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@INPROCEEDINGS{Ringwald:600649,
      author       = {Ringwald, Andreas},
      title        = {{P}rospects to scrutinise or smash {SM}*{A}*{S}*{H}},
      journal      = {Proceedings of Science / International School for Advanced
                      Studies},
      volume       = {(COSMICWISPers)},
      issn         = {1824-8039},
      address      = {Trieste},
      publisher    = {SISSA},
      reportid     = {PUBDB-2023-08072, DESY-23-225. arXiv:2312.14679},
      series       = {2740324},
      pages        = {003},
      year         = {2024},
      note         = {13 pages, 9 pages, contribution to the proceedings of the
                      1st General Meeting and 1st Training School of the COST
                      Action COSMIC WISPers (COSMICWISPers)},
      abstract     = {SM*A*S*H is an extension of the Standard Model of particle
                      physics which has just the minimal number of fields in order
                      to solve six puzzles of particle physics and cosmology in
                      one smash: vacuum stability, inflation, baryon asymmetry,
                      neutrino masses, strong CP, and dark matter. The parameters
                      of SM*A*S*H are constrained by symmetries and requirements
                      to solve these puzzles.This provides various firm
                      predictions for observables which can be confronted with
                      experiments. We discuss the prospects and timeline to
                      scrutinise or smash SM*A*S*H by cosmic microwave background
                      polarisation experiments, axion haloscopes, and future
                      space-borne gravitational wave detectors.},
      month         = {Sep},
      date          = {2023-09-05},
      organization  = {1st General Meeting and 1st Training
                       School of the COST Action COSMIC
                       WISPers, Bari (Italy), 5 Sep 2023 - 14
                       Sep 2023},
      keywords     = {neutrino: mass (INSPIRE) / cosmic background radiation:
                      polarization (INSPIRE) / vacuum: stability (INSPIRE) /
                      baryon: asymmetry (INSPIRE) / dark matter (INSPIRE) /
                      gravitational radiation detector (INSPIRE) / inflation:
                      model (INSPIRE) / axion (INSPIRE) / cosmological model:
                      parameter space (INSPIRE)},
      cin          = {T / ALPS},
      ddc          = {530},
      cid          = {I:(DE-H253)T-20120731 / I:(DE-H253)ALPS-20130318},
      pnm          = {611 - Fundamental Particles and Forces (POF4-611) / DFG
                      project G:(GEPRIS)390833306 - EXC 2121: Quantum Universe
                      (390833306)},
      pid          = {G:(DE-HGF)POF4-611 / G:(GEPRIS)390833306},
      experiment   = {EXP:(DE-H253)MADMAX-20210101 / EXP:(DE-MLZ)NOSPEC-20140101},
      typ          = {PUB:(DE-HGF)16 / PUB:(DE-HGF)8 / PUB:(DE-HGF)7},
      eprint       = {2312.14679},
      howpublished = {arXiv:2312.14679},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:2312.14679;\%\%$},
      doi          = {10.22323/1.454.0003},
      url          = {https://bib-pubdb1.desy.de/record/600649},
}