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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3989
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dc.contributor.authorSivaram, C-
dc.contributor.authorSinha, K. P-
dc.date.accessioned2008-10-27T15:25:36Z-
dc.date.available2008-10-27T15:25:36Z-
dc.date.issued1977-09-
dc.identifier.citationPhysical Review D, Vol. 16, pp. 1975 - 1978en
dc.identifier.issn0556-2821-
dc.identifier.urihttp://hdl.handle.net/2248/3989-
dc.description.abstractCertain similarities and analogies between the properties of black holes and elementary particles are considered in the framework of the strong gravitational field. Properties examined include measurable parameters (mass, angular momentum, charge), the metrical properties of space-time in the region near an elementary particle, mass formulas, thermodynamical phenomena, and black-hole radiation. An upper limit for the temperature of black holes is derived which is the same as the limiting temperature arising in thermodynamic bootstrap models of hadrons.en
dc.language.isoenen
dc.publisherAmerican Physical Societyen
dc.relation.urihttp://link.aps.org/abstract/PRD/v16/p1975en
dc.subjectAstrophysicsen
dc.subjectBlack Holes (Astronomy)en
dc.subjectGravitation Theoryen
dc.subjectHadronsen
dc.subjectHigh Gravity Environmentsen
dc.subjectAstronomical Modelsen
dc.subjectRelativityen
dc.subjectSpace-Time Functionsen
dc.subjectStellar Temperatureen
dc.subjectThermodynamicsen
dc.titleStrong gravity, black holes, and hadronsen
dc.typeArticleen
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