000169207 001__ 169207
000169207 005__ 20250717112550.0
000169207 0247_ $$2doi$$a10.1007/JHEP06(2014)037
000169207 0247_ $$2ISSN$$a1029-8479
000169207 0247_ $$2ISSN$$a1126-6708
000169207 0247_ $$2WOS$$aWOS:000337032000002
000169207 0247_ $$2inspire$$ainspire:1286910
000169207 0247_ $$2altmetric$$aaltmetric:2209504
000169207 0247_ $$2arXiv$$aarXiv:1403.5760
000169207 0247_ $$2openalex$$aopenalex:W2033241389
000169207 037__ $$aDESY-2014-02855
000169207 041__ $$aEnglish
000169207 082__ $$a530
000169207 088__ $$2DESY$$aDESY-14-020
000169207 088__ $$2arXiv$$aarXiv:1403.5760
000169207 1001_ $$0P:(DE-HGF)0$$aDias, A. G.$$b0
000169207 245__ $$aThe quest for an intermediate-scale accidental axion and further ALPs
000169207 260__ $$aBerlin$$bSpringer$$c2014
000169207 3367_ $$2DRIVER$$aarticle
000169207 3367_ $$2DataCite$$aOutput Types/Journal article
000169207 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$bjournal$$mjournal$$s1601389441_5071
000169207 3367_ $$2BibTeX$$aARTICLE
000169207 3367_ $$2ORCID$$aJOURNAL_ARTICLE
000169207 3367_ $$00$$2EndNote$$aJournal Article
000169207 500__ $$3POF3_Assignment on 2016-02-09
000169207 520__ $$aThe recent detection of the cosmic microwave background polarimeter experiment BICEP2 of tensor fluctuations in the B-mode power spectrum basically excludes all plausible axion models where its decay constant is above $10^{13}$ GeV. Moreover, there are strong theoretical, astrophysical, and cosmological motivations for models involving, in addition to the axion, also axion-like particles (ALPs), with decay constants in the intermediate scale range, between $10^9$ GeV and $10^{13}$ GeV. Here, we present a general analysis of models with an axion and further ALPs and derive bounds on the relative size of the axion and ALP photon (and electron) coupling. We discuss what we can learn from measurements of the axion and ALP photon couplings about the fundamental parameters of the underlying ultraviolet completion of the theory. For the latter we consider extensions of the Standard Model in which the axion and the ALP(s) appear as pseudo Nambu-Goldstone bosons from the breaking of global chiral $U(1)$ (Peccei-Quinn (PQ)) symmetries, occuring accidentally as low energy remnants from exact discrete symmetries. In such models, the axion and the further ALP are protected from disastrous explicit symmetry breaking effects due to Planck-scale suppressed operators. The scenarios considered exploit heavy right handed neutrinos getting their mass via PQ symmetry breaking and thus explain the small mass of the active neutrinos via a seesaw relation between the electroweak and an intermediate PQ symmetry breaking scale. We show some models that can accommodate simultaneously an axion dark matter candidate, an ALP explaining the anomalous transparency of the universe for $\gamma$-rays, and an ALP explaining the recently reported 3.55 keV gamma line from galaxies and clusters of galaxies, if the respective decay constants are of intermediate scale.
000169207 536__ $$0G:(DE-HGF)POF2-514$$a514 - Theoretical Particle Physics (POF2-514)$$cPOF2-514$$fPOF II$$x0
000169207 588__ $$aDataset connected to CrossRef, bib-pubdb1.desy.de
000169207 650_7 $$2INSPIRE$$asymmetry: Peccei-Quinn
000169207 650_7 $$2INSPIRE$$amodel: axion
000169207 650_7 $$2INSPIRE$$aaxion: dark matter
000169207 650_7 $$2INSPIRE$$asymmetry breaking: scale
000169207 650_7 $$2INSPIRE$$asymmetry breaking: effect
000169207 650_7 $$2INSPIRE$$aphoton: coupling
000169207 650_7 $$2INSPIRE$$aelectron: energy: low
000169207 650_7 $$2INSPIRE$$aneutrino: right-handed
000169207 650_7 $$2INSPIRE$$aneutrino: energy: low
000169207 650_7 $$2INSPIRE$$aoperator: suppression
000169207 650_7 $$2INSPIRE$$afluctuation: tensor
000169207 650_7 $$2INSPIRE$$asymmetry: discrete
000169207 650_7 $$2INSPIRE$$agalaxy: cluster
000169207 650_7 $$2INSPIRE$$aenergy: low
000169207 650_7 $$2INSPIRE$$abeam: polarization
000169207 650_7 $$2INSPIRE$$acosmic background radiation
000169207 650_7 $$2INSPIRE$$aelectroweak interaction
000169207 650_7 $$2INSPIRE$$aaxion-like particles
000169207 650_7 $$2INSPIRE$$aGoldstone particle
000169207 650_7 $$2INSPIRE$$apower spectrum
000169207 650_7 $$2INSPIRE$$adecay constant
000169207 650_7 $$2INSPIRE$$atransparency
000169207 650_7 $$2INSPIRE$$aseesaw model
000169207 650_7 $$2INSPIRE$$aultraviolet
000169207 650_7 $$2INSPIRE$$aB-mode
000169207 650_7 $$2INSPIRE$$achiral
000169207 650_7 $$2INSPIRE$$aU(1)
000169207 65020 $$2Author$$aBeyond Standard Model 
000169207 65020 $$2Author$$aDiscrete and Finite Symmetries 
000169207 65020 $$2Author$$aGlobal Symmetries 
000169207 693__ $$0EXP:(DE-MLZ)NOSPEC-20140101$$5EXP:(DE-MLZ)NOSPEC-20140101$$eNo specific instrument$$x0
000169207 7001_ $$aMachado, A. C. B.$$b1
000169207 7001_ $$aNishi, C. C.$$b2
000169207 7001_ $$0P:(DE-H253)PIP1001650$$aRingwald, A.$$b3
000169207 7001_ $$0P:(DE-H253)PIP1015641$$aVaudrevange, P.$$b4
000169207 773__ $$0PERI:(DE-600)2027350-2$$a10.1007/JHEP06(2014)037$$gVol. 2014, no. 6, p. 37$$n6$$p37$$tJournal of high energy physics$$v2014$$x1029-8479$$y2014
000169207 7870_ $$0DESY-2014-02535$$aDias, Alex et.al.$$d2014$$iIsParent$$rDESY-14-020 ; arXiv:1403.5760$$tThe Quest for an Intermediate-Scale Accidental Axion and Further ALPs
000169207 8564_ $$uhttp://dx.doi.org/10.1007/JHEP06(2014)037
000169207 8564_ $$uhttps://bib-pubdb1.desy.de/record/169207/files/DESY-2014-02855.pdf$$yOpenAccess
000169207 8564_ $$uhttps://bib-pubdb1.desy.de/record/169207/files/DESY-2014-02855.jpg?subformat=icon-1440$$xicon-1440$$yOpenAccess
000169207 8564_ $$uhttps://bib-pubdb1.desy.de/record/169207/files/DESY-2014-02855.jpg?subformat=icon-180$$xicon-180$$yOpenAccess
000169207 8564_ $$uhttps://bib-pubdb1.desy.de/record/169207/files/DESY-2014-02855.jpg?subformat=icon-640$$xicon-640$$yOpenAccess
000169207 909CO $$ooai:bib-pubdb1.desy.de:169207$$pdnbdelivery$$pdriver$$pVDB$$popen_access$$popenaire
000169207 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1001650$$aDeutsches Elektronen-Synchrotron$$b3$$kDESY
000169207 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1015641$$aDeutsches Elektronen-Synchrotron$$b4$$kDESY
000169207 9132_ $$0G:(DE-HGF)POF3-611$$1G:(DE-HGF)POF3-610$$2G:(DE-HGF)POF3-600$$aDE-HGF$$bForschungsbereich Materie$$lMaterie und Universum$$vFundamental Particles and Forces $$x0
000169207 9131_ $$0G:(DE-HGF)POF2-514$$1G:(DE-HGF)POF2-510$$2G:(DE-HGF)POF2-500$$3G:(DE-HGF)POF2$$4G:(DE-HGF)POF$$aDE-HGF$$bStruktur der Materie$$lElementarteilchenphysik$$vTheoretical Particle Physics$$x0
000169207 9141_ $$y2014
000169207 915__ $$0StatID:(DE-HGF)0150$$2StatID$$aDBCoverage$$bWeb of Science Core Collection
000169207 915__ $$0LIC:(DE-HGF)CCBY4$$2HGFVOC$$aCreative Commons Attribution CC BY 4.0
000169207 915__ $$0StatID:(DE-HGF)0100$$2StatID$$aJCR
000169207 915__ $$0StatID:(DE-HGF)0200$$2StatID$$aDBCoverage$$bSCOPUS
000169207 915__ $$0StatID:(DE-HGF)0110$$2StatID$$aWoS$$bScience Citation Index
000169207 915__ $$0StatID:(DE-HGF)0111$$2StatID$$aWoS$$bScience Citation Index Expanded
000169207 915__ $$0StatID:(DE-HGF)0510$$2StatID$$aOpenAccess
000169207 915__ $$0StatID:(DE-HGF)0010$$2StatID$$aJCR/ISI refereed
000169207 915__ $$0StatID:(DE-HGF)1020$$2StatID$$aDBCoverage$$bCurrent Contents - Social and Behavioral Sciences
000169207 915__ $$0StatID:(DE-HGF)0420$$2StatID$$aNationallizenz
000169207 915__ $$0StatID:(DE-HGF)0199$$2StatID$$aDBCoverage$$bThomson Reuters Master Journal List
000169207 915__ $$0StatID:(DE-HGF)0570$$2StatID$$aSCOAP3
000169207 9201_ $$0I:(DE-H253)T-20120731$$kT$$lTheorie-Gruppe$$x0
000169207 9201_ $$0I:(DE-H253)ALPS-20130318$$kALPS$$lAny Light Particle Search$$x1
000169207 980__ $$ajournal
000169207 980__ $$aVDB
000169207 980__ $$aUNRESTRICTED
000169207 980__ $$aI:(DE-H253)T-20120731
000169207 980__ $$aI:(DE-H253)ALPS-20130318
000169207 9801_ $$aFullTexts