The University of Southampton
University of Southampton Institutional Repository

Pair creation of de Sitter black holes on a cosmic string background

Pair creation of de Sitter black holes on a cosmic string background
Pair creation of de Sitter black holes on a cosmic string background
We analyze the quantum process in which a cosmic string breaks in a de Sitter (dS) background, and a pair of neutral or charged black holes is produced at the ends of the string. The energy to materialize and accelerate the pair comes from the positive cosmological constant and, in addition, from the string tension. The compact saddle point solutions without conical singularities (instantons) or with conical singularities (submaximal instantons) that describe this process are constructed through the analytical continuation of the dS C metric. Then, we explicitly compute the pair creation rate of the process. In particular, we find the nucleation rate of a cosmic string in a dS background, and the probability that it breaks and a pair of black holes is produced. Finally we verify that, as occurs with pair production processes in other background fields, the pair creation rate of black holes is proportional to eS, where the gravitational entropy of the black hole, S, is given by one-quarter of the area of the horizons present in the saddle point solution that mediates the process.
Dias, Oscar J.C.
f01a8d9b-9597-4c32-9226-53a6e5500a54
Lemos, Jose P.S.
4e94199c-42b9-4592-9da9-f5035913088c
Dias, Oscar J.C.
f01a8d9b-9597-4c32-9226-53a6e5500a54
Lemos, Jose P.S.
4e94199c-42b9-4592-9da9-f5035913088c

Dias, Oscar J.C. and Lemos, Jose P.S. (2004) Pair creation of de Sitter black holes on a cosmic string background. Phys.Rev.D, 69 (8), [084006]. (doi:10.1103/PhysRevD.69.084006).

Record type: Article

Abstract

We analyze the quantum process in which a cosmic string breaks in a de Sitter (dS) background, and a pair of neutral or charged black holes is produced at the ends of the string. The energy to materialize and accelerate the pair comes from the positive cosmological constant and, in addition, from the string tension. The compact saddle point solutions without conical singularities (instantons) or with conical singularities (submaximal instantons) that describe this process are constructed through the analytical continuation of the dS C metric. Then, we explicitly compute the pair creation rate of the process. In particular, we find the nucleation rate of a cosmic string in a dS background, and the probability that it breaks and a pair of black holes is produced. Finally we verify that, as occurs with pair production processes in other background fields, the pair creation rate of black holes is proportional to eS, where the gravitational entropy of the black hole, S, is given by one-quarter of the area of the horizons present in the saddle point solution that mediates the process.

This record has no associated files available for download.

More information

e-pub ahead of print date: 8 April 2004
Published date: 15 April 2004
Additional Information: ©2004 American Physical Society

Identifiers

Local EPrints ID: 468107
URI: http://eprints.soton.ac.uk/id/eprint/468107
PURE UUID: 321c54eb-e153-461c-b26e-86490976579a
ORCID for Oscar J.C. Dias: ORCID iD orcid.org/0000-0003-4855-4750

Catalogue record

Date deposited: 02 Aug 2022 17:06
Last modified: 17 Mar 2024 03:35

Export record

Altmetrics

Contributors

Author: Oscar J.C. Dias ORCID iD
Author: Jose P.S. Lemos

Download statistics

Downloads from ePrints over the past year. Other digital versions may also be available to download e.g. from the publisher's website.

View more statistics

Atom RSS 1.0 RSS 2.0

Contact ePrints Soton: eprints@soton.ac.uk

ePrints Soton supports OAI 2.0 with a base URL of http://eprints.soton.ac.uk/cgi/oai2

This repository has been built using EPrints software, developed at the University of Southampton, but available to everyone to use.

We use cookies to ensure that we give you the best experience on our website. If you continue without changing your settings, we will assume that you are happy to receive cookies on the University of Southampton website.

×