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001     395469
005     20211110145211.0
020 _ _ |a 978-3-945931-06-6
020 _ _ |a 978-3-945931-06-6
024 7 _ |a 10.3204/DESY-PROC-2009-03/Branca_Antonio
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024 7 _ |a 1435-8077
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037 _ _ |a PUBDB-2017-12134
041 _ _ |a English
088 1 _ |a DESY-PROC-2016-03
088 _ _ |a DESY-PROC-2016-03
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100 1 _ |a Branca, Antonio
|0 P:(DE-HGF)0
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111 2 _ |a 12th Patras Workshop on Axions, WIMPs and WISPs
|c Jeju Island
|d 2016-06-20 - 2016-06-24
|g AXION-WIMP 2016
|0 C16-06-20.4
|2 inspire
|w South Korea
245 _ _ |a Light Dark Matter Search with AURIGA
260 _ _ |a Hamburg
|c 2017
|b Verlag Deutsches Elektronen-Synchrotron
295 1 0 |a Branca, 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
300 _ _ |a 9-13
336 7 _ |a CONFERENCE_PAPER
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490 0 _ |a DESY-PROC
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520 _ _ |a We 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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693 _ _ |0 EXP:(DE-MLZ)NOSPEC-20140101
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700 1 _ |a AURIGA Collaboration
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787 0 _ |a Kim, Younglm et. al.
|d Verlag Deutsches Elektronen-Synchrotron
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|0 PUBDB-2017-11637
|r DESY-PROC-2016-03
|t 12th "Patras" Workshop on Axions, WIMPs and WISPs, PATRAS 2016
856 4 _ |u https://bib-pubdb1.desy.de/record/395469/files/fulltext.pdf
|y OpenAccess
909 C O |o oai:bib-pubdb1.desy.de:395469
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910 1 _ |a INFN - Sezione di Padova - Via Marzolo 8 - I-35131 Padova - Italy
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914 1 _ |y 2017
915 _ _ |a OpenAccess
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915 _ _ |a Creative Commons Attribution CC BY 4.0
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