strange rule opens a loophole. One incoming body can split, with one piece swallowed while the other escapes with more energy than it came in with. A Penrose-style heist where the difference is paid for by the black hole’s rotation. The same idea shows up in wave form. A coherent packet can skim that region and return brighter, as if the geometry itself acted like an amplifier. Split near the ergosphere and you can steal spin. Skim it as a wave and you can come back louder.

Mathelirium

20,314 views • 6 months ago