Strong electroweak phase transition in t-channel simplified dark matter models - INSPIRE

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Strong electroweak phase transition in t-channel simplified dark matter models

Simone Biondini
(
- Basel U.
)
,
Philipp Schicho
(
- Helsinki Inst. of Phys.
)
,
Tuomas V.I. Tenkanen
(
- Nordita and
- Royal Inst. Tech., Stockholm and
- Tsung-Dao Lee Inst., Shanghai and
- Shanghai Jiao Tong U.
)

Jul 25, 2022

54 pages

Published in:

JCAP 10 (2022) 044,
JCAP 10 (2022) 044

Published: Oct 13, 2022

e-Print:

2207.12207 [hep-ph]

DOI:

10.1088/1475-7516/2022/10/044

Report number:

HIP-2022-19/TH,
NORDITA 2022-050

View in:

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Abstract: (IOP)

Beyond the Standard Model physics is required to explain both dark matter and the baryon asymmetry of the universe, the latter possibly generated during a strong first-order electroweak phase transition. While many proposed models tackle these problems independently, it is interesting to inquire whether the same model can explain both. In this context, we link state-of-the-art perturbative assessments of the phase transition thermodynamics with the extraction of the dark matter energy density. These techniques are applied to a next-to-minimal dark matter model containing an inert Majorana fermion that is coupled to Standard Model leptons via a scalar mediator, where the mediator interacts directly with the Higgs boson. For dark matter masses 180 GeV < M

_{χ}

≲ 300 GeV, we discern regions of the model parameter space that reproduce the observed dark matter energy density and allow for a first-order phase transition, while evading the most stringent collider constraints.

Note:

54 pages, 12 figures, 1 table; v2: Journal version, extended section 3.2

cosmological phase transitions
cosmology of theories beyond the SM
dark matter theory
physics of the early universe
baryon: asymmetry
effective potential
electroweak interaction: critical phenomena
thermodynamics: critical phenomena
dark matter: freeze-out
dark matter: relic density

References(156)

Figures(15)

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