Black Holes from Nucleating Strings

Details Black Holes from Nucleating Strings Black Holes from Nucleating Strings

1992-08-06

arxiv.org/abs/hep-ph/9208212v1

Phys.Rev. D47 (1993) 3265-3274

Physics

High Energy Physics

High Energy Physics - Phenomenology

27 pages, tutp-92-6

Scientific paper

10.1103/PhysRevD.47.3265

We evaluate the probability that a loop of string that has spontaneously nucleated during inflation will form a black hole upon collapse, after the end of inflation. We then use the observational bounds on the density of primordial black holes to put constraints on the parameters of the model. Other constraints from the distortions of the microwave background and emission of gravitational radiation by the loops are considered. Also, observational constraints on domain wall nucleation and monopole pair production during inflation are briefly discussed.

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