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Black Holes
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Lecture notes for a 'Part III' course 'Black Holes' given in DAMTP, Cambridge. The course covers some of the developments in Black Hole physics of the 1960s and 1970s.
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Cited by 10 Pith papers
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Derivation of the Smarr formula from the Komar charge in Einstein-nonlinear electrodynamics theories and applications to regular black holes
Derives Smarr formula from generalized Komar charge in 4D Einstein-NLED theories by treating coupling constant as dynamical field, and analyzes thermodynamics of regular Bardeen black hole.
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Bekenstein-Hawking temperature from the Schwarzian
Bekenstein-Hawking temperature is completely determined from the projective structure on the Killing horizon because the Schwarzian of the affine parameter equals minus half the square of surface gravity.
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The Smarr Formula is Gauss's Law: A Kerr-Schild Single-Copy Perspective
The Smarr formula is structurally identical to the single-copy Gauss's law for Kerr-Schild black holes, with the AdS pressure-volume term arising from gauge background subtraction.
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Strings near BTZ black holes: A Carrollian Chronicle
The paper classifies families of closed bosonic string solutions in the near-horizon non-extremal BTZ spacetime and identifies novel features via string-Carroll expansion.
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Gravity as emergent phenomena for spherically symmetric black hole accretion of multi-component flow with relativistic equation of state
Spherical accretion of a multi-species relativistic fluid with variable gamma produces an acoustic black hole metric whose surface gravity grows with flow energy and proton fraction.
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Modular quantization and black holes
Modular quantization of a single holographic CFT reproduces exact Hartle-Hawking correlators of smooth BTZ black holes in the semiclassical limit while yielding non-smooth stretched-horizon descriptions at finite GN.
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Null geodesics, causal structure, and matter accretion in Lorentzian-Euclidean black holes
In the Lorentzian-Euclidean black hole, photons and massive particles are claimed to be unable to cross the event horizon, making the spacetime geodesically complete and avoiding the central singularity.
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Gravastars with Kuchowicz Metric Potential in $f(R, \Sigma, T)$ Gravity
A gravastar model with a Kuchowicz metric potential is solved in f(R,Σ,T) gravity, yielding an allegedly singularity-free three-region solution with an ultra-relativistic shell.
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On the nature of the black hole information problem
The paper reviews the classical and semiclassical arguments behind the black hole information problem and catalogs the assumptions that the problem depends on.
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The physics of gravitational waves
Lecture notes deriving gravitational wave physics from first principles in general relativity for PhD and advanced MSc students.
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