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Title: Cosmology in Mirror Twin Higgs and neutrino masses

Abstract

We explore a simple solution to the cosmological challenges of the original Mirror Twin Higgs (MTH) model that leads to interesting implications for experiment. We consider theories in which both the standard model and mirror neutrinos acquire masses through the familiar seesaw mechanism, but with a low right-handed neutrino mass scale of order a few GeV. In these $$\nu$$MTH models, the right-handed neutrinos leave the thermal bath while still relativistic. As the universe expands, these particles eventually become nonrelativistic, and come to dominate the energy density of the universe before decaying. Decays to standard model states are preferred, with the result that the visible sector is left at a higher temperature than the twin sector. Consequently the contribution of the twin sector to the radiation density in the early universe is suppressed, allowing the current bounds on this scenario to be satisfied. However, the energy density in twin radiation remains large enough to be discovered in future cosmic microwave background experiments. Finally, in addition, the twin neutrinos are significantly heavier than their standard model counterparts, resulting in a sizable contribution to the overall mass density in neutrinos that can be detected in upcoming experiments designed to probe the large scale structure of the universe.

Authors:
 [1];  [2];  [3];  [3]
  1. Univ. of Maryland, College Park, MD (United States). Maryland Center for Fundamental Physics, Dept. of Physics
  2. Univ. of California, Santa Barbara, CA (United States). Dept. of Physcis
  3. Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
Publication Date:
Research Org.:
Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
Sponsoring Org.:
USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25); National Science Foundation (NSF)
OSTI Identifier:
1368364
Report Number(s):
FERMILAB-PUB-16-555-T
Journal ID: ISSN 1029-8479; 1500212
Grant/Contract Number:  
AC02-07CH11359; SC0014129; PHY-1620074
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: 2017; 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; Cosmology of Theories beyond the SM; Beyond Standard Model

Citation Formats

Chacko, Zackaria, Craig, Nathaniel, Fox, Patrick J., and Harnik, Roni. Cosmology in Mirror Twin Higgs and neutrino masses. United States: N. p., 2017. Web. doi:10.1007/JHEP07(2017)023.
Chacko, Zackaria, Craig, Nathaniel, Fox, Patrick J., & Harnik, Roni. Cosmology in Mirror Twin Higgs and neutrino masses. United States. doi:10.1007/JHEP07(2017)023.
Chacko, Zackaria, Craig, Nathaniel, Fox, Patrick J., and Harnik, Roni. Thu . "Cosmology in Mirror Twin Higgs and neutrino masses". United States. doi:10.1007/JHEP07(2017)023. https://www.osti.gov/servlets/purl/1368364.
@article{osti_1368364,
title = {Cosmology in Mirror Twin Higgs and neutrino masses},
author = {Chacko, Zackaria and Craig, Nathaniel and Fox, Patrick J. and Harnik, Roni},
abstractNote = {We explore a simple solution to the cosmological challenges of the original Mirror Twin Higgs (MTH) model that leads to interesting implications for experiment. We consider theories in which both the standard model and mirror neutrinos acquire masses through the familiar seesaw mechanism, but with a low right-handed neutrino mass scale of order a few GeV. In these $\nu$MTH models, the right-handed neutrinos leave the thermal bath while still relativistic. As the universe expands, these particles eventually become nonrelativistic, and come to dominate the energy density of the universe before decaying. Decays to standard model states are preferred, with the result that the visible sector is left at a higher temperature than the twin sector. Consequently the contribution of the twin sector to the radiation density in the early universe is suppressed, allowing the current bounds on this scenario to be satisfied. However, the energy density in twin radiation remains large enough to be discovered in future cosmic microwave background experiments. Finally, in addition, the twin neutrinos are significantly heavier than their standard model counterparts, resulting in a sizable contribution to the overall mass density in neutrinos that can be detected in upcoming experiments designed to probe the large scale structure of the universe.},
doi = {10.1007/JHEP07(2017)023},
journal = {Journal of High Energy Physics (Online)},
number = 7,
volume = 2017,
place = {United States},
year = {2017},
month = {7}
}

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Cited by: 15 works
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    Works referencing / citing this record:

    Signatures of mirror stars
    journal, March 2020