All-flavor search for a diffuse flux of cosmic neutrinos with nine years of ANTARES data
The ANTARES detector is at present the most sensitive neutrino telescope in the northern hemisphere. The highly significant cosmic neutrino excess observed by the Antarctic IceCube detector can be studied with ANTARES, exploiting its complementing field of view, exposure, and lower energy threshold....
Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
---|---|
Format: | Text |
Language: | English |
Published: |
2018
|
Subjects: | |
Online Access: | http://www.documentation.ird.fr/hor/fdi:010081634 |
id |
ftird:oai:ird.fr:fdi:010081634 |
---|---|
record_format |
openpolar |
institution |
Open Polar |
collection |
IRD (Institute de recherche pour le développement): Horizon |
op_collection_id |
ftird |
language |
English |
topic |
astroparticle physics neutrinos |
spellingShingle |
astroparticle physics neutrinos Albert, A. Andre, M. Anghinolfi, M. Anton, G. Ardid, M. Aubert, J. J. Aublin, J. Avgitas, T. Baret, B. Barrios-Marti, J. Basa, S. Belhorma, B. Bertin, V. Biagi, S. Bormuth, R. Bourret, S. Bouwhuis, M. C. Branzas, H. Bruijn, R. Brunner, J. Busto, J. Capone, A. Caramete, L. Carr, J. Celli, S. El Moursli, R. C. Chiarusi, T. Circella, M. Coelho, J. A. B. Coleiro, A. Coniglione, R. Costantini, H. Coyle, P. Creusot, A. Diaz, A. F. Deschamps, A. De Bonis, G. Distefano, C. Di Palma, I. Domi, A. Donzaud, C. Dornic, D. Drouhin, D. Eberl, T. El Bojaddaini, I. El Khayati, N. Elsasser, D. Enzenhofer, A. Ettahiri, A. Fassi, F. Felis, I. Fusco, L. A. Gay, P. Giordano, V. Glotin, H. Gregoire, T. Ruiz, R. G. Graf, K. Hallmann, S. van Haren, H. Heijboer, A. J. Hello, Yann Hernandez-Rey, J. J. Hossl, J. Hofestadt, J. Illuminati, G. James, C. W. de Jong, M. Jongen, M. Kadler, M. Kalekin, O. Katz, U. Kiessling, D. Kouchner, A. Kreter, M. Kreykenbohm, I. Kulikovskiy, V. Lachaud, C. Lahmann, R. Lefevre, D. Leonora, E. Lotze, M. Loucatos, S. Marcelin, M. Margiotta, A. Marinelli, A. Martinez-Mora, J. A. Mele, R. Melis, K. Michael, T. Migliozzi, P. Moussa, A. Navas, S. Nezri, E. Organokov, M. Pavalas, G. E. Pellegrino, C. Perrina, C. Piattelli, P. Popa, V. Pradier, T. Quinn, L. Racca, C. Riccobene, G. Sanchez-Losa, A. Saldana, M. Salvadori, I. Samtleben, D. F. E. Sanguineti, M. Sapienza, P. Schussler, F. Sieger, C. Spurio, M. Stolarczyk, T. Taiuti, M. Tayalati, Y. Trovato, A. Turpin, D. Tonnis, C. Vallage, B. Van Elewyck, V. Versari, F. Vivolo, D. Vizzoca, A. Wilms, J. Zornoza, J. D. Zuniga, J. ANTARES Collaboration All-flavor search for a diffuse flux of cosmic neutrinos with nine years of ANTARES data |
topic_facet |
astroparticle physics neutrinos |
description |
The ANTARES detector is at present the most sensitive neutrino telescope in the northern hemisphere. The highly significant cosmic neutrino excess observed by the Antarctic IceCube detector can be studied with ANTARES, exploiting its complementing field of view, exposure, and lower energy threshold. Searches for an all-flavor diffuse neutrino signal, covering nine years of ANTARES data taking, are presented in this Letter. Upward-going events are used to reduce the atmospheric muon background. This work includes for the first time in ANTARES both track-like (mainly nu mu) and shower-like (mainly nu(e)) events in this kind of analysis. Track-like events allow for an increase of the effective volume of the detector thanks to the long path traveled by muons in rock and/ or sea water. Shower-like events are well reconstructed only when the neutrino interaction vertex is close to, or inside, the instrumented volume. A mild excess of high-energy events over the expected background is observed in nine years of ANTARES data in both samples. The best fit for a single power-law cosmic neutrino spectrum, in terms of perflavor flux at 100 TeV, is Phi(1f)(0) (100 TeV) = (1.7 +/- 1.0) x 10(-18) GeV-1 cm(-2) s(-1) sr(-1) with spectral index Gamma = 2.4(-0.4)(+0.5) .The null cosmic flux assumption is rejected with a significance of 1.6 sigma . |
format |
Text |
author |
Albert, A. Andre, M. Anghinolfi, M. Anton, G. Ardid, M. Aubert, J. J. Aublin, J. Avgitas, T. Baret, B. Barrios-Marti, J. Basa, S. Belhorma, B. Bertin, V. Biagi, S. Bormuth, R. Bourret, S. Bouwhuis, M. C. Branzas, H. Bruijn, R. Brunner, J. Busto, J. Capone, A. Caramete, L. Carr, J. Celli, S. El Moursli, R. C. Chiarusi, T. Circella, M. Coelho, J. A. B. Coleiro, A. Coniglione, R. Costantini, H. Coyle, P. Creusot, A. Diaz, A. F. Deschamps, A. De Bonis, G. Distefano, C. Di Palma, I. Domi, A. Donzaud, C. Dornic, D. Drouhin, D. Eberl, T. El Bojaddaini, I. El Khayati, N. Elsasser, D. Enzenhofer, A. Ettahiri, A. Fassi, F. Felis, I. Fusco, L. A. Gay, P. Giordano, V. Glotin, H. Gregoire, T. Ruiz, R. G. Graf, K. Hallmann, S. van Haren, H. Heijboer, A. J. Hello, Yann Hernandez-Rey, J. J. Hossl, J. Hofestadt, J. Illuminati, G. James, C. W. de Jong, M. Jongen, M. Kadler, M. Kalekin, O. Katz, U. Kiessling, D. Kouchner, A. Kreter, M. Kreykenbohm, I. Kulikovskiy, V. Lachaud, C. Lahmann, R. Lefevre, D. Leonora, E. Lotze, M. Loucatos, S. Marcelin, M. Margiotta, A. Marinelli, A. Martinez-Mora, J. A. Mele, R. Melis, K. Michael, T. Migliozzi, P. Moussa, A. Navas, S. Nezri, E. Organokov, M. Pavalas, G. E. Pellegrino, C. Perrina, C. Piattelli, P. Popa, V. Pradier, T. Quinn, L. Racca, C. Riccobene, G. Sanchez-Losa, A. Saldana, M. Salvadori, I. Samtleben, D. F. E. Sanguineti, M. Sapienza, P. Schussler, F. Sieger, C. Spurio, M. Stolarczyk, T. Taiuti, M. Tayalati, Y. Trovato, A. Turpin, D. Tonnis, C. Vallage, B. Van Elewyck, V. Versari, F. Vivolo, D. Vizzoca, A. Wilms, J. Zornoza, J. D. Zuniga, J. ANTARES Collaboration |
author_facet |
Albert, A. Andre, M. Anghinolfi, M. Anton, G. Ardid, M. Aubert, J. J. Aublin, J. Avgitas, T. Baret, B. Barrios-Marti, J. Basa, S. Belhorma, B. Bertin, V. Biagi, S. Bormuth, R. Bourret, S. Bouwhuis, M. C. Branzas, H. Bruijn, R. Brunner, J. Busto, J. Capone, A. Caramete, L. Carr, J. Celli, S. El Moursli, R. C. Chiarusi, T. Circella, M. Coelho, J. A. B. Coleiro, A. Coniglione, R. Costantini, H. Coyle, P. Creusot, A. Diaz, A. F. Deschamps, A. De Bonis, G. Distefano, C. Di Palma, I. Domi, A. Donzaud, C. Dornic, D. Drouhin, D. Eberl, T. El Bojaddaini, I. El Khayati, N. Elsasser, D. Enzenhofer, A. Ettahiri, A. Fassi, F. Felis, I. Fusco, L. A. Gay, P. Giordano, V. Glotin, H. Gregoire, T. Ruiz, R. G. Graf, K. Hallmann, S. van Haren, H. Heijboer, A. J. Hello, Yann Hernandez-Rey, J. J. Hossl, J. Hofestadt, J. Illuminati, G. James, C. W. de Jong, M. Jongen, M. Kadler, M. Kalekin, O. Katz, U. Kiessling, D. Kouchner, A. Kreter, M. Kreykenbohm, I. Kulikovskiy, V. Lachaud, C. Lahmann, R. Lefevre, D. Leonora, E. Lotze, M. Loucatos, S. Marcelin, M. Margiotta, A. Marinelli, A. Martinez-Mora, J. A. Mele, R. Melis, K. Michael, T. Migliozzi, P. Moussa, A. Navas, S. Nezri, E. Organokov, M. Pavalas, G. E. Pellegrino, C. Perrina, C. Piattelli, P. Popa, V. Pradier, T. Quinn, L. Racca, C. Riccobene, G. Sanchez-Losa, A. Saldana, M. Salvadori, I. Samtleben, D. F. E. Sanguineti, M. Sapienza, P. Schussler, F. Sieger, C. Spurio, M. Stolarczyk, T. Taiuti, M. Tayalati, Y. Trovato, A. Turpin, D. Tonnis, C. Vallage, B. Van Elewyck, V. Versari, F. Vivolo, D. Vizzoca, A. Wilms, J. Zornoza, J. D. Zuniga, J. ANTARES Collaboration |
author_sort |
Albert, A. |
title |
All-flavor search for a diffuse flux of cosmic neutrinos with nine years of ANTARES data |
title_short |
All-flavor search for a diffuse flux of cosmic neutrinos with nine years of ANTARES data |
title_full |
All-flavor search for a diffuse flux of cosmic neutrinos with nine years of ANTARES data |
title_fullStr |
All-flavor search for a diffuse flux of cosmic neutrinos with nine years of ANTARES data |
title_full_unstemmed |
All-flavor search for a diffuse flux of cosmic neutrinos with nine years of ANTARES data |
title_sort |
all-flavor search for a diffuse flux of cosmic neutrinos with nine years of antares data |
publishDate |
2018 |
url |
http://www.documentation.ird.fr/hor/fdi:010081634 |
geographic |
Antarctic The Antarctic |
geographic_facet |
Antarctic The Antarctic |
genre |
Antarc* Antarctic |
genre_facet |
Antarc* Antarctic |
op_relation |
http://www.documentation.ird.fr/hor/fdi:010081634 oai:ird.fr:fdi:010081634 Albert A., Andre M., Anghinolfi M., Anton G., Ardid M., Aubert J. J., Aublin J., Avgitas T., Baret B., Barrios-Marti J., Basa S., Belhorma B., Bertin V., Biagi S., Bormuth R., Bourret S., Bouwhuis M. C., Branzas H., Bruijn R., Brunner J., Busto J., Capone A., Caramete L., Carr J., Celli S., El Moursli R. C., Chiarusi T., Circella M., Coelho J. A. B., Coleiro A., Coniglione R., Costantini H., Coyle P., Creusot A., Diaz A. F., Deschamps A., De Bonis G., Distefano C., Di Palma I., Domi A., Donzaud C., Dornic D., Drouhin D., Eberl T., El Bojaddaini I., El Khayati N., Elsasser D., Enzenhofer A., Ettahiri A., Fassi F., Felis I., Fusco L. A., Gay P., Giordano V., Glotin H., Gregoire T., Ruiz R. G., Graf K., Hallmann S., van Haren H., Heijboer A. J., Hello Yann, Hernandez-Rey J. J., Hossl J., Hofestadt J., Illuminati G., James C. W., de Jong M., Jongen M., Kadler M., Kalekin O., Katz U., Kiessling D., Kouchner A., Kreter M., Kreykenbohm I., Kulikovskiy V., Lachaud C., Lahmann R., Lefevre D., Leonora E., Lotze M., Loucatos S., Marcelin M., Margiotta A., Marinelli A., Martinez-Mora J. A., Mele R., Melis K., Michael T., Migliozzi P., Moussa A., Navas S., Nezri E., Organokov M., Pavalas G. E., Pellegrino C., Perrina C., Piattelli P., Popa V., Pradier T., Quinn L., Racca C., Riccobene G., Sanchez-Losa A., Saldana M., Salvadori I., Samtleben D. F. E., Sanguineti M., Sapienza P., Schussler F., Sieger C., Spurio M., Stolarczyk T., Taiuti M., Tayalati Y., Trovato A., Turpin D., Tonnis C., Vallage B., Van Elewyck V., Versari F., Vivolo D., Vizzoca A., Wilms J., Zornoza J. D., Zuniga J., ANTARES Collaboration. All-flavor search for a diffuse flux of cosmic neutrinos with nine years of ANTARES data. Astrophysical Journal Letters, 2018, 853 (1), p. L7. |
_version_ |
1766252892603285504 |
spelling |
ftird:oai:ird.fr:fdi:010081634 2023-05-15T13:50:05+02:00 All-flavor search for a diffuse flux of cosmic neutrinos with nine years of ANTARES data Albert, A. Andre, M. Anghinolfi, M. Anton, G. Ardid, M. Aubert, J. J. Aublin, J. Avgitas, T. Baret, B. Barrios-Marti, J. Basa, S. Belhorma, B. Bertin, V. Biagi, S. Bormuth, R. Bourret, S. Bouwhuis, M. C. Branzas, H. Bruijn, R. Brunner, J. Busto, J. Capone, A. Caramete, L. Carr, J. Celli, S. El Moursli, R. C. Chiarusi, T. Circella, M. Coelho, J. A. B. Coleiro, A. Coniglione, R. Costantini, H. Coyle, P. Creusot, A. Diaz, A. F. Deschamps, A. De Bonis, G. Distefano, C. Di Palma, I. Domi, A. Donzaud, C. Dornic, D. Drouhin, D. Eberl, T. El Bojaddaini, I. El Khayati, N. Elsasser, D. Enzenhofer, A. Ettahiri, A. Fassi, F. Felis, I. Fusco, L. A. Gay, P. Giordano, V. Glotin, H. Gregoire, T. Ruiz, R. G. Graf, K. Hallmann, S. van Haren, H. Heijboer, A. J. Hello, Yann Hernandez-Rey, J. J. Hossl, J. Hofestadt, J. Illuminati, G. James, C. W. de Jong, M. Jongen, M. Kadler, M. Kalekin, O. Katz, U. Kiessling, D. Kouchner, A. Kreter, M. Kreykenbohm, I. Kulikovskiy, V. Lachaud, C. Lahmann, R. Lefevre, D. Leonora, E. Lotze, M. Loucatos, S. Marcelin, M. Margiotta, A. Marinelli, A. Martinez-Mora, J. A. Mele, R. Melis, K. Michael, T. Migliozzi, P. Moussa, A. Navas, S. Nezri, E. Organokov, M. Pavalas, G. E. Pellegrino, C. Perrina, C. Piattelli, P. Popa, V. Pradier, T. Quinn, L. Racca, C. Riccobene, G. Sanchez-Losa, A. Saldana, M. Salvadori, I. Samtleben, D. F. E. Sanguineti, M. Sapienza, P. Schussler, F. Sieger, C. Spurio, M. Stolarczyk, T. Taiuti, M. Tayalati, Y. Trovato, A. Turpin, D. Tonnis, C. Vallage, B. Van Elewyck, V. Versari, F. Vivolo, D. Vizzoca, A. Wilms, J. Zornoza, J. D. Zuniga, J. ANTARES Collaboration 2018 text/pdf http://www.documentation.ird.fr/hor/fdi:010081634 EN eng http://www.documentation.ird.fr/hor/fdi:010081634 oai:ird.fr:fdi:010081634 Albert A., Andre M., Anghinolfi M., Anton G., Ardid M., Aubert J. J., Aublin J., Avgitas T., Baret B., Barrios-Marti J., Basa S., Belhorma B., Bertin V., Biagi S., Bormuth R., Bourret S., Bouwhuis M. C., Branzas H., Bruijn R., Brunner J., Busto J., Capone A., Caramete L., Carr J., Celli S., El Moursli R. C., Chiarusi T., Circella M., Coelho J. A. B., Coleiro A., Coniglione R., Costantini H., Coyle P., Creusot A., Diaz A. F., Deschamps A., De Bonis G., Distefano C., Di Palma I., Domi A., Donzaud C., Dornic D., Drouhin D., Eberl T., El Bojaddaini I., El Khayati N., Elsasser D., Enzenhofer A., Ettahiri A., Fassi F., Felis I., Fusco L. A., Gay P., Giordano V., Glotin H., Gregoire T., Ruiz R. G., Graf K., Hallmann S., van Haren H., Heijboer A. J., Hello Yann, Hernandez-Rey J. J., Hossl J., Hofestadt J., Illuminati G., James C. W., de Jong M., Jongen M., Kadler M., Kalekin O., Katz U., Kiessling D., Kouchner A., Kreter M., Kreykenbohm I., Kulikovskiy V., Lachaud C., Lahmann R., Lefevre D., Leonora E., Lotze M., Loucatos S., Marcelin M., Margiotta A., Marinelli A., Martinez-Mora J. A., Mele R., Melis K., Michael T., Migliozzi P., Moussa A., Navas S., Nezri E., Organokov M., Pavalas G. E., Pellegrino C., Perrina C., Piattelli P., Popa V., Pradier T., Quinn L., Racca C., Riccobene G., Sanchez-Losa A., Saldana M., Salvadori I., Samtleben D. F. E., Sanguineti M., Sapienza P., Schussler F., Sieger C., Spurio M., Stolarczyk T., Taiuti M., Tayalati Y., Trovato A., Turpin D., Tonnis C., Vallage B., Van Elewyck V., Versari F., Vivolo D., Vizzoca A., Wilms J., Zornoza J. D., Zuniga J., ANTARES Collaboration. All-flavor search for a diffuse flux of cosmic neutrinos with nine years of ANTARES data. Astrophysical Journal Letters, 2018, 853 (1), p. L7. astroparticle physics neutrinos text 2018 ftird 2021-04-06T22:52:18Z The ANTARES detector is at present the most sensitive neutrino telescope in the northern hemisphere. The highly significant cosmic neutrino excess observed by the Antarctic IceCube detector can be studied with ANTARES, exploiting its complementing field of view, exposure, and lower energy threshold. Searches for an all-flavor diffuse neutrino signal, covering nine years of ANTARES data taking, are presented in this Letter. Upward-going events are used to reduce the atmospheric muon background. This work includes for the first time in ANTARES both track-like (mainly nu mu) and shower-like (mainly nu(e)) events in this kind of analysis. Track-like events allow for an increase of the effective volume of the detector thanks to the long path traveled by muons in rock and/ or sea water. Shower-like events are well reconstructed only when the neutrino interaction vertex is close to, or inside, the instrumented volume. A mild excess of high-energy events over the expected background is observed in nine years of ANTARES data in both samples. The best fit for a single power-law cosmic neutrino spectrum, in terms of perflavor flux at 100 TeV, is Phi(1f)(0) (100 TeV) = (1.7 +/- 1.0) x 10(-18) GeV-1 cm(-2) s(-1) sr(-1) with spectral index Gamma = 2.4(-0.4)(+0.5) .The null cosmic flux assumption is rejected with a significance of 1.6 sigma . Text Antarc* Antarctic IRD (Institute de recherche pour le développement): Horizon Antarctic The Antarctic |