Dark matter, dark radiation and gravitational waves from mirror Higgs parity
Abstract
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 λSM(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 et 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 ΔNeff~ 0.03–0.4. With a low reheat temperature after inflation, the e' dark matter abundance is determinedmore »
- Authors:
-
- Univ. of California, Berkeley, CA (United States); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Princeton Univ., NJ (United States)
- Publication Date:
- Research Org.:
- Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC); National Science Foundation (NSF)
- OSTI Identifier:
- 1735537
- Grant/Contract Number:
- AC02-05CH11231; SC0009988; PHY-1316783; PHY-1521446; PHY-1607611
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Journal of High Energy Physics (Online)
- Additional Journal Information:
- Journal Name: Journal of High Energy Physics (Online); Journal Volume: 2020; Journal Issue: 2; Journal ID: ISSN 1029-8479
- Publisher:
- Springer Berlin
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; Beyond Standard Model; Cosmology of theories beyond the SM; Higgs physics
Citation Formats
Dunsky, David, Hall, Lawrence J., and Harigaya, Keisuke. Dark matter, dark radiation and gravitational waves from mirror Higgs parity. United States: N. p., 2020.
Web. doi:10.1007/jhep02(2020)078.
Dunsky, David, Hall, Lawrence J., & Harigaya, Keisuke. Dark matter, dark radiation and gravitational waves from mirror Higgs parity. United States. https://doi.org/10.1007/jhep02(2020)078
Dunsky, David, Hall, Lawrence J., and Harigaya, Keisuke. Wed .
"Dark matter, dark radiation and gravitational waves from mirror Higgs parity". United States. https://doi.org/10.1007/jhep02(2020)078. https://www.osti.gov/servlets/purl/1735537.
@article{osti_1735537,
title = {Dark matter, dark radiation and gravitational waves from mirror Higgs parity},
author = {Dunsky, David and Hall, Lawrence J. and Harigaya, Keisuke},
abstractNote = {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 λSM(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 et 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 ΔNeff~ 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.},
doi = {10.1007/jhep02(2020)078},
journal = {Journal of High Energy Physics (Online)},
number = 2,
volume = 2020,
place = {United States},
year = {Wed Feb 12 00:00:00 EST 2020},
month = {Wed Feb 12 00:00:00 EST 2020}
}
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