dc.contributor.author |
Irastorza, G |
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, M |
en |
dc.contributor.author |
Cetin, A |
en |
dc.contributor.author |
Collar, I |
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 |
Gardikiotis, A |
en |
dc.contributor.author |
Gazis, N |
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, D |
en |
dc.contributor.author |
Hoffmann, H |
en |
dc.contributor.author |
Iguaz, J |
en |
dc.contributor.author |
Jacoby, J |
en |
dc.contributor.author |
Jakovic, K |
en |
dc.contributor.author |
Karuza, M |
en |
dc.contributor.author |
Konigsmann, K |
en |
dc.contributor.author |
Kotthaus, R |
en |
dc.contributor.author |
Krmar, M |
en |
dc.contributor.author |
Kuster, M |
en |
dc.contributor.author |
Lakic, B |
en |
dc.contributor.author |
Laurent, M |
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, J |
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, S |
en |
dc.contributor.author |
Solanki, K |
en |
dc.contributor.author |
Soufli, R |
en |
dc.contributor.author |
Stewart, L |
en |
dc.contributor.author |
Toms, 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, C |
en |
dc.contributor.author |
Zioutas, K |
en |
dc.date.accessioned |
2014-03-01T02:53:20Z |
|
dc.date.available |
2014-03-01T02:53:20Z |
|
dc.date.issued |
2011 |
en |
dc.identifier.issn |
17426588 |
en |
dc.identifier.uri |
https://dspace.lib.ntua.gr/xmlui/handle/123456789/36244 |
|
dc.subject.other |
CERN axion solar telescopes |
en |
dc.subject.other |
High magnetic fields |
en |
dc.subject.other |
Large Hadron collider LHC |
en |
dc.subject.other |
Phase I |
en |
dc.subject.other |
Magnetic fields |
en |
dc.subject.other |
Magnets |
en |
dc.subject.other |
Optical telescopes |
en |
dc.subject.other |
Photons |
en |
dc.subject.other |
Solar energy |
en |
dc.subject.other |
Stars |
en |
dc.subject.other |
Superconducting magnets |
en |
dc.subject.other |
Telescopes |
en |
dc.subject.other |
Experiments |
en |
dc.title |
Latest results and prospects of the CERN Axion Solar Telescope |
en |
heal.type |
conferenceItem |
en |
heal.identifier.primary |
10.1088/1742-6596/309/1/012001 |
en |
heal.identifier.secondary |
http://dx.doi.org/10.1088/1742-6596/309/1/012001 |
en |
heal.identifier.secondary |
012001 |
en |
heal.publicationDate |
2011 |
en |
heal.abstract |
The CERN Axion Solar Telescope (CAST) experiment searches for axions from the Sun converted into few keV photons via the inverse Primakoff effect in the high magnetic field of a superconducting Large Hadron Collider (LHC) decommissioned test magnet. After results obtained with vacuum in the magnet pipes (phase I of the experiment) as well as with4He the collaboration is now immersed in the data taking with3He, to be finished in 2011. The status of the experiment will be presented, including a preliminary exclusion plot of the first3He data. CAST is currently sensitive to realistic QCD axion models at the sub-eV scale, and with axion-photon couplings down to the ∼ 2 × 10-10 GeV-1, compatible with solar life limits. Future plans include revisiting vaccuum and4He configurations with improved sensitivity, as well as possible additional search for non-standard signals from chamaleons, paraphotons or other WISPs. For the longer term, we study the feasibility of an altogether improved version of the axion helioscope concept, with a jump in sensitivity of about one order of magnitude in gaγ beyond CAST. |
en |
heal.journalName |
Journal of Physics: Conference Series |
en |
dc.identifier.doi |
10.1088/1742-6596/309/1/012001 |
en |
dc.identifier.volume |
309 |
en |
dc.identifier.issue |
1 |
en |