Sterile neutrino dark matter and leptogenesis in Left-Right Higgs Parity

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

doi:10.1007/jhep01(2021)125

Title: Sterile neutrino dark matter and leptogenesis in Left-Right Higgs Parity

Journal Article · Thu Jan 21 00:00:00 EST 2021 · Journal of High Energy Physics (Online)

DOI:https://doi.org/10.1007/jhep01(2021)125· OSTI ID:1798759

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)
Institute for Advanced Study, Princeton, NJ (United States)

The standard model Higgs quartic coupling vanishes at (10⁹ – 10¹³) GeV. We study SU(2)_L × SU(2)_R × U(1)_B–L theories that incorporate the Higgs Parity mechanism, where this becomes the scale of Left-Right symmetry breaking, $$v_R$$. Furthermore, these theories solve the strong CP problem and predict three right-handed neutrinos. We introduce cosmologies where SU(2)_R × U(1)_B–L gauge interactions produce right-handed neutrinos via the freeze-out or freeze-in mechanisms. In both cases, we find the parameter space where the lightest right-handed neutrino is dark matter and the decay of a heavier one creates the baryon asymmetry of the universe via leptogenesis. A theory of flavor is constructed that naturally accounts for the lightness and stability of the right-handed neutrino dark matter, while maintaining sufficient baryon asymmetry. The dark matter abundance and successful natural leptogenesis require vR to be in the range (10¹⁰ – 10¹³) GeV for freeze-out, in remarkable agreement with the scale where the Higgs quartic coupling vanishes, whereas freeze-in requires $$v_R$$ ≳ 109 GeV. The allowed parameter space can be probed by the warmness of dark matter, precise determinations of the top quark mass and QCD coupling by future colliders and lattice computations, and measurement of the neutrino mass hierarchy.

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

Sponsoring Organization:: USDOE Office of Science (SC), High Energy Physics (HEP); USDOE Office of Science (SC), Nuclear Physics (NP); National Science Foundation (NSF); Raymond and Beverly Sackler Foundation Fund (KH)

Grant/Contract Number:: AC02-05CH11231; SC0009988; PHY-1316783; PHY-1521446

OSTI ID:: 1798759

Journal Information:: Journal of High Energy Physics (Online), Vol. 2021, Issue 1; ISSN 1029-8479

Publisher:: Springer BerlinCopyright Statement

Country of Publication:: United States

Language:: English

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