Pregled bibliografske jedinice broj: 304450
Prospects for the CERN Axion Solar Telescope sensitivity to 14.4 keV axions
Prospects for the CERN Axion Solar Telescope sensitivity to 14.4 keV axions // Nuclear Instruments and Methods in Physics Research Section A - Accelerators Spectrometers Detectors and Associated Equipment, 580 (2007), 1; 37-39 (međunarodna recenzija, članak, znanstveni)
CROSBI ID: 304450 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
Prospects for the CERN Axion Solar Telescope sensitivity to 14.4 keV axions
Autori
Jakovčić, Krešimir ; Andriamonje, S. ; Aune, S. ; Avignone, F. ; Barth, K. ; Belov, A. ; Beltrán, B. ; Bräuninger, H. ; Carmona, J. M. ; Cebrián, S. ; Collar, J. I. ; Dafni, T. ; Davenport, M. ; Di Lella, L. ; Eleftheriadis, C. ; Fanourakis, G. ; Ferrer Ribas, E. ; Fischer, H. ; Franz, J. ; Friedrich, P. ; Geralis, T. ; Giomataris, I. ; Gninenko, S. ; Hasinoff, M. D. ; Heinsius, F. H. ; Hoffmann, D. H. H. ; Irastorza, I. G. ; Jacoby, J. ; Kang, D. ; Königsmann, K. ; Kotthaus, R. ; Krčmar, Milica ; Kousouris, K. ; Kuster, M. ; Lakić, Biljana ; Lasseur, C. ; Liolios, A. ; Ljubičić, Ante ; Lutz, G. ; Luzón, G. ; Miller, D. W. ; Morales, A. ; Morales, J. ; Ortiz, A. ; Papaevangelou, T. ; Placci, A. ; Raffelt, G. ; Ruz, J. ; Riege, H. ; Semertzidis, Y. ; Serpico, P. ; Stewart, L. ; Vieira, J. D. ; Villar, J. ; Vogel, J. ; Walckiers, L. ; Zioutas K.
Izvornik
Nuclear Instruments and Methods in Physics Research Section A - Accelerators Spectrometers Detectors and Associated Equipment (0168-9002) 580
(2007), 1;
37-39
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni
Ključne riječi
solar axions; axion-photon coupling; axion-nucleon coupling; dark matter
Sažetak
The CERN Axion Solar Telescope (CAST) is searching for solar axions using the 9.0 T strong and 9.26 m long transverse magnetic field of a twin aperture LHC test magnet, where axions could be converted into X-rays via reverse Primakoff process. Here we explore the potential of CAST to search for 14.4 keV axions that could be emitted from the Sun in M1 nuclear transition between the first, thermally excited state, and the ground state of 57Fe nuclide. Calculations of the expected signals, with respect to the axion– photon coupling, axion– nucleon coupling and axion mass, are presented in comparison with the experimental sensitivity.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
Napomena
Proceedings of the 10th International Symposium on Radiation Physics - ISRP 10 Coimbra, Portugal 17-22 September 2006 Edited by M.I. Lopes, J.E. Fernández, W.L. Dunn and M.M.R. Costa
POVEZANOST RADA
Projekti:
098-0982887-2872 - Masivni neutrini i astročestice: od fizike čestica do kozmologije (Ljubičić, Ante, MZOS ) ( CroRIS)
Ustanove:
Institut "Ruđer Bošković", Zagreb
Profili:
Milica Krčmar
(autor)
Ante Ljubičić
(autor)
Biljana Lakić
(autor)
Krešimir Jakovčić
(autor)
Citiraj ovu publikaciju:
Časopis indeksira:
- Current Contents Connect (CCC)
- Web of Science Core Collection (WoSCC)
- Science Citation Index Expanded (SCI-EXP)
- SCI-EXP, SSCI i/ili A&HCI
- Scopus