TY - JOUR
T1 - Vanishing Higgs potential at the Planck scale in a singlet extension of the standard model
AU - Haba, Naoyuki
AU - Ishida, Hiroyuki
AU - Kaneta, Kunio
AU - Takahashi, Ryo
PY - 2014/8/25
Y1 - 2014/8/25
N2 - We discuss the realization of a vanishing effective Higgs potential at the Planck scale, which is required by the multiple-point criticality principle (MPCP), in the standard model with singlet scalar dark matter and a right-handed neutrino. We find the scalar dark matter and the right-handed neutrino play crucial roles for realization of the MPCP, where a neutrino Yukawa becomes effective above the Majorana mass of the right-handed neutrino. Once the top mass is fixed, the MPCP at the (reduced) Planck scale and the suitable dark matter relic abundance determine the dark matter mass, mS, and the Majorana mass of the right-handed neutrino, MR, as 8.5(8.0)×102GeV≤mS≤1.4(1.2) ×103GeV and 6.3(5.5)×1013GeV≤MR≤1.6(1.2)×1014GeV within current experimental values of the Higgs and top masses. This scenario is consistent with current dark matter direct search experiments and will be checked by future experiments such as LUX with further exposure and/or the XENON1T.
AB - We discuss the realization of a vanishing effective Higgs potential at the Planck scale, which is required by the multiple-point criticality principle (MPCP), in the standard model with singlet scalar dark matter and a right-handed neutrino. We find the scalar dark matter and the right-handed neutrino play crucial roles for realization of the MPCP, where a neutrino Yukawa becomes effective above the Majorana mass of the right-handed neutrino. Once the top mass is fixed, the MPCP at the (reduced) Planck scale and the suitable dark matter relic abundance determine the dark matter mass, mS, and the Majorana mass of the right-handed neutrino, MR, as 8.5(8.0)×102GeV≤mS≤1.4(1.2) ×103GeV and 6.3(5.5)×1013GeV≤MR≤1.6(1.2)×1014GeV within current experimental values of the Higgs and top masses. This scenario is consistent with current dark matter direct search experiments and will be checked by future experiments such as LUX with further exposure and/or the XENON1T.
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U2 - 10.1103/PhysRevD.90.036006
DO - 10.1103/PhysRevD.90.036006
M3 - Article
AN - SCOPUS:84918807638
SN - 1550-7998
VL - 90
JO - Physical Review D - Particles, Fields, Gravitation and Cosmology
JF - Physical Review D - Particles, Fields, Gravitation and Cosmology
IS - 3
M1 - 036006
ER -