2021MNRAS.500.5614A

Query : 2021MNRAS.500.5614A

2021MNRAS.500.5614A - Mon. Not. R. Astron. Soc., 500, 5614-5628 (2021/February-1)

Constraining the contribution of Gamma-Ray Bursts to the high-energy diffuse neutrino flux with 10 yr of ANTARES data.

ALBERT A., ANDRE M., ANGHINOLFI M., ANTON G., ARDID M., AUBERT J.-J., AUBLIN J., BARET B., BASA S., BELHORMA B., BERTIN V., BIAGI S., BISSINGER M., BOUMAAZA J., BOUTA M., BOUWHUIS M.C., BRANZAS H., BRUIJN R., BRUNNER J., BUSTO J., CAPONE A., CARAMETE L., CARR J., CELLI S., CHABAB M., CHAU T.N., CHERKAOUI EL MOURSLI R., CHIARUSI T., CIRCELLA M., COLEIRO A., COLOMER-MOLLA M., CONIGLIONE R., COYLE P., CREUSOT A., DIAZ A.F., DE WASSEIGE G., DESCHAMPS A., DISTEFANO C., DI PALMA I., DOMI A., DONZAUD C., DORNIC D., DROUHIN D., EBERL T., EL KHAYATI N., ENZENHOFER A., ETTAHIRI A., FERMANI P., FERRARA G., FILIPPINI F., FUSCO L.A., GAY P., GLOTIN H., GOZZINI R., GRAF K., GUIDI C., HALLMANN S., VAN HAREN H., HEIJBOER A.J., HELLO Y., HERNANDEZ-REY J.J., HOSSL J., HOFESTADT J., HUANG F., ILLUMINATI G., JAMES C.W., DE JONG M., DE JONG P., JONGEN M., KADLER M., KALEKIN O., KATZ U., KHAN-CHOWDHURY N.R., KOUCHNER A., KREYKENBOHM I., KULIKOVSKIY V., LAHMANN R., LE BRETON R., LEFEVRE D., LEONORA E., LEVI G., LINCETTO M., LOPEZ-COTO D., LOUCATOS S., MAGGI G., MANCZAK J., MARCELIN M., MARGIOTTA A., MARINELLI A., MARTINEZ-MORA J.A., MAZZOU S., MELIS K., MIGLIOZZI P., MOSER M., MOUSSA A., MULLER R., NAUTA L., NAVAS S., NEZRI E., NUNEZ-CASTINEYRA A., O'FEARRAIGH B., ORGANOKOV M., PAVALAS G.E., PELLEGRINO C., PERRIN-TERRIN M., PIATTELLI P., POIRE C., POPA V., PRADIER T., RANDAZZO N., RECK S., RICCOBENE G., SANCHEZ-LOSA A., SAMTLEBEN D.F.E., SANGUINETI M., SAPIENZA P., SCHNABEL J., SCHUSSLER F., SPURIO M., STOLARCZYK T., STRANDBERG B., TAIUTI M., TAYALATI Y., THAKORE T., TINGAY S.J., TROVATO A., VALLAGE B., VAN ELEWYCK V., VERSARI F., VIOLA S., VIVOLO D., WILMS J., ZEGARELLI A., ZORNOZA J.D. and ZUNIGA J.

Abstract (from CDS):

Addressing the origin of the astrophysical neutrino flux observed by IceCube is of paramount importance. Gamma-Ray Bursts (GRBs) are among the few astrophysical sources capable of achieving the required energy to contribute to such neutrino flux through pγ interactions. In this work, ANTARES data have been used to search for upward going muon neutrinos in spatial and temporal coincidence with 784 GRBs occurred from 2007 to 2017. For each GRB, the expected neutrino flux has been calculated in the framework of the internal shock model and the impact of the lack of knowledge on the majority of source redshifts and on other intrinsic parameters of the emission mechanism has been quantified. It is found that the model parameters that set the radial distance where shock collisions occur have the largest impact on neutrino flux expectations. In particular, the bulk Lorentz factor of the source ejecta and the minimum variability time-scale are found to contribute significantly to the GRB-neutrino flux uncertainty. For the selected sources, ANTARES data have been analysed by maximizing the discovery probability of the stacking sample through an extended maximum-likelihood strategy. Since no neutrino event passed the quality cuts set by the optimization procedure, 90 per cent confidence level upper limits (with their uncertainty) on the total expected diffuse neutrino flux have been derived, according to the model. The GRB contribution to the observed diffuse astrophysical neutrino flux around 100 TeV is constrained to be less than 10 per cent.

Abstract Copyright: © 2020 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

Journal keyword(s): acceleration of particles - neutrinos - transients: gamma-ray bursts - astroparticle physics

Simbad objects: 17

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Number of rows : 17
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 GRB 180720B gB 00 02 06.99 -02 55 07.8           ~ 215 0
2 GRB 140416A gB 02 22 +43.9           ~ 17 0
3 SN 2019oyw SN* 02 58 10.510 -08 57 27.20           ~ 218 0
4 GRB 190114C gB 03 38 01.18 -26 56 47.8           ~ 343 0
5 GRB 171010A gB 04 26 19.41 -10 27 47.9           SNIc-BL 109 0
6 Fermi bn100728095 gB 05 55 02.00 -15 15 20.2           ~ 157 0
7 Fermi bn140810782 gB 07 56 +27.5           ~ 19 0
8 GRB 081028 gB 08 07 34.40 +02 18 16.8           ~ 125 0
9 Fermi bn111228657 gB 10 00 16.04 +18 17 52.2           ~ 201 0
10 GRB 111123A gB 10 19 23.17 -20 38 41.9           ~ 83 0
11 SN 2013cq SN* 11 32 32.84 +27 41 56.2           SNIc 613 1
12 Fermi bn090720276 gB 13 34 46.6 -10 20 06           ~ 24 0
13 GRB 080212 gB 15 24 35.400 -22 44 29.50           ~ 58 0
14 Fermi bn100910818 gB 15 52.4 -34 37           ~ 17 0
15 GRB 110928A gB 17 10 55.91 +36 32 08.5           ~ 24 0
16 GRB 120707A gB 19 24 -34.4           ~ 21 0
17 GRB 141028A gB 21 30 24.46 -00 13 55.6           ~ 109 0

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