Cargando…

Search for solar axions with the Time Projection Chamber of the CERN Axion Solar Telescope with 4-Helium as buffer gas

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...

Descripción completa

Detalles Bibliográficos
Autor principal: Ruz, J
Lenguaje:eng
Publicado: 2009
Materias:
Acceso en línea:http://cds.cern.ch/record/1164157
_version_ 1780915975272529920
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 and, therefore, different X-ray detectors are mounted on both ends of the magnet waiting for a photon from axion-to-photon conversion due to the Primakoff effect. During its First Phase, which concluded in 2004, the TPC detector of CAST looked for axions with masses up to 0.02 eV. By using a Helium-4 buffer gas, CAST's TPC detector has been able to re-establish the coherence needed to scan for axions with masses up to 0.39 eV, technique that allows CAST to look into the theoretical regions for axions.
id cern-1164157
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2009
record_format invenio
spelling cern-11641572019-09-30T06:29:59Zhttp://cds.cern.ch/record/1164157engRuz, JSearch for solar axions with the Time Projection Chamber of the CERN Axion Solar Telescope with 4-Helium as buffer gasAstrophysics 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 and, therefore, different X-ray detectors are mounted on both ends of the magnet waiting for a photon from axion-to-photon conversion due to the Primakoff effect. During its First Phase, which concluded in 2004, the TPC detector of CAST looked for axions with masses up to 0.02 eV. By using a Helium-4 buffer gas, CAST's TPC detector has been able to re-establish the coherence needed to scan for axions with masses up to 0.39 eV, technique that allows CAST to look into the theoretical regions for axions.CERN-THESIS-2009-010oai:cds.cern.ch:11641572009-02-27T12:03:32Z
spellingShingle Astrophysics and Astronomy
Ruz, J
Search for solar axions with the Time Projection Chamber of the CERN Axion Solar Telescope with 4-Helium as buffer gas
title Search for solar axions with the Time Projection Chamber of the CERN Axion Solar Telescope with 4-Helium as buffer gas
title_full Search for solar axions with the Time Projection Chamber of the CERN Axion Solar Telescope with 4-Helium as buffer gas
title_fullStr Search for solar axions with the Time Projection Chamber of the CERN Axion Solar Telescope with 4-Helium as buffer gas
title_full_unstemmed Search for solar axions with the Time Projection Chamber of the CERN Axion Solar Telescope with 4-Helium as buffer gas
title_short Search for solar axions with the Time Projection Chamber of the CERN Axion Solar Telescope with 4-Helium as buffer gas
title_sort search for solar axions with the time projection chamber of the cern axion solar telescope with 4-helium as buffer gas
topic Astrophysics and Astronomy
url http://cds.cern.ch/record/1164157
work_keys_str_mv AT ruzj searchforsolaraxionswiththetimeprojectionchamberofthecernaxionsolartelescopewith4heliumasbuffergas