000297011 001__ 297011 000297011 005__ 20211110133939.0 000297011 0247_ $$2datacite_doi$$a10.3204/DESY-PROC-2008-02/raffelt_georg 000297011 0247_ $$2arXiv$$aarXiv:0808.0814 000297011 0247_ $$2WOS$$aWOS:00 000297011 0247_ $$2inspire$$ainspire:792521 000297011 037__ $$aPUBDB-2016-01764 000297011 041__ $$aen 000297011 0881_ $$aarXiv:0808.0814; MPP-2008-99 000297011 088__ $$2arXiv$$aarXiv:0808.0814 000297011 088__ $$2MPG$$aMPP-2008-99 000297011 1001_ $$0P:(DE-HGF)0$$aRaffelt, G.$$b0 000297011 1112_ $$a4th Patras Workshop on Axions, WIMPs and WISPs$$cHamburg$$d2008-06-18 - 2008-06-21$$gAXION-WIMP 2008$$wGermany 000297011 245__ $$aAxion hot dark matter bounds 000297011 260__ $$aHamburg$$bDeutsches Elektronen-Synchrotron, DESY$$c2009 000297011 300__ $$a27-30 000297011 3367_ $$033$$2EndNote$$aConference Paper 000297011 3367_ $$2DRIVER$$aconferenceObject 000297011 3367_ $$0PUB:(DE-HGF)8$$2PUB:(DE-HGF)$$aContribution to a conference proceedings$$bcontrib$$mcontrib$$s1461653565_23562 000297011 3367_ $$0PUB:(DE-HGF)15$$2PUB:(DE-HGF)$$aInternal Report$$mintrep 000297011 3367_ $$2BibTeX$$aINPROCEEDINGS 000297011 520__ $$aWe derive cosmological limits on two-component hot dark matter consisting of neutrinos and axions. We restrict the large-scale structure data to the safely linear regime, excluding the Lyman-alpha forest. We derive Bayesian credible regions in the two-parameter space consisting of m_a and sum(m_nu). Marginalizing over sum(m_nu) provides m_a<1.02 eV (95% CL). In the absence of axions the same data and methods give sum(m_nu)< 0.63 eV (95% CL). 000297011 536__ $$0G:(DE-HGF)POF3-899$$a899 - ohne Topic (POF3-899)$$cPOF3-899$$fPOF III$$x0 000297011 588__ $$aDataset connected to DataCite, INSPIRE 000297011 693__ $$0EXP:(DE-H253)HERA(machine)-20150101$$1EXP:(DE-588)4159571-3$$5EXP:(DE-H253)HERA(machine)-20150101$$aHERA$$eFacility (machine) HERA$$x0 000297011 7001_ $$0P:(DE-HGF)0$$aHannestad, S.$$b1 000297011 7001_ $$0P:(DE-HGF)0$$aMirizzi, A.$$b2 000297011 7001_ $$0P:(DE-HGF)0$$aWong, Y. Y. Y.$$b3 000297011 773__ $$a10.3204/DESY-PROC-2008-02/raffelt_georg 000297011 7870_ $$0PUBDB-2016-01759$$aLindner, Axel et.al.$$dVerlag Deutsches Elektronen-Synchrotron, 2008$$iIsPartOf$$rDESY-PROC-2008-02$$tProceedings, 4th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2008) 000297011 8564_ $$uhttps://bib-pubdb1.desy.de/record/297011/files/raffelt_georg.pdf$$yOpenAccess 000297011 8564_ $$uhttps://bib-pubdb1.desy.de/record/297011/files/raffelt_georg.gif?subformat=icon$$xicon$$yOpenAccess 000297011 8564_ $$uhttps://bib-pubdb1.desy.de/record/297011/files/raffelt_georg.jpg?subformat=icon-1440$$xicon-1440$$yOpenAccess 000297011 8564_ $$uhttps://bib-pubdb1.desy.de/record/297011/files/raffelt_georg.jpg?subformat=icon-180$$xicon-180$$yOpenAccess 000297011 8564_ $$uhttps://bib-pubdb1.desy.de/record/297011/files/raffelt_georg.jpg?subformat=icon-640$$xicon-640$$yOpenAccess 000297011 8564_ $$uhttps://bib-pubdb1.desy.de/record/297011/files/raffelt_georg.pdf?subformat=pdfa$$xpdfa$$yOpenAccess 000297011 909CO $$ooai:bib-pubdb1.desy.de:297011$$pdnbdelivery$$pdriver$$popen_access$$popenaire$$pVDB 000297011 9131_ $$0G:(DE-HGF)POF3-899$$1G:(DE-HGF)POF3-890$$2G:(DE-HGF)POF3-800$$3G:(DE-HGF)POF3$$4G:(DE-HGF)POF$$aDE-HGF$$bProgrammungebundene Forschung$$lohne Programm$$vohne Topic$$x0 000297011 915__ $$0StatID:(DE-HGF)0510$$2StatID$$aOpenAccess 000297011 9201_ $$0I:(DE-H253)L-20120731$$kL$$lBibliothek und Dokumentation$$x0 000297011 980__ $$acontrib 000297011 980__ $$aVDB 000297011 980__ $$aUNRESTRICTED 000297011 980__ $$aintrep 000297011 980__ $$aI:(DE-H253)L-20120731 000297011 9801_ $$aUNRESTRICTED 000297011 9801_ $$aFullTexts