The search for high-energy neutrinos coincident with fast radio bursts with the ANTARES neutrino telescope

In the past decade, a new class of bright transient radio sources with millisecond duration has been discovered. The origin of these so-called fast radio bursts (FRBs) is still a mystery, despite the growing observational efforts made by various multiwavelength and multimessenger facilities. To date...

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Main Authors:	Albert, A., Andre, M., Anghinolfi, M., Anton, G., Ardid, M., Aubert, J., Aublin, J., Avgitas, T., Baret, B., Barrios-Marti, J., Basa, S., Belhorma, B., Bertin, V., Biagi, S., Bormuth, R., Boumaaza, J., Bourret, S., Bouwhuis, M., Branzas, H., Bruijn, R., Brunner, J., Busto, J., Capone, A., Caramete, L., Carr, J., Celli, S., Chabab, M., Cherkaoui El Moursli, R., Chiarusi, T., Circella, M., Coelho, J., Coleiro, A., Colomer, M., Coniglione, R., Costantini, H., Coyle, P., Creusot, A., Diaz, A., Deschamps, A., Distefano, C., Di Palma, I., Domi, A., Donzaud, C., Dornic, D., Drouhin, D., Eberl, T., El Bojaddaini, I., El Khayati, N., Elsaesser, D., Enzenhoefer, A., Ettahiri, A., Fassi, F., Felis, I., Fermani, P., Ferrara, G., Fusco, L., Gay, P., Glotin, H., Gregoire, T., Gracia-Ruiz, R., Graf, K., Hallmann, S., van Haren, H., Heijboer, A., Hello, Y., Hernandez-Rey, J., Hoessl, J., Hofestaedt, J., Illuminati, G., James, Clancy, de Jong, M., Jongen, M., Kadler, M., Kalekin, O., Katz, U., Kouchner, A., Kreter, M., Kreykenbohm, I., Kulikovskiy, V., Lachaud, C., Lahmann, R., Lefevre, D., Leonora, E., Levi, G., Lotze, M., Loucatos, S., Marcelin, M., Margiotta, A., Marinelli, A., Martinez-Mora, J., Mele, R., Melis, K., Migliozzi, P., Moussa, A., Navas, S., Nezri, E., Nunez, A., Organokov, M., Pavalas, G., Pellegrino, C., Piattelli, P., Popa, V., Pradier, T., Quinn, L., Racca, C., Randazzo, N., Riccobene, G., Sanchez-Losa, A., Saldana, M., Salvadori, I., Samtleben, D., Sanguineti, M., Sapienza, P., Schussler, F., Spurio, M., Stolarczyk, T., Taiuti, M., Tayalati, Y., Trovato, A., Turpin, D., Vallage, B., Van Elewyck, V., Versari, F., Vivolo, D., Wilms, J., Zaborov, D., Zornoza, J., Zuniga, J.
Format:	Journal Article
Published:	Oxford University Press 2019
Online Access:	http://hdl.handle.net/20.500.11937/74440

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author	Albert, A. Andre, M. Anghinolfi, M. Anton, G. Ardid, M. Aubert, J. Aublin, J. Avgitas, T. Baret, B. Barrios-Marti, J. Basa, S. Belhorma, B. Bertin, V. Biagi, S. Bormuth, R. Boumaaza, J. Bourret, S. Bouwhuis, M. Branzas, H. Bruijn, R. Brunner, J. Busto, J. Capone, A. Caramete, L. Carr, J. Celli, S. Chabab, M. Cherkaoui El Moursli, R. Chiarusi, T. Circella, M. Coelho, J. Coleiro, A. Colomer, M. Coniglione, R. Costantini, H. Coyle, P. Creusot, A. Diaz, A. Deschamps, A. Distefano, C. Di Palma, I. Domi, A. Donzaud, C. Dornic, D. Drouhin, D. Eberl, T. El Bojaddaini, I. El Khayati, N. Elsaesser, D. Enzenhoefer, A. Ettahiri, A. Fassi, F. Felis, I. Fermani, P. Ferrara, G. Fusco, L. Gay, P. Glotin, H. Gregoire, T. Gracia-Ruiz, R. Graf, K. Hallmann, S. van Haren, H. Heijboer, A. Hello, Y. Hernandez-Rey, J. Hoessl, J. Hofestaedt, J. Illuminati, G. James, Clancy de Jong, M. Jongen, M. Kadler, M. Kalekin, O. Katz, U. Kouchner, A. Kreter, M. Kreykenbohm, I. Kulikovskiy, V. Lachaud, C. Lahmann, R. Lefevre, D. Leonora, E. Levi, G. Lotze, M. Loucatos, S. Marcelin, M. Margiotta, A. Marinelli, A. Martinez-Mora, J. Mele, R. Melis, K. Migliozzi, P. Moussa, A. Navas, S. Nezri, E. Nunez, A. Organokov, M. Pavalas, G. Pellegrino, C. Piattelli, P. Popa, V. Pradier, T. Quinn, L. Racca, C. Randazzo, N. Riccobene, G. Sanchez-Losa, A. Saldana, M. Salvadori, I. Samtleben, D. Sanguineti, M. Sapienza, P. Schussler, F. Spurio, M. Stolarczyk, T. Taiuti, M. Tayalati, Y. Trovato, A. Turpin, D. Vallage, B. Van Elewyck, V. Versari, F. Vivolo, D. Wilms, J. Zaborov, D. Zornoza, J. Zuniga, J.
author_facet	Albert, A. Andre, M. Anghinolfi, M. Anton, G. Ardid, M. Aubert, J. Aublin, J. Avgitas, T. Baret, B. Barrios-Marti, J. Basa, S. Belhorma, B. Bertin, V. Biagi, S. Bormuth, R. Boumaaza, J. Bourret, S. Bouwhuis, M. Branzas, H. Bruijn, R. Brunner, J. Busto, J. Capone, A. Caramete, L. Carr, J. Celli, S. Chabab, M. Cherkaoui El Moursli, R. Chiarusi, T. Circella, M. Coelho, J. Coleiro, A. Colomer, M. Coniglione, R. Costantini, H. Coyle, P. Creusot, A. Diaz, A. Deschamps, A. Distefano, C. Di Palma, I. Domi, A. Donzaud, C. Dornic, D. Drouhin, D. Eberl, T. El Bojaddaini, I. El Khayati, N. Elsaesser, D. Enzenhoefer, A. Ettahiri, A. Fassi, F. Felis, I. Fermani, P. Ferrara, G. Fusco, L. Gay, P. Glotin, H. Gregoire, T. Gracia-Ruiz, R. Graf, K. Hallmann, S. van Haren, H. Heijboer, A. Hello, Y. Hernandez-Rey, J. Hoessl, J. Hofestaedt, J. Illuminati, G. James, Clancy de Jong, M. Jongen, M. Kadler, M. Kalekin, O. Katz, U. Kouchner, A. Kreter, M. Kreykenbohm, I. Kulikovskiy, V. Lachaud, C. Lahmann, R. Lefevre, D. Leonora, E. Levi, G. Lotze, M. Loucatos, S. Marcelin, M. Margiotta, A. Marinelli, A. Martinez-Mora, J. Mele, R. Melis, K. Migliozzi, P. Moussa, A. Navas, S. Nezri, E. Nunez, A. Organokov, M. Pavalas, G. Pellegrino, C. Piattelli, P. Popa, V. Pradier, T. Quinn, L. Racca, C. Randazzo, N. Riccobene, G. Sanchez-Losa, A. Saldana, M. Salvadori, I. Samtleben, D. Sanguineti, M. Sapienza, P. Schussler, F. Spurio, M. Stolarczyk, T. Taiuti, M. Tayalati, Y. Trovato, A. Turpin, D. Vallage, B. Van Elewyck, V. Versari, F. Vivolo, D. Wilms, J. Zaborov, D. Zornoza, J. Zuniga, J.
author_sort	Albert, A.
building	Curtin Institutional Repository
collection	Online Access
description	In the past decade, a new class of bright transient radio sources with millisecond duration has been discovered. The origin of these so-called fast radio bursts (FRBs) is still a mystery, despite the growing observational efforts made by various multiwavelength and multimessenger facilities. To date, many models have been proposed to explain FRBs, but neither the progenitors nor the radiative and the particle acceleration processes at work have been clearly identified. In this paper, we assess whether hadronic processes may occur in the vicinity of the FRB source. If they do, FRBs may contribute to the high-energy cosmic-ray and neutrino fluxes. A search for these hadronic signatures was carried out using the ANTARES neutrino telescope. The analysis consists in looking for high-energy neutrinos, in the TeV–PeV regime, that are spatially and temporally coincident with the detected FRBs. Most of the FRBs discovered in the period 2013–2017 were in the field of view of the ANTARES detector, which is sensitive mostly to events originating from the Southern hemisphere. From this period, 12 FRBs were selected and no coincident neutrino candidate was observed. Upper limits on the per-burst neutrino fluence were derived using a power-law spectrum, dN/dEν∝E−γν⁠, for the incoming neutrino flux, assuming spectral indexes γ = 1.0, 2.0, 2.5. Finally, the neutrino energy was constrained by computing the total energy radiated in neutrinos, assuming different distances for the FRBs. Constraints on the neutrino fluence and on the energy released were derived from the associated null results.
first_indexed	2025-11-14T11:00:52Z
format	Journal Article
id	curtin-20.500.11937-74440
institution	Curtin University Malaysia
institution_category	Local University
last_indexed	2025-11-14T11:00:52Z
publishDate	2019
publisher	Oxford University Press
recordtype	eprints
repository_type	Digital Repository
spelling	curtin-20.500.11937-744402019-03-13T02:10:21Z The search for high-energy neutrinos coincident with fast radio bursts with the ANTARES neutrino telescope Albert, A. Andre, M. Anghinolfi, M. Anton, G. Ardid, M. Aubert, J. Aublin, J. Avgitas, T. Baret, B. Barrios-Marti, J. Basa, S. Belhorma, B. Bertin, V. Biagi, S. Bormuth, R. Boumaaza, J. Bourret, S. Bouwhuis, M. Branzas, H. Bruijn, R. Brunner, J. Busto, J. Capone, A. Caramete, L. Carr, J. Celli, S. Chabab, M. Cherkaoui El Moursli, R. Chiarusi, T. Circella, M. Coelho, J. Coleiro, A. Colomer, M. Coniglione, R. Costantini, H. Coyle, P. Creusot, A. Diaz, A. Deschamps, A. Distefano, C. Di Palma, I. Domi, A. Donzaud, C. Dornic, D. Drouhin, D. Eberl, T. El Bojaddaini, I. El Khayati, N. Elsaesser, D. Enzenhoefer, A. Ettahiri, A. Fassi, F. Felis, I. Fermani, P. Ferrara, G. Fusco, L. Gay, P. Glotin, H. Gregoire, T. Gracia-Ruiz, R. Graf, K. Hallmann, S. van Haren, H. Heijboer, A. Hello, Y. Hernandez-Rey, J. Hoessl, J. Hofestaedt, J. Illuminati, G. James, Clancy de Jong, M. Jongen, M. Kadler, M. Kalekin, O. Katz, U. Kouchner, A. Kreter, M. Kreykenbohm, I. Kulikovskiy, V. Lachaud, C. Lahmann, R. Lefevre, D. Leonora, E. Levi, G. Lotze, M. Loucatos, S. Marcelin, M. Margiotta, A. Marinelli, A. Martinez-Mora, J. Mele, R. Melis, K. Migliozzi, P. Moussa, A. Navas, S. Nezri, E. Nunez, A. Organokov, M. Pavalas, G. Pellegrino, C. Piattelli, P. Popa, V. Pradier, T. Quinn, L. Racca, C. Randazzo, N. Riccobene, G. Sanchez-Losa, A. Saldana, M. Salvadori, I. Samtleben, D. Sanguineti, M. Sapienza, P. Schussler, F. Spurio, M. Stolarczyk, T. Taiuti, M. Tayalati, Y. Trovato, A. Turpin, D. Vallage, B. Van Elewyck, V. Versari, F. Vivolo, D. Wilms, J. Zaborov, D. Zornoza, J. Zuniga, J. In the past decade, a new class of bright transient radio sources with millisecond duration has been discovered. The origin of these so-called fast radio bursts (FRBs) is still a mystery, despite the growing observational efforts made by various multiwavelength and multimessenger facilities. To date, many models have been proposed to explain FRBs, but neither the progenitors nor the radiative and the particle acceleration processes at work have been clearly identified. In this paper, we assess whether hadronic processes may occur in the vicinity of the FRB source. If they do, FRBs may contribute to the high-energy cosmic-ray and neutrino fluxes. A search for these hadronic signatures was carried out using the ANTARES neutrino telescope. The analysis consists in looking for high-energy neutrinos, in the TeV–PeV regime, that are spatially and temporally coincident with the detected FRBs. Most of the FRBs discovered in the period 2013–2017 were in the field of view of the ANTARES detector, which is sensitive mostly to events originating from the Southern hemisphere. From this period, 12 FRBs were selected and no coincident neutrino candidate was observed. Upper limits on the per-burst neutrino fluence were derived using a power-law spectrum, dN/dEν∝E−γν⁠, for the incoming neutrino flux, assuming spectral indexes γ = 1.0, 2.0, 2.5. Finally, the neutrino energy was constrained by computing the total energy radiated in neutrinos, assuming different distances for the FRBs. Constraints on the neutrino fluence and on the energy released were derived from the associated null results. 2019 Journal Article http://hdl.handle.net/20.500.11937/74440 10.1093/mnras/sty2621 Oxford University Press fulltext
spellingShingle	Albert, A. Andre, M. Anghinolfi, M. Anton, G. Ardid, M. Aubert, J. Aublin, J. Avgitas, T. Baret, B. Barrios-Marti, J. Basa, S. Belhorma, B. Bertin, V. Biagi, S. Bormuth, R. Boumaaza, J. Bourret, S. Bouwhuis, M. Branzas, H. Bruijn, R. Brunner, J. Busto, J. Capone, A. Caramete, L. Carr, J. Celli, S. Chabab, M. Cherkaoui El Moursli, R. Chiarusi, T. Circella, M. Coelho, J. Coleiro, A. Colomer, M. Coniglione, R. Costantini, H. Coyle, P. Creusot, A. Diaz, A. Deschamps, A. Distefano, C. Di Palma, I. Domi, A. Donzaud, C. Dornic, D. Drouhin, D. Eberl, T. El Bojaddaini, I. El Khayati, N. Elsaesser, D. Enzenhoefer, A. Ettahiri, A. Fassi, F. Felis, I. Fermani, P. Ferrara, G. Fusco, L. Gay, P. Glotin, H. Gregoire, T. Gracia-Ruiz, R. Graf, K. Hallmann, S. van Haren, H. Heijboer, A. Hello, Y. Hernandez-Rey, J. Hoessl, J. Hofestaedt, J. Illuminati, G. James, Clancy de Jong, M. Jongen, M. Kadler, M. Kalekin, O. Katz, U. Kouchner, A. Kreter, M. Kreykenbohm, I. Kulikovskiy, V. Lachaud, C. Lahmann, R. Lefevre, D. Leonora, E. Levi, G. Lotze, M. Loucatos, S. Marcelin, M. Margiotta, A. Marinelli, A. Martinez-Mora, J. Mele, R. Melis, K. Migliozzi, P. Moussa, A. Navas, S. Nezri, E. Nunez, A. Organokov, M. Pavalas, G. Pellegrino, C. Piattelli, P. Popa, V. Pradier, T. Quinn, L. Racca, C. Randazzo, N. Riccobene, G. Sanchez-Losa, A. Saldana, M. Salvadori, I. Samtleben, D. Sanguineti, M. Sapienza, P. Schussler, F. Spurio, M. Stolarczyk, T. Taiuti, M. Tayalati, Y. Trovato, A. Turpin, D. Vallage, B. Van Elewyck, V. Versari, F. Vivolo, D. Wilms, J. Zaborov, D. Zornoza, J. Zuniga, J. The search for high-energy neutrinos coincident with fast radio bursts with the ANTARES neutrino telescope
title	The search for high-energy neutrinos coincident with fast radio bursts with the ANTARES neutrino telescope
title_full	The search for high-energy neutrinos coincident with fast radio bursts with the ANTARES neutrino telescope
title_fullStr	The search for high-energy neutrinos coincident with fast radio bursts with the ANTARES neutrino telescope
title_full_unstemmed	The search for high-energy neutrinos coincident with fast radio bursts with the ANTARES neutrino telescope
title_short	The search for high-energy neutrinos coincident with fast radio bursts with the ANTARES neutrino telescope
title_sort	search for high-energy neutrinos coincident with fast radio bursts with the antares neutrino telescope
url	http://hdl.handle.net/20.500.11937/74440

The search for high-energy neutrinos coincident with fast radio bursts with the ANTARES neutrino telescope

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