λL ≤ 2πkBT/ℏ
A scientific exploration of black hole physics through quantum chaos theory, covering Schwarzschild and Kerr geometries, information scrambling dynamics, the MSS bound, and holographic correspondences.
Real black holes from EHT, LIGO/Virgo, and multi-wavelength observations. Select one to see calculated properties.
rs = 2GM/c²
TH = ℏc³/(8πGMkB)
SBH = kBA/(4lP²)
λL ≤ 2πkBT/ℏ
Fundamental structure and properties of black holes based on Einstein's general relativity.
A point of infinite density at the center of a black hole. All known laws of physics break down here.
ρ → ∞
Singularity density
The boundary from which nothing, including light, can escape. Radius determined by mass.
rs = 2GM/c²
Schwarzschild radius
Unstable circular orbit for photons at r = 1.5rs. Light can temporarily orbit.
rph = 3GM/c²
Photon sphere radius
Matter spinning and falling into the black hole, emitting intense radiation due to frictional heating.
L = ηṀc²
Accretion luminosity (η ≈ 0.1)
Region outside the event horizon of a rotating (Kerr) black hole where spacetime is dragged by rotation.
re = M + √(M² - a²cos²θ)
Ergosphere outer boundary
Innermost Stable Circular Orbit - the deepest stable circular orbit before matter spirals inward.
rISCO = 6GM/c² (Schwarzschild)
3rs for non-rotating
Non-rotating, uncharged. The simplest solution to Einstein's equations.
ds² = -(1-2M/r)dt² + (1-2M/r)⁻¹dr² + r²dΩ²
Rotating, uncharged. The most realistic model for astrophysical black holes.
Has spin parameter a = J/Mc
Non-rotating, charged. Has two horizons (inner & outer).
r± = M ± √(M² - Q²)
Rotating and charged. The most general solution for electrovacuum black holes.
Combination of parameters M, J, Q
Black holes as maximally chaotic systems - quantum information scrambling and connection with holography.
In classical chaotic systems, distance between trajectories grows exponentially: δx(t) ~ eλt. Black holes have a maximal Lyapunov exponent bounded by quantum mechanics.
λL ≤ 2πkBT/ℏ
Maldacena-Shenker-Stanford bound (2016). Black holes saturate this bound in holographic theories.
λBH = 2πTH = κ
(surface gravity)
Out-of-Time-Order Correlator - the main diagnostic for quantum chaos.
C(t) = ⟨[W(t), V]†[W(t), V]⟩
Measures how fast perturbations spread in a quantum system.
Time required for information to "scramble" evenly throughout the system.
t* ~ (ℏ/2πT) log S
S = Bekenstein-Hawking entropy. For BH: t* ~ rs log(S)
Black hole oscillation modes that decay exponentially - fingerprint of chaos.
ω = ωR - iωI
Poles in Green's function, related to Lyapunov exponent.
Duality between gravity in Anti-de Sitter (AdS) space and Conformal Field Theory (CFT) on its boundary. Black hole in bulk ↔ thermal state on boundary.
Sachdev-Ye-Kitaev model - system of N fermions with random interactions. Maximally chaotic and has a gravitational dual in nearly-AdS₂.
H = Σijkl Jijkl ψiψjψkψl
In holography, small perturbations at the boundary "fall" into the black hole and spread chaotically.
vB = √(d/2(d-1)) × 2πT
vB = butterfly velocity
Study of how quantum information spreads within the horizon - key to understanding the information paradox.
Connection between volume of the region behind the horizon and computational complexity of the dual quantum state.
How individual black hole eigenstates encode thermal physics - ETH in gravitational systems.
Level spacing statistics of quasinormal modes follow random matrix distributions (GUE/GOE).
Fundamental relationship between gravity, thermodynamics, and quantum mechanics.
Surface gravity κ is constant on the event horizon of a stationary black hole.
Mass change is related to area change, angular momentum, and charge.
dM = (κ/8π)dA + ΩdJ + ΦdQ
Event horizon area never decreases in any classical process.
δA ≥ 0
It is impossible to reduce surface gravity κ to zero through any finite physical process.
Hawking's discovery (1974) that black holes radiate thermally demonstrated that the thermodynamic analogy is remarkably precise - black holes truly have temperature and entropy.
TH = ℏκ/2πkBc = ℏc³/8πGMkB
For M = M☉: T ≈ 60 nanoKelvin
SBH = kBA/4lP² = kBc³A/4Gℏ
Entropy proportional to AREA, not volume!
tevap ≈ 5120πG²M³/ℏc⁴
For M = M☉: t ≈ 10⁶⁷ years
Virtual pair creation near horizon
If a black hole fully evaporates via Hawking radiation (which is thermal/random), where does the information about what fell in go? This conflicts with quantum mechanical unitarity!
Radiation entropy initially rises, then falls after "Page time" - information exits gradually.
Generalized entropy formula with "quantum extremal surfaces" reproduces the Page curve.
Entanglement (EPR) is equivalent to wormholes (Einstein-Rosen bridge) - Maldacena & Susskind.
AMPS paradox: is there a "firewall" at the horizon that destroys infalling observers?
Observational evidence for the existence of black holes from various astronomical methods.
First direct image of a supermassive black hole at the center of Messier 87 galaxy. Mass ~6.5 billion M☉, distance 55 million light years.
Supermassive black hole at the center of the Milky Way. Orbits of S-stars provide undeniable evidence.
LIGO/Virgo detects binary black hole mergers. GW150914: ~36 + 29 M☉ → 62 M☉
Binary star systems with stellar-mass black holes. Matter accretion emits intense X-rays.
Active galactic nuclei powered by supermassive black holes - the most luminous sources in the universe.
Collection of black hole images and visualizations from NASA and global observatories.
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"A bound on chaos" - arXiv:1503.01409
SYK model foundations - Phys. Rev. Lett. 70, 3339
"Black hole explosions?" - Nature 248, 30-31
"Black holes and entropy" - Phys. Rev. D 7, 2333
"Jerusalem Lectures on Black Holes and Quantum Information"
"An Introduction to Black Holes, Information and the String Theory Revolution"