First axion results from the XENON100 experiment

E. Aprile, F. Agostini, M. Alfonsi, K. Arisaka, Francesco Arneodo, M. Auger, C. Balan, P. Barrow, L. Baudis, B. Bauermeister, A. Behrens, P. Beltrame, K. Bokeloh, A. Brown, E. Brown, S. Bruenner, G. Bruno, R. Budnik, J. M.R. Cardoso, A. P. ColijnH. Contreras, J. P. Cussonneau, M. P. Decowski, E. Duchovni, S. Fattori, A. D. Ferella, W. Fulgione, F. Gao, M. Garbini, C. Geis, L. W. Goetzke, C. Grignon, E. Gross, W. Hampel, R. Itay, F. Kaether, G. Kessler, A. Kish, H. Landsman, R. F. Lang, M. Le Calloch, D. Lellouch, C. Levy, S. Lindemann, M. Lindner, J. A.M. Lopes, K. Lung, A. Lyashenko, S. Macmullin, T. Marrodán Undagoitia, J. Masbou, F. V. Massoli, D. Mayani Paras, A. J. Melgarejo Fernandez, Y. Meng, M. Messina, B. Miguez, A. Molinario, M. Murra, J. Naganoma, K. Ni, U. Oberlack, S. E.A. Orrigo, E. Pantic, R. Persiani, F. Piastra, J. Pienaar, G. Plante, N. Priel, S. Reichard, C. Reuter, A. Rizzo, S. Rosendahl, J. M.F. Dos Santos, G. Sartorelli, S. Schindler, J. Schreiner, M. Schumann, L. Scotto Lavina, M. Selvi, P. Shagin, H. Simgen, A. Teymourian, D. Thers, A. Tiseni, G. Trinchero, O. Vitells, H. Wang, M. Weber, C. Weinheimer

Research output: Contribution to journalArticle

Abstract

We present the first results of searches for axions and axionlike particles with the XENON100 experiment. The axion-electron coupling constant, gAe, has been probed by exploiting the axioelectric effect in liquid xenon. A profile likelihood analysis of 224.6 live days × 34-kg exposure has shown no evidence for a signal. By rejecting gAe larger than 7.7×10-12 (90% C.L.) in the solar axion search, we set the best limit to date on this coupling. In the frame of the DFSZ and KSVZ models, we exclude QCD axions heavier than 0.3 and 80eV/c2, respectively. For axionlike particles, under the assumption that they constitute the whole abundance of dark matter in our galaxy, we constrain gAe to be lower than 1×10-12 (90% C.L.) for masses between 5 and 10keV/c2.

Original languageEnglish (US)
Article number062009
JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
Volume90
Issue number6
DOIs
StatePublished - Sep 9 2014

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xenon
dark matter
quantum chromodynamics
galaxies
liquids
profiles
electrons

ASJC Scopus subject areas

  • Nuclear and High Energy Physics
  • Physics and Astronomy (miscellaneous)

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First axion results from the XENON100 experiment. / Aprile, E.; Agostini, F.; Alfonsi, M.; Arisaka, K.; Arneodo, Francesco; Auger, M.; Balan, C.; Barrow, P.; Baudis, L.; Bauermeister, B.; Behrens, A.; Beltrame, P.; Bokeloh, K.; Brown, A.; Brown, E.; Bruenner, S.; Bruno, G.; Budnik, R.; Cardoso, J. M.R.; Colijn, A. P.; Contreras, H.; Cussonneau, J. P.; Decowski, M. P.; Duchovni, E.; Fattori, S.; Ferella, A. D.; Fulgione, W.; Gao, F.; Garbini, M.; Geis, C.; Goetzke, L. W.; Grignon, C.; Gross, E.; Hampel, W.; Itay, R.; Kaether, F.; Kessler, G.; Kish, A.; Landsman, H.; Lang, R. F.; Le Calloch, M.; Lellouch, D.; Levy, C.; Lindemann, S.; Lindner, M.; Lopes, J. A.M.; Lung, K.; Lyashenko, A.; Macmullin, S.; Marrodán Undagoitia, T.; Masbou, J.; Massoli, F. V.; Mayani Paras, D.; Melgarejo Fernandez, A. J.; Meng, Y.; Messina, M.; Miguez, B.; Molinario, A.; Murra, M.; Naganoma, J.; Ni, K.; Oberlack, U.; Orrigo, S. E.A.; Pantic, E.; Persiani, R.; Piastra, F.; Pienaar, J.; Plante, G.; Priel, N.; Reichard, S.; Reuter, C.; Rizzo, A.; Rosendahl, S.; Dos Santos, J. M.F.; Sartorelli, G.; Schindler, S.; Schreiner, J.; Schumann, M.; Scotto Lavina, L.; Selvi, M.; Shagin, P.; Simgen, H.; Teymourian, A.; Thers, D.; Tiseni, A.; Trinchero, G.; Vitells, O.; Wang, H.; Weber, M.; Weinheimer, C.

In: Physical Review D - Particles, Fields, Gravitation and Cosmology, Vol. 90, No. 6, 062009, 09.09.2014.

Research output: Contribution to journalArticle

Aprile, E, Agostini, F, Alfonsi, M, Arisaka, K, Arneodo, F, Auger, M, Balan, C, Barrow, P, Baudis, L, Bauermeister, B, Behrens, A, Beltrame, P, Bokeloh, K, Brown, A, Brown, E, Bruenner, S, Bruno, G, Budnik, R, Cardoso, JMR, Colijn, AP, Contreras, H, Cussonneau, JP, Decowski, MP, Duchovni, E, Fattori, S, Ferella, AD, Fulgione, W, Gao, F, Garbini, M, Geis, C, Goetzke, LW, Grignon, C, Gross, E, Hampel, W, Itay, R, Kaether, F, Kessler, G, Kish, A, Landsman, H, Lang, RF, Le Calloch, M, Lellouch, D, Levy, C, Lindemann, S, Lindner, M, Lopes, JAM, Lung, K, Lyashenko, A, Macmullin, S, Marrodán Undagoitia, T, Masbou, J, Massoli, FV, Mayani Paras, D, Melgarejo Fernandez, AJ, Meng, Y, Messina, M, Miguez, B, Molinario, A, Murra, M, Naganoma, J, Ni, K, Oberlack, U, Orrigo, SEA, Pantic, E, Persiani, R, Piastra, F, Pienaar, J, Plante, G, Priel, N, Reichard, S, Reuter, C, Rizzo, A, Rosendahl, S, Dos Santos, JMF, Sartorelli, G, Schindler, S, Schreiner, J, Schumann, M, Scotto Lavina, L, Selvi, M, Shagin, P, Simgen, H, Teymourian, A, Thers, D, Tiseni, A, Trinchero, G, Vitells, O, Wang, H, Weber, M & Weinheimer, C 2014, 'First axion results from the XENON100 experiment', Physical Review D - Particles, Fields, Gravitation and Cosmology, vol. 90, no. 6, 062009. https://doi.org/10.1103/PhysRevD.90.062009
Aprile, E. ; Agostini, F. ; Alfonsi, M. ; Arisaka, K. ; Arneodo, Francesco ; Auger, M. ; Balan, C. ; Barrow, P. ; Baudis, L. ; Bauermeister, B. ; Behrens, A. ; Beltrame, P. ; Bokeloh, K. ; Brown, A. ; Brown, E. ; Bruenner, S. ; Bruno, G. ; Budnik, R. ; Cardoso, J. M.R. ; Colijn, A. P. ; Contreras, H. ; Cussonneau, J. P. ; Decowski, M. P. ; Duchovni, E. ; Fattori, S. ; Ferella, A. D. ; Fulgione, W. ; Gao, F. ; Garbini, M. ; Geis, C. ; Goetzke, L. W. ; Grignon, C. ; Gross, E. ; Hampel, W. ; Itay, R. ; Kaether, F. ; Kessler, G. ; Kish, A. ; Landsman, H. ; Lang, R. F. ; Le Calloch, M. ; Lellouch, D. ; Levy, C. ; Lindemann, S. ; Lindner, M. ; Lopes, J. A.M. ; Lung, K. ; Lyashenko, A. ; Macmullin, S. ; Marrodán Undagoitia, T. ; Masbou, J. ; Massoli, F. V. ; Mayani Paras, D. ; Melgarejo Fernandez, A. J. ; Meng, Y. ; Messina, M. ; Miguez, B. ; Molinario, A. ; Murra, M. ; Naganoma, J. ; Ni, K. ; Oberlack, U. ; Orrigo, S. E.A. ; Pantic, E. ; Persiani, R. ; Piastra, F. ; Pienaar, J. ; Plante, G. ; Priel, N. ; Reichard, S. ; Reuter, C. ; Rizzo, A. ; Rosendahl, S. ; Dos Santos, J. M.F. ; Sartorelli, G. ; Schindler, S. ; Schreiner, J. ; Schumann, M. ; Scotto Lavina, L. ; Selvi, M. ; Shagin, P. ; Simgen, H. ; Teymourian, A. ; Thers, D. ; Tiseni, A. ; Trinchero, G. ; Vitells, O. ; Wang, H. ; Weber, M. ; Weinheimer, C. / First axion results from the XENON100 experiment. In: Physical Review D - Particles, Fields, Gravitation and Cosmology. 2014 ; Vol. 90, No. 6.
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abstract = "We present the first results of searches for axions and axionlike particles with the XENON100 experiment. The axion-electron coupling constant, gAe, has been probed by exploiting the axioelectric effect in liquid xenon. A profile likelihood analysis of 224.6 live days × 34-kg exposure has shown no evidence for a signal. By rejecting gAe larger than 7.7×10-12 (90{\%} C.L.) in the solar axion search, we set the best limit to date on this coupling. In the frame of the DFSZ and KSVZ models, we exclude QCD axions heavier than 0.3 and 80eV/c2, respectively. For axionlike particles, under the assumption that they constitute the whole abundance of dark matter in our galaxy, we constrain gAe to be lower than 1×10-12 (90{\%} C.L.) for masses between 5 and 10keV/c2.",
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TY - JOUR

T1 - First axion results from the XENON100 experiment

AU - Aprile, E.

AU - Agostini, F.

AU - Alfonsi, M.

AU - Arisaka, K.

AU - Arneodo, Francesco

AU - Auger, M.

AU - Balan, C.

AU - Barrow, P.

AU - Baudis, L.

AU - Bauermeister, B.

AU - Behrens, A.

AU - Beltrame, P.

AU - Bokeloh, K.

AU - Brown, A.

AU - Brown, E.

AU - Bruenner, S.

AU - Bruno, G.

AU - Budnik, R.

AU - Cardoso, J. M.R.

AU - Colijn, A. P.

AU - Contreras, H.

AU - Cussonneau, J. P.

AU - Decowski, M. P.

AU - Duchovni, E.

AU - Fattori, S.

AU - Ferella, A. D.

AU - Fulgione, W.

AU - Gao, F.

AU - Garbini, M.

AU - Geis, C.

AU - Goetzke, L. W.

AU - Grignon, C.

AU - Gross, E.

AU - Hampel, W.

AU - Itay, R.

AU - Kaether, F.

AU - Kessler, G.

AU - Kish, A.

AU - Landsman, H.

AU - Lang, R. F.

AU - Le Calloch, M.

AU - Lellouch, D.

AU - Levy, C.

AU - Lindemann, S.

AU - Lindner, M.

AU - Lopes, J. A.M.

AU - Lung, K.

AU - Lyashenko, A.

AU - Macmullin, S.

AU - Marrodán Undagoitia, T.

AU - Masbou, J.

AU - Massoli, F. V.

AU - Mayani Paras, D.

AU - Melgarejo Fernandez, A. J.

AU - Meng, Y.

AU - Messina, M.

AU - Miguez, B.

AU - Molinario, A.

AU - Murra, M.

AU - Naganoma, J.

AU - Ni, K.

AU - Oberlack, U.

AU - Orrigo, S. E.A.

AU - Pantic, E.

AU - Persiani, R.

AU - Piastra, F.

AU - Pienaar, J.

AU - Plante, G.

AU - Priel, N.

AU - Reichard, S.

AU - Reuter, C.

AU - Rizzo, A.

AU - Rosendahl, S.

AU - Dos Santos, J. M.F.

AU - Sartorelli, G.

AU - Schindler, S.

AU - Schreiner, J.

AU - Schumann, M.

AU - Scotto Lavina, L.

AU - Selvi, M.

AU - Shagin, P.

AU - Simgen, H.

AU - Teymourian, A.

AU - Thers, D.

AU - Tiseni, A.

AU - Trinchero, G.

AU - Vitells, O.

AU - Wang, H.

AU - Weber, M.

AU - Weinheimer, C.

PY - 2014/9/9

Y1 - 2014/9/9

N2 - We present the first results of searches for axions and axionlike particles with the XENON100 experiment. The axion-electron coupling constant, gAe, has been probed by exploiting the axioelectric effect in liquid xenon. A profile likelihood analysis of 224.6 live days × 34-kg exposure has shown no evidence for a signal. By rejecting gAe larger than 7.7×10-12 (90% C.L.) in the solar axion search, we set the best limit to date on this coupling. In the frame of the DFSZ and KSVZ models, we exclude QCD axions heavier than 0.3 and 80eV/c2, respectively. For axionlike particles, under the assumption that they constitute the whole abundance of dark matter in our galaxy, we constrain gAe to be lower than 1×10-12 (90% C.L.) for masses between 5 and 10keV/c2.

AB - We present the first results of searches for axions and axionlike particles with the XENON100 experiment. The axion-electron coupling constant, gAe, has been probed by exploiting the axioelectric effect in liquid xenon. A profile likelihood analysis of 224.6 live days × 34-kg exposure has shown no evidence for a signal. By rejecting gAe larger than 7.7×10-12 (90% C.L.) in the solar axion search, we set the best limit to date on this coupling. In the frame of the DFSZ and KSVZ models, we exclude QCD axions heavier than 0.3 and 80eV/c2, respectively. For axionlike particles, under the assumption that they constitute the whole abundance of dark matter in our galaxy, we constrain gAe to be lower than 1×10-12 (90% C.L.) for masses between 5 and 10keV/c2.

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