Comments on "Thermodynamics and/of horizons : A comparison of Schwarzschild, Rindler and de Sitter spacetimes" (ArXiv : gr-qc/0202078), by T.Padmanabhan

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dc.creatorCuletu, Hristu
dc.date2005-02-10
dc.date2005-02-14
dc.date.accessioned2026-07-07T04:18:03Z
dc.date.available2026-07-07T04:18:03Z
dc.descriptionWe show in this note that the Padmanabhan expression $E = a/2$ for the energy of the Schwarzschild and de Sitter spacetimes (a - the horizon radius) is also valid for the Rindler horizon, using an analogy with the electrostatic case.
dc.description5 pages, references added, no figures
dc.identifierhttps://arxiv.org/abs/hep-th/0502098
dc.identifierhttp://arxiv.org/abs/hep-th/0502098
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/53018
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleComments on "Thermodynamics and/of horizons : A comparison of Schwarzschild, Rindler and de Sitter spacetimes" (ArXiv : gr-qc/0202078), by T.Padmanabhan
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