Black holes and the second law
By J. Bekenstein. Jacob Bekenstein, 2019
874 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/b71b417b0b74447440f2bfc22f4f3c70d71587c7
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Citations in the corpus
- Quantum extremal islands made easy. Part II. Black holes on the brane (2020, background): “On the other hand, unitary evolution would require that the thermodynamic entropy of the black hole, which is proportional to its horizon area [9–11], set an upper bound on the the entanglement entropy of the radiation.”
- The Swampland: Introduction and Review (2019, background): “The covariant entropy bound is closely related to the Bekenstein bound [40–42] which states that given some matter with total mass-energy E, inside a sphere of radius R, the entropy of that matter Smatter is bounded by Smatter ≤ 2πER .”
- Entanglement islands in higher dimensions (2019, background): “The generalized entropy functional [4,5] depends on a codimension-two surface and equals the area of this surface, plus the entropy of matter fields on the outer half of a Cauchy slice passing through this surface.”
- Quantum extremal islands made easy. Part I. Entanglement on the brane (2020, background): “Almost half a century ago, it was discovered that black holes behave as quantum objects, with an associated temperature, entropy and other thermodynamic properties [1–5].”
- Ruppeiner geometry, phase transitions, and the microstructure of charged AdS black holes (2019, methodology): “[13] J.”
- An algebra of observables for de Sitter space (2022, background): “By contrast, in the case of a black hole, the Bekenstein-Hawking entropy A/4GN possibly determines the size of a Hilbert space that describes the black hole as seen from outside, but this Hilbert space does not describe particles and fields outside the black hole horizon.”
- Black Holes in 4D N=4 Super-Yang-Mills Field Theory (2018, background): “Of particular importance is the fact that black holes carry a macroscopic entropy [1–5], classically determined in terms of the horizon area.”