TY - JOUR
T1 - Hidden monopole dark matter via axion portal and its implications for direct detection searches, beam-dump experiments, and the H 0 tension
AU - Daido, Ryuji
AU - Ho, Shu Yu
AU - Takahashi, Fuminobu
N1 - Funding Information:
This article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0), which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited
Publisher Copyright:
© 2020, The Author(s).
PY - 2020/1/1
Y1 - 2020/1/1
N2 - Hidden monopole is a plausible dark matter candidate due to its stability, but its direct experimental search is extremely difficult due to feeble interactions with the standard model particles in the minimal form. Then, we introduce an axion, a, connecting the hidden monopole and the standard model particles and examine the current limits and future prospects of direct dark matter searches and beam-dump experiments. We find two parameter regions around ma = O(10) MeV, fa = O(105) GeV and ma = O(100) MeV, fa = O(104) GeV where monopole dark matter and the axion are respectively within the reach of the future experiments such as PICO-500 and SHiP. We also note that the hidden photons mainly produced by the axion decay contribute to dark radiation with ∆Neff ≃ 0.6 which can relax the H0 tension.
AB - Hidden monopole is a plausible dark matter candidate due to its stability, but its direct experimental search is extremely difficult due to feeble interactions with the standard model particles in the minimal form. Then, we introduce an axion, a, connecting the hidden monopole and the standard model particles and examine the current limits and future prospects of direct dark matter searches and beam-dump experiments. We find two parameter regions around ma = O(10) MeV, fa = O(105) GeV and ma = O(100) MeV, fa = O(104) GeV where monopole dark matter and the axion are respectively within the reach of the future experiments such as PICO-500 and SHiP. We also note that the hidden photons mainly produced by the axion decay contribute to dark radiation with ∆Neff ≃ 0.6 which can relax the H0 tension.
KW - Phenomenological Models
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U2 - 10.1007/JHEP01(2020)185
DO - 10.1007/JHEP01(2020)185
M3 - Article
AN - SCOPUS:85078765014
SN - 1126-6708
VL - 2020
JO - Journal of High Energy Physics
JF - Journal of High Energy Physics
IS - 1
M1 - 185
ER -