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Latest results of the CAST axion search
/ Irastorza, I G (DAPNIA, Saclay ; Zaragoza U.) ; Arik, E (Dogus U., Kadikoy) ; Aune, S (DAPNIA, Saclay) ; Autiero, D (CERN) ; Barth, K (CERN) ; Belov, A (Moscow, INR) ; Beltran, B (Zaragoza U.) ; Borghi, S (CERN) ; Bourlis, G (Hellenic Open U., Patras) ; Boydag, F S (Dogus U., Kadikoy) et al.
/CAST
2007 - 9 p.
- Published in : , pp. 301-310
Fulltext: PDF;
In : 42nd Rencontres de Moriond, La Thuile, Italy, 10 - 17 Mar 2007, pp.301-310
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Solar axion search with the CAST experiment
/ Borghi, S (CERN ; Glasgow U.) ; Arik, E (Dogus U., Kadikoy ; Bogazici U.) ; Aune, S (IRFU, Saclay) ; Autiero, D (CERN ; Lyon, IPN) ; Barth, K (CERN) ; Belov, A (Moscow, INR) ; Beltrán, B (Zaragoza U.) ; Bourlis, G (Hellenic Open U., Patras) ; Boydag, F S (Dogus U., Kadikoy ; Bogazici U.) ; Bräuninger, H (Garching, Max Planck Inst., MPE) et al.
/CAST
The CAST (CERN Axion Solar Telescope) experiment is searching for solar axions by their conversion into photons inside the magnet pipe of a LHC prototype dipole. In the phase II, CAST is operating with a buffer gas inside the magnet bore apertures in order to extent the sensitivity of the experiment to larger axion masses. [...]
Paris, France : Moriond, 2008 - 8 p.
- Published in : , pp. 465-472
Fulltext: PDF;
In : 43rd Rencontres de Moriond, La Thuile, Italy, 01 - 08 Mar 2008, pp.465-472
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Search for Solar Axions with the CAST-Experiment
/ Vogel, J. (Freiburg U.) ; Arik, E. (Dogus U., Kadikoy) ; Aune, S. (CEA, DSM, Saclay) ; Autiero, D. (CERN) ; Barth, K. (CERN) ; Belov, A. (Moscow, INR) ; Beltran, B. (U. Zaragoza (main)) ; Borghi, S. (CERN) ; Bourlis, G. ; Boydag, F. S. (Dogus U., Kadikoy) et al.
Solar axions can be produced in the Sun via the so-called Primakoff effect. The CERN Axion Solar Telescope (CAST) uses an LHC prototype magnet of about 9 T to reconvert these axions into photons. [...]
2008
- Published in : 10.1142/9789812819093_0049
In : 10th ICATPP Conference on Astroparticle, Particle, Space Physics, Detectors and Medical Physics Applications, Villa Olmo, Como, Italy, 8 - 12 Oct 2007, pp.282-286
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CAST constraints on the axion-electron coupling
/ Barth, K. (CERN) ; Belov, A. (Moscow, INR) ; Beltran, B. (Zaragoza U.) ; Bräuninger, H. (Garching, Max Planck Inst., MPE) ; Carmona, J.M. (Zaragoza U.) ; Collar, J.I. (Chicago U., EFI ; Chicago U., KICP) ; Dafni, T. (Zaragoza U. ; IRFU, Saclay ; Darmstadt, Tech. U.) ; Davenport, M. (CERN) ; Di Lella, L. (CERN) ; Eleftheriadis, C. (Thessaloniki U.) et al.
In non-hadronic axion models, which have a tree-level axion-electron interaction, the Sun produces a strong axion flux by bremsstrahlung, Compton scattering, and axio-recombination, the "BCA processes." Based on a new calculation of this flux, including for the first time axio-recombination, we derive limits on the axion-electron Yukawa coupling g_ae and axion-photon interaction strength g_ag using the CAST phase-I data (vacuum phase). For m_a < 10 meV/c2 we find g_ag x g_ae< 8.1 x 10^-23 GeV^-1 at 95% CL. [...]
arXiv:1302.6283.-
2013 - 16 p.
- Published in : JCAP 05 (2013) 010
Fulltext: PDF; External link: Preprint
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The CERN Axion Solar Telescope (CAST) : An Update
/ Andriamonje, Samuel A (DAPNIA, CEA Saclay) ; Arsov, V ; Aune, S ; Aume, T ; Avignone, F T ; Barth, K (CERN) ; Belov, A ; Beltran, B ; Bräuninger, H ; Carmona, J et al.
2005
- Published in : Nucl. Phys. B, Proc. Suppl. 138 (2005) 41-44
In : 8th International Workshop on Topics in Astroparticle and Underground Physics, Seattle, WA, USA, 5 - 9 Sep 2003, pp.41-44
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Background studies and shielding effects for the TPC detector of the CAST experiment
/ Luzon, G. (U. Zaragoza (main)) ; Beltran, B. (Queen's U., Kingston ; U. Zaragoza (main)) ; Carmona, J.M. (U. Zaragoza (main)) ; Cebrian, S. ; Gomez, H. (U. Zaragoza (main)) ; Irastorza, I.G. (U. Zaragoza (main)) ; Morales, J. (U. Zaragoza (main)) ; Ortiz, A. (U. Zaragoza (main)) ; Rodriguez, A. (U. Zaragoza (main)) ; Ruz, J. (U. Zaragoza (main)) et al.
Sunset solar axions traversing the intense magnetic field of the CERN Axion Solar Telescope (CAST) experiment may be detected in a Time Projection Chamber (TPC) detector, as X-rays signals. These signals could be masked, however, by the inhomogeneous background of materials in the experimental site. [...]
arXiv:0706.1636.-
2007 - 14 p.
- Published in : New J. Phys. 9 (2007) 208
Fulltext: njp7_7_208 - PDF; arXiv:0706.1636 - PDF; External link: Fulltext
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