Report/Contribution to a conference proceedings/Contribution to a book PUBDB-2017-12134

http://join2-wiki.gsi.de/foswiki/pub/Main/Artwork/join2_logo100x88.png
Light Dark Matter Search with AURIGA

 ;

2017
Verlag Deutsches Elektronen-Synchrotron Hamburg
ISBN: 978-3-945931-06-6, 978-3-945931-06-6

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
12th Patras Workshop on Axions, WIMPs and WISPs, AXION-WIMP 2016, Jeju IslandJeju Island, South Korea, 20 Jun 2016 - 24 Jun 20162016-06-202016-06-24
Hamburg : Verlag Deutsches Elektronen-Synchrotron, DESY-PROC 9-13 () [10.3204/DESY-PROC-2009-03/Branca_Antonio]  GO

This record in other databases:

Please use a persistent id in citations: doi:

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 $m_{\Phi}=3.6\cdot10^{-12}\,\mathrm{eV}$.


Contributing Institute(s):
  1. Bibliothek und Dokumentation (L)
Research Program(s):
  1. 899 - ohne Topic (POF3-899) (POF3-899)
Experiment(s):
  1. No specific instrument

Appears in the scientific report 2017
Database coverage:
Creative Commons Attribution CC BY 4.0 ; OpenAccess
Click to display QR Code for this record

The record appears in these collections:
Private Collections > >DESY > >FH > L
Document types > Events > Contributions to a conference proceedings
Document types > Books > Contribution to a book
Document types > Reports > Reports
Public records
Publications database
OpenAccess


Linked articles:

http://join2-wiki.gsi.de/foswiki/pub/Main/Artwork/join2_logo100x88.png 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 20162016-06-202016-06-24 Hamburg : Verlag Deutsches Elektronen-Synchrotron, DESY-PROC () [10.3204/PUBDB-2017-11637]  GO OpenAccess  Download fulltext Files BibTeX | EndNote: XML, Text | RIS


 Record created 2017-11-20, last modified 2021-11-10


OpenAccess:
Download fulltext PDF
Rate this document:

Rate this document:
1
2
3
 
(Not yet reviewed)