Published May 10, 2018 | Version v1
Journal article

Higher-order Skyrme hair of black holes

  • 1. Institute of Modern Physics, Chinese Academy of Sciences,Lanzhou 730000 (China)
  • 2. Department of Physics, and Research and Education Center for Natural Sciences, Keio University,Hiyoshi 4-1-1, Yokohama, Kanagawa 223-8521 (Japan)

Description

Higher-order derivative terms are considered as replacement for the Skyrme term in an Einstein-Skyrme-like model in order to pinpoint which properties are necessary for a black hole to possess stable static scalar hair. We find two new models able to support stable black hole hair in the limit of the Skyrme term being turned off. They contain 8 and 12 derivatives, respectively, and are roughly the Skyrme-term squared and the so-called BPS-Skyrme-term squared. In the twelfth-order model we find that the lower branches, which are normally unstable, become stable in the limit where the Skyrme term is turned off. We check this claim with a linear stability analysis. Finally, we find for a certain range of the gravitational coupling and horizon radius, that the twelfth-order model contains 4 solutions as opposed to 2. More surprisingly, the lowest part of the would-be unstable branch turns out to be the stable one of the 4 solutions.

Availability note (English)

Available from http://dx.doi.org/10.1007/JHEP05(2018)071; Available from http://repo.scoap3.org/record/25492

Additional details

Identifiers

Publishing Information

Journal Title
Journal of High Energy Physics (Online)
Journal Volume
2018
Journal Issue
05
Journal Page Range
p. 71
ISSN
1029-8479

INIS

Country of Publication
Germany
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
49093960
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
BLACK HOLES; FIELD THEORIES; HAIR; MATHEMATICAL SOLUTIONS; SKYRME POTENTIAL
Descriptors DEC
BODY; NUCLEON-NUCLEON POTENTIAL; ORGANS; POTENTIALS; SKIN

Optional Information

Copyright
Copyright (c) OPEN ACCESS, © The Authors
Notes
PUBLISHER-ID: JHEP05(2018)071; ARXIV:1803.10786; OAI: oai:repo.scoap3.org:25492
Funding organization
SCOAP3, CERN, Geneva (Switzerland)