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First results from the CERN axion solar telescope.

Authors :
Zioutas K
Andriamonje S
Arsov V
Aune S
Autiero D
Avignone FT
Barth K
Belov A
Beltrán B
Bräuninger H
Carmona JM
Cebrián S
Chesi E
Collar JI
Creswick R
Dafni T
Davenport M
Di Lella L
Eleftheriadis C
Englhauser J
Fanourakis G
Farach H
Ferrer E
Fischer H
Franz J
Friedrich P
Geralis T
Giomataris I
Gninenko S
Goloubev N
Hasinoff MD
Heinsius FH
Hoffmann DH
Irastorza IG
Jacoby J
Kang D
Königsmann K
Kotthaus R
Krcmar M
Kousouris K
Kuster M
Lakić B
Lasseur C
Liolios A
Ljubicić A
Lutz G
Luzón G
Miller DW
Morales A
Morales J
Mutterer M
Nikolaidis A
Ortiz A
Papaevangelou T
Placci A
Raffelt G
Ruz J
Riege H
Sarsa ML
Savvidis I
Serber W
Serpico P
Semertzidis Y
Stewart L
Vieira JD
Villar J
Walckiers L
Zachariadou K
Source :
Physical review letters [Phys Rev Lett] 2005 Apr 01; Vol. 94 (12), pp. 121301. Date of Electronic Publication: 2005 Apr 01.
Publication Year :
2005

Abstract

Hypothetical axionlike particles with a two-photon interaction would be produced in the sun by the Primakoff process. In a laboratory magnetic field ("axion helioscope"), they would be transformed into x-rays with energies of a few keV. Using a decommissioned Large Hadron Collider test magnet, the CERN Axion Solar Telescope ran for about 6 months during 2003. The first results from the analysis of these data are presented here. No signal above background was observed, implying an upper limit to the axion-photon coupling g(agamma)<1.16x10(-10) GeV-1 at 95% C.L. for m(a) less, similar 0.02 eV. This limit, assumption-free, is comparable to the limit from stellar energy-loss arguments and considerably more restrictive than any previous experiment over a broad range of axion masses.

Details

Language :
English
ISSN :
0031-9007
Volume :
94
Issue :
12
Database :
MEDLINE
Journal :
Physical review letters
Publication Type :
Academic Journal
Accession number :
15903903
Full Text :
https://doi.org/10.1103/PhysRevLett.94.121301