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000408369 0247_ $$2datacite_doi$$a10.3204/DESY-PROC-2013-04/ko_pyungwon
000408369 0247_ $$2ISSN$$a1435-8077
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000408369 0881_ $$aDESY-PROC-2013-04
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000408369 1001_ $$0P:(DE-HGF)0$$aBaek, S.$$b0
000408369 1112_ $$0C13-06-24.5$$2inspire$$a9th Patras Workshop on Axions, WIMPs and WISPs$$cMainz$$d2013-06-24 - 2013-06-28$$gAXION-WIMP 2013$$wGermany
000408369 245__ $$aSinglet portal extensions of the standard seesaw models to dark sector with local dark symmetry: An alternative to the new minimal standard model
000408369 260__ $$aHamburg$$bVerlag Deutsches Elektronen-Synchrotron$$c2013
000408369 29510 $$aBaek, S. "Singlet portal extensions of the standard seesaw models to dark sector with local dark symmetry: An alternative to the new minimal standard model" in Proceedings, 9th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2013) / Oberlack, Uwe, Sissol, Pierre (eds.), 2013 ; AXION-WIMP 2013 : 9th Patras Workshop on Axions, WIMPs and WISPs , 2013-06-23 - 2013-06-28, Mainz
000408369 300__ $$a247-251
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000408369 520__ $$aAssuming 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 N eff = 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. 
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000408369 7001_ $$0P:(DE-HGF)0$$aKo, P.$$b1$$eCorresponding author
000408369 7001_ $$0P:(DE-HGF)0$$aPark, W.-I.$$b2
000408369 7870_ $$0PUBDB-2015-05816$$aOberlack, Uwe et. al.$$iisPartOf$$rDESY-PROC-2013-04$$tProceedings, 9th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2013)
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