Phase transitions in twin Higgs models
Abstract
We study twin Higgs models at non-zero temperature and discuss cosmological phase transitions as well as their implications on electroweak baryogenesis and gravitational waves. It is shown that the expectation value of the Higgs field at the critical temperature of the electroweak phase transition is much smaller than the critical temperature, which indicates two important facts: (i) the electroweak phase transition cannot be analyzed perturbatively (ii) the electroweak baryogenesis is hardly realized in the typical realizations of twin Higgs models. We also analyze the phase transition associated with the global symmetry breaking, through which the Standard Model Higgs is identified with one of the pseudo-Nambu-Goldstone bosons in terms of its linear realization, with and without supersymmetry. For this phase transition, we show that, only in the supersymmetric case, there are still some parameter spaces, in which the perturbative approach is validated and the phase transition is the first order. We find that the stochastic gravitational wave background is generated through this first order phase transition, but it is impossible to be detected by DECIGO or BBO in the linear realization and the decoupling limit. The detection of stochastic gravitational wave background with the feature of first order phase transition, therefore,more »
- Authors:
-
- Tokyo Inst. of Technology (Japan)
- Inst. for Basics Science (IBS), Daejeon (Korea); Univ. of Tokyo (Japan)
- Rutgers Univ., Piscataway, NJ (United States)
- Publication Date:
- Research Org.:
- Rutgers Univ., Piscataway, NJ (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC); Japan Society for the Promotion of Science (JSPS)
- OSTI Identifier:
- 1611322
- Grant/Contract Number:
- SC0010008; JP25287054; JP15H05888; JP18H04579; JP18K18764
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Journal of High Energy Physics (Online)
- Additional Journal Information:
- Journal Name: Journal of High Energy Physics (Online); Journal Volume: 2018; Journal Issue: 12; Journal ID: ISSN 1029-8479
- Publisher:
- Springer Berlin
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; physics; Beyond Standard Model; Thermal Field Theory
Citation Formats
Fujikura, Kohei, Kamada, Kohei, Nakai, Yuichiro, and Yamaguchi, Masahide. Phase transitions in twin Higgs models. United States: N. p., 2018.
Web. doi:10.1007/jhep12(2018)018.
Fujikura, Kohei, Kamada, Kohei, Nakai, Yuichiro, & Yamaguchi, Masahide. Phase transitions in twin Higgs models. United States. https://doi.org/10.1007/jhep12(2018)018
Fujikura, Kohei, Kamada, Kohei, Nakai, Yuichiro, and Yamaguchi, Masahide. Tue .
"Phase transitions in twin Higgs models". United States. https://doi.org/10.1007/jhep12(2018)018. https://www.osti.gov/servlets/purl/1611322.
@article{osti_1611322,
title = {Phase transitions in twin Higgs models},
author = {Fujikura, Kohei and Kamada, Kohei and Nakai, Yuichiro and Yamaguchi, Masahide},
abstractNote = {We study twin Higgs models at non-zero temperature and discuss cosmological phase transitions as well as their implications on electroweak baryogenesis and gravitational waves. It is shown that the expectation value of the Higgs field at the critical temperature of the electroweak phase transition is much smaller than the critical temperature, which indicates two important facts: (i) the electroweak phase transition cannot be analyzed perturbatively (ii) the electroweak baryogenesis is hardly realized in the typical realizations of twin Higgs models. We also analyze the phase transition associated with the global symmetry breaking, through which the Standard Model Higgs is identified with one of the pseudo-Nambu-Goldstone bosons in terms of its linear realization, with and without supersymmetry. For this phase transition, we show that, only in the supersymmetric case, there are still some parameter spaces, in which the perturbative approach is validated and the phase transition is the first order. We find that the stochastic gravitational wave background is generated through this first order phase transition, but it is impossible to be detected by DECIGO or BBO in the linear realization and the decoupling limit. The detection of stochastic gravitational wave background with the feature of first order phase transition, therefore, will give strong constraints on twin Higgs models.},
doi = {10.1007/jhep12(2018)018},
journal = {Journal of High Energy Physics (Online)},
number = 12,
volume = 2018,
place = {United States},
year = {Tue Dec 04 00:00:00 EST 2018},
month = {Tue Dec 04 00:00:00 EST 2018}
}
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