First Searches for Axions and Axionlike Particles with the LUX Experiment

D. S. Akerib; S. Alsum; C. Aquino; H. M. Araújo; X. Bai; A. J. Bailey; J. Balajthy; P. Beltrame; E. P. Bernard; A. Bernstein; T. P. Biesiadzinski; E. M. Boulton; P. Brás; D. Byram; S. B. Cahn; M. C. Carmona-Benitez; C. Chan; A. A. Chiller; C. Chiller; A. Currie; J. E. Cutter; T. J.R. Davison; A. Dobi; J. E.Y. Dobson; E. Druszkiewicz; B. N. Edwards; C. H. Faham; S. R. Fallon; S. Fiorucci; R. J. Gaitskell; V. M. Gehman; C. Ghag; K. R. Gibson; M. G.D. Gilchriese; C. R. Hall; M. Hanhardt; S. J. Haselschwardt; S. A. Hertel; D. P. Hogan; M. Horn; D. Q. Huang; C. M. Ignarra; R. G. Jacobsen; W. Ji; K. Kamdin; K. Kazkaz; D. Khaitan; R. Knoche; N. A. Larsen; C. Lee; B. G. Lenardo; K. T. Lesko; A. Lindote; M. I. Lopes; A. Manalaysay; R. L. Mannino; M. F. Marzioni; D. N. McKinsey; D. M. Mei; J. Mock; M. Moongweluwan; J. A. Morad; A. St J. Murphy; C. Nehrkorn; H. N. Nelson; F. Neves; K. O'Sullivan; K. C. Oliver-Mallory; K. J. Palladino; E. K. Pease; L. Reichhart; C. Rhyne; S. Shaw; T. A. Shutt; C. Silva; M. Solmaz; V. N. Solovov; P. Sorensen; S. Stephenson; T. J. Sumner; M. Szydagis; D. J. Taylor; W. C. Taylor; B. P. Tennyson; P. A. Terman; D. R. Tiedt; W. H. To; M. Tripathi; L. Tvrznikova; S. Uvarov; V. Velan; J. R. Verbus; R. C. Webb; J. T. White; T. J. Whitis; M. S. Witherell; F. L.H. Wolfs; J. Xu; K. Yazdani; S. K. Young; C. Zhang

doi:10.1103/PhysRevLett.118.261301

First Searches for Axions and Axionlike Particles with the LUX Experiment

D. S. Akerib, S. Alsum, C. Aquino, H. M. Araújo, X. Bai, A. J. Bailey, J. Balajthy, P. Beltrame, E. P. Bernard, A. Bernstein, T. P. Biesiadzinski, E. M. Boulton, P. Brás, D. Byram, S. B. Cahn, M. C. Carmona-Benitez, C. Chan, A. A. Chiller, C. Chiller, A. CurrieJ. E. Cutter, T. J.R. Davison, A. Dobi, J. E.Y. Dobson, E. Druszkiewicz, B. N. Edwards, C. H. Faham, S. R. Fallon, S. Fiorucci, R. J. Gaitskell, V. M. Gehman, C. Ghag, K. R. Gibson, M. G.D. Gilchriese, C. R. Hall, M. Hanhardt, S. J. Haselschwardt, S. A. Hertel, D. P. Hogan, M. Horn, D. Q. Huang, C. M. Ignarra, R. G. Jacobsen, W. Ji, K. Kamdin, K. Kazkaz, D. Khaitan, R. Knoche, N. A. Larsen, C. Lee, B. G. Lenardo, K. T. Lesko, A. Lindote, M. I. Lopes, A. Manalaysay, R. L. Mannino, M. F. Marzioni, D. N. McKinsey, D. M. Mei, J. Mock, M. Moongweluwan, J. A. Morad, A. St J. Murphy, C. Nehrkorn, H. N. Nelson, F. Neves, K. O'Sullivan, K. C. Oliver-Mallory, K. J. Palladino, E. K. Pease, L. Reichhart, C. Rhyne, S. Shaw, T. A. Shutt, C. Silva, M. Solmaz, V. N. Solovov, P. Sorensen, S. Stephenson, T. J. Sumner, M. Szydagis, D. J. Taylor, W. C. Taylor, B. P. Tennyson, P. A. Terman, D. R. Tiedt, W. H. To, M. Tripathi, L. Tvrznikova, S. Uvarov, V. Velan, J. R. Verbus, R. C. Webb, J. T. White, T. J. Whitis, M. S. Witherell, F. L.H. Wolfs, J. Xu, K. Yazdani, S. K. Young, C. Zhang

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Abstract

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 gAe is tested using data collected in 2013 with an exposure totaling 95 live days ×118 kg. A double-sided, profile likelihood ratio statistic test excludes gAe larger than 3.5×10-12 (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/c2, while for the Kim-Shifman-Vainshtein-Zhakharov description masses above 36.6 eV/c2 are excluded. For galactic axionlike particles, values of gAe larger than 4.2×10-13 are excluded for particle masses in the range 1-16 keV/c2. These are the most stringent constraints to date for these interactions.

Original language	English (US)
Article number	261301
Journal	Physical review letters
Volume	118
Issue number	26
DOIs	https://doi.org/10.1103/PhysRevLett.118.261301
State	Published - Jun 29 2017

All Science Journal Classification (ASJC) codes

General Physics and Astronomy

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10.1103/PhysRevLett.118.261301

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Akerib, D. S., Alsum, S., Aquino, C., Araújo, H. M., Bai, X., Bailey, A. J., Balajthy, J., Beltrame, P., Bernard, E. P., Bernstein, A., Biesiadzinski, T. P., Boulton, E. M., Brás, P., Byram, D., Cahn, S. B., Carmona-Benitez, M. C., Chan, C., Chiller, A. A., Chiller, C., ... Zhang, C. (2017). First Searches for Axions and Axionlike Particles with the LUX Experiment. Physical review letters, 118(26), Article 261301. https://doi.org/10.1103/PhysRevLett.118.261301

@article{52a1ff3af0e54eb488816ca21dc88335,

title = "First Searches for Axions and Axionlike Particles with the LUX Experiment",

abstract = "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 gAe is tested using data collected in 2013 with an exposure totaling 95 live days ×118 kg. A double-sided, profile likelihood ratio statistic test excludes gAe larger than 3.5×10-12 (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/c2, while for the Kim-Shifman-Vainshtein-Zhakharov description masses above 36.6 eV/c2 are excluded. For galactic axionlike particles, values of gAe larger than 4.2×10-13 are excluded for particle masses in the range 1-16 keV/c2. These are the most stringent constraints to date for these interactions.",

author = "Akerib, {D. S.} and S. Alsum and C. Aquino and Ara{\'u}jo, {H. M.} and X. Bai and Bailey, {A. J.} and J. Balajthy and P. Beltrame and Bernard, {E. P.} and A. Bernstein and Biesiadzinski, {T. P.} and Boulton, {E. M.} and P. Br{\'a}s and D. Byram and Cahn, {S. B.} and Carmona-Benitez, {M. C.} and C. Chan and Chiller, {A. A.} and C. Chiller and A. Currie and Cutter, {J. E.} and Davison, {T. J.R.} and A. Dobi and Dobson, {J. E.Y.} and E. Druszkiewicz and Edwards, {B. N.} and Faham, {C. H.} and Fallon, {S. R.} and S. Fiorucci and Gaitskell, {R. J.} and Gehman, {V. M.} and C. Ghag and Gibson, {K. R.} and Gilchriese, {M. G.D.} and Hall, {C. R.} and M. Hanhardt and Haselschwardt, {S. J.} and Hertel, {S. A.} and Hogan, {D. P.} and M. Horn and Huang, {D. Q.} and Ignarra, {C. M.} and Jacobsen, {R. G.} and W. Ji and K. Kamdin and K. Kazkaz and D. Khaitan and R. Knoche and Larsen, {N. A.} and C. Lee and Lenardo, {B. G.} and Lesko, {K. T.} and A. Lindote and Lopes, {M. I.} and A. Manalaysay and Mannino, {R. L.} and Marzioni, {M. F.} and McKinsey, {D. N.} and Mei, {D. M.} and J. Mock and M. Moongweluwan and Morad, {J. A.} and Murphy, {A. St J.} and C. Nehrkorn and Nelson, {H. N.} and F. Neves and K. O'Sullivan and Oliver-Mallory, {K. C.} and Palladino, {K. J.} and Pease, {E. K.} and L. Reichhart and C. Rhyne and S. Shaw and Shutt, {T. A.} and C. Silva and M. Solmaz and Solovov, {V. N.} and P. Sorensen and S. Stephenson and Sumner, {T. J.} and M. Szydagis and Taylor, {D. J.} and Taylor, {W. C.} and Tennyson, {B. P.} and Terman, {P. A.} and Tiedt, {D. R.} and To, {W. H.} and M. Tripathi and L. Tvrznikova and S. Uvarov and V. Velan and Verbus, {J. R.} and Webb, {R. C.} and White, {J. T.} and Whitis, {T. J.} and Witherell, {M. S.} and Wolfs, {F. L.H.} and J. Xu and K. Yazdani and Young, {S. K.} and C. Zhang",

note = "Publisher Copyright: {\textcopyright} 2017 American Physical Society.",

year = "2017",

month = jun,

day = "29",

doi = "10.1103/PhysRevLett.118.261301",

language = "English (US)",

volume = "118",

journal = "Physical review letters",

issn = "0031-9007",

publisher = "American Physical Society",

number = "26",

}

Akerib, DS, Alsum, S, Aquino, C, Araújo, HM, Bai, X, Bailey, AJ, Balajthy, J, Beltrame, P, Bernard, EP, Bernstein, A, Biesiadzinski, TP, Boulton, EM, Brás, P, Byram, D, Cahn, SB, Carmona-Benitez, MC, Chan, C, Chiller, AA, Chiller, C, Currie, A, Cutter, JE, Davison, TJR, Dobi, A, Dobson, JEY, Druszkiewicz, E, Edwards, BN, Faham, CH, Fallon, SR, Fiorucci, S, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, CR, Hanhardt, M, Haselschwardt, SJ, Hertel, SA, Hogan, DP, Horn, M, Huang, DQ, Ignarra, CM, Jacobsen, RG, Ji, W, Kamdin, K, Kazkaz, K, Khaitan, D, Knoche, R, Larsen, NA, Lee, C, Lenardo, BG, Lesko, KT, Lindote, A, Lopes, MI, Manalaysay, A, Mannino, RL, Marzioni, MF, McKinsey, DN, Mei, DM, Mock, J, Moongweluwan, M, Morad, JA, Murphy, ASJ, Nehrkorn, C, Nelson, HN, Neves, F, O'Sullivan, K, Oliver-Mallory, KC, Palladino, KJ, Pease, EK, Reichhart, L, Rhyne, C, Shaw, S, Shutt, TA, Silva, C, Solmaz, M, Solovov, VN, Sorensen, P, Stephenson, S, Sumner, TJ, Szydagis, M, Taylor, DJ, Taylor, WC, Tennyson, BP, Terman, PA, Tiedt, DR, To, WH, Tripathi, M, Tvrznikova, L, Uvarov, S, Velan, V, Verbus, JR, Webb, RC, White, JT, Whitis, TJ, Witherell, MS, Wolfs, FLH, Xu, J, Yazdani, K, Young, SK & Zhang, C 2017, 'First Searches for Axions and Axionlike Particles with the LUX Experiment', Physical review letters, vol. 118, no. 26, 261301. https://doi.org/10.1103/PhysRevLett.118.261301

TY - JOUR

T1 - First Searches for Axions and Axionlike Particles with the LUX Experiment

AU - Akerib, D. S.

AU - Alsum, S.

AU - Aquino, C.

AU - Araújo, H. M.

AU - Bai, X.

AU - Bailey, A. J.

AU - Balajthy, J.

AU - Beltrame, P.

AU - Bernard, E. P.

AU - Bernstein, A.

AU - Biesiadzinski, T. P.

AU - Boulton, E. M.

AU - Brás, P.

AU - Byram, D.

AU - Cahn, S. B.

AU - Carmona-Benitez, M. C.

AU - Chan, C.

AU - Chiller, A. A.

AU - Chiller, C.

AU - Currie, A.

AU - Cutter, J. E.

AU - Davison, T. J.R.

AU - Dobi, A.

AU - Dobson, J. E.Y.

AU - Druszkiewicz, E.

AU - Edwards, B. N.

AU - Faham, C. H.

AU - Fallon, S. R.

AU - Fiorucci, S.

AU - Gaitskell, R. J.

AU - Gehman, V. M.

AU - Ghag, C.

AU - Gibson, K. R.

AU - Gilchriese, M. G.D.

AU - Hall, C. R.

AU - Hanhardt, M.

AU - Haselschwardt, S. J.

AU - Hertel, S. A.

AU - Hogan, D. P.

AU - Horn, M.

AU - Huang, D. Q.

AU - Ignarra, C. M.

AU - Jacobsen, R. G.

AU - Ji, W.

AU - Kamdin, K.

AU - Kazkaz, K.

AU - Khaitan, D.

AU - Knoche, R.

AU - Larsen, N. A.

AU - Lee, C.

AU - Lenardo, B. G.

AU - Lesko, K. T.

AU - Lindote, A.

AU - Lopes, M. I.

AU - Manalaysay, A.

AU - Mannino, R. L.

AU - Marzioni, M. F.

AU - McKinsey, D. N.

AU - Mei, D. M.

AU - Mock, J.

AU - Moongweluwan, M.

AU - Morad, J. A.

AU - Murphy, A. St J.

AU - Nehrkorn, C.

AU - Nelson, H. N.

AU - Neves, F.

AU - O'Sullivan, K.

AU - Oliver-Mallory, K. C.

AU - Palladino, K. J.

AU - Pease, E. K.

AU - Reichhart, L.

AU - Rhyne, C.

AU - Shaw, S.

AU - Shutt, T. A.

AU - Silva, C.

AU - Solmaz, M.

AU - Solovov, V. N.

AU - Sorensen, P.

AU - Stephenson, S.

AU - Sumner, T. J.

AU - Szydagis, M.

AU - Taylor, D. J.

AU - Taylor, W. C.

AU - Tennyson, B. P.

AU - Terman, P. A.

AU - Tiedt, D. R.

AU - To, W. H.

AU - Tripathi, M.

AU - Tvrznikova, L.

AU - Uvarov, S.

AU - Velan, V.

AU - Verbus, J. R.

AU - Webb, R. C.

AU - White, J. T.

AU - Whitis, T. J.

AU - Witherell, M. S.

AU - Wolfs, F. L.H.

AU - Xu, J.

AU - Yazdani, K.

AU - Young, S. K.

AU - Zhang, C.

PY - 2017/6/29

Y1 - 2017/6/29

N2 - 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 gAe is tested using data collected in 2013 with an exposure totaling 95 live days ×118 kg. A double-sided, profile likelihood ratio statistic test excludes gAe larger than 3.5×10-12 (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/c2, while for the Kim-Shifman-Vainshtein-Zhakharov description masses above 36.6 eV/c2 are excluded. For galactic axionlike particles, values of gAe larger than 4.2×10-13 are excluded for particle masses in the range 1-16 keV/c2. These are the most stringent constraints to date for these interactions.

AB - 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 gAe is tested using data collected in 2013 with an exposure totaling 95 live days ×118 kg. A double-sided, profile likelihood ratio statistic test excludes gAe larger than 3.5×10-12 (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/c2, while for the Kim-Shifman-Vainshtein-Zhakharov description masses above 36.6 eV/c2 are excluded. For galactic axionlike particles, values of gAe larger than 4.2×10-13 are excluded for particle masses in the range 1-16 keV/c2. These are the most stringent constraints to date for these interactions.

UR - http://www.scopus.com/inward/record.url?scp=85021760141&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85021760141&partnerID=8YFLogxK

U2 - 10.1103/PhysRevLett.118.261301

DO - 10.1103/PhysRevLett.118.261301

M3 - Article

C2 - 28707937

AN - SCOPUS:85021760141

SN - 0031-9007

VL - 118

JO - Physical review letters

JF - Physical review letters

IS - 26

M1 - 261301

ER -

First Searches for Axions and Axionlike Particles with the LUX Experiment

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