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Report number arXiv:1702.08909 ; CERN-TH-2017-050
Title Electroweak baryogenesis from a dark sector
Related titleElectroweak baryogenesis from a dark sector
Author(s) Cline, James M. (CERN ; McGill U.) ; Kainulainen, Kimmo (Jyvaskyla U. ; Helsinki Inst. of Phys.) ; Tucker-Smith, David (Williams Coll.)
Publication 2017-06-07
Imprint 2017-02-28
Number of pages 16
Note 16 pages, 15 figures; v2: added references; v3: corrected eq.7, improved treatment of nucleation and wall velocity, added section on indirect detection; published version
In: Phys. Rev. D 95 (2017) 115006
DOI 10.1103/PhysRevD.95.115006
Subject category astro-ph.CO ; Astrophysics and Astronomy ; hep-ph ; Particle Physics - Phenomenology
Abstract Adding an extra singlet scalar $S$ to the Higgs sector can provide a barrier at tree level between a false vacuum with restored electroweak symmetry and the true one. This has been demonstrated to readily give a strong phase transition as required for electroweak baryogenesis. We show that with the addition of a fermionic dark matter particle $\chi$ coupling to $S$, a simple UV-complete model can realize successful electroweak baryogenesis. The dark matter gets a CP asymmetry that is transferred to the standard model through a $CP\ portal\ interaction$, which we take to be a coupling of $\chi$ to $\tau$ leptons and an inert Higgs doublet. The CP asymmetry induced in left-handed $\tau$ leptons biases sphalerons to produce the baryon asymmetry. The model has promising discovery potential at the LHC, while robustly providing a large enough baryon asymmetry and correct dark matter relic density with reasonable values of the couplings.
Copyright/License arXiv nonexclusive-distrib. 1.0
Preprint: © 2017-2025 CERN (License: CC-BY-4.0)



Corresponding record in: Inspire


 レコード 生成: 2017-03-10, 最終変更: 2023-03-12


フルテキスト:
arXiv:1702.08909 - Download fulltextPDF
10.1103_PhysRevD.95.115006 - Download fulltextPDF