Dark matter, dark radiation and gravitational waves from mirror Higgs parity

Dunsky, David; Hall, Lawrence J.; Harigaya, Keisuke

doi:10.1007/jhep02(2020)078

Dark matter, dark radiation and gravitational waves from mirror Higgs parity

Journal Article · Wed Feb 12 00:00:00 EST 2020 · Journal of High Energy Physics (Online)

DOI:https://doi.org/10.1007/jhep02(2020)078· OSTI ID:1735537

Dunsky, David ^[1]; Hall, Lawrence J. ^[1]; Harigaya, Keisuke ^[2]

Univ. of California, Berkeley, CA (United States); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
Princeton Univ., NJ (United States)

An exact parity replicates the Standard Model giving a Mirror Standard Model, SM ↔ SM^'. This “Higgs Parity” and the mirror electroweak symmetry are spontaneously broken by the mirror Higgs, (H^') = v^' >> (H), yielding the Standard Model Higgs as a Pseudo-Nambu-Goldstone Boson of an approximate SU (4) symmetry, with a quartic coupling λ_SM(v^') ~ 10^-3. Mirror electromagnetism is unbroken and dark matter is composed of e^' and \( {\overline{e}}^{\prime } \). Direct detection may be possible via the kinetic mixing portal, and in unified theories this rate is correlated with the proton decay rate. With a high reheat temperature after inflation, the e^t dark matter abundance is determined by freeze-out followed by dilution from decays of mirror neutrinos, ν^'→ ℓH . Remarkably, this requires v^'~ (10⁸–10¹⁰) GeV, predicting a Higgs mass of 123 ± 3 GeV at 1σ and a Standard Model neutrino mass of (10^-2–10^-1) eV, consistent with observed neutrino masses. The mirror QCD sector exhibits a first order phase transition producing gravitational waves that may be detected by future observations. Mirror glueballs decay to mirror photons giving dark radiation with ΔN_eff~ 0.03–0.4. With a low reheat temperature after inflation, the e^' dark matter abundance is determined by freeze-in from the SM sector by either the Higgs or kinetic mixing portal.

View Accepted Manuscript (DOE)

Research Organization:: Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)

Sponsoring Organization:: National Science Foundation (NSF); USDOE Office of Science (SC)

Grant/Contract Number:: AC02-05CH11231; SC0009988

OSTI ID:: 1735537

Journal Information:: Journal of High Energy Physics (Online), Journal Name: Journal of High Energy Physics (Online) Journal Issue: 2 Vol. 2020; ISSN 1029-8479

Publisher:: Springer BerlinCopyright Statement

Country of Publication:: United States

Language:: English

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