The Energy Density of a Gas of Photons Surrounding a Spherical Mass $M$ at a Non-Zero Temperature

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dc.creatorSpeliotopoulos, Achilles D.
dc.date1993-05-24
dc.date.accessioned2026-07-07T03:56:05Z
dc.date.available2026-07-07T03:56:05Z
dc.descriptionThe equations determining the energy density $ρ$ of a gas of photons in thermodynamic equilibrium with a spherical mass $M$ at a non-zero temperature $T_s>0$ is derived from Einstein's equations. It is found that for large $r$, $ρ\sim 1/r^2$ where the proportionality constant is a {\it fundamental constant\/} and is the same for all spherical masses at all temperatures.
dc.descriptionPlain TeX 16 pages, IP-ASTP-12-93
dc.identifierhttps://arxiv.org/abs/hep-ph/9305302
dc.identifierhttp://arxiv.org/abs/hep-ph/9305302
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/44810
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleThe Energy Density of a Gas of Photons Surrounding a Spherical Mass $M$ at a Non-Zero Temperature
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