Defining Entropy Bounds

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dc.creatorPage, Don N.
dc.date2000-07-28
dc.date2008-09-19
dc.date.accessioned2026-07-07T12:03:36Z
dc.date.available2026-07-07T12:03:36Z
dc.descriptionBekenstein's conjectured entropy bound for a system of linear size R and energy E, S < 2 pi E R, has counterexamples for many of the ways in which the "system," R, E, and S may be defined. Here new ways are proposed to define these quantities for arbitrary nongravitational quantum field theories in flat spacetime, such as defining R as the smallest radius outside of which only vacuum expectation values occur. Difficulties of extending these definitions to gravitational quantum theories are noted.
dc.description30 pages, LaTeX, rewritten Introduction and references added
dc.identifierhttps://arxiv.org/abs/hep-th/0007238
dc.identifierhttp://arxiv.org/abs/hep-th/0007238
dc.identifierJHEP0810:007,2008
dc.identifierdoi:10.1088/1126-6708/2008/10/007
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/207839
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleDefining Entropy Bounds
dc.typetext

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