Strong gravity, black holes, and hadrons

dc.contributor.author	Sivaram, C
dc.contributor.author	Sinha, K. P
dc.date.accessioned	2008-10-27T15:25:36Z
dc.date.available	2008-10-27T15:25:36Z
dc.date.issued	1977-09
dc.identifier.citation	Physical Review D, Vol. 16, pp. 1975 - 1978	en
dc.identifier.issn	0556-2821
dc.identifier.uri	http://hdl.handle.net/2248/3989
dc.description.abstract	Certain 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.iso	en	en
dc.publisher	American Physical Society	en
dc.relation.uri	http://link.aps.org/abstract/PRD/v16/p1975	en
dc.subject	Astrophysics	en
dc.subject	Black Holes (Astronomy)	en
dc.subject	Gravitation Theory	en
dc.subject	Hadrons	en
dc.subject	High Gravity Environments	en
dc.subject	Astronomical Models	en
dc.subject	Relativity	en
dc.subject	Space-Time Functions	en
dc.subject	Stellar Temperature	en
dc.subject	Thermodynamics	en
dc.title	Strong gravity, black holes, and hadrons	en
dc.type	Article	en