000315491 001__ 315491
000315491 005__ 20211110140132.0
000315491 020__ $$a978-3-935702-59-1
000315491 0247_ $$2datacite_doi$$a10.3204/DESY-PROC-2014-03/balazs_csaba
000315491 0247_ $$2ISSN$$a1435-8077
000315491 037__ $$aPUBDB-2016-05898
000315491 041__ $$aEnglish
000315491 1001_ $$0P:(DE-HGF)0$$aBalázs, Csaba$$b0
000315491 1112_ $$0C14-06-29.1$$2inspire$$a10th Patras Workshop on Axions, WIMPs and WISPs$$cGeneva$$d2014-06-29 - 2014-07-04$$gAXION-WIMP 2014$$wSwitzerland
000315491 245__ $$aObservations are confirming the WIMP paradigm
000315491 260__ $$aHamburg$$bVerlag Deutsches Elektronen-Synchrotron$$c2014
000315491 29510 $$aBalázs, Csaba "Observations are confirming the WIMP paradigm" in Proceedings, 10th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2014)  / Tsesmelis, Emmanuel, Maroudas, Marios (eds.), Verlag Deutsches Elektronen-Synchrotron : 2014 ; AXION-WIMP 2014 : 10th Patras Workshop on Axions, WIMPs and WISPs, 2014-06-29 - 2014-07-04, Geneva
000315491 300__ $$a3-6
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000315491 4900_ $$0PERI:(DE-600)2450075-6$$aDESY-PROC
000315491 520__ $$aWe present a model independent analysis of thermal dark matter constraining its mass and interaction strengths with data from astro- and particle physics experiments. We show that the observationally favored dark matter particle mass region is 1-1000 GeV with effective interactions that have a cut-off in the range of 1-10 TeV.
000315491 7001_ $$0P:(DE-HGF)0$$aLi, Tong$$b1
000315491 7001_ $$0P:(DE-HGF)0$$aNewstead, Jayden L.$$b2
000315491 7870_ $$0PUBDB-2016-05897$$aTsesmelis, Emmanuel et. al.$$dVerlag Deutsches Elektronen-Synchrotron$$iisPartOf$$rDESY-PROC-2014-03$$tProceedings, 10th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2014) : Geneva, Switzerland, June 29-July 4, 2014
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000315491 9101_ $$0I:(DE-HGF)0$$6P:(DE-HGF)0$$a Monash U.$$b0
000315491 9101_ $$0I:(DE-HGF)0$$6P:(DE-HGF)0$$a Monash U.$$b1
000315491 9101_ $$0I:(DE-HGF)0$$6P:(DE-HGF)0$$a  	 Arizona State U.$$b2
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