A decommissioned LHC model magnet as an axion telescope

被引:132
作者
Zioutas, K
Aalseth, CE
Abriola, D
Avignone, FT
Brodzinski, RL
Collar, JI [1 ]
Creswick, R
Di Gregorio, DE
Farach, H
Gattone, AO
Guérard, CK
Hasenbalg, F
Hasinoff, M
Huck, H
Liolios, A
Miley, HS
Morales, A
Morales, J
Nikas, D
Nussinov, S
Ortiz, A
Savvidis, E
Scopel, S
Sievers, P
Villar, JA
Walckiers, L
机构
[1] CERN, CH-1211 Geneva 23, Switzerland
[2] Univ Thessaloniki, Dept Phys, GR-54006 Thessaloniki, Greece
[3] Univ S Carolina, Dept Phys & Astron, Columbia, SC 29208 USA
[4] CNEA, TANDAR Lab, Dept Phys, Buenos Aires, DF, Argentina
[5] Pacific NW Lab, Richland, WA 99352 USA
[6] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z1, Canada
[7] Univ Zaragoza, Fac Ciencias, Lab Fis Nucl & Atlas Energias, E-50009 Zaragoza, Spain
[8] Tel Aviv Univ, Dept Phys, Tel Aviv, Israel
关键词
solar axions; LHC; superconducting magnets; dark matter;
D O I
10.1016/S0168-9002(98)01442-9
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
The 8.4 T, 10 m long transverse magnetic field of a twin aperture LHC bending magnet can be utilized as a macroscopic coherent solar axion-to-photon converter. Numerical calculations show that the integrated time of alignment with the Sun would be 33 days/yr with the magnet on a tracking table capable of +/ -5 degrees in the vertical direction and +/- 40 degrees in the horizontal direction. The existing lower bound on the axion-to-photon coupling constant can be improved by a factor between 30 and 100 in 3 yr, i.e.. g(a gamma gamma) less than or similar to 9 X 10(-11) GeV-1 for axion masses less than or similar to 1 eV. This value falls within the existing open axion mass window. The same set-up can simultaneously search for low- and high-energy celestial axions, or axion-like particles, scanning the sky as the Earth rotates and orbits the Sun. (C) 1999 Elsevier Science B.V. All rights reserved.
引用
收藏
页码:480 / 487
页数:8
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