ホーム > Electroweak baryogenesis from a dark sector |
Published Articles | |
Report number | arXiv:1702.08909 ; CERN-TH-2017-050 |
Title | Electroweak baryogenesis from a dark sector |
Related title | Electroweak 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) |