First Searches for Axions and Axionlike Particles with the LUX Experiment

被引：56

作者：

Akerib, D. S. ^{[1
,2
,3
]}

Alsum, S. ^{[4
]}

Aquino, C. ^{[5
]}

Araujo, H. M. ^{[6
]}

Bai, X. ^{[7
]}

Bailey, A. J. ^{[6
]}

Balajthy, J. ^{[8
]}

Beltrame, P. ^{[5
]}

Bernard, E. P. ^{[9
,10
]}

Bernstein, A. ^{[11
]}

Biesiadzinski, T. P. ^{[1
,2
,3
]}

Boulton, E. M. ^{[9
,10
]}

Bras, P. ^{[12
]}

Byram, D. ^{[13
,14
]}

Cahn, S. B. ^{[10
]}

Carmona-Benitez, M. C. ^{[15
]}

Chan, C. ^{[16
]}

Chiller, A. A. ^{[13
]}

Chiller, C.

Currie, A. ^{[6
]}

Cutter, J. E. ^{[17
]}

Davison, T. J. R. ^{[5
]}

Dobi, A. ^{[18
]}

Dobson, J. E. Y. ^{[19
]}

Druszkiewicz, E. ^{[20
]}

Edwards, B. N. ^{[10
]}

Faham, C. H. ^{[18
]}

Fallon, S. R. ^{[21
]}

Fiorucci, S. ^{[18
]}

Gaitskell, R. J. ^{[16
]}

Gehman, V. M. ^{[16
,18
]}

Ghag, C. ^{[19
]}

Gibson, K. R. ^{[1
]}

Gilchriese, M. G. D. ^{[18
]}

Hall, C. R. ^{[8
]}

Hanhardt, M. ^{[7
,14
]}

Haselschwardt, S. J. ^{[22
]}

Hertel, S. A. ^{[23
]}

Hogan, D. P. ^{[9
]}

Horn, M. ^{[9
,14
]}

Huang, D. Q. ^{[16
]}

Ignarra, C. M. ^{[2
,3
]}

Jacobsen, R. G. ^{[9
]}

Ji, W. ^{[1
,2
,3
]}

Kamdin, K. ^{[9
]}

Kazkaz, K. ^{[11
]}

Khaitan, D. ^{[20
]}

Knoche, R. ^{[8
]}

Larsen, N. A. ^{[10
]}

Lee, C. ^{[1
,2
,3
]}

机构：

[1] Case Western Reserve Univ, Dept Phys, 10900 Euclid Ave, Cleveland, OH 44106 USA

[2] SLAC Natl Accelerator Lab, 2575 Sand Hill Rd, Menlo Pk, CA 94205 USA

[3] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, 452 Lomita Mall, Stanford, CA 94309 USA

[4] Univ Wisconsin, Dept Phys, 1150 Univ Ave, Madison, WI 53706 USA

[5] Univ Edinburgh, Sch Phys & Astron, SUPA, Edinburgh EH9 3FD, Midlothian, Scotland

[6] Imperial Coll London, Blackett Lab, High Energy Phys, London SW7 2BZ, England

[7] South Dakota Sch Mines & Technol, 501 E St Joseph St, Rapid City, SD 57701 USA

[8] Univ Maryland, Dept Phys, College Pk, MD 20742 USA

[9] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA

[10] Yale Univ, Dept Phys, 217 Prospect St, New Haven, CT 06511 USA

[11] Lawrence Livermore Natl Lab, 7000 East Ave, Livermore, CA 94551 USA

[12] Univ Coimbra, Dept Phys, LIP Coimbra, Rua Larga, P-3004516 Coimbra, Portugal

[13] Univ South Dakota, Dept Phys, 414E Clark St, Vermillion, SD 57069 USA

[14] South Dakota Sci & Technol Author, Sanford Underground Res Facil, Lead, SD 57754 USA

[15] Penn State Univ, Dept Phys, 104 Davey Lab, University Pk, PA 16802 USA

[16] Brown Univ, Dept Phys, 182 Hope St, Providence, RI 02912 USA

[17] Univ Calif Davis, Dept Phys, One Shields Ave, Davis, CA 95616 USA

[18] Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA 94720 USA

[19] UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, England

[20] Univ Rochester, Dept Phys & Astron, Rochester, NY 14627 USA

[21] SUNY Albany, Dept Phys, 1400 Washington Ave, Albany, NY 12222 USA

[22] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA

[23] Univ Massachusetts, Dept Phys, Amherst, MA 01003 USA

[24] Texas A&M Univ, Dept Phys, College Stn, TX 77843 USA

来源：

PHYSICAL REVIEW LETTERS | 2017年 / 118卷 / 26期

基金：

美国国家科学基金会;

关键词：

INVARIANCE;

D O I：

10.1103/PhysRevLett.118.261301

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

The first searches for axions and axionlike particles with the Large Underground Xenon experiment are presented. Under the assumption of an axioelectric interaction in xenon, the coupling constant between axions and electrons g(Ae) is tested using data collected in 2013 with an exposure totaling 95 live days x 118 kg. A double-sided, profile likelihood ratio statistic test excludes gAe larger than 3.5 x 10(-12) (90% C.L.) for solar axions. Assuming the Dine-Fischler-Srednicki-Zhitnitsky theoretical description, the upper limit in coupling corresponds to an upper limit on axion mass of 0.12 eV/c(2), while for the Kim-Shifman-Vainshtein-Zhakharov description masses above 36.6 eV/c(2) are excluded. For galactic axionlike particles, values of gAe larger than 4.2 x 10(-13) are excluded for particle masses in the range 1-16 keV/c(2). These are the most stringent constraints to date for these interactions.

引用

页数：7

共 46 条

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