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001     408357
005     20211110151245.0
010 _ _ |a
020 _ _ |a 978-3-935702-83-6
024 7 _ |a 10.3204/DESY-PROC-2013-04/marrodan_undagoitia_teresa
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024 7 _ |a 1435-8077
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037 _ _ |a PUBDB-2018-02810
041 _ _ |a English
088 1 _ |a DESY-PROC-2013-04
088 _ _ |a DESY-PROC-2013-04
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100 1 _ |a Marrodán Undagoitia, T.
|0 P:(DE-HGF)0
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111 2 _ |a 9th Patras Workshop on Axions, WIMPs and WISPs
|c Mainz
|d 2013-06-24 - 2013-06-28
|g AXION-WIMP 2013
|0 C13-06-24.5
|2 inspire
|w Germany
245 _ _ |a Direct Dark Matter Search with XENON
260 _ _ |a Hamburg
|c 2013
|b Verlag Deutsches Elektronen-Synchrotron
295 1 0 |a Undagoitia, T.Marrodán "Direct Dark Matter Search with XENON" in Proceedings, 9th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2013) / Oberlack, Uwe, Sissol, Pierre (eds.), 2013 ; AXION-WIMP 2013 : 9th Patras Workshop on Axions, WIMPs and WISPs , 2013-06-23 - 2013-06-28, Mainz
300 _ _ |a 189-194
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490 0 _ |a DESY-PROC
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500 _ _ |a Literaturangaben; English
520 _ _ |a Direct dark matter searches using liquid xenon have shown a great potential to detect WIMPs (Weakly Interacting Massive Particles) via elastic scattering off the target nuclei. XENON100 operates with an active volume of 62 kg liquid xenon and it is located at the Gran Sasso underground laboratory in Italy. So far the data released provides no evidence for dark matter. The resulting exclusion limits on the WIMP-nucleon cross section for spin-dependent and-independent interactions probe already significant regions of the cross section and WIMP mass parameter space. The XENON1T experiment currently under construction will improve the current sensitivity by two orders of magnitude.
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650 _ 7 |a Hypothetisches Teilchen
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693 _ _ |0 EXP:(DE-MLZ)NOSPEC-20140101
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700 1 _ |a XENON Collaboration
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787 0 _ |a Oberlack, Uwe et. al.
|0 PUBDB-2015-05816
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|t Proceedings, 9th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2013)
856 4 _ |u https://bib-pubdb1.desy.de/record/408357/files/fulltext.pdf
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