Electroweak baryogenesis in the ℤ3 $$ {\mathbb{Z}}_3 $$-invariant NMSSM

Abstract We calculate the baryon asymmetry of the Universe in the ℤ3 $$ {\mathbb{Z}}_3 $$-invariant Next-to-Minimal Supersymmetric Standard Model where the interactions of the singlino provide the necessary source of charge and parity violation. Using the closed time path formalism, we derive and so...

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Main Authors: Sujeet Akula, Csaba Balázs, Liam Dunn, Graham White
Format: Article
Language:English
Published: SpringerOpen 2017-11-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP11(2017)051
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author Sujeet Akula
Csaba Balázs
Liam Dunn
Graham White
author_facet Sujeet Akula
Csaba Balázs
Liam Dunn
Graham White
author_sort Sujeet Akula
collection DOAJ
description Abstract We calculate the baryon asymmetry of the Universe in the ℤ3 $$ {\mathbb{Z}}_3 $$-invariant Next-to-Minimal Supersymmetric Standard Model where the interactions of the singlino provide the necessary source of charge and parity violation. Using the closed time path formalism, we derive and solve transport equations for the cases where the singlet acquires a vacuum expectation value (VEV) before and during the electroweak phase transition. We perform a detailed scan to show how the baryon asymmetry varies throughout the relevant parameter space. Our results show that the case where the singlet acquires a VEV during the electroweak phase transition typically generates a larger baryon asymmetry, although we expect that the case where the singlet acquires a VEV first is far more common for any model in which parameters unify at a high scale. Finally, we examine the dependence of the baryon asymmetry on the three-body interactions involving gauge singlets.
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spelling doaj.art-bcd71db35e1049aeb629f042a67778a12022-12-22T00:09:34ZengSpringerOpenJournal of High Energy Physics1029-84792017-11-0120171112610.1007/JHEP11(2017)051Electroweak baryogenesis in the ℤ3 $$ {\mathbb{Z}}_3 $$-invariant NMSSMSujeet Akula0Csaba Balázs1Liam Dunn2Graham White3School of Physics and Astronomy, Monash UniversitySchool of Physics and Astronomy, Monash UniversitySchool of Physics and Astronomy, Monash UniversitySchool of Physics and Astronomy, Monash UniversityAbstract We calculate the baryon asymmetry of the Universe in the ℤ3 $$ {\mathbb{Z}}_3 $$-invariant Next-to-Minimal Supersymmetric Standard Model where the interactions of the singlino provide the necessary source of charge and parity violation. Using the closed time path formalism, we derive and solve transport equations for the cases where the singlet acquires a vacuum expectation value (VEV) before and during the electroweak phase transition. We perform a detailed scan to show how the baryon asymmetry varies throughout the relevant parameter space. Our results show that the case where the singlet acquires a VEV during the electroweak phase transition typically generates a larger baryon asymmetry, although we expect that the case where the singlet acquires a VEV first is far more common for any model in which parameters unify at a high scale. Finally, we examine the dependence of the baryon asymmetry on the three-body interactions involving gauge singlets.http://link.springer.com/article/10.1007/JHEP11(2017)051Supersymmetry Phenomenology
spellingShingle Sujeet Akula
Csaba Balázs
Liam Dunn
Graham White
Electroweak baryogenesis in the ℤ3 $$ {\mathbb{Z}}_3 $$-invariant NMSSM
Journal of High Energy Physics
Supersymmetry Phenomenology
title Electroweak baryogenesis in the ℤ3 $$ {\mathbb{Z}}_3 $$-invariant NMSSM
title_full Electroweak baryogenesis in the ℤ3 $$ {\mathbb{Z}}_3 $$-invariant NMSSM
title_fullStr Electroweak baryogenesis in the ℤ3 $$ {\mathbb{Z}}_3 $$-invariant NMSSM
title_full_unstemmed Electroweak baryogenesis in the ℤ3 $$ {\mathbb{Z}}_3 $$-invariant NMSSM
title_short Electroweak baryogenesis in the ℤ3 $$ {\mathbb{Z}}_3 $$-invariant NMSSM
title_sort electroweak baryogenesis in the z3 mathbb z 3 invariant nmssm
topic Supersymmetry Phenomenology
url http://link.springer.com/article/10.1007/JHEP11(2017)051
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AT csababalazs electroweakbaryogenesisinthez3mathbbz3invariantnmssm
AT liamdunn electroweakbaryogenesisinthez3mathbbz3invariantnmssm
AT grahamwhite electroweakbaryogenesisinthez3mathbbz3invariantnmssm