ANTARES upper limits on the multi-TeV neutrino emission from the GRBs   detected by IACTs

ANTARES Collaboration: A. Albert; M. Andr\'e; M. Anghinolfi; G. Anton,; M. Ardid; J.-J. Aubert; J. Aublin; B. Baret; S. Basa; B. Belhorma; V. Bertin,; S. Biagi; M. Bissinger; J. Boumaaza; M. Bouta; M.C. Bouwhuis; H.; Br\^anza\c{s}; R. Bruijn; J. Brunner; J. Busto; A. Capone; L. Caramete; J.; Carr; V. Carretero; S. Celli; M. Chabab; T. N. Chau; R. Cherkaoui El Moursli,; T. Chiarusi; M. Circella; A. Coleiro; M. Colomer-Molla; R. Coniglione; P.; Coyle; A. Creusot; A. F. D\'iaz; G. de Wasseige; A. Deschamps; C. Distefano,; I. Di Palma; A. Domi; C. Donzaud; D. Dornic; D. Drouhin; T. Eberl; N. El; Khayati; A. Enzenh\"ofer; A. Ettahiri; P. Fermani; G. Ferrara; F. Filippini,; L. Fusco; R. Garc\'ia; P. Gay; H. Glotin; R. Gozzini; K. Graf; C. Guidi; S.; Hallmann; H. van Haren; A.J. Heijboer; Y. Hello; J.J. Hern\'andez-Rey; J.; H\"o{\ss}l; J. Hofest\"adt; F. Huang; G. Illuminati; C. W. James; B.; Jisse-Jung; M. de Jong; P. de Jong; M. Jongen; M. Kadler; O. Kalekin; U.; Katz; N.R. Khan-Chowdhury; A. Kouchner; I. Kreykenbohm; V. Kulikovskiy; R.; Lahmann; R. Le Breton; D. Lef\`evre; E. Leonora; G. Levi; M. Lincetto; D.; Lopez-Coto; S. Loucatos; L. Maderer; J. Manczak; M. Marcelin; A. Margiotta,; A. Marinelli; J.A. Mart\'inez-Mora; S. Mazzou; K. Melis; P. Migliozzi; M.; Moser; A. Moussa; R. Muller; L. Nauta; S. Navas; E. Nezri; A.; Nu\~nez-Casti\~neyra; B. O'Fearraigh; M. Organokov; G.E. P\u{a}v\u{a}la\c{s},; C. Pellegrino; M. Perrin-Terrin; P. Piattelli; C. Pieterse; C. Poir\`e; V.; Popa; T. Pradier; N. Randazzo; S. Reck; G. Riccobene; A. S\'anchez-Losa; D.; F. E. Samtleben; M. Sanguineti; P. Sapienza; J. Schnabel; F. Sch\"ussler; M.; Spurio; Th. Stolarczyk; M. Taiuti; Y. Tayalati; T. Thakore; S.J. Tingay; B.; Vallage; V. Van Elewyck; F. Versari; S. Viola; D. Vivolo; J. Wilms; A.; Zegarelli; J.D. Zornoza; J. Z\'u\~niga

arXiv:2011.11411·astro-ph.HE·March 31, 2021

ANTARES upper limits on the multi-TeV neutrino emission from the GRBs detected by IACTs

ANTARES Collaboration: A. Albert, M. Andr\'e, M. Anghinolfi, G. Anton,, M. Ardid, J.-J. Aubert, J. Aublin, B. Baret, S. Basa, B. Belhorma, V. Bertin,, S. Biagi, M. Bissinger, J. Boumaaza, M. Bouta, M.C. Bouwhuis, H., Br\^anza\c{s}, R. Bruijn, J. Brunner, J. Busto, A. Capone

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TL;DR

This study used ANTARES data to search for neutrinos coinciding with three gamma-ray bursts detected by IACTs, but found no neutrinos, setting upper limits that do not constrain existing models.

Contribution

First dedicated search for neutrinos in coincidence with recent IACT-detected GRBs using ANTARES, establishing upper limits on neutrino emission.

Findings

01

No neutrinos detected in coincidence with the GRBs

02

Upper limits are above gamma-ray emission levels

03

Results do not constrain current neutrino emission models

Abstract

The first gamma-ray burst detections by Imaging Atmospheric Cherenkov Telescopes have been recently announced: GRB 190114C, detected by MAGIC, GRB 180720B and GRB 190829A, observed by H.E.S.S. A dedicated search for neutrinos in space and time coincidence with the gamma-ray emission observed by IACTs has been performed using ANTARES data. The search covers both the prompt and afterglow phases, yielding no neutrinos in coincidence with the three GRBs studied. Upper limits on the energetics of the neutrino emission are inferred. The resulting upper limits are several orders of magnitude above the observed gamma-ray emission, and they do not allow to constrain the available models.

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