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000395468 0247_ $$2datacite_doi$$a10.3204/DESY-PROC-2009-03/Ringwald_Andreas
000395468 0247_ $$2ISSN$$a1435-8077
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000395468 0881_ $$aDESY-PROC-2016-03
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000395468 1001_ $$0P:(DE-H253)PIP1001650$$aRingwald, Andreas$$b0$$eCorresponding author$$udesy
000395468 1112_ $$0C16-06-20.4$$2inspire$$a12th Patras Workshop on Axions, WIMPs and WISPs$$cJeju Island$$d2016-06-20 - 2016-06-24$$gAXION-WIMP 2016$$wSouth Korea
000395468 245__ $$aSM*A*S*H
000395468 260__ $$aHamburg$$bVerlag Deutsches Elektronen-Synchrotron$$c2017
000395468 29510 $$aRingwald, Andreas "SM*A*S*H" in 12th "Patras" Workshop on Axions, WIMPs and WISPs, PATRAS 2016 / Kim, Younglm, Lindner, Axel, Semertzidis, Yannis K. (eds.), Verlag Deutsches Elektronen-Synchrotron : 2017 ; PATRAS 2016 : 12th "Patras" Workshop on Axions, WIMPs and WISPs, 2016-06-20 - 2016-06-24, Jeju Island
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000395468 520__ $$aWe present a minimal model for particle physics and cosmology. The Standard Model (SM) particle content is extended by three right-handed SM-singlet neutrinos $N_i$ and a vector-like quark $Q$, all of them being charged under a global lepton number and Peccei-Quinn (PQ) $U(1)$ symmetry which is spontaneously broken by the vacuum expectation value $v_\sigma \sim 10^{11}$ GeV of a SM-singlet complex scalar field $\sigma$. Five fundamental problems -- neutrino oscillations, baryogenesis, dark matter, inflation, strong CP problem -- are solved at one stroke in this model, dubbed ``SM*A*S*H" (Standard Model*Axion*Seesaw*Higgs portal inflation). It can be probed decisively by upcoming cosmic microwave background and axion dark matter experiments.
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000395468 7870_ $$0PUBDB-2017-11637$$aKim, Younglm et. al.$$dVerlag Deutsches Elektronen-Synchrotron$$iisPartOf$$rDESY-PROC-2016-03$$t12th "Patras" Workshop on Axions, WIMPs and WISPs, PATRAS 2016
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