Thermodynamics and Evaporation of Closed Black Cosmic Strings

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dc.creatorDeBenedictis, Andrew
dc.date1998-09-04
dc.date.accessioned2026-07-07T03:32:38Z
dc.date.available2026-07-07T03:32:38Z
dc.descriptionBoth the canonical and microcanonical ensembles are utilized to study the thermodynamic and evaporation properties of a closed black cosmic string whose spacetime is asymptotically anti deSitter. There are similarities and differences to the Schwarzschild-anti deSitter and 2+1 BTZ black hole solutions. It is found that there exist regimes of black string/thermal radiation equilibrium as well as stable remnant regimes. The relevance to black hole evaporation is discussed.
dc.description10 pages with AMS packages. 1 figure
dc.identifierhttps://arxiv.org/abs/gr-qc/9809025
dc.identifierhttp://arxiv.org/abs/gr-qc/9809025
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/36306
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleThermodynamics and Evaporation of Closed Black Cosmic Strings
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