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In our paper, we presented searches for solar axions and galactic axionlike particles (ALPs) in the data collected by the XENON100 experiment (with an exposure of 224.6 days). We recently found a bug in the code to calculate the exclusion limit for galactic ALPs. This resulted in an underestimation of the ALP expected rate, which in turn led to an overly conservative limit, compared to what it should really be. We corrected the code, and the result of the XENON100 90% C.L. exclusion limit on galactic ALPs (shown in Fig. 1) was reevaluated. The corrected limit is stronger than the one previously published by approximately a factor of 5 across all masses and sets the best published limit on the axion-electron coupling, gAe, in the ð1–40Þ keV=c2 mass range.

Erratum: First axion results from the XENON100 experiment [Phys. Rev. D 90, 062009 (2014)] / 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, 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. - ISSN 2470-0010. - ELETTRONICO. - 95:2(2017), pp. 029904(E).1-029904(E).1. [10.1103/PhysRevD.95.029904]

Erratum: First axion results from the XENON100 experiment [Phys. Rev. D 90, 062009 (2014)]

Garbini, M.;SARTORELLI, GABRIELLA;SELVI, MARCO;
2017

Abstract

In our paper, we presented searches for solar axions and galactic axionlike particles (ALPs) in the data collected by the XENON100 experiment (with an exposure of 224.6 days). We recently found a bug in the code to calculate the exclusion limit for galactic ALPs. This resulted in an underestimation of the ALP expected rate, which in turn led to an overly conservative limit, compared to what it should really be. We corrected the code, and the result of the XENON100 90% C.L. exclusion limit on galactic ALPs (shown in Fig. 1) was reevaluated. The corrected limit is stronger than the one previously published by approximately a factor of 5 across all masses and sets the best published limit on the axion-electron coupling, gAe, in the ð1–40Þ keV=c2 mass range.
2017
Erratum: First axion results from the XENON100 experiment [Phys. Rev. D 90, 062009 (2014)] / 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, 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. - ISSN 2470-0010. - ELETTRONICO. - 95:2(2017), pp. 029904(E).1-029904(E).1. [10.1103/PhysRevD.95.029904]
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, 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.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/599419
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