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Report/Contribution to a conference proceedings/Contribution to a book | PUBDB-2017-12134 |
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2017
Verlag Deutsches Elektronen-Synchrotron
Hamburg
ISBN: 978-3-945931-06-6, 978-3-945931-06-6
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Please use a persistent id in citations: doi:10.3204/DESY-PROC-2009-03/Branca_Antonio
Report No.: DESY-PROC-2016-03
Abstract: 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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Book/Proceedings/Report
12th "Patras" Workshop on Axions, WIMPs and WISPs, PATRAS 2016
12th "Patras" Workshop on Axions, WIMPs and WISPs, PATRAS 2016, Jeju IslandJeju Island, South Korea, 20 Jun 2016 - 24 Jun 2016
Hamburg : Verlag Deutsches Elektronen-Synchrotron, DESY-PROC (2017) [10.3204/PUBDB-2017-11637]
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