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000395469 020__ $$a978-3-945931-06-6
000395469 0247_ $$2datacite_doi$$a10.3204/DESY-PROC-2009-03/Branca_Antonio
000395469 0247_ $$2ISSN$$a1435-8077
000395469 037__ $$aPUBDB-2017-12134
000395469 041__ $$aEnglish
000395469 0881_ $$aDESY-PROC-2016-03
000395469 088__ $$2DESY$$aDESY-PROC-2016-03
000395469 1001_ $$0P:(DE-HGF)0$$aBranca, Antonio$$b0
000395469 1112_ $$0C16-06-20.4$$2inspire$$a12th Patras Workshop on Axions, WIMPs and WISPs$$cJeju Island$$d2016-06-20 - 2016-06-24$$gAXION-WIMP 2016$$wSouth Korea
000395469 245__ $$aLight Dark Matter Search with AURIGA
000395469 260__ $$aHamburg$$bVerlag Deutsches Elektronen-Synchrotron$$c2017
000395469 29510 $$aBranca, Antonio "Light Dark Matter Search with AURIGA" in 12th "Patras" Workshop on Axions, WIMPs and WISPs, PATRAS 2016 / Kim, Younglm, Lindner, Axel, Semertzidis, Yannis K. (eds.), Verlag Deutsches Elektronen-Synchrotron : 2017 ; PATRAS 2016 : 12th "Patras" Workshop on Axions, WIMPs and WISPs, 2016-06-20 - 2016-06-24, Jeju Island
000395469 300__ $$a9-13
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000395469 520__ $$aWe present a search for a new scalar particle, called moduli, performed using the cryogenic resonant-mass gravitational wave detector AURIGA. This particle may give a significant contribution to the Dark Matter (DM) in our Universe. DM clusters under the galaxies gravitational effect, forming the so called galactic halo. The interaction of ordinary matter with a DM halo composed by moduli causes the oscillation of solids with a frequency equal to the mass of the DM particle. In particular, the putative signal would appear as a narrow peak ($\triangle f\sim1\,\mathrm{mHz}$) in the sensitive band of AURIGA, some $100\,\mathrm{Hz}$ at about $1\,\mathrm{kHz}$. We used high quality data, selected out of an acquisition of years of continuous running. The search sets upper limits at $95\%\,C.L.$ on the moduli coupling to matter $d_{i}\lesssim10^{-5}$ around moduli masses $m_{\Phi}=3.6\cdot10^{-12}\,\mathrm{eV}$.
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000395469 7001_ $$0P:(DE-HGF)0$$aAURIGA Collaboration$$b1$$eCollaboration author
000395469 7870_ $$0PUBDB-2017-11637$$aKim, Younglm et. al.$$dVerlag Deutsches Elektronen-Synchrotron$$iisPartOf$$rDESY-PROC-2016-03$$t12th "Patras" Workshop on Axions, WIMPs and WISPs, PATRAS 2016
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