F(R) gravity equation of state

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dc.creatorElizalde, Emilio
dc.creatorSilva, Pedro J.
dc.date2008-04-23
dc.date2008-05-16
dc.date.accessioned2026-07-07T11:50:09Z
dc.date.available2026-07-07T11:50:09Z
dc.descriptionThe ${\bf f}(R)$ gravity field equations are derived as an equation of state of local space-time thermodynamics. Jacobson's arguments are non-trivially extended, by means of a more general definition of local entropy, for which Wald's definition of dynamic black hole entropy is used, as well as the concept of an effective Newton constant for graviton exchange, recently appeared in the literature.
dc.identifierhttps://arxiv.org/abs/0804.3721
dc.identifierhttp://arxiv.org/abs/0804.3721
dc.identifierPhys.Rev.D78:061501,2008
dc.identifierdoi:10.1103/PhysRevD.78.061501
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/203474
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectMathematical Physics
dc.subjectQuantum Physics
dc.titleF(R) gravity equation of state
dc.typetext

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