Nalazite se na CroRIS probnoj okolini. Ovdje evidentirani podaci neće biti pohranjeni u Informacijskom sustavu znanosti RH. Ako je ovo greška, CroRIS produkcijskoj okolini moguće je pristupi putem poveznice www.croris.hr
izvor podataka: crosbi

The CAST Experiment (CROSBI ID 545368)

Prilog sa skupa u časopisu | izvorni znanstveni rad | međunarodna recenzija

(CAST Collaboration) Ruz, J. ; Arik, E. ; Aune, S. ; Autiero, D. ; Barth, K. ; Belov, A. ; Beltran, B. ; Borghi, S. ; Bourlis, G. ; Boydag, F.S. et al. The CAST Experiment // Journal of physics. Conference series. 2008. doi: 10.1088/1742-6596/110/6/062023

Podaci o odgovornosti

Ruz, J. ; Arik, E. ; Aune, S. ; Autiero, D. ; Barth, K. ; Belov, A. ; Beltran, B. ; Borghi, S. ; Bourlis, G. ; Boydag, F.S. ; Brauninger, H. ; Carmona, J. ; Cebrian, S. ; Cetin, S.A. ; Collar, J.I. ; Dafni, T. ; Davenport, M. ; Di Lella, L. ; Dogan, O.B. ; Eleftheriadis, C. ; Fanourakis, G. ; Ferrer Ribas, E. ; Fischer, H. ; Franz, J. ; Galan, J. ; Geralis, T. ; Giomataris, I. ; Gninenko, S. ; Gomez, H. ; Hasinoff, M. ; Heinsius, F.H. ; Hikmet, I. ; Gazis, E. ; Hoffmann, D.H.H. ; Irastorza, I.G. ; Jacoby, J. ; Jakovčić, Krešimir ; Kang, D. ; Konigsmann, K. ; Kotthaus, R. ; Krčmar, Milica ; Kousouris, K. ; Kuster, M. ; Lakić, Biljana ; Lasseur, C. ; Liolios, A. ; Ljubičić, Ante ; Lutz, G. ; Luzon, G. ; Miller, D. ; Morales, A. ; Morales, J. ; Niinikoski, T. ; Nordt, A. ; Ortiz, A. ; Papaevangelou, T. ; Pivovaroff, M. ; Placci, A. ; Raitieri, G. ; Raffelt, G. ; Riege, H. ; Rodriguez, A. ; Savvidis, I. ; Semertzidis, Y. ; Serpico, P. ; Soufli, R. ; Stewart, L. ; Tzamarias, K. ; van Bibber, K. ; Villar, J. ; Vogel, J. ; Walckiers, L. ; Zioutas, K.

CAST Collaboration

engleski

The CAST Experiment

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 three 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, CAST has been looking for axions with masses up to 0.02 eV. CAST’ s second phase manages to re-establish the coherence needed to scan for axions with masses up to 1.16 eV by using a buffer gas. This technique enables the experiment to look into the theoretical regions for axions. During the years 2005 and 2006, the use of 4He in CAST has already provided coherence in order to look for axions with masses up to 0.4 eV.

axions ; axion-photon coupling ; solar axion telescope

nije evidentirano

nije evidentirano

nije evidentirano

nije evidentirano

nije evidentirano

nije evidentirano

Podaci o prilogu

062023

2008.

nije evidentirano

objavljeno

10.1088/1742-6596/110/6/062023

Podaci o matičnoj publikaciji

Journal of physics. Conference series

IOP Publishing

1742-6588

1742-6596

Podaci o skupu

Nepoznat skup

predavanje

29.02.1904-29.02.2096

Povezanost rada

Fizika

Poveznice
Indeksiranost