Simulations of Cold Electroweak Baryogenesis: hypercharge U(1) and the creation of helical magnetic fields

We perform numerical simulations of Cold Electroweak Baryogenesis, including for the first time in the Bosonic sector the full electroweak gauge group SU(2)×U(1) and CP-violation. We find that the maximum generated baryon asymmetry is reduced by a factor of three relative to the SU(2)-only model, bu...

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Main Authors: Mou, Zong-Gang, Saffin, Paul M., Tranberg, Anders
Format: Article
Published: Springer Verlag 2017
Online Access:https://eprints.nottingham.ac.uk/43972/
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author Mou, Zong-Gang
Saffin, Paul M.
Tranberg, Anders
author_facet Mou, Zong-Gang
Saffin, Paul M.
Tranberg, Anders
author_sort Mou, Zong-Gang
building Nottingham Research Data Repository
collection Online Access
description We perform numerical simulations of Cold Electroweak Baryogenesis, including for the first time in the Bosonic sector the full electroweak gauge group SU(2)×U(1) and CP-violation. We find that the maximum generated baryon asymmetry is reduced by a factor of three relative to the SU(2)-only model, but that the quench time dependence is very similar. In addition, we compute the magnitude of the helical magnetic fields, and find that it is proportional to the strength of CP-violation and dependent on quench time, but is not proportional to the magnitude of the baryon asymmetry as proposed in the literature. Astrophysical signatures of primordial magnetic helicity can therefore not in general be used as evidence that electroweak baryogenesis has taken place.
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institution University of Nottingham Malaysia Campus
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spelling nottingham-439722020-05-04T18:50:25Z https://eprints.nottingham.ac.uk/43972/ Simulations of Cold Electroweak Baryogenesis: hypercharge U(1) and the creation of helical magnetic fields Mou, Zong-Gang Saffin, Paul M. Tranberg, Anders We perform numerical simulations of Cold Electroweak Baryogenesis, including for the first time in the Bosonic sector the full electroweak gauge group SU(2)×U(1) and CP-violation. We find that the maximum generated baryon asymmetry is reduced by a factor of three relative to the SU(2)-only model, but that the quench time dependence is very similar. In addition, we compute the magnitude of the helical magnetic fields, and find that it is proportional to the strength of CP-violation and dependent on quench time, but is not proportional to the magnitude of the baryon asymmetry as proposed in the literature. Astrophysical signatures of primordial magnetic helicity can therefore not in general be used as evidence that electroweak baryogenesis has taken place. Springer Verlag 2017-06-14 Article PeerReviewed Mou, Zong-Gang, Saffin, Paul M. and Tranberg, Anders (2017) Simulations of Cold Electroweak Baryogenesis: hypercharge U(1) and the creation of helical magnetic fields. Journal of High Energy Physics, 2017 (6). pp. 1-27. ISSN 1029-8479 https://link.springer.com/article/10.1007%2FJHEP06%282017%29075 doi:10.1007/JHEP06(2017)075 doi:10.1007/JHEP06(2017)075
spellingShingle Mou, Zong-Gang
Saffin, Paul M.
Tranberg, Anders
Simulations of Cold Electroweak Baryogenesis: hypercharge U(1) and the creation of helical magnetic fields
title Simulations of Cold Electroweak Baryogenesis: hypercharge U(1) and the creation of helical magnetic fields
title_full Simulations of Cold Electroweak Baryogenesis: hypercharge U(1) and the creation of helical magnetic fields
title_fullStr Simulations of Cold Electroweak Baryogenesis: hypercharge U(1) and the creation of helical magnetic fields
title_full_unstemmed Simulations of Cold Electroweak Baryogenesis: hypercharge U(1) and the creation of helical magnetic fields
title_short Simulations of Cold Electroweak Baryogenesis: hypercharge U(1) and the creation of helical magnetic fields
title_sort simulations of cold electroweak baryogenesis: hypercharge u(1) and the creation of helical magnetic fields
url https://eprints.nottingham.ac.uk/43972/
https://eprints.nottingham.ac.uk/43972/
https://eprints.nottingham.ac.uk/43972/