Unified explanation for dark matter and electroweak baryogenesis with direct detection and gravitational wave signatures

Mikael Chala, Germano Nardini, and Ivan Sobolev
Phys. Rev. D 94, 055006 – Published 8 September 2016

Abstract

A minimal extension of the Standard Model that provides both a dark matter candidate and a strong first-order electroweak phase transition (EWPT) consists of two additional Lorentz and gauge singlets. In this paper we work out a composite Higgs version of this scenario, based on the coset SO(7)/SO(6). We show that by embedding the elementary fermions in appropriate representations of SO(7), all dominant interactions are described by only three free effective parameters. Within the model dependencies of the embedding, the theory predicts one of the singlets to be stable and responsible for the observed dark matter abundance. At the same time, the second singlet introduces new CP-violation phases and triggers a strong first-order EWPT, making electroweak baryogenesis feasible. It turns out that this scenario does not conflict with current observations and it is promising for solving the dark matter and baryon asymmetry puzzles. The tight predictions of the model will be accessible at the forthcoming dark matter direct detection and gravitational wave experiments.

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  • Received 9 June 2016

DOI:https://doi.org/10.1103/PhysRevD.94.055006

© 2016 American Physical Society

Physics Subject Headings (PhySH)

Particles & FieldsGravitation, Cosmology & Astrophysics

Authors & Affiliations

Mikael Chala1, Germano Nardini2, and Ivan Sobolev3,4

  • 1DESY, Notkestrasse 85, D-22607 Hamburg, Germany
  • 2Albert Einstein Center, Institute for Theoretical Physics, University of Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland
  • 3Institute for Nuclear Research of the Russian Academy of Sciences, 60th October Anniversary prospect 7a, Moscow 117312, Russia
  • 4Department of Particle Physics and Cosmology, Physics Faculty, M. V. Lomonosov Moscow State University, Vorobjevy Gory, 119991 Moscow, Russia

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Issue

Vol. 94, Iss. 5 — 1 September 2016

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