Classical and quantum thermodynamics of horizons in spherically symmetric spacetimes
By Thanu Padmanabhan. 2002
455 citations recorded by the source corpus.
Subfields: Atomic and Molecular Physics, and Optics, Nuclear and High Energy Physics, Statistical and Nonlinear Physics
View Paper: https://www.semanticscholar.org/paper/269c7e1c8f5687f5b1afa70ba94c4d4d74ae8fe4
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Citations in the corpus
- Gravity and the Thermodynamics of Horizons (2003, methodology): “The background material relevant to this review can be found in several text books (Birrel and Davies, 1982; Fulling, 1989; Wald, 1994) and review articles (Bousso, 2002; Brout et al., 1995b; Dewitt, 1975; Sciama et al., 1981; Sriramkumar and Padmanabhan, 2002; Takagi, 1986; Wald, 2001).”
- Black hole chemistry: thermodynamics with Lambda (2016, methodology): “r a positive cosmological constant > 0 (extending the concepts presented in Sec.1and Sec.2) [50,245], asymptotically Lifshitz spacetimes [58], and connections with so-called horizon thermodynamics [45]. 6.1 Thermodynamics of de Sitter black holes The thermodynamics of asymptotically de Sitter (dS”
- Friedmann Equations from Entropic Force (2010, background): “Padmanabhan [11] first noticed that the gravitational field equation in a static, spherically symmetric spacetime can be rewritten as a form of the ordinary first law of thermodynamics at a black hole”
- Thermodynamics of Rotating Black Holes and Black Rings: Phase Transitions and Thermodynamic Volume (2014, background): “Extensions of this idea to asymptotically de Sitter space times have also been recently explored, with the resultant thermodynamic notions for black holes remaining intact [40] (see also [41–49]).”
- Gravity and the thermodynamics of horizons (2005, background): “−H2L3 and S= πHL3 from (154) and (153). Once again, equation (157) holds since β= −2π/H. We should, therefore, be able to rewrite Einstein’s equations in a form analogous to the TdS− dU= PdV equation [75,163]. It is fairly straight forward to achieve this in the case of spacetimes of the form: ds 2=”
- Black Hole Chemistry (2014, unknown): “ding M = M(A,Λ), Euler’s theorem implies that (d −3)M = (d −2) ∂M ∂A A −2 ∂M ∂Λ Λ, (2) and since T = 4∂M ∂A , eq. (2) suggests that we regard P = − Λ 8π = ( d−1)( 2) 16πℓ2 as a thermodynamic variable [5, 6], whose conjugate is V = −8π∂M ∂Λ . Putting this together, we have (d −3)M = (d −2)TS −2PV and”