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Newtorites in bar detectors of gravitational wave
The detection of particles with only gravitational interactions (Newtorites) in gravitational bar detectors was studied in 1984 by Bernard, De Rujula and Lautrup. The negative results of dark matter searches suggest to look to exotic possibilities like Newtorites. The limits obtained with the Nautil...
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Lenguaje: | eng |
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2015
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Acceso en línea: | https://dx.doi.org/10.1088/1742-6596/718/7/072006 http://cds.cern.ch/record/2103007 |
_version_ | 1780948753114464256 |
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author | Ronga, F |
author_facet | Ronga, F |
author_sort | Ronga, F |
collection | CERN |
description | The detection of particles with only gravitational interactions (Newtorites) in gravitational bar detectors was studied in 1984 by Bernard, De Rujula and Lautrup. The negative results of dark matter searches suggest to look to exotic possibilities like Newtorites. The limits obtained with the Nautilus bar detector will be presented and the possible improvements will be discussed. Since the gravitational coupling is very weak, the possible limits are very far from what is needed for dark matter, but for large masses are the best limits obtained on the Earth. An update of limits for MACRO particles will be given. |
id | cern-2103007 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2015 |
record_format | invenio |
spelling | cern-21030072022-08-17T13:31:43Zdoi:10.1088/1742-6596/718/7/072006http://cds.cern.ch/record/2103007engRonga, FNewtorites in bar detectors of gravitational waveDetectors and Experimental TechniquesThe detection of particles with only gravitational interactions (Newtorites) in gravitational bar detectors was studied in 1984 by Bernard, De Rujula and Lautrup. The negative results of dark matter searches suggest to look to exotic possibilities like Newtorites. The limits obtained with the Nautilus bar detector will be presented and the possible improvements will be discussed. Since the gravitational coupling is very weak, the possible limits are very far from what is needed for dark matter, but for large masses are the best limits obtained on the Earth. An update of limits for MACRO particles will be given.arXiv:1511.04882oai:cds.cern.ch:21030072015-11-16 |
spellingShingle | Detectors and Experimental Techniques Ronga, F Newtorites in bar detectors of gravitational wave |
title | Newtorites in bar detectors of gravitational wave |
title_full | Newtorites in bar detectors of gravitational wave |
title_fullStr | Newtorites in bar detectors of gravitational wave |
title_full_unstemmed | Newtorites in bar detectors of gravitational wave |
title_short | Newtorites in bar detectors of gravitational wave |
title_sort | newtorites in bar detectors of gravitational wave |
topic | Detectors and Experimental Techniques |
url | https://dx.doi.org/10.1088/1742-6596/718/7/072006 http://cds.cern.ch/record/2103007 |
work_keys_str_mv | AT rongaf newtoritesinbardetectorsofgravitationalwave |