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Title: Higgs Parity, strong CP and dark matter

Abstract

An exact spacetime parity replicates the $$SU(2) \times U(1)$$ electroweak interaction, the Higgs boson $H$, and the matter of the Standard Model. This "Higgs Parity" and the mirror electroweak symmetry are spontaneously broken at scale $$v' = \left\langle{H'} \right\rangle \gg \left\langle{H}\right\rangle$$, yielding the Standard Model below $v'$ with a quartic coupling that essentially vanishes at $v'$: $$\lambda_{SM}(v') \sim 10^{-3}$$. The strong CP problem is solved as Higgs parity forces the masses of mirror quarks and ordinary quarks to have opposite phases. Dark matter is composed of mirror electrons, $e'$, stabilized by unbroken mirror electromagnetism. These interact with Standard Model particles via kinetic mixing between the photon and the mirror photon, which arises at four-loop level and is a firm prediction of the theory. Physics below $v'$, including the mass and interaction of $e'$ dark matter, is described by $$\textit{one fewer parameter}$$ than in the Standard Model. The allowed range of $$m_{e'}$$ is determined by uncertainties in $$(\alpha_s, m_t, m_h)$$, so that future precision measurements of these will be correlated with the direct detection rate of $e'$ dark matter, which, together with the neutron electric dipole moment, will probe the entire parameter space.

Authors:
 [1];  [1];  [2]
  1. Univ. of California, Berkeley, CA (United States). Dept. of Physics; Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States). Theoretical Physics Group
  2. Univ. of California, Berkeley, CA (United States). Dept. of Physics; Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States). Theoretical Physics Group; Inst. for Advanced Study, Princeton, NJ (United States). School of Natural Sciences
Publication Date:
Research Org.:
Institute for Advanced Study, Princeton, NJ (United States); Univ. of California, Berkeley, CA (United States)
Sponsoring Org.:
USDOE Office of Science (SC), High Energy Physics (HEP); National Science Foundation (NSF)
OSTI Identifier:
1596654
Grant/Contract Number:  
SC0009988; AC02-05CH11231; PHY-1316783; PHY-1521446
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: 2019; Journal Issue: 7; 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; Higgs Physics

Citation Formats

Dunsky, David, Hall, Lawrence J., and Harigaya, Keisuke. Higgs Parity, strong CP and dark matter. United States: N. p., 2019. Web. doi:10.1007/JHEP07(2019)016.
Dunsky, David, Hall, Lawrence J., & Harigaya, Keisuke. Higgs Parity, strong CP and dark matter. United States. https://doi.org/10.1007/JHEP07(2019)016
Dunsky, David, Hall, Lawrence J., and Harigaya, Keisuke. Wed . "Higgs Parity, strong CP and dark matter". United States. https://doi.org/10.1007/JHEP07(2019)016. https://www.osti.gov/servlets/purl/1596654.
@article{osti_1596654,
title = {Higgs Parity, strong CP and dark matter},
author = {Dunsky, David and Hall, Lawrence J. and Harigaya, Keisuke},
abstractNote = {An exact spacetime parity replicates the $SU(2) \times U(1)$ electroweak interaction, the Higgs boson $H$, and the matter of the Standard Model. This "Higgs Parity" and the mirror electroweak symmetry are spontaneously broken at scale $v' = \left\langle{H'} \right\rangle \gg \left\langle{H}\right\rangle$, yielding the Standard Model below $v'$ with a quartic coupling that essentially vanishes at $v'$: $\lambda_{SM}(v') \sim 10^{-3}$. The strong CP problem is solved as Higgs parity forces the masses of mirror quarks and ordinary quarks to have opposite phases. Dark matter is composed of mirror electrons, $e'$, stabilized by unbroken mirror electromagnetism. These interact with Standard Model particles via kinetic mixing between the photon and the mirror photon, which arises at four-loop level and is a firm prediction of the theory. Physics below $v'$, including the mass and interaction of $e'$ dark matter, is described by $\textit{one fewer parameter}$ than in the Standard Model. The allowed range of $m_{e'}$ is determined by uncertainties in $(\alpha_s, m_t, m_h)$, so that future precision measurements of these will be correlated with the direct detection rate of $e'$ dark matter, which, together with the neutron electric dipole moment, will probe the entire parameter space.},
doi = {10.1007/JHEP07(2019)016},
journal = {Journal of High Energy Physics (Online)},
number = 7,
volume = 2019,
place = {United States},
year = {2019},
month = {7}
}

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