dc.contributor.author |
Lakic, B |
en |
dc.contributor.author |
Arik, M |
en |
dc.contributor.author |
Aune, S |
en |
dc.contributor.author |
Barth, K |
en |
dc.contributor.author |
Belov, A |
en |
dc.contributor.author |
Borghi, S |
en |
dc.contributor.author |
Brauninger, H |
en |
dc.contributor.author |
Cantatore, G |
en |
dc.contributor.author |
Carmona, JM |
en |
dc.contributor.author |
Cetin, SA |
en |
dc.contributor.author |
Collar, JI |
en |
dc.contributor.author |
Dafni, T |
en |
dc.contributor.author |
Davenport, M |
en |
dc.contributor.author |
Eleftheriadis, C |
en |
dc.contributor.author |
Elias, N |
en |
dc.contributor.author |
Ezer, C |
en |
dc.contributor.author |
Fanourakis, G |
en |
dc.contributor.author |
Ferrer-Ribas, E |
en |
dc.contributor.author |
Friedrich, P |
en |
dc.contributor.author |
Galan, J |
en |
dc.contributor.author |
Garcia, JA |
en |
dc.contributor.author |
Gardikiotis, A |
en |
dc.contributor.author |
Gazis, EN |
en |
dc.contributor.author |
Geralis, T |
en |
dc.contributor.author |
Giomataris, I |
en |
dc.contributor.author |
Gninenko, S |
en |
dc.contributor.author |
Gomez, H |
en |
dc.contributor.author |
Gruber, E |
en |
dc.contributor.author |
Guthorl, T |
en |
dc.contributor.author |
Hartmann, R |
en |
dc.contributor.author |
Haug, F |
en |
dc.contributor.author |
Hasinoff, MD |
en |
dc.contributor.author |
Hoffmann, DHH |
en |
dc.contributor.author |
Iguaz, FJ |
en |
dc.contributor.author |
Irastorza, IG |
en |
dc.contributor.author |
Jacoby, J |
en |
dc.contributor.author |
Jakovcic, K |
en |
dc.contributor.author |
Karuza, M |
en |
dc.contributor.author |
Konigsmann, K |
en |
dc.contributor.author |
Kotthaus, R |
en |
dc.contributor.author |
Krcmar, M |
en |
dc.contributor.author |
Kuster, M |
en |
dc.contributor.author |
Laurent, JM |
en |
dc.contributor.author |
Liolios, A |
en |
dc.contributor.author |
Ljubicic, A |
en |
dc.contributor.author |
Lozza, V |
en |
dc.contributor.author |
Lutz, G |
en |
dc.contributor.author |
Luzon, G |
en |
dc.contributor.author |
Morales, J |
en |
dc.contributor.author |
Niinikoski, T |
en |
dc.contributor.author |
Nordt, A |
en |
dc.contributor.author |
Papaevangelou, T |
en |
dc.contributor.author |
Pivovaroff, MJ |
en |
dc.contributor.author |
Raffelt, G |
en |
dc.contributor.author |
Rashba, T |
en |
dc.contributor.author |
Riege, H |
en |
dc.contributor.author |
Rodriguez, A |
en |
dc.contributor.author |
Rosu, M |
en |
dc.contributor.author |
Ruz, J |
en |
dc.contributor.author |
Savvidis, I |
en |
dc.contributor.author |
Silva, PS |
en |
dc.contributor.author |
Solanki, K |
en |
dc.contributor.author |
Stewart, L |
en |
dc.contributor.author |
Tomas, A |
en |
dc.contributor.author |
Tsagri, M |
en |
dc.contributor.author |
Van Bibber, K |
en |
dc.contributor.author |
Vafeiadis, T |
en |
dc.contributor.author |
Villar, J |
en |
dc.contributor.author |
Vogel, K |
en |
dc.contributor.author |
Yildiz, SC |
en |
dc.contributor.author |
Zioutas, K |
en |
dc.date.accessioned |
2014-03-01T02:54:01Z |
|
dc.date.available |
2014-03-01T02:54:01Z |
|
dc.date.issued |
2012 |
en |
dc.identifier.issn |
17426588 |
en |
dc.identifier.uri |
https://dspace.lib.ntua.gr/xmlui/handle/123456789/36543 |
|
dc.subject.other |
Buffer gas |
en |
dc.subject.other |
CERN axion solar telescopes |
en |
dc.subject.other |
Coupling constants |
en |
dc.subject.other |
Large Hadron collider LHC |
en |
dc.subject.other |
Phase I |
en |
dc.subject.other |
Phase II |
en |
dc.subject.other |
Various densities |
en |
dc.subject.other |
Bosons |
en |
dc.subject.other |
Experiments |
en |
dc.subject.other |
Magnets |
en |
dc.title |
Status and perspectives of the CAST experiment |
en |
heal.type |
conferenceItem |
en |
heal.identifier.primary |
10.1088/1742-6596/375/1/022001 |
en |
heal.identifier.secondary |
http://dx.doi.org/10.1088/1742-6596/375/1/022001 |
en |
heal.identifier.secondary |
022001 |
en |
heal.publicationDate |
2012 |
en |
heal.abstract |
The CERN Axion Solar Telescope (CAST) is currently the most sensitive axion helioscope designed to search for axions produced by the Primakoff process in the solar core. CAST is using a Large Hadron Collider (LHC) test magnet where axions could be converted into X-rays with energies up to 10 keV. During the phase I, the experiment operated with vacuum inside the magnet bores and covered axion masses up to 0.02 eV. In the phase II, the magnet bores were filled with a buffer gas (first4He and later3He) at various densities in order to extend the sensitivity to higher axion masses (up to f .18 eV). The phase II data taking was completed in 2011. So far, no evidence of axion signal has been found and CAST set the most restrictive experimental limit on the axion-photon coupling constant over a broad range of axion masses. The latest CAST results with3He data in the mass range 0.39 eV < ma < 0.64 eV will be presented. |
en |
heal.journalName |
Journal of Physics: Conference Series |
en |
dc.identifier.doi |
10.1088/1742-6596/375/1/022001 |
en |
dc.identifier.volume |
375 |
en |
dc.identifier.issue |
PART 2 |
en |