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|Correlations between black holes formed in cosmic string breaking
|Emparan García de Salazar, Roberto A.
|Teoria de camps (Física)
Forats negres (Astronomia)
Field theory (Physics)
Black holes (Astronomy)
|The American Physical Society
|An analysis of cosmic string breaking with the formation of black holes attached to the ends reveals a remarkable feature: the black holes can be correlated or uncorrelated. We find that, as a consequence, the number-of-states enhancement factor in the action governing the formation of uncorrelated black holes is twice the one for a correlated pair. We argue that when an uncorrelated pair forms at the ends of the string, the physics involved is more analogous to thermal nucleation than to particle-antiparticle creation. Also, we analyze the process of intercommuting strings induced by black hole annihilation and merging. Finally, we discuss the consequences for grand unified strings. The process whereby uncorrelated black holes are formed yields a rate which significantly improves over those previously considered, but still not enough to modify string cosmology. 1995 The American Physical Society.
|Reproducció digital del document publicat en format paper, proporcionada per PROLA i http://dx.doi.org/10.1103/PhysRevD.52.6976
|It is part of:
|Physical Review D, 1995, vol. 52, núm. 12, p. 6976-6981
|Appears in Collections:
|Articles publicats en revistes (Física de la Matèria Condensada)
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