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Probing eV-scale axions with CAST
CAST (CERN Axion Solar Telescope) is a helioscope looking for axions coming from the solar core to the Earth. The experiment, located at CERN, is based on the Primakoff effect and uses a magnetic field of 9 Tesla provided by a decommissioned LHC magnet. CAST is able to follow the Sun during sunrise...
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Lenguaje: | eng |
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2009
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Acceso en línea: | http://cds.cern.ch/record/2283110 |
_version_ | 1780955691916197888 |
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author | Ruz, J |
author_facet | Ruz, J |
author_sort | Ruz, J |
collection | CERN |
description | CAST (CERN Axion Solar Telescope) is a helioscope looking for axions coming from the solar core to the Earth. The experiment, located at CERN, is based on the Primakoff effect and uses a magnetic field of 9 Tesla provided by a decommissioned LHC magnet. CAST is able to follow the Sun during sunrise and sunset having four X-ray detectors mounted on both ends of the magnet to look for photons from axion-to-photon conversions. During its First Phase, which concluded in 2004, CAST searched for axions with masses up to 0.02 eV. By using a buffer gas the coherence needed to scan for axions with masses up to 1.20 eV is re-established in CAST’s Second Phase. This technique enables the experiment to study the theoretical regions for axions. During the years 2005 and 2006, the use of 4He has already enabled the search for axions with masses up to 0.39 eV. Up to present time, CAST has upgraded its experimental setup to operate with 3He in the magnetic field. |
id | oai-inspirehep.net-1385535 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2009 |
record_format | invenio |
spelling | oai-inspirehep.net-13855352019-09-30T06:29:59Zhttp://cds.cern.ch/record/2283110engRuz, JProbing eV-scale axions with CASTAstrophysics and AstronomyCAST (CERN Axion Solar Telescope) is a helioscope looking for axions coming from the solar core to the Earth. The experiment, located at CERN, is based on the Primakoff effect and uses a magnetic field of 9 Tesla provided by a decommissioned LHC magnet. CAST is able to follow the Sun during sunrise and sunset having four X-ray detectors mounted on both ends of the magnet to look for photons from axion-to-photon conversions. During its First Phase, which concluded in 2004, CAST searched for axions with masses up to 0.02 eV. By using a buffer gas the coherence needed to scan for axions with masses up to 1.20 eV is re-established in CAST’s Second Phase. This technique enables the experiment to study the theoretical regions for axions. During the years 2005 and 2006, the use of 4He has already enabled the search for axions with masses up to 0.39 eV. Up to present time, CAST has upgraded its experimental setup to operate with 3He in the magnetic field.oai:inspirehep.net:13855352009 |
spellingShingle | Astrophysics and Astronomy Ruz, J Probing eV-scale axions with CAST |
title | Probing eV-scale axions with CAST |
title_full | Probing eV-scale axions with CAST |
title_fullStr | Probing eV-scale axions with CAST |
title_full_unstemmed | Probing eV-scale axions with CAST |
title_short | Probing eV-scale axions with CAST |
title_sort | probing ev-scale axions with cast |
topic | Astrophysics and Astronomy |
url | http://cds.cern.ch/record/2283110 |
work_keys_str_mv | AT ruzj probingevscaleaxionswithcast |