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
相关论文
共 54 条
[21]   New astrophysical constraints on the light-pseudoscalar-photon coupling [J].
Krasnikov, SV .
PHYSICAL REVIEW LETTERS, 1996, 76 (15) :2633-2636
[22]   SEARCH FOR SOLAR AXIONS [J].
LAZARUS, DM ;
SMITH, GC ;
CAMERON, R ;
MELISSINOS, AC ;
RUOSO, G ;
SEMERTZIDIS, YK ;
NEZRICK, FA .
PHYSICAL REVIEW LETTERS, 1992, 69 (16) :2333-2336
[23]   LIGHT SPINLESS PARTICLE COUPLED TO PHOTONS [J].
MASSO, E ;
TOLDRA, R .
PHYSICAL REVIEW D, 1995, 52 (04) :1755-1763
[24]  
MASSO E, ASTROPH9704056
[25]   LOW-BACKGROUND COUNTING SYSTEMS COMPARED [J].
MILEY, HS ;
BRODZINSKI, RL ;
REEVES, JH .
JOURNAL OF RADIOANALYTICAL AND NUCLEAR CHEMISTRY-ARTICLES, 1992, 160 (02) :371-385
[26]   FILTERING MICROPHONICS IN DARK MATTER GERMANIUM EXPERIMENTS [J].
MORALES, J ;
GARCIA, E ;
DESOLORZANO, AO ;
MORALES, A ;
NUNEZLAGOS, R ;
PUIMEDON, J ;
SAENZ, C ;
VILLAR, JA .
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, 1992, 321 (1-2) :410-414
[27]   PROPOSAL TO SEARCH FOR A MONOCHROMATIC COMPONENT OF SOLAR AXIONS USING FE-57 [J].
MORIYAMA, S .
PHYSICAL REVIEW LETTERS, 1995, 75 (18) :3222-3225
[28]   Direct search for solar axions by using strong magnetic field and X-ray detectors [J].
Moriyama, S ;
Minowa, M ;
Namba, T ;
Inoue, Y ;
Takasu, Y ;
Yamamoto, A .
PHYSICS LETTERS B, 1998, 434 (1-2) :147-152
[29]  
MORIYAMA S, 1997, THESIS U TOKIO
[30]   Interactions of cosmic axions with Rydberg atoms in resonant cavities via the Primakoff process [J].
Ogawa, I ;
Matsuki, S ;
Yamamoto, K .
PHYSICAL REVIEW D, 1996, 53 (04) :R1740-R1744