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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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Autor principal: Ruz, J
Lenguaje:eng
Publicado: 2009
Materias:
Acceso en línea:http://cds.cern.ch/record/2283110
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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.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2009
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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