An Algorithm for the Reconstruction of Neutrino-induced Showers in the ANTARES Neutrino Telescope

Muons created by nm charged current (CC) interactions in the water surrounding the ANTARES neutrino telescope have been almost exclusively used so far in searches for cosmic neutrino sources. Due to their long range, highly energetic muons inducing Cherenkov radiation in the water are reconstructed...

Full description

Bibliographic Details
Main Authors: Albert, A., André, M., Anghinolfi, M., Anton, G., Ardid, M., Aubert, J., Avgitas, T., Baret, B., Barrios-Marti, J., Basa, S., Belhorma, B., Bertin, V., Biagi, S., Bormuth, R., Bourret, S., Bouwhuis, M., Branzas, H., Bruijn, R., Brunner, J., Busto, J., Capone, A., Caramete, L., Carr, J., Celli, S., El Moursli, R., Chiarusi, T., Circella, M., Coelho, J., Coleiro, A., Coniglione, R., Costantini, H., Coyle, P., Creusot, A., Diaz, A., Deschamps, A., Bonis, G., Distefano, C., Palma, I., Domi, A., Donzaud, C., Dornic, D., Drouhin, D., Eberl, T., Bojaddaini, I., Khayati, N., Elsasser, D., Enzenhöfer, A., Ettahiri, A., Fassi, F., Felis, I., Fusco, L., Gay, P., Giordano, V., Glotin, H., Grégoire, T., Ruiz, R., Graf, K., Hallmann, S., Haren, H., Heijboer, A., Hello, Y., Hernández-Rey, J., Hößl, J., Hofestadt, J., Hugon, C., Illuminati, G., James, Clancy, 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.
Format: Journal Article
Published: Institute of Physics Publishing 2017
Online Access:http://hdl.handle.net/20.500.11937/73345
_version_ 1848762990040449024
author Albert, A.
André, M.
Anghinolfi, M.
Anton, G.
Ardid, M.
Aubert, J.
Avgitas, T.
Baret, B.
Barrios-Marti, J.
Basa, S.
Belhorma, B.
Bertin, V.
Biagi, S.
Bormuth, R.
Bourret, S.
Bouwhuis, M.
Branzas, H.
Bruijn, R.
Brunner, J.
Busto, J.
Capone, A.
Caramete, L.
Carr, J.
Celli, S.
El Moursli, R.
Chiarusi, T.
Circella, M.
Coelho, J.
Coleiro, A.
Coniglione, R.
Costantini, H.
Coyle, P.
Creusot, A.
Diaz, A.
Deschamps, A.
Bonis, G.
Distefano, C.
Palma, I.
Domi, A.
Donzaud, C.
Dornic, D.
Drouhin, D.
Eberl, T.
Bojaddaini, I.
Khayati, N.
Elsasser, D.
Enzenhöfer, A.
Ettahiri, A.
Fassi, F.
Felis, I.
Fusco, L.
Gay, P.
Giordano, V.
Glotin, H.
Grégoire, T.
Ruiz, R.
Graf, K.
Hallmann, S.
Haren, H.
Heijboer, A.
Hello, Y.
Hernández-Rey, J.
Hößl, J.
Hofestadt, J.
Hugon, C.
Illuminati, G.
James, Clancy
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.
author_facet Albert, A.
André, M.
Anghinolfi, M.
Anton, G.
Ardid, M.
Aubert, J.
Avgitas, T.
Baret, B.
Barrios-Marti, J.
Basa, S.
Belhorma, B.
Bertin, V.
Biagi, S.
Bormuth, R.
Bourret, S.
Bouwhuis, M.
Branzas, H.
Bruijn, R.
Brunner, J.
Busto, J.
Capone, A.
Caramete, L.
Carr, J.
Celli, S.
El Moursli, R.
Chiarusi, T.
Circella, M.
Coelho, J.
Coleiro, A.
Coniglione, R.
Costantini, H.
Coyle, P.
Creusot, A.
Diaz, A.
Deschamps, A.
Bonis, G.
Distefano, C.
Palma, I.
Domi, A.
Donzaud, C.
Dornic, D.
Drouhin, D.
Eberl, T.
Bojaddaini, I.
Khayati, N.
Elsasser, D.
Enzenhöfer, A.
Ettahiri, A.
Fassi, F.
Felis, I.
Fusco, L.
Gay, P.
Giordano, V.
Glotin, H.
Grégoire, T.
Ruiz, R.
Graf, K.
Hallmann, S.
Haren, H.
Heijboer, A.
Hello, Y.
Hernández-Rey, J.
Hößl, J.
Hofestadt, J.
Hugon, C.
Illuminati, G.
James, Clancy
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.
author_sort Albert, A.
building Curtin Institutional Repository
collection Online Access
description Muons created by nm charged current (CC) interactions in the water surrounding the ANTARES neutrino telescope have been almost exclusively used so far in searches for cosmic neutrino sources. Due to their long range, highly energetic muons inducing Cherenkov radiation in the water are reconstructed with dedicated algorithms that allow for the determination of the parent neutrino direction with a median angular resolution of about 0.4 for an E-2 neutrino spectrum. In this paper, an algorithm optimized for accurate reconstruction of energy and direction of shower events in the ANTARES detector is presented. Hadronic showers of electrically charged particles are produced by the disintegration of the nucleus both in CC and neutral current interactions of neutrinos in water. In addition, electromagnetic showers result from the CC interactions of electron neutrinos while the decay of a tau lepton produced in nt CC interactions will, in most cases, lead to either a hadronic or an electromagnetic shower. A shower can be approximated as a point source of photons. With the presented method, the shower position is reconstructed with a precision of about 1 m; the neutrino direction is reconstructed with a median angular resolution between 2 and 3 in the energy range of 11000 TeV. In this energy interval, the uncertainty on the reconstructed neutrino energy is about 5%10%. The increase in the detector sensitivity due to the use of additional information from shower events in the searches for a cosmic neutrino flux is also presented.
first_indexed 2025-11-14T10:56:20Z
format Journal Article
id curtin-20.500.11937-73345
institution Curtin University Malaysia
institution_category Local University
last_indexed 2025-11-14T10:56:20Z
publishDate 2017
publisher Institute of Physics Publishing
recordtype eprints
repository_type Digital Repository
spelling curtin-20.500.11937-733452018-12-13T09:35:41Z An Algorithm for the Reconstruction of Neutrino-induced Showers in the ANTARES Neutrino Telescope Albert, A. André, M. Anghinolfi, M. Anton, G. Ardid, M. Aubert, J. Avgitas, T. Baret, B. Barrios-Marti, J. Basa, S. Belhorma, B. Bertin, V. Biagi, S. Bormuth, R. Bourret, S. Bouwhuis, M. Branzas, H. Bruijn, R. Brunner, J. Busto, J. Capone, A. Caramete, L. Carr, J. Celli, S. El Moursli, R. Chiarusi, T. Circella, M. Coelho, J. Coleiro, A. Coniglione, R. Costantini, H. Coyle, P. Creusot, A. Diaz, A. Deschamps, A. Bonis, G. Distefano, C. Palma, I. Domi, A. Donzaud, C. Dornic, D. Drouhin, D. Eberl, T. Bojaddaini, I. Khayati, N. Elsasser, D. Enzenhöfer, A. Ettahiri, A. Fassi, F. Felis, I. Fusco, L. Gay, P. Giordano, V. Glotin, H. Grégoire, T. Ruiz, R. Graf, K. Hallmann, S. Haren, H. Heijboer, A. Hello, Y. Hernández-Rey, J. Hößl, J. Hofestadt, J. Hugon, C. Illuminati, G. James, Clancy 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. Muons created by nm charged current (CC) interactions in the water surrounding the ANTARES neutrino telescope have been almost exclusively used so far in searches for cosmic neutrino sources. Due to their long range, highly energetic muons inducing Cherenkov radiation in the water are reconstructed with dedicated algorithms that allow for the determination of the parent neutrino direction with a median angular resolution of about 0.4 for an E-2 neutrino spectrum. In this paper, an algorithm optimized for accurate reconstruction of energy and direction of shower events in the ANTARES detector is presented. Hadronic showers of electrically charged particles are produced by the disintegration of the nucleus both in CC and neutral current interactions of neutrinos in water. In addition, electromagnetic showers result from the CC interactions of electron neutrinos while the decay of a tau lepton produced in nt CC interactions will, in most cases, lead to either a hadronic or an electromagnetic shower. A shower can be approximated as a point source of photons. With the presented method, the shower position is reconstructed with a precision of about 1 m; the neutrino direction is reconstructed with a median angular resolution between 2 and 3 in the energy range of 11000 TeV. In this energy interval, the uncertainty on the reconstructed neutrino energy is about 5%10%. The increase in the detector sensitivity due to the use of additional information from shower events in the searches for a cosmic neutrino flux is also presented. 2017 Journal Article http://hdl.handle.net/20.500.11937/73345 10.3847/1538-3881/aa9709 Institute of Physics Publishing restricted
spellingShingle Albert, A.
André, M.
Anghinolfi, M.
Anton, G.
Ardid, M.
Aubert, J.
Avgitas, T.
Baret, B.
Barrios-Marti, J.
Basa, S.
Belhorma, B.
Bertin, V.
Biagi, S.
Bormuth, R.
Bourret, S.
Bouwhuis, M.
Branzas, H.
Bruijn, R.
Brunner, J.
Busto, J.
Capone, A.
Caramete, L.
Carr, J.
Celli, S.
El Moursli, R.
Chiarusi, T.
Circella, M.
Coelho, J.
Coleiro, A.
Coniglione, R.
Costantini, H.
Coyle, P.
Creusot, A.
Diaz, A.
Deschamps, A.
Bonis, G.
Distefano, C.
Palma, I.
Domi, A.
Donzaud, C.
Dornic, D.
Drouhin, D.
Eberl, T.
Bojaddaini, I.
Khayati, N.
Elsasser, D.
Enzenhöfer, A.
Ettahiri, A.
Fassi, F.
Felis, I.
Fusco, L.
Gay, P.
Giordano, V.
Glotin, H.
Grégoire, T.
Ruiz, R.
Graf, K.
Hallmann, S.
Haren, H.
Heijboer, A.
Hello, Y.
Hernández-Rey, J.
Hößl, J.
Hofestadt, J.
Hugon, C.
Illuminati, G.
James, Clancy
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.
An Algorithm for the Reconstruction of Neutrino-induced Showers in the ANTARES Neutrino Telescope
title An Algorithm for the Reconstruction of Neutrino-induced Showers in the ANTARES Neutrino Telescope
title_full An Algorithm for the Reconstruction of Neutrino-induced Showers in the ANTARES Neutrino Telescope
title_fullStr An Algorithm for the Reconstruction of Neutrino-induced Showers in the ANTARES Neutrino Telescope
title_full_unstemmed An Algorithm for the Reconstruction of Neutrino-induced Showers in the ANTARES Neutrino Telescope
title_short An Algorithm for the Reconstruction of Neutrino-induced Showers in the ANTARES Neutrino Telescope
title_sort algorithm for the reconstruction of neutrino-induced showers in the antares neutrino telescope
url http://hdl.handle.net/20.500.11937/73345