Search for non-standard neutrino interactions with 10 years of ANTARES data
Abstract Non-standard interactions of neutrinos arising in many theories beyond the Standard Model can significantly alter matter effects in atmospheric neutrino propagation through the Earth. In this paper, a search for deviations from the prediction of the standard 3-flavour atmospheric neutrino o...
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Gespeichert in:
| Autor*in: |
Albert, A. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2022 |
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| Schlagwörter: |
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| Anmerkung: |
© The Author(s) 2022 |
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| Übergeordnetes Werk: |
Enthalten in: Journal of high energy physics - Berlin : Springer, 1997, 2022(2022), 7 vom: 08. Juli |
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| Übergeordnetes Werk: |
volume:2022 ; year:2022 ; number:7 ; day:08 ; month:07 |
| Links: |
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| DOI / URN: |
10.1007/JHEP07(2022)048 |
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| Katalog-ID: |
SPR047540214 |
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| 100 | 1 | |a Albert, A. |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a Search for non-standard neutrino interactions with 10 years of ANTARES data |
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| 520 | |a Abstract Non-standard interactions of neutrinos arising in many theories beyond the Standard Model can significantly alter matter effects in atmospheric neutrino propagation through the Earth. In this paper, a search for deviations from the prediction of the standard 3-flavour atmospheric neutrino oscillations using the data taken by the ANTARES neutrino telescope is presented. Ten years of atmospheric neutrino data collected from 2007 to 2016, with reconstructed energies in the range from ∼16 GeV to 100 GeV, have been analysed. A log-likelihood ratio test of the dimensionless coefficients εμτ and εττ − εμμ does not provide clear evidence of deviations from standard interactions. For normal neutrino mass ordering, the combined fit of both coefficients yields a value 1.7σ away from the null result. However, the 68% and 95% confidence level intervals for εμτ and εττ − εμμ, respectively, contain the null value. Best fit values, one standard deviation errors and bounds at the 90% confidence level for these coefficients are given for both normal and inverted mass orderings. The constraint on εμτ is among the most stringent to date and it further restrains the strength of possible non-standard interactions in the μ − τ sector. | ||
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10.1007/JHEP07(2022)048 doi (DE-627)SPR047540214 (SPR)JHEP07(2022)048-e DE-627 ger DE-627 rakwb eng Albert, A. verfasserin aut Search for non-standard neutrino interactions with 10 years of ANTARES data 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2022 Abstract Non-standard interactions of neutrinos arising in many theories beyond the Standard Model can significantly alter matter effects in atmospheric neutrino propagation through the Earth. In this paper, a search for deviations from the prediction of the standard 3-flavour atmospheric neutrino oscillations using the data taken by the ANTARES neutrino telescope is presented. Ten years of atmospheric neutrino data collected from 2007 to 2016, with reconstructed energies in the range from ∼16 GeV to 100 GeV, have been analysed. A log-likelihood ratio test of the dimensionless coefficients εμτ and εττ − εμμ does not provide clear evidence of deviations from standard interactions. For normal neutrino mass ordering, the combined fit of both coefficients yields a value 1.7σ away from the null result. However, the 68% and 95% confidence level intervals for εμτ and εττ − εμμ, respectively, contain the null value. Best fit values, one standard deviation errors and bounds at the 90% confidence level for these coefficients are given for both normal and inverted mass orderings. The constraint on εμτ is among the most stringent to date and it further restrains the strength of possible non-standard interactions in the μ − τ sector. Neutrino Detectors and Telescopes (experiments) (dpeaa)DE-He213 Alves, S. aut André, M. aut Anghinolfi, M. aut Anton, G. aut Ardid, M. aut Ardid, S. aut Aubert, J.-J. aut Aublin, J. aut Baret, B. aut Basa, S. aut Belhorma, B. aut Bendahman, M. aut Benfenati, F. aut Bertin, V. aut Biagi, S. aut Bissinger, M. aut Boumaaza, J. aut Bouta, M. aut Bouwhuis, M. C. aut Brânzaş, H. aut Bruijn, R. aut Brunner, J. aut Busto, J. aut Caiffi, B. aut Calvo, D. aut Capone, A. aut Caramete, L. aut Carr, J. aut Carretero, V. aut Celli, S. aut Chabab, M. aut Chau, T. N. aut Cherkaoui El Moursli, R. aut Chiarusi, T. aut Circella, M. aut Coleiro, A. aut Coniglione, R. aut Coyle, P. aut Creusot, A. aut Díaz, A. F. aut de Wasseige, G. aut Distefano, C. aut Di Palma, I. aut Domi, A. aut Donzaud, C. aut Dornic, D. aut Drouhin, D. aut Eberl, T. aut van Eeden, T. aut van Eijk, D. aut El Khayati, N. aut Enzenhöfer, A. aut Fermani, P. aut Ferrara, G. aut Filippini, F. aut Fusco, L. aut Gatelet, Y. aut Gay, P. aut Glotin, H. aut Gozzini, R. aut Gracia Ruiz, R. aut Graf, K. aut Guidi, C. aut Hallmann, S. aut van Haren, H. aut Heijboer, A. J. aut Hello, Y. aut Hernández-Rey, J. J. aut Hößl, J. aut Hofestädt, J. aut Huang, F. aut Illuminati, G. aut James, C. W. aut Jisse-Jung, B. aut de Jong, M. aut de Jong, P. aut Kadler, M. aut Kalekin, O. aut Katz, U. aut Khan-Chowdhury, N. R. aut Kouchner, A. aut Kreykenbohm, I. aut Kulikovskiy, V. aut Lahmann, R. aut Le Breton, R. aut LeStum, S. aut Lefèvre, D. aut Leonora, E. aut Levi, G. aut Lincetto, M. aut Lopez-Coto, D. aut Loucatos, S. aut Maderer, L. aut Manczak, J. aut Marcelin, M. aut Margiotta, A. aut Marinelli, A. aut Martínez-Mora, J. A. aut Martino, B. aut Melis, K. aut Migliozzi, P. aut Moussa, A. aut Muller, R. aut Nauta, L. aut Navas, S. aut Nezri, E. aut Fearraigh, B. Ó aut Păun, A. aut Păvălaş, G. E. aut Pellegrino, C. aut Perrin-Terrin, M. aut Pestel, V. aut Piattelli, P. aut Pieterse, C. aut Poirè, C. aut Popa, V. aut Pradier, T. aut Randazzo, N. aut Real, D. aut Reck, S. aut Riccobene, G. aut Romanov, A. aut Sánchez-Losa, A. aut Salesa Greus, F. aut Samtleben, D. F. E. aut Sanguineti, M. aut Sapienza, P. aut Schnabel, J. aut Schumann, J. aut Schüssler, F. aut Seneca, J. aut Spurio, M. aut Stolarczyk, Th. aut Taiuti, M. aut Tayalati, Y. aut Thakore, T. aut Tingay, S. J. aut Vallage, B. aut Van Elewyck, V. aut Versari, F. aut Viola, S. aut Vivolo, D. aut Wilms, J. aut Zavatarelli, S. aut Zegarelli, A. aut Zornoza, J. D. aut Zúñiga, J. aut Enthalten in Journal of high energy physics Berlin : Springer, 1997 2022(2022), 7 vom: 08. Juli (DE-627)320910571 (DE-600)2027350-2 1029-8479 nnns volume:2022 year:2022 number:7 day:08 month:07 https://dx.doi.org/10.1007/JHEP07(2022)048 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_2020 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 2022 2022 7 08 07 |
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10.1007/JHEP07(2022)048 doi (DE-627)SPR047540214 (SPR)JHEP07(2022)048-e DE-627 ger DE-627 rakwb eng Albert, A. verfasserin aut Search for non-standard neutrino interactions with 10 years of ANTARES data 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2022 Abstract Non-standard interactions of neutrinos arising in many theories beyond the Standard Model can significantly alter matter effects in atmospheric neutrino propagation through the Earth. In this paper, a search for deviations from the prediction of the standard 3-flavour atmospheric neutrino oscillations using the data taken by the ANTARES neutrino telescope is presented. Ten years of atmospheric neutrino data collected from 2007 to 2016, with reconstructed energies in the range from ∼16 GeV to 100 GeV, have been analysed. A log-likelihood ratio test of the dimensionless coefficients εμτ and εττ − εμμ does not provide clear evidence of deviations from standard interactions. For normal neutrino mass ordering, the combined fit of both coefficients yields a value 1.7σ away from the null result. However, the 68% and 95% confidence level intervals for εμτ and εττ − εμμ, respectively, contain the null value. Best fit values, one standard deviation errors and bounds at the 90% confidence level for these coefficients are given for both normal and inverted mass orderings. The constraint on εμτ is among the most stringent to date and it further restrains the strength of possible non-standard interactions in the μ − τ sector. Neutrino Detectors and Telescopes (experiments) (dpeaa)DE-He213 Alves, S. aut André, M. aut Anghinolfi, M. aut Anton, G. aut Ardid, M. aut Ardid, S. aut Aubert, J.-J. aut Aublin, J. aut Baret, B. aut Basa, S. aut Belhorma, B. aut Bendahman, M. aut Benfenati, F. aut Bertin, V. aut Biagi, S. aut Bissinger, M. aut Boumaaza, J. aut Bouta, M. aut Bouwhuis, M. C. aut Brânzaş, H. aut Bruijn, R. aut Brunner, J. aut Busto, J. aut Caiffi, B. aut Calvo, D. aut Capone, A. aut Caramete, L. aut Carr, J. aut Carretero, V. aut Celli, S. aut Chabab, M. aut Chau, T. N. aut Cherkaoui El Moursli, R. aut Chiarusi, T. aut Circella, M. aut Coleiro, A. aut Coniglione, R. aut Coyle, P. aut Creusot, A. aut Díaz, A. F. aut de Wasseige, G. aut Distefano, C. aut Di Palma, I. aut Domi, A. aut Donzaud, C. aut Dornic, D. aut Drouhin, D. aut Eberl, T. aut van Eeden, T. aut van Eijk, D. aut El Khayati, N. aut Enzenhöfer, A. aut Fermani, P. aut Ferrara, G. aut Filippini, F. aut Fusco, L. aut Gatelet, Y. aut Gay, P. aut Glotin, H. aut Gozzini, R. aut Gracia Ruiz, R. aut Graf, K. aut Guidi, C. aut Hallmann, S. aut van Haren, H. aut Heijboer, A. J. aut Hello, Y. aut Hernández-Rey, J. J. aut Hößl, J. aut Hofestädt, J. aut Huang, F. aut Illuminati, G. aut James, C. W. aut Jisse-Jung, B. aut de Jong, M. aut de Jong, P. aut Kadler, M. aut Kalekin, O. aut Katz, U. aut Khan-Chowdhury, N. R. aut Kouchner, A. aut Kreykenbohm, I. aut Kulikovskiy, V. aut Lahmann, R. aut Le Breton, R. aut LeStum, S. aut Lefèvre, D. aut Leonora, E. aut Levi, G. aut Lincetto, M. aut Lopez-Coto, D. aut Loucatos, S. aut Maderer, L. aut Manczak, J. aut Marcelin, M. aut Margiotta, A. aut Marinelli, A. aut Martínez-Mora, J. A. aut Martino, B. aut Melis, K. aut Migliozzi, P. aut Moussa, A. aut Muller, R. aut Nauta, L. aut Navas, S. aut Nezri, E. aut Fearraigh, B. Ó aut Păun, A. aut Păvălaş, G. E. aut Pellegrino, C. aut Perrin-Terrin, M. aut Pestel, V. aut Piattelli, P. aut Pieterse, C. aut Poirè, C. aut Popa, V. aut Pradier, T. aut Randazzo, N. aut Real, D. aut Reck, S. aut Riccobene, G. aut Romanov, A. aut Sánchez-Losa, A. aut Salesa Greus, F. aut Samtleben, D. F. E. aut Sanguineti, M. aut Sapienza, P. aut Schnabel, J. aut Schumann, J. aut Schüssler, F. aut Seneca, J. aut Spurio, M. aut Stolarczyk, Th. aut Taiuti, M. aut Tayalati, Y. aut Thakore, T. aut Tingay, S. J. aut Vallage, B. aut Van Elewyck, V. aut Versari, F. aut Viola, S. aut Vivolo, D. aut Wilms, J. aut Zavatarelli, S. aut Zegarelli, A. aut Zornoza, J. D. aut Zúñiga, J. aut Enthalten in Journal of high energy physics Berlin : Springer, 1997 2022(2022), 7 vom: 08. Juli (DE-627)320910571 (DE-600)2027350-2 1029-8479 nnns volume:2022 year:2022 number:7 day:08 month:07 https://dx.doi.org/10.1007/JHEP07(2022)048 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_2020 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 2022 2022 7 08 07 |
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10.1007/JHEP07(2022)048 doi (DE-627)SPR047540214 (SPR)JHEP07(2022)048-e DE-627 ger DE-627 rakwb eng Albert, A. verfasserin aut Search for non-standard neutrino interactions with 10 years of ANTARES data 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2022 Abstract Non-standard interactions of neutrinos arising in many theories beyond the Standard Model can significantly alter matter effects in atmospheric neutrino propagation through the Earth. In this paper, a search for deviations from the prediction of the standard 3-flavour atmospheric neutrino oscillations using the data taken by the ANTARES neutrino telescope is presented. Ten years of atmospheric neutrino data collected from 2007 to 2016, with reconstructed energies in the range from ∼16 GeV to 100 GeV, have been analysed. A log-likelihood ratio test of the dimensionless coefficients εμτ and εττ − εμμ does not provide clear evidence of deviations from standard interactions. For normal neutrino mass ordering, the combined fit of both coefficients yields a value 1.7σ away from the null result. However, the 68% and 95% confidence level intervals for εμτ and εττ − εμμ, respectively, contain the null value. Best fit values, one standard deviation errors and bounds at the 90% confidence level for these coefficients are given for both normal and inverted mass orderings. The constraint on εμτ is among the most stringent to date and it further restrains the strength of possible non-standard interactions in the μ − τ sector. Neutrino Detectors and Telescopes (experiments) (dpeaa)DE-He213 Alves, S. aut André, M. aut Anghinolfi, M. aut Anton, G. aut Ardid, M. aut Ardid, S. aut Aubert, J.-J. aut Aublin, J. aut Baret, B. aut Basa, S. aut Belhorma, B. aut Bendahman, M. aut Benfenati, F. aut Bertin, V. aut Biagi, S. aut Bissinger, M. aut Boumaaza, J. aut Bouta, M. aut Bouwhuis, M. C. aut Brânzaş, H. aut Bruijn, R. aut Brunner, J. aut Busto, J. aut Caiffi, B. aut Calvo, D. aut Capone, A. aut Caramete, L. aut Carr, J. aut Carretero, V. aut Celli, S. aut Chabab, M. aut Chau, T. N. aut Cherkaoui El Moursli, R. aut Chiarusi, T. aut Circella, M. aut Coleiro, A. aut Coniglione, R. aut Coyle, P. aut Creusot, A. aut Díaz, A. F. aut de Wasseige, G. aut Distefano, C. aut Di Palma, I. aut Domi, A. aut Donzaud, C. aut Dornic, D. aut Drouhin, D. aut Eberl, T. aut van Eeden, T. aut van Eijk, D. aut El Khayati, N. aut Enzenhöfer, A. aut Fermani, P. aut Ferrara, G. aut Filippini, F. aut Fusco, L. aut Gatelet, Y. aut Gay, P. aut Glotin, H. aut Gozzini, R. aut Gracia Ruiz, R. aut Graf, K. aut Guidi, C. aut Hallmann, S. aut van Haren, H. aut Heijboer, A. J. aut Hello, Y. aut Hernández-Rey, J. J. aut Hößl, J. aut Hofestädt, J. aut Huang, F. aut Illuminati, G. aut James, C. W. aut Jisse-Jung, B. aut de Jong, M. aut de Jong, P. aut Kadler, M. aut Kalekin, O. aut Katz, U. aut Khan-Chowdhury, N. R. aut Kouchner, A. aut Kreykenbohm, I. aut Kulikovskiy, V. aut Lahmann, R. aut Le Breton, R. aut LeStum, S. aut Lefèvre, D. aut Leonora, E. aut Levi, G. aut Lincetto, M. aut Lopez-Coto, D. aut Loucatos, S. aut Maderer, L. aut Manczak, J. aut Marcelin, M. aut Margiotta, A. aut Marinelli, A. aut Martínez-Mora, J. A. aut Martino, B. aut Melis, K. aut Migliozzi, P. aut Moussa, A. aut Muller, R. aut Nauta, L. aut Navas, S. aut Nezri, E. aut Fearraigh, B. Ó aut Păun, A. aut Păvălaş, G. E. aut Pellegrino, C. aut Perrin-Terrin, M. aut Pestel, V. aut Piattelli, P. aut Pieterse, C. aut Poirè, C. aut Popa, V. aut Pradier, T. aut Randazzo, N. aut Real, D. aut Reck, S. aut Riccobene, G. aut Romanov, A. aut Sánchez-Losa, A. aut Salesa Greus, F. aut Samtleben, D. F. E. aut Sanguineti, M. aut Sapienza, P. aut Schnabel, J. aut Schumann, J. aut Schüssler, F. aut Seneca, J. aut Spurio, M. aut Stolarczyk, Th. aut Taiuti, M. aut Tayalati, Y. aut Thakore, T. aut Tingay, S. J. aut Vallage, B. aut Van Elewyck, V. aut Versari, F. aut Viola, S. aut Vivolo, D. aut Wilms, J. aut Zavatarelli, S. aut Zegarelli, A. aut Zornoza, J. D. aut Zúñiga, J. aut Enthalten in Journal of high energy physics Berlin : Springer, 1997 2022(2022), 7 vom: 08. Juli (DE-627)320910571 (DE-600)2027350-2 1029-8479 nnns volume:2022 year:2022 number:7 day:08 month:07 https://dx.doi.org/10.1007/JHEP07(2022)048 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_2020 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 2022 2022 7 08 07 |
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10.1007/JHEP07(2022)048 doi (DE-627)SPR047540214 (SPR)JHEP07(2022)048-e DE-627 ger DE-627 rakwb eng Albert, A. verfasserin aut Search for non-standard neutrino interactions with 10 years of ANTARES data 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2022 Abstract Non-standard interactions of neutrinos arising in many theories beyond the Standard Model can significantly alter matter effects in atmospheric neutrino propagation through the Earth. In this paper, a search for deviations from the prediction of the standard 3-flavour atmospheric neutrino oscillations using the data taken by the ANTARES neutrino telescope is presented. Ten years of atmospheric neutrino data collected from 2007 to 2016, with reconstructed energies in the range from ∼16 GeV to 100 GeV, have been analysed. A log-likelihood ratio test of the dimensionless coefficients εμτ and εττ − εμμ does not provide clear evidence of deviations from standard interactions. For normal neutrino mass ordering, the combined fit of both coefficients yields a value 1.7σ away from the null result. However, the 68% and 95% confidence level intervals for εμτ and εττ − εμμ, respectively, contain the null value. Best fit values, one standard deviation errors and bounds at the 90% confidence level for these coefficients are given for both normal and inverted mass orderings. The constraint on εμτ is among the most stringent to date and it further restrains the strength of possible non-standard interactions in the μ − τ sector. Neutrino Detectors and Telescopes (experiments) (dpeaa)DE-He213 Alves, S. aut André, M. aut Anghinolfi, M. aut Anton, G. aut Ardid, M. aut Ardid, S. aut Aubert, J.-J. aut Aublin, J. aut Baret, B. aut Basa, S. aut Belhorma, B. aut Bendahman, M. aut Benfenati, F. aut Bertin, V. aut Biagi, S. aut Bissinger, M. aut Boumaaza, J. aut Bouta, M. aut Bouwhuis, M. C. aut Brânzaş, H. aut Bruijn, R. aut Brunner, J. aut Busto, J. aut Caiffi, B. aut Calvo, D. aut Capone, A. aut Caramete, L. aut Carr, J. aut Carretero, V. aut Celli, S. aut Chabab, M. aut Chau, T. N. aut Cherkaoui El Moursli, R. aut Chiarusi, T. aut Circella, M. aut Coleiro, A. aut Coniglione, R. aut Coyle, P. aut Creusot, A. aut Díaz, A. F. aut de Wasseige, G. aut Distefano, C. aut Di Palma, I. aut Domi, A. aut Donzaud, C. aut Dornic, D. aut Drouhin, D. aut Eberl, T. aut van Eeden, T. aut van Eijk, D. aut El Khayati, N. aut Enzenhöfer, A. aut Fermani, P. aut Ferrara, G. aut Filippini, F. aut Fusco, L. aut Gatelet, Y. aut Gay, P. aut Glotin, H. aut Gozzini, R. aut Gracia Ruiz, R. aut Graf, K. aut Guidi, C. aut Hallmann, S. aut van Haren, H. aut Heijboer, A. J. aut Hello, Y. aut Hernández-Rey, J. J. aut Hößl, J. aut Hofestädt, J. aut Huang, F. aut Illuminati, G. aut James, C. W. aut Jisse-Jung, B. aut de Jong, M. aut de Jong, P. aut Kadler, M. aut Kalekin, O. aut Katz, U. aut Khan-Chowdhury, N. R. aut Kouchner, A. aut Kreykenbohm, I. aut Kulikovskiy, V. aut Lahmann, R. aut Le Breton, R. aut LeStum, S. aut Lefèvre, D. aut Leonora, E. aut Levi, G. aut Lincetto, M. aut Lopez-Coto, D. aut Loucatos, S. aut Maderer, L. aut Manczak, J. aut Marcelin, M. aut Margiotta, A. aut Marinelli, A. aut Martínez-Mora, J. A. aut Martino, B. aut Melis, K. aut Migliozzi, P. aut Moussa, A. aut Muller, R. aut Nauta, L. aut Navas, S. aut Nezri, E. aut Fearraigh, B. Ó aut Păun, A. aut Păvălaş, G. E. aut Pellegrino, C. aut Perrin-Terrin, M. aut Pestel, V. aut Piattelli, P. aut Pieterse, C. aut Poirè, C. aut Popa, V. aut Pradier, T. aut Randazzo, N. aut Real, D. aut Reck, S. aut Riccobene, G. aut Romanov, A. aut Sánchez-Losa, A. aut Salesa Greus, F. aut Samtleben, D. F. E. aut Sanguineti, M. aut Sapienza, P. aut Schnabel, J. aut Schumann, J. aut Schüssler, F. aut Seneca, J. aut Spurio, M. aut Stolarczyk, Th. aut Taiuti, M. aut Tayalati, Y. aut Thakore, T. aut Tingay, S. J. aut Vallage, B. aut Van Elewyck, V. aut Versari, F. aut Viola, S. aut Vivolo, D. aut Wilms, J. aut Zavatarelli, S. aut Zegarelli, A. aut Zornoza, J. D. aut Zúñiga, J. aut Enthalten in Journal of high energy physics Berlin : Springer, 1997 2022(2022), 7 vom: 08. Juli (DE-627)320910571 (DE-600)2027350-2 1029-8479 nnns volume:2022 year:2022 number:7 day:08 month:07 https://dx.doi.org/10.1007/JHEP07(2022)048 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_2020 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 2022 2022 7 08 07 |
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10.1007/JHEP07(2022)048 doi (DE-627)SPR047540214 (SPR)JHEP07(2022)048-e DE-627 ger DE-627 rakwb eng Albert, A. verfasserin aut Search for non-standard neutrino interactions with 10 years of ANTARES data 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2022 Abstract Non-standard interactions of neutrinos arising in many theories beyond the Standard Model can significantly alter matter effects in atmospheric neutrino propagation through the Earth. In this paper, a search for deviations from the prediction of the standard 3-flavour atmospheric neutrino oscillations using the data taken by the ANTARES neutrino telescope is presented. Ten years of atmospheric neutrino data collected from 2007 to 2016, with reconstructed energies in the range from ∼16 GeV to 100 GeV, have been analysed. A log-likelihood ratio test of the dimensionless coefficients εμτ and εττ − εμμ does not provide clear evidence of deviations from standard interactions. For normal neutrino mass ordering, the combined fit of both coefficients yields a value 1.7σ away from the null result. However, the 68% and 95% confidence level intervals for εμτ and εττ − εμμ, respectively, contain the null value. Best fit values, one standard deviation errors and bounds at the 90% confidence level for these coefficients are given for both normal and inverted mass orderings. The constraint on εμτ is among the most stringent to date and it further restrains the strength of possible non-standard interactions in the μ − τ sector. Neutrino Detectors and Telescopes (experiments) (dpeaa)DE-He213 Alves, S. aut André, M. aut Anghinolfi, M. aut Anton, G. aut Ardid, M. aut Ardid, S. aut Aubert, J.-J. aut Aublin, J. aut Baret, B. aut Basa, S. aut Belhorma, B. aut Bendahman, M. aut Benfenati, F. aut Bertin, V. aut Biagi, S. aut Bissinger, M. aut Boumaaza, J. aut Bouta, M. aut Bouwhuis, M. C. aut Brânzaş, H. aut Bruijn, R. aut Brunner, J. aut Busto, J. aut Caiffi, B. aut Calvo, D. aut Capone, A. aut Caramete, L. aut Carr, J. aut Carretero, V. aut Celli, S. aut Chabab, M. aut Chau, T. N. aut Cherkaoui El Moursli, R. aut Chiarusi, T. aut Circella, M. aut Coleiro, A. aut Coniglione, R. aut Coyle, P. aut Creusot, A. aut Díaz, A. F. aut de Wasseige, G. aut Distefano, C. aut Di Palma, I. aut Domi, A. aut Donzaud, C. aut Dornic, D. aut Drouhin, D. aut Eberl, T. aut van Eeden, T. aut van Eijk, D. aut El Khayati, N. aut Enzenhöfer, A. aut Fermani, P. aut Ferrara, G. aut Filippini, F. aut Fusco, L. aut Gatelet, Y. aut Gay, P. aut Glotin, H. aut Gozzini, R. aut Gracia Ruiz, R. aut Graf, K. aut Guidi, C. aut Hallmann, S. aut van Haren, H. aut Heijboer, A. J. aut Hello, Y. aut Hernández-Rey, J. J. aut Hößl, J. aut Hofestädt, J. aut Huang, F. aut Illuminati, G. aut James, C. W. aut Jisse-Jung, B. aut de Jong, M. aut de Jong, P. aut Kadler, M. aut Kalekin, O. aut Katz, U. aut Khan-Chowdhury, N. R. aut Kouchner, A. aut Kreykenbohm, I. aut Kulikovskiy, V. aut Lahmann, R. aut Le Breton, R. aut LeStum, S. aut Lefèvre, D. aut Leonora, E. aut Levi, G. aut Lincetto, M. aut Lopez-Coto, D. aut Loucatos, S. aut Maderer, L. aut Manczak, J. aut Marcelin, M. aut Margiotta, A. aut Marinelli, A. aut Martínez-Mora, J. A. aut Martino, B. aut Melis, K. aut Migliozzi, P. aut Moussa, A. aut Muller, R. aut Nauta, L. aut Navas, S. aut Nezri, E. aut Fearraigh, B. Ó aut Păun, A. aut Păvălaş, G. E. aut Pellegrino, C. aut Perrin-Terrin, M. aut Pestel, V. aut Piattelli, P. aut Pieterse, C. aut Poirè, C. aut Popa, V. aut Pradier, T. aut Randazzo, N. aut Real, D. aut Reck, S. aut Riccobene, G. aut Romanov, A. aut Sánchez-Losa, A. aut Salesa Greus, F. aut Samtleben, D. F. E. aut Sanguineti, M. aut Sapienza, P. aut Schnabel, J. aut Schumann, J. aut Schüssler, F. aut Seneca, J. aut Spurio, M. aut Stolarczyk, Th. aut Taiuti, M. aut Tayalati, Y. aut Thakore, T. aut Tingay, S. J. aut Vallage, B. aut Van Elewyck, V. aut Versari, F. aut Viola, S. aut Vivolo, D. aut Wilms, J. aut Zavatarelli, S. aut Zegarelli, A. aut Zornoza, J. D. aut Zúñiga, J. aut Enthalten in Journal of high energy physics Berlin : Springer, 1997 2022(2022), 7 vom: 08. Juli (DE-627)320910571 (DE-600)2027350-2 1029-8479 nnns volume:2022 year:2022 number:7 day:08 month:07 https://dx.doi.org/10.1007/JHEP07(2022)048 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_2020 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 2022 2022 7 08 07 |
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Albert, A. Alves, S. André, M. Anghinolfi, M. Anton, G. Ardid, M. Ardid, S. Aubert, J.-J. Aublin, J. Baret, B. Basa, S. Belhorma, B. Bendahman, M. Benfenati, F. Bertin, V. Biagi, S. Bissinger, M. Boumaaza, J. Bouta, M. Bouwhuis, M. C. Brânzaş, H. Bruijn, R. Brunner, J. Busto, J. Caiffi, B. Calvo, D. Capone, A. Caramete, L. Carr, J. Carretero, V. Celli, S. Chabab, M. Chau, T. N. Cherkaoui El Moursli, R. Chiarusi, T. Circella, M. Coleiro, A. Coniglione, R. Coyle, P. Creusot, A. Díaz, A. F. de Wasseige, G. Distefano, C. Di Palma, I. Domi, A. Donzaud, C. Dornic, D. Drouhin, D. Eberl, T. van Eeden, T. van Eijk, D. El Khayati, N. Enzenhöfer, A. Fermani, P. Ferrara, G. Filippini, F. Fusco, L. Gatelet, Y. Gay, P. Glotin, H. Gozzini, R. Gracia Ruiz, R. Graf, K. Guidi, C. Hallmann, S. van Haren, H. Heijboer, A. J. Hello, Y. Hernández-Rey, J. J. Hößl, J. Hofestädt, J. Huang, F. Illuminati, G. James, C. W. Jisse-Jung, B. de Jong, M. de Jong, P. Kadler, M. Kalekin, O. Katz, U. Khan-Chowdhury, N. R. Kouchner, A. Kreykenbohm, I. Kulikovskiy, V. Lahmann, R. Le Breton, R. LeStum, S. Lefèvre, D. Leonora, E. Levi, G. Lincetto, M. Lopez-Coto, D. Loucatos, S. Maderer, L. Manczak, J. Marcelin, M. Margiotta, A. Marinelli, A. Martínez-Mora, J. A. Martino, B. Melis, K. Migliozzi, P. Moussa, A. Muller, R. Nauta, L. Navas, S. Nezri, E. Fearraigh, B. Ó Păun, A. Păvălaş, G. E. Pellegrino, C. Perrin-Terrin, M. Pestel, V. Piattelli, P. Pieterse, C. Poirè, C. Popa, V. Pradier, T. Randazzo, N. Real, D. Reck, S. Riccobene, G. Romanov, A. Sánchez-Losa, A. Salesa Greus, F. Samtleben, D. F. E. Sanguineti, M. Sapienza, P. Schnabel, J. Schumann, J. Schüssler, F. Seneca, J. Spurio, M. Stolarczyk, Th. Taiuti, M. Tayalati, Y. Thakore, T. Tingay, S. J. Vallage, B. Van Elewyck, V. Versari, F. Viola, S. Vivolo, D. Wilms, J. Zavatarelli, S. Zegarelli, A. Zornoza, J. D. Zúñiga, J. |
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search for non-standard neutrino interactions with 10 years of antares data |
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Search for non-standard neutrino interactions with 10 years of ANTARES data |
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Abstract Non-standard interactions of neutrinos arising in many theories beyond the Standard Model can significantly alter matter effects in atmospheric neutrino propagation through the Earth. In this paper, a search for deviations from the prediction of the standard 3-flavour atmospheric neutrino oscillations using the data taken by the ANTARES neutrino telescope is presented. Ten years of atmospheric neutrino data collected from 2007 to 2016, with reconstructed energies in the range from ∼16 GeV to 100 GeV, have been analysed. A log-likelihood ratio test of the dimensionless coefficients εμτ and εττ − εμμ does not provide clear evidence of deviations from standard interactions. For normal neutrino mass ordering, the combined fit of both coefficients yields a value 1.7σ away from the null result. However, the 68% and 95% confidence level intervals for εμτ and εττ − εμμ, respectively, contain the null value. Best fit values, one standard deviation errors and bounds at the 90% confidence level for these coefficients are given for both normal and inverted mass orderings. The constraint on εμτ is among the most stringent to date and it further restrains the strength of possible non-standard interactions in the μ − τ sector. © The Author(s) 2022 |
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Abstract Non-standard interactions of neutrinos arising in many theories beyond the Standard Model can significantly alter matter effects in atmospheric neutrino propagation through the Earth. In this paper, a search for deviations from the prediction of the standard 3-flavour atmospheric neutrino oscillations using the data taken by the ANTARES neutrino telescope is presented. Ten years of atmospheric neutrino data collected from 2007 to 2016, with reconstructed energies in the range from ∼16 GeV to 100 GeV, have been analysed. A log-likelihood ratio test of the dimensionless coefficients εμτ and εττ − εμμ does not provide clear evidence of deviations from standard interactions. For normal neutrino mass ordering, the combined fit of both coefficients yields a value 1.7σ away from the null result. However, the 68% and 95% confidence level intervals for εμτ and εττ − εμμ, respectively, contain the null value. Best fit values, one standard deviation errors and bounds at the 90% confidence level for these coefficients are given for both normal and inverted mass orderings. The constraint on εμτ is among the most stringent to date and it further restrains the strength of possible non-standard interactions in the μ − τ sector. © The Author(s) 2022 |
| abstract_unstemmed |
Abstract Non-standard interactions of neutrinos arising in many theories beyond the Standard Model can significantly alter matter effects in atmospheric neutrino propagation through the Earth. In this paper, a search for deviations from the prediction of the standard 3-flavour atmospheric neutrino oscillations using the data taken by the ANTARES neutrino telescope is presented. Ten years of atmospheric neutrino data collected from 2007 to 2016, with reconstructed energies in the range from ∼16 GeV to 100 GeV, have been analysed. A log-likelihood ratio test of the dimensionless coefficients εμτ and εττ − εμμ does not provide clear evidence of deviations from standard interactions. For normal neutrino mass ordering, the combined fit of both coefficients yields a value 1.7σ away from the null result. However, the 68% and 95% confidence level intervals for εμτ and εττ − εμμ, respectively, contain the null value. Best fit values, one standard deviation errors and bounds at the 90% confidence level for these coefficients are given for both normal and inverted mass orderings. The constraint on εμτ is among the most stringent to date and it further restrains the strength of possible non-standard interactions in the μ − τ sector. © The Author(s) 2022 |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">SPR047540214</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230507225833.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">220710s2022 xx |||||o 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/JHEP07(2022)048</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)SPR047540214</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(SPR)JHEP07(2022)048-e</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Albert, A.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Search for non-standard neutrino interactions with 10 years of ANTARES data</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2022</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© The Author(s) 2022</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract Non-standard interactions of neutrinos arising in many theories beyond the Standard Model can significantly alter matter effects in atmospheric neutrino propagation through the Earth. In this paper, a search for deviations from the prediction of the standard 3-flavour atmospheric neutrino oscillations using the data taken by the ANTARES neutrino telescope is presented. Ten years of atmospheric neutrino data collected from 2007 to 2016, with reconstructed energies in the range from ∼16 GeV to 100 GeV, have been analysed. A log-likelihood ratio test of the dimensionless coefficients εμτ and εττ − εμμ does not provide clear evidence of deviations from standard interactions. For normal neutrino mass ordering, the combined fit of both coefficients yields a value 1.7σ away from the null result. However, the 68% and 95% confidence level intervals for εμτ and εττ − εμμ, respectively, contain the null value. Best fit values, one standard deviation errors and bounds at the 90% confidence level for these coefficients are given for both normal and inverted mass orderings. The constraint on εμτ is among the most stringent to date and it further restrains the strength of possible non-standard interactions in the μ − τ sector.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Neutrino Detectors and Telescopes (experiments)</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Alves, S.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">André, M.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Anghinolfi, M.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Anton, G.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ardid, M.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ardid, S.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Aubert, J.-J.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Aublin, J.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Baret, B.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Basa, S.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Belhorma, B.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Bendahman, M.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Benfenati, F.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Bertin, V.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Biagi, S.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Bissinger, M.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Boumaaza, J.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Bouta, M.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Bouwhuis, M. 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