TY - GEN
T1 - Singlet portal extensions of the standard seesaw models to dark sector with local dark symmetry
T2 - 9th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2013
AU - Baek, S.
AU - Ko, P.
AU - Park, W. I.
N1 - Publisher Copyright:
© 2013 Proceedings of the 9th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2013. All rights reserved.
PY - 2020
Y1 - 2020
N2 - Assuming dark matter is absolutely stable due to unbroken dark gauge symmetry and singlet operators are portals to the dark sector, we present a simple extension of the standard seesaw model that can accommodate all the cosmological observations as well as terrestrial experiments available as of now, including leptogenesis, extra dark radiation of ∼ 8% (resulting in Neff = 3.130 the effective number of neutrino species), Higgs inflation, small and large scale structure formation, and current relic density of scalar DM (X). The Higgs signal strength is equal to one as in the SM for unbroken U(1)X case with a scalar dark matter, but it could be less than one independent of decay channels if the dark matter is a dark sector fermion or if U(1)X is spontaneously broken, because of a mixing with a new neutral scalar boson in the models.
AB - Assuming dark matter is absolutely stable due to unbroken dark gauge symmetry and singlet operators are portals to the dark sector, we present a simple extension of the standard seesaw model that can accommodate all the cosmological observations as well as terrestrial experiments available as of now, including leptogenesis, extra dark radiation of ∼ 8% (resulting in Neff = 3.130 the effective number of neutrino species), Higgs inflation, small and large scale structure formation, and current relic density of scalar DM (X). The Higgs signal strength is equal to one as in the SM for unbroken U(1)X case with a scalar dark matter, but it could be less than one independent of decay channels if the dark matter is a dark sector fermion or if U(1)X is spontaneously broken, because of a mixing with a new neutral scalar boson in the models.
UR - https://www.scopus.com/pages/publications/85085942045
U2 - 10.3204/DESY-PROC-2013-04/ko_pyungwon
DO - 10.3204/DESY-PROC-2013-04/ko_pyungwon
M3 - Conference paper
AN - SCOPUS:85085942045
T3 - Proceedings of the 9th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2013
SP - 247
EP - 251
BT - Proceedings of the 9th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2013
A2 - Uwe, Oberlack
A2 - Pierre, Sissol
PB - Verlag Deutsches Elektronen-Synchrotron
Y2 - 24 June 2013 through 28 June 2013
ER -