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.2017.04.008Additional 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.