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Title: Gravitational wave, collider and dark matter signals from a scalar singlet electroweak baryogenesis

Abstract

We analyse a simple extension of the SM with just an additional scalar singlet coupled to the Higgs boson. Here, we discuss the possible probes for electroweak baryogenesis in this model including collider searches, gravitational wave and direct dark matter detection signals. We show that a large portion of the model parameter space exists where the observation of gravitational waves would allow detection while the indirect collider searches would not.

Authors:
ORCiD logo [1]; ORCiD logo [2]; ORCiD logo [3];  [1]; ORCiD logo [1]
  1. Univ. of Adelaide, SA (Australia). ARC Centre of Excellence for Particle Physics at the Terascale (CoEPP) & CSSM, Dept. of Physics
  2. Univ. of Adelaide, SA (Australia). ARC Centre of Excellence for Particle Physics at the Terascale (CoEPP) & CSSM, Dept. of Physics; Univ. of Warsaw (Poland). Faculty of Physics
  3. Univ. of Michigan, Ann Arbor, MI (United States). Michigan Center for Theoretical Physics; Deutsches Elektronen-Synchrotron (DESY), Hamburg (Germany)
Publication Date:
Research Org.:
Univ. of Michigan, Ann Arbor, MI (United States)
Sponsoring Org.:
USDOE Office of Science (SC); ARC Centre of Excellence for Particle Physics at the Terascale (CoEPP); Alexander von Humboldt Foundation; Australian Research Council
OSTI Identifier:
1425641
Grant/Contract Number:  
SC0007859; IP2015 043174
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: 2017; Journal Issue: 8; Journal ID: ISSN 1029-8479
Publisher:
Springer Berlin
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; Beyond Standard Model; Cosmology of Theories beyond the SM; Higgs Physics; Solitons Monopoles and Instantons

Citation Formats

Beniwal, Ankit, Lewicki, Marek, Wells, James D., White, Martin, and Williams, Anthony G. Gravitational wave, collider and dark matter signals from a scalar singlet electroweak baryogenesis. United States: N. p., 2017. Web. doi:10.1007/JHEP08(2017)108.
Beniwal, Ankit, Lewicki, Marek, Wells, James D., White, Martin, & Williams, Anthony G. Gravitational wave, collider and dark matter signals from a scalar singlet electroweak baryogenesis. United States. https://doi.org/10.1007/JHEP08(2017)108
Beniwal, Ankit, Lewicki, Marek, Wells, James D., White, Martin, and Williams, Anthony G. Wed . "Gravitational wave, collider and dark matter signals from a scalar singlet electroweak baryogenesis". United States. https://doi.org/10.1007/JHEP08(2017)108. https://www.osti.gov/servlets/purl/1425641.
@article{osti_1425641,
title = {Gravitational wave, collider and dark matter signals from a scalar singlet electroweak baryogenesis},
author = {Beniwal, Ankit and Lewicki, Marek and Wells, James D. and White, Martin and Williams, Anthony G.},
abstractNote = {We analyse a simple extension of the SM with just an additional scalar singlet coupled to the Higgs boson. Here, we discuss the possible probes for electroweak baryogenesis in this model including collider searches, gravitational wave and direct dark matter detection signals. We show that a large portion of the model parameter space exists where the observation of gravitational waves would allow detection while the indirect collider searches would not.},
doi = {10.1007/JHEP08(2017)108},
journal = {Journal of High Energy Physics (Online)},
number = 8,
volume = 2017,
place = {United States},
year = {Wed Aug 23 00:00:00 EDT 2017},
month = {Wed Aug 23 00:00:00 EDT 2017}
}

Journal Article:
Free Publicly Available Full Text
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Cited by: 108 works
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Figures / Tables:

Figure 1 Figure 1: Parameter space of the scalar singlet model relevant for EWBG. The yellow region is excluded because in that region, the electroweak minimum is not the global minimum at zero temperature. The blue region realises a strong first-order phase transition whereas the light blue region can still be allowedmore » due to the cosmological modification. The solid red line marks the boundary between the regions where $μ^{2}_{S}$($T$$c$) < 0 and $μ^{2}_{S}$($T$$c$) > 0 (see text for more details).« less

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