Black holes from nucleating strings

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. Combi...

Full description

Bibliographic Details
Authors: Garriga Torres, Jaume, Vilenkin, A. (Alexander)
Format: article
Status:Published version
Publication Date:1993
Country:España
Institution:Varias* (Consorci de Biblioteques Universitáries de Catalunya, Centre de Serveis Científics i Acadèmics de Catalunya)
Repository:Recercat. Dipósit de la Recerca de Catalunya
OAI Identifier:oai:recercat.cat:2445/12330
Online Access:https://hdl.handle.net/2445/12330
Access Level:Open access
Keyword:Forats negres (Astronomia)
Teoria quàntica de camps
Black holes (Astronomy)
Quantum field theory
id ES_2b84ef9fe9c8d42791cd34a21e1dc5ed
oai_identifier_str oai:recercat.cat:2445/12330
network_acronym_str ES
network_name_str España
repository_id_str
spelling Black holes from nucleating stringsGarriga Torres, JaumeVilenkin, A. (Alexander)Forats negres (Astronomia)Teoria quàntica de campsBlack holes (Astronomy)Quantum field theoryWe 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. Combining these constraints with current upper limits on the expansion rate during inflation, we conclude that the density of black holes formed from nucleating strings is too low to be observed. Also, constraints on domain wall nucleation and monopole pair production during inflation are briefly discussed.The American Physical Society201020101993info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersion10 p.application/pdfapplication/pdfhttps://hdl.handle.net/2445/12330Articles publicats en revistes (Física de la Matèria Condensada)reponame:Recercat. Dipósit de la Recerca de Catalunyainstname:Varias* (Consorci de Biblioteques Universitáries de Catalunya, Centre de Serveis Científics i Acadèmics de Catalunya)InglésReproducció digital del document publicat en format paper, proporcionada per PROLA i http://dx.doi.org/10.1103/PhysRevD.47.3265Physical Review D, 1993, vol. 47, núm. 8, p. 3265-3274http://dx.doi.org/10.1103/PhysRevD.47.3265(c) The American Physical Society, 1993info:eu-repo/semantics/openAccessoai:recercat.cat:2445/123302026-05-29T05:05:01Z
dc.title.none.fl_str_mv Black holes from nucleating strings
title Black holes from nucleating strings
spellingShingle Black holes from nucleating strings
Garriga Torres, Jaume
Forats negres (Astronomia)
Teoria quàntica de camps
Black holes (Astronomy)
Quantum field theory
title_short Black holes from nucleating strings
title_full Black holes from nucleating strings
title_fullStr Black holes from nucleating strings
title_full_unstemmed Black holes from nucleating strings
title_sort Black holes from nucleating strings
dc.creator.none.fl_str_mv Garriga Torres, Jaume
Vilenkin, A. (Alexander)
author Garriga Torres, Jaume
author_facet Garriga Torres, Jaume
Vilenkin, A. (Alexander)
author_role author
author2 Vilenkin, A. (Alexander)
author2_role author
dc.subject.none.fl_str_mv Forats negres (Astronomia)
Teoria quàntica de camps
Black holes (Astronomy)
Quantum field theory
topic Forats negres (Astronomia)
Teoria quàntica de camps
Black holes (Astronomy)
Quantum field theory
description 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. Combining these constraints with current upper limits on the expansion rate during inflation, we conclude that the density of black holes formed from nucleating strings is too low to be observed. Also, constraints on domain wall nucleation and monopole pair production during inflation are briefly discussed.
publishDate 1993
dc.date.none.fl_str_mv 1993
2010
2010
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv https://hdl.handle.net/2445/12330
url https://hdl.handle.net/2445/12330
dc.language.none.fl_str_mv Inglés
language_invalid_str_mv Inglés
dc.relation.none.fl_str_mv Reproducció digital del document publicat en format paper, proporcionada per PROLA i http://dx.doi.org/10.1103/PhysRevD.47.3265
Physical Review D, 1993, vol. 47, núm. 8, p. 3265-3274
http://dx.doi.org/10.1103/PhysRevD.47.3265
dc.rights.none.fl_str_mv (c) The American Physical Society, 1993
info:eu-repo/semantics/openAccess
rights_invalid_str_mv (c) The American Physical Society, 1993
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 10 p.
application/pdf
application/pdf
dc.publisher.none.fl_str_mv The American Physical Society
publisher.none.fl_str_mv The American Physical Society
dc.source.none.fl_str_mv Articles publicats en revistes (Física de la Matèria Condensada)
reponame:Recercat. Dipósit de la Recerca de Catalunya
instname:Varias* (Consorci de Biblioteques Universitáries de Catalunya, Centre de Serveis Científics i Acadèmics de Catalunya)
instname_str Varias* (Consorci de Biblioteques Universitáries de Catalunya, Centre de Serveis Científics i Acadèmics de Catalunya)
reponame_str Recercat. Dipósit de la Recerca de Catalunya
collection Recercat. Dipósit de la Recerca de Catalunya
repository.name.fl_str_mv
repository.mail.fl_str_mv
_version_ 1869405154031173632
score 15.81155

Similar Items