• Open Access

Baryogenesis and gravity waves from a UV-completed electroweak phase transition

Benoit Laurent, James M. Cline, Avi Friedlander, Dong-Ming He, Kimmo Kainulainen, and David Tucker-Smith
Phys. Rev. D 103, 123529 – Published 10 June 2021

Abstract

We study gravity wave production and baryogenesis at the electroweak phase transition in a real singlet scalar extension of the Standard Model, including vectorlike top partners, to generate the CP violation needed for electroweak baryogenesis (EWBG). The singlet makes the phase transition strongly first order through its coupling to the Higgs boson, and it spontaneously breaks CP invariance through a dimension-five contribution to the top quark mass term, generated by integrating out the heavy top quark partners. We improve on previous studies by incorporating updated transport equations, compatible with large bubble wall velocities. The wall speed and thickness are computed directly from the microphysical parameters rather than treating them as free parameters, allowing for a first-principles computation of the baryon asymmetry. The size of the CP-violating dimension-five operator needed for EWBG is constrained by collider, electroweak precision, and renormalization group running constraints. We identify regions of parameter space that can produce the observed baryon asymmetry or observable gravitational wave (GW) signals. Contrary to standard lore, we find that for strong deflagrations, the efficiencies of large baryon asymmetry production and strong GW signals can be positively correlated. However, we find the overall likelihood of observably large GW signals to be smaller than estimated in previous studies. In particular, only detonation-type transitions are predicted to produce observably large gravitational waves.

  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
3 More
  • Received 8 March 2021
  • Accepted 11 May 2021

DOI:https://doi.org/10.1103/PhysRevD.103.123529

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & AstrophysicsParticles & Fields

Authors & Affiliations

Benoit Laurent* and James M. Cline

  • McGill University, Department of Physics, 3600 University St., Montréal, Quebec, H3A2T8 Canada

Avi Friedlander

  • Queen’s University, Department of Physics & Engineering Physics Astronomy Kingston, Ontario, K7L 3N6 Kingston, Canada

Dong-Ming He§

  • University of Science and Technology of China, Hefei, Anhui 230026 and Universiteit van Amsterdam, Science Park 904, Amsterdam 1098XH, Netherlands

Kimmo Kainulainen

  • Department of Physics, P.O.Box 35 (YFL), FIN-40014 University of Jyväskylä, Finland and Helsinki Institute of Physics, P.O. Box 64, FIN-00014 University of Helsinki, Finland

David Tucker-Smith

  • Department of Physics, Williams College, Williamstown, Massachusetts 01267, USA

  • *benoit.laurent@mail.mcgill.ca
  • avi.friedlander@queensu.ca
  • dong-ming.he@student.uva.nl
  • §jcline@physics.mcgill.ca
  • kimmo.kainulainen@jyu.fi
  • dtuckers@williams.edu

Article Text

Click to Expand

References

Click to Expand
Issue

Vol. 103, Iss. 12 — 15 June 2021

Reuse & Permissions
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review D

Reuse & Permissions

It is not necessary to obtain permission to reuse this article or its components as it is available under the terms of the Creative Commons Attribution 4.0 International license. This license permits unrestricted use, distribution, and reproduction in any medium, provided attribution to the author(s) and the published article's title, journal citation, and DOI are maintained. Please note that some figures may have been included with permission from other third parties. It is your responsibility to obtain the proper permission from the rights holder directly for these figures.

×

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×