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Prospects for the CERN Axion Solar Telescope sensitivity to 14.4 keV axions

Authors :
José Villar
A. Liolios
L. Di Lella
Thomas Papaevangelou
H. Riege
J. Franz
G. Fanourakis
Joachim Jacoby
Milica Krčmar
A. Morales
Ante Ljubičić
S. Andriamonje
J. M. Carmona
Pasquale D. Serpico
E. Ferrer Ribas
T. Dafni
Theodoros Geralis
L. Stewart
Y. Semertzidis
Julia Vogel
Biljana Lakić
K. Barth
G. Luzón
S. Cebrián
F. T. Avignone
B. Beltrán
Krešimir Jakovčić
A. Placci
Konstantinos Kousouris
Georg G. Raffelt
H. Fischer
A. Belov
K. Königsmann
M. D. Hasinoff
J. I. Collar
C. Lasseur
H. Bräuninger
J. Morales
David Miller
C. Eleftheriadis
Louis Walckiers
Markus Kuster
J. Ruz
Peter Friedrich
Konstantin Zioutas
S. Aune
Dieter H. H. Hoffmann
I. G. Irastorza
M. Davenport
Gerhard Lutz
Ioannis Giomataris
Joaquin Vieira
D. Kang
R. Kotthaus
F.H. Heinsius
A. Ortiz
S. N. Gninenko
Publication Year :
2007

Abstract

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.<br />Comment: 4 pages, 1 figure. Submitted to Nucl. Instr. and Meth. A

Details

Language :
English
Database :
OpenAIRE
Accession number :
edsair.doi.dedup.....8e0414d22503e4832f6873afe79ec5a6