Published June 10, 2017 | Version v1
Journal article

Hairs of discrete symmetries and gravity

  • 1. Center for Fields, Gravity and Strings, CTPU, Institute for Basic Sciences, Yuseong-Gu, Daejeon 34047 (Korea, Republic of)
  • 2. Scranton Honors Program, Ewha Womans University, Seodaemun-Gu, Seoul 03760 (Korea, Republic of)
  • 3. Center for Axion and Precision Physics Research (IBS), 291 Daehakro, Yuseong-Gu, Daejeon 34141 (Korea, Republic of)
  • 4. Department of Physics, Kyung Hee University, 26 Gyungheedaero, Dongdaemun-Gu, Seoul 02447 (Korea, Republic of)
  • 5. Department of Physics, Pusan National University, 2 Busandaehakro-63-Gil, Geumjeong-Gu, Busan 46241 (Korea, Republic of)

Description

Gauge symmetries are known to be respected by gravity because gauge charges carry flux lines, but global charges do not carry flux lines and are not conserved by gravitational interaction. For discrete symmetries, they are spontaneously broken in the Universe, forming domain walls. Since the realization of discrete symmetries in the Universe must involve the vacuum expectation values of Higgs fields, a string-like configuration (hair) at the intersection of domain walls in the Higgs vacua can be realized. Therefore, we argue that discrete charges are also respected by gravity.

Availability note (English)

Available from http://dx.doi.org/10.1016/j.physletb.2017.04.008

Additional details

Identifiers

DOI
10.1016/j.physletb.2017.04.008;
arXiv
arXiv:1703.05389v2;
PII
S0370-2693(17)30282-4;

Publishing Information

Journal Title
Physics Letters. Section B
Journal Volume
769
Journal Page Range
p. 430-435
ISSN
0370-2693
CODEN
PYLBAJ

INIS

Country of Publication
Netherlands
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
48086135
Subject category
S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
Descriptors DEI
GAUGE INVARIANCE; GRAVITATION; GRAVITATIONAL INTERACTIONS; HIGGS MODEL; SYMMETRY; UNIVERSE
Descriptors DEC
FUNDAMENTAL INTERACTIONS; INTERACTIONS; INVARIANCE PRINCIPLES; MATHEMATICAL MODELS; PARTICLE MODELS

Optional Information

Copyright
Copyright (c) 2017 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.