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001     600649
005     20250801212026.0
024 7 _ |a 10.22323/1.454.0003
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024 7 _ |a arXiv:2312.14679
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088 _ _ |a arXiv:2312.14679
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100 1 _ |a Ringwald, Andreas
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111 2 _ |a 1st General Meeting and 1st Training School of the COST Action COSMIC WISPers
|g (COSMICWISPers)
|c Bari
|d 2023-09-05 - 2023-09-14
|w Italy
245 _ _ |a Prospects to scrutinise or smash SM*A*S*H
260 _ _ |a Trieste
|c 2024
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300 _ _ |a 13
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500 _ _ |a 13 pages, 9 pages, contribution to the proceedings of the 1st General Meeting and 1st Training School of the COST Action COSMIC WISPers (COSMICWISPers)
520 _ _ |a 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.
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588 _ _ |a Dataset connected to CrossRef Conference
650 _ 7 |a neutrino: mass
|2 INSPIRE
650 _ 7 |a cosmic background radiation: polarization
|2 INSPIRE
650 _ 7 |a vacuum: stability
|2 INSPIRE
650 _ 7 |a baryon: asymmetry
|2 INSPIRE
650 _ 7 |a dark matter
|2 INSPIRE
650 _ 7 |a gravitational radiation detector
|2 INSPIRE
650 _ 7 |a inflation: model
|2 INSPIRE
650 _ 7 |a axion
|2 INSPIRE
650 _ 7 |a cosmological model: parameter space
|2 INSPIRE
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693 _ _ |0 EXP:(DE-MLZ)NOSPEC-20140101
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773 1 8 |a 10.22323/1.454.0003
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|t Proceedings of 1st General Meeting and 1st Training School of the COST Action COSMIC WSIPers — PoS(COSMICWISPers)
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773 _ _ |a 10.22323/1.454.0003
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787 0 _ |a Ringwald, Andreas
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|t Prospects to scrutinise or smash SM*A*S*H
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914 1 _ |y 2024
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