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Search for Axions with Micromegas Detectors in the CERN CAST Experiment

The CAST experiment is searching for the axion, which is a light, weakly interacting pseudoscalar particle, that is proposed to solve the so called Strong Charge-Parity Problem. The axions CAST is looking for are produced from photons in the solar core and CAST aims to convert them back into photons...

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Autor principal: YILDIZ, Suleyman Cenk
Lenguaje:eng
Publicado: 2013
Materias:
Acceso en línea:http://cds.cern.ch/record/1629526
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author YILDIZ, Suleyman Cenk
author_facet YILDIZ, Suleyman Cenk
author_sort YILDIZ, Suleyman Cenk
collection CERN
description The CAST experiment is searching for the axion, which is a light, weakly interacting pseudoscalar particle, that is proposed to solve the so called Strong Charge-Parity Problem. The axions CAST is looking for are produced from photons in the solar core and CAST aims to convert them back into photons in a superconducting LHC dipole magnet and detect the photons in the x-ray detectors attached to ends of each magnet bore. CAST uses three micromegas and a CCD detector and can track the Sun during sunset and sunrise. The two of the micromegas take tracking data during the sunset solar tracking, and were used for the first time in 2008. The analysis of the data taken in 2008 with these two detectors show no signal of axions, and new upper limits on the axion mass-coupling constant parameter space are established due to sensitivity of detectors for the axion mass range of $0.38\eV$ to $0.65\eV$.
id cern-1629526
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2013
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spelling cern-16295262019-09-30T06:29:59Zhttp://cds.cern.ch/record/1629526engYILDIZ, Suleyman CenkSearch for Axions with Micromegas Detectors in the CERN CAST ExperimentParticle Physics - ExperimentThe CAST experiment is searching for the axion, which is a light, weakly interacting pseudoscalar particle, that is proposed to solve the so called Strong Charge-Parity Problem. The axions CAST is looking for are produced from photons in the solar core and CAST aims to convert them back into photons in a superconducting LHC dipole magnet and detect the photons in the x-ray detectors attached to ends of each magnet bore. CAST uses three micromegas and a CCD detector and can track the Sun during sunset and sunrise. The two of the micromegas take tracking data during the sunset solar tracking, and were used for the first time in 2008. The analysis of the data taken in 2008 with these two detectors show no signal of axions, and new upper limits on the axion mass-coupling constant parameter space are established due to sensitivity of detectors for the axion mass range of $0.38\eV$ to $0.65\eV$.CERN-THESIS-2013-205oai:cds.cern.ch:16295262013-11-18T14:07:33Z
spellingShingle Particle Physics - Experiment
YILDIZ, Suleyman Cenk
Search for Axions with Micromegas Detectors in the CERN CAST Experiment
title Search for Axions with Micromegas Detectors in the CERN CAST Experiment
title_full Search for Axions with Micromegas Detectors in the CERN CAST Experiment
title_fullStr Search for Axions with Micromegas Detectors in the CERN CAST Experiment
title_full_unstemmed Search for Axions with Micromegas Detectors in the CERN CAST Experiment
title_short Search for Axions with Micromegas Detectors in the CERN CAST Experiment
title_sort search for axions with micromegas detectors in the cern cast experiment
topic Particle Physics - Experiment
url http://cds.cern.ch/record/1629526
work_keys_str_mv AT yildizsuleymancenk searchforaxionswithmicromegasdetectorsinthecerncastexperiment