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Latest results of cast and future prospects

CERN Axion Solar Telescope (CAST) is currently the most sensitive axion helioscope designed to search for axions and axion-like particles produced in the Sun. CAST completed successfully the second part of CAST phase II where the magnet bores were lled with 3He gas at variable pressure scanning axio...

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Autor principal: Vafeiadis, Theodoros
Lenguaje:eng
Publicado: 2014
Materias:
Acceso en línea:http://cds.cern.ch/record/2025911
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author Vafeiadis, Theodoros
author_facet Vafeiadis, Theodoros
author_sort Vafeiadis, Theodoros
collection CERN
description CERN Axion Solar Telescope (CAST) is currently the most sensitive axion helioscope designed to search for axions and axion-like particles produced in the Sun. CAST completed successfully the second part of CAST phase II where the magnet bores were lled with 3He gas at variable pressure scanning axion masses up to 1.2 eV In the absence of signal it has set the best experimental limit on the axion-photon coupling constant over a broad range of axion masses. In 2013 CAST has improved its sensitivity to solar axions with rest mass below 0.02 eV by upgrading the Micromegas detectors and it will continue in 2014 with the implementation of a second X-ray optic and a new type detector (InGRID). In addition, CAST has extended its sensitivity into the sub-keV energy range using a silicon detector (SDD), to search for solar chameleons. Thus, CAST also became sensitive to dark energy particles. A new generation axion helioscope (IAXO) aims to improve the current axion-photon coupling by 1-1.5 orders of magnitude. This will be possible by building a dedicated magnet and dedicated optics and X-ray detectors
id oai-inspirehep.net-1338147
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2014
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spelling oai-inspirehep.net-13381472019-09-30T06:29:59Zhttp://cds.cern.ch/record/2025911engVafeiadis, TheodorosLatest results of cast and future prospectsAstrophysics and AstronomyCERN Axion Solar Telescope (CAST) is currently the most sensitive axion helioscope designed to search for axions and axion-like particles produced in the Sun. CAST completed successfully the second part of CAST phase II where the magnet bores were lled with 3He gas at variable pressure scanning axion masses up to 1.2 eV In the absence of signal it has set the best experimental limit on the axion-photon coupling constant over a broad range of axion masses. In 2013 CAST has improved its sensitivity to solar axions with rest mass below 0.02 eV by upgrading the Micromegas detectors and it will continue in 2014 with the implementation of a second X-ray optic and a new type detector (InGRID). In addition, CAST has extended its sensitivity into the sub-keV energy range using a silicon detector (SDD), to search for solar chameleons. Thus, CAST also became sensitive to dark energy particles. A new generation axion helioscope (IAXO) aims to improve the current axion-photon coupling by 1-1.5 orders of magnitude. This will be possible by building a dedicated magnet and dedicated optics and X-ray detectorsoai:inspirehep.net:13381472014
spellingShingle Astrophysics and Astronomy
Vafeiadis, Theodoros
Latest results of cast and future prospects
title Latest results of cast and future prospects
title_full Latest results of cast and future prospects
title_fullStr Latest results of cast and future prospects
title_full_unstemmed Latest results of cast and future prospects
title_short Latest results of cast and future prospects
title_sort latest results of cast and future prospects
topic Astrophysics and Astronomy
url http://cds.cern.ch/record/2025911
work_keys_str_mv AT vafeiadistheodoros latestresultsofcastandfutureprospects