XENON100 Results on WIMP and non-WIMP Searches

Priel, Nadav; XENON Collaboration

Contribution to a conference proceedings/Contribution to a book

PUBDB-2016-05906

XENON100 Results on WIMP and non-WIMP Searches

Priel, N. ; XENON Collaboration (Collaboration author)

2014
Verlag Deutsches Elektronen-Synchrotron Hamburg
ISBN: 978-3-935702-59-1

Priel, Nadav "XENON100 Results on WIMP and non-WIMP Searches" 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
10th Patras Workshop on Axions, WIMPs and WISPs, AXION-WIMP 2014, Geneva, Switzerland, 29 Jun 2014 - 4 Jul 2014 Hamburg : Verlag Deutsches Elektronen-Synchrotron, DESY-PROC 37-40 (2014) [10.3204/DESY-PROC-2014-03/priel_nadav]

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Please use a persistent id in citations: doi:10.3204/DESY-PROC-2014-03/priel_nadav

Abstract: XENON100 is the second phase of the XENON direct Dark Matter search program. It consists of an ultra-low background double phase (liquid-gas) xenon filled time projection chamber, and is installed at the Laboratori Nazionali del Gran Sasso. The results from the 224.6 live days of data taken between March 2011 and April 2012 are reported. The experiment sets one of the most stringent limits on the WIMP-nucleon spin-independent cross section, and the most stringent limit on the spin-dependent WIMP-neutron interaction. With the same dataset, XENON100 sets the best limit to date on the axion coupling to electrons for solar and for galactic axions.

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