000154830 001__ 154830
000154830 005__ 20211110122639.0
000154830 0247_ $$2arXiv$$aarXiv:1310.1774
000154830 0247_ $$2altmetric$$aaltmetric:1809598
000154830 0247_ $$2inspire$$ainspire:1257348
000154830 037__ $$aDESY-2013-01123
000154830 0881_ $$aDESY-13-181; arXiv:1310.1774; TU-948; ICRR-661-2013-10; IPMU13-0197
000154830 088__ $$2DESY$$aDESY-13-181
000154830 088__ $$2arXiv$$aarXiv:1310.1774
000154830 088__ $$2Other$$aTU-948
000154830 088__ $$2Other$$aICRR-661-2013-10
000154830 088__ $$2Other$$aIPMU13-0197
000154830 1001_ $$0P:(DE-H253)PIP1020876$$aJeong, Kwangsik$$b0
000154830 245__ $$aAxions as Hot and Cold Dark Matter
000154830 260__ $$c2013
000154830 3367_ $$2DRIVER$$apreprint
000154830 3367_ $$028$$2EndNote$$aElectronic Article
000154830 3367_ $$0PUB:(DE-HGF)25$$2PUB:(DE-HGF)$$aPreprint$$bpreprint$$mpreprint$$s154830
000154830 3367_ $$2BibTeX$$aARTICLE
000154830 3367_ $$0PUB:(DE-HGF)15$$2PUB:(DE-HGF)$$aInternal Report$$mintrep
000154830 520__ $$aThe presence of a hot dark matter component has been hinted at 3 sigma by a combination of the results from different cosmological observations. We examine a possibility that pseudo Nambu-Goldstone bosons account for both hot and cold dark matter components. We show that the QCD axions can do the job for the axion decay constant f_a < O(10^10) GeV, if they are produced by the saxion decay and the domain wall annihilation. We also investigate the cases of thermal QCD axions, pseudo Nambu-Goldstone bosons coupled to the standard model sector through the Higgs portal, and axions produced by modulus decay.
000154830 536__ $$0G:(DE-HGF)POF2-514$$a514 - Theoretical Particle Physics (POF2-514)$$cPOF2-514$$fPOF II$$x0
000154830 693__ $$0EXP:(DE-MLZ)NOSPEC-20140101$$5EXP:(DE-MLZ)NOSPEC-20140101$$eNo specific instrument$$x0
000154830 7001_ $$0P:(DE-HGF)0$$aKawasaki, Masahiro$$b1
000154830 7001_ $$0P:(DE-HGF)0$$aTakahashi, Fuminobu$$b2
000154830 8564_ $$uhttps://arxiv.org/abs/1310.1774
000154830 8564_ $$uhttps://bib-pubdb1.desy.de/record/154830/files/DESY-2013-01123.pdf$$yRestricted
000154830 8564_ $$uhttps://bib-pubdb1.desy.de/record/154830/files/DESY-2013-01123.jpg?subformat=icon-1440$$xicon-1440$$yRestricted
000154830 8564_ $$uhttps://bib-pubdb1.desy.de/record/154830/files/DESY-2013-01123.jpg?subformat=icon-180$$xicon-180$$yRestricted
000154830 8564_ $$uhttps://bib-pubdb1.desy.de/record/154830/files/DESY-2013-01123.jpg?subformat=icon-640$$xicon-640$$yRestricted
000154830 909CO $$ooai:bib-pubdb1.desy.de:154830$$pVDB
000154830 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-HGF)0$$aDeutsches Elektronen-Synchrotron$$b0$$kDESY
000154830 9131_ $$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$$x0
000154830 9141_ $$y2013
000154830 915__ $$0StatID:(DE-HGF)0580$$2StatID$$aPublished
000154830 9201_ $$0I:(DE-H253)T-20120731$$kT$$lTheorie-Gruppe$$x0
000154830 980__ $$apreprint
000154830 980__ $$aVDB
000154830 980__ $$aUNRESTRICTED
000154830 980__ $$aintrep
000154830 980__ $$aI:(DE-H253)T-20120731