Home > Publications database > Prospects to scrutinise or smash SM*A*S*H |
Journal Article/Contribution to a conference proceedings/Contribution to a book | PUBDB-2023-08072 |
2024
SISSA
Trieste
This record in other databases:
Please use a persistent id in citations: doi:10.22323/1.454.0003 doi:10.3204/PUBDB-2023-08072
Report No.: DESY-23-225; arXiv:2312.14679
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.
Keyword(s): neutrino: mass ; cosmic background radiation: polarization ; vacuum: stability ; baryon: asymmetry ; dark matter ; gravitational radiation detector ; inflation: model ; axion ; cosmological model: parameter space
![]() |
The record appears in these collections: |
Preprint
Prospects to scrutinise or smash SM*A*S*H
[10.3204/PUBDB-2024-00400]
Files
Fulltext by arXiv.org
BibTeX |
EndNote:
XML,
Text |
RIS