000600649 001__ 600649
000600649 005__ 20250801212026.0
000600649 0247_ $$2doi$$a10.22323/1.454.0003
000600649 0247_ $$2datacite_doi$$a10.3204/PUBDB-2023-08072
000600649 0247_ $$2arXiv$$aarXiv:2312.14679
000600649 0247_ $$2openalex$$aopenalex:W4391449673
000600649 037__ $$aPUBDB-2023-08072
000600649 041__ $$aEnglish
000600649 082__ $$a530
000600649 088__ $$2DESY$$aDESY-23-225
000600649 088__ $$2arXiv$$aarXiv:2312.14679
000600649 1001_ $$0P:(DE-H253)PIP1001650$$aRingwald, Andreas$$b0$$eCorresponding author$$udesy
000600649 1112_ $$a1st General Meeting and 1st Training School of the COST Action COSMIC WISPers$$cBari$$d2023-09-05 - 2023-09-14$$g(COSMICWISPers)$$wItaly
000600649 245__ $$aProspects to scrutinise or smash SM*A*S*H
000600649 260__ $$aTrieste$$bSISSA$$c2024
000600649 300__ $$a13
000600649 3367_ $$2ORCID$$aCONFERENCE_PAPER
000600649 3367_ $$033$$2EndNote$$aConference Paper
000600649 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$mjournal
000600649 3367_ $$2BibTeX$$aINPROCEEDINGS
000600649 3367_ $$2DRIVER$$aconferenceObject
000600649 3367_ $$2DataCite$$aOutput Types/Conference Paper
000600649 3367_ $$0PUB:(DE-HGF)8$$2PUB:(DE-HGF)$$aContribution to a conference proceedings$$bcontrib$$mcontrib$$s1754057013_3349141
000600649 3367_ $$0PUB:(DE-HGF)7$$2PUB:(DE-HGF)$$aContribution to a book$$mcontb
000600649 4900_ $$2Author$$a2740324
000600649 500__ $$a13 pages, 9 pages, contribution to the proceedings of the 1st General Meeting and 1st Training School of the COST Action COSMIC WISPers (COSMICWISPers)
000600649 520__ $$aSM*A*S*H is an extension of the Standard Model of particle physics which has just the minimal number of fields in order to solve six puzzles of particle physics and cosmology in one smash: vacuum stability, inflation, baryon asymmetry, neutrino masses, strong CP, and dark matter. The parameters of SM*A*S*H are constrained by symmetries and requirements to solve these puzzles.This provides various firm predictions for observables which can be confronted with experiments. We discuss the prospects and timeline to scrutinise or smash SM*A*S*H by cosmic microwave background polarisation experiments, axion haloscopes, and future space-borne gravitational wave detectors.
000600649 536__ $$0G:(DE-HGF)POF4-611$$a611 - Fundamental Particles and Forces (POF4-611)$$cPOF4-611$$fPOF IV$$x0
000600649 536__ $$0G:(GEPRIS)390833306$$aDFG project G:(GEPRIS)390833306 - EXC 2121: Quantum Universe (390833306)$$c390833306$$x1
000600649 588__ $$aDataset connected to CrossRef Conference
000600649 650_7 $$2INSPIRE$$aneutrino: mass
000600649 650_7 $$2INSPIRE$$acosmic background radiation: polarization
000600649 650_7 $$2INSPIRE$$avacuum: stability
000600649 650_7 $$2INSPIRE$$abaryon: asymmetry
000600649 650_7 $$2INSPIRE$$adark matter
000600649 650_7 $$2INSPIRE$$agravitational radiation detector
000600649 650_7 $$2INSPIRE$$ainflation: model
000600649 650_7 $$2INSPIRE$$aaxion
000600649 650_7 $$2INSPIRE$$acosmological model: parameter space
000600649 693__ $$0EXP:(DE-H253)MADMAX-20210101$$5EXP:(DE-H253)MADMAX-20210101$$eMAgnetized Disc and Mirror Axion eXperiment$$x0
000600649 693__ $$0EXP:(DE-MLZ)NOSPEC-20140101$$5EXP:(DE-MLZ)NOSPEC-20140101$$eNo specific instrument$$x1
000600649 77318 $$2Crossref$$3proceedings-article$$a10.22323/1.454.0003$$bSissa Medialab$$d2024-02-01$$p003$$tProceedings of 1st General Meeting and 1st Training School of the COST Action COSMIC WSIPers — PoS(COSMICWISPers)$$y2024
000600649 773__ $$0PERI:(DE-600)2642026-0$$a10.22323/1.454.0003$$p003$$tProceedings of Science / International School for Advanced Studies$$v(COSMICWISPers)$$x1824-8039$$y2024
000600649 7870_ $$0PUBDB-2024-00400$$aRingwald, Andreas$$d2023$$iIsParent$$rarXiv:2312.14679 ; DESY-23-225$$tProspects to scrutinise or smash SM*A*S*H
000600649 8564_ $$uhttps://bib-pubdb1.desy.de/record/600649/files/HTML-Approval_of_scientific_publication.html
000600649 8564_ $$uhttps://bib-pubdb1.desy.de/record/600649/files/PDF-Approval_of_scientific_publication.pdf
000600649 8564_ $$uhttps://bib-pubdb1.desy.de/record/600649/files/COSMICWISPers_003.pdf$$yRestricted$$zStatID:(DE-HGF)0599
000600649 8564_ $$uhttps://bib-pubdb1.desy.de/record/600649/files/smash_SMASH.pdf$$yOpenAccess$$zStatID:(DE-HGF)0510
000600649 8564_ $$uhttps://bib-pubdb1.desy.de/record/600649/files/COSMICWISPers_003.pdf?subformat=pdfa$$xpdfa$$yRestricted$$zStatID:(DE-HGF)0599
000600649 8564_ $$uhttps://bib-pubdb1.desy.de/record/600649/files/smash_SMASH.pdf?subformat=pdfa$$xpdfa$$yOpenAccess$$zStatID:(DE-HGF)0510
000600649 909CO $$ooai:bib-pubdb1.desy.de:600649$$pVDB$$popen_access$$popenaire$$pdnbdelivery$$pdriver
000600649 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1001650$$aDeutsches Elektronen-Synchrotron$$b0$$kDESY
000600649 9131_ $$0G:(DE-HGF)POF4-611$$1G:(DE-HGF)POF4-610$$2G:(DE-HGF)POF4-600$$3G:(DE-HGF)POF4$$4G:(DE-HGF)POF$$aDE-HGF$$bForschungsbereich Materie$$lMatter and the Universe$$vFundamental Particles and Forces$$x0
000600649 9141_ $$y2024
000600649 915__ $$0LIC:(DE-HGF)CCBYNCND4$$2HGFVOC$$aCreative Commons Attribution-NonCommercial-NoDerivs CC BY-NC-ND 4.0
000600649 915__ $$0StatID:(DE-HGF)0501$$2StatID$$aDBCoverage$$bDOAJ Seal$$d2021-04-20T14:42:38Z
000600649 915__ $$0StatID:(DE-HGF)0500$$2StatID$$aDBCoverage$$bDOAJ$$d2021-04-20T14:42:38Z
000600649 915__ $$0StatID:(DE-HGF)0510$$2StatID$$aOpenAccess
000600649 915__ $$0StatID:(DE-HGF)0030$$2StatID$$aPeer Review$$bDOAJ : Editorial review$$d2021-04-20T14:42:38Z
000600649 915__ $$0StatID:(DE-HGF)0200$$2StatID$$aDBCoverage$$bSCOPUS$$d2025-01-02
000600649 915__ $$0StatID:(DE-HGF)0300$$2StatID$$aDBCoverage$$bMedline$$d2025-01-02
000600649 9201_ $$0I:(DE-H253)T-20120731$$kT$$lTheorie-Gruppe$$x0
000600649 9201_ $$0I:(DE-H253)ALPS-20130318$$kALPS$$lAny Light Particle Search$$x1
000600649 980__ $$acontrib
000600649 980__ $$aVDB
000600649 980__ $$ajournal
000600649 980__ $$acontb
000600649 980__ $$aI:(DE-H253)T-20120731
000600649 980__ $$aI:(DE-H253)ALPS-20130318
000600649 980__ $$aUNRESTRICTED
000600649 9801_ $$aFullTexts