000315497 001__ 315497
000315497 005__ 20211110140133.0
000315497 020__ $$a978-3-935702-59-1
000315497 0247_ $$2datacite_doi$$a10.3204/DESY-PROC-2014-03/kozlov_valentin
000315497 0247_ $$2ISSN$$a1435-8077
000315497 037__ $$aPUBDB-2016-05904
000315497 041__ $$aEnglish
000315497 1001_ $$0P:(DE-HGF)0$$aKozlov, Valentin$$b0$$eCorresponding author
000315497 1112_ $$0C14-06-29.1$$2inspire$$a10th Patras Workshop on Axions, WIMPs and WISPs$$cGeneva$$d2014-06-29 - 2014-07-04$$gAXION-WIMP 2014$$wSwitzerland
000315497 245__ $$aDirect Dark matter search with the Edelweiss experiment
000315497 260__ $$aHamburg$$bVerlag Deutsches Elektronen-Synchrotron$$c2014
000315497 29510 $$aKozlov, Valentin "Direct Dark matter search with the Edelweiss experiment" in Proceedings, 10th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2014)  / Tsesmelis, Emmanuel, Maroudas, Marios (eds.), Verlag Deutsches Elektronen-Synchrotron : 2014 ; AXION-WIMP 2014 : 10th Patras Workshop on Axions, WIMPs and WISPs, 2014-06-29 - 2014-07-04, Geneva
000315497 300__ $$a29-32
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000315497 4900_ $$0PERI:(DE-600)2450075-6$$aDESY-PROC
000315497 520__ $$aThe EDELWEISS experiment searches for Dark Matter particles by means of Ge-bolometers with a powerful rejection of background. The setup is installed in the Modane underground laboratory (LSM, France) in French-Italian Alps. The second phase of the experiment was completed in 2011, and results are published setting new limits on the spin-independent WIMP-nucleon scattering cross-section. The same data set was also analyzed to search for axion-induced electron recoils down to 2.5~keV. We set new limits on ALP parameters for different scenarios, some of which provide one of the best bounds for direct axion searches. Recently the setup was upgraded towards significantly higher sensitivity and 36 new Ge-detectors of 800~g each were installed. The detector background rejection capabilities and performances, and improvements of the background will be presented. The status and scientific goals of the current \EDW\ program will be described as well as further plans for a next generation experiment, EURECA.
000315497 7001_ $$0P:(DE-HGF)0$$aEDELWEISS Collaboration$$b1$$eCollaboration author
000315497 7870_ $$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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