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@INPROCEEDINGS{Ringwald:395468,
      author       = {Ringwald, Andreas},
      title        = {{SM}*{A}*{S}*{H}},
      address      = {Hamburg},
      publisher    = {Verlag Deutsches Elektronen-Synchrotron},
      reportid     = {PUBDB-2017-12133, DESY-PROC-2016-03},
      isbn         = {978-3-945931-06-6},
      series       = {DESY-PROC},
      pages        = {3-8},
      year         = {2017},
      comment      = {Ringwald, 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},
      booktitle     = {Ringwald, 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},
      abstract     = {We 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.},
      month         = {Jun},
      date          = {2016-06-20},
      organization  = {12th Patras Workshop on Axions, WIMPs
                       and WISPs, Jeju Island (South Korea),
                       20 Jun 2016 - 24 Jun 2016},
      cin          = {L},
      cid          = {I:(DE-H253)L-20120731},
      pnm          = {899 - ohne Topic (POF3-899)},
      pid          = {G:(DE-HGF)POF3-899},
      experiment   = {EXP:(DE-MLZ)NOSPEC-20140101},
      typ          = {PUB:(DE-HGF)29 / PUB:(DE-HGF)8 / PUB:(DE-HGF)7},
      doi          = {10.3204/DESY-PROC-2009-03/Ringwald_Andreas},
      url          = {https://bib-pubdb1.desy.de/record/395468},
}