Search for high-energy neutrinos from bright GRBs with ANTARES

Albert, A.; André, M.; Anghinolfi, M.; Anton, G.; Ardid, M.; Aubert, Jean-Jacques; Avgitas, T.; Baret, B.; Barrios-Martí, J.; Basa, S.; Bertín, V.; Biagi, S.; Bormuth, R.; Bourret, S.; Bouwhuis, M. C.; Bruijn, R.; Brünner, J.; Busto, J.; Capone, A.; Caramete, L.; Carr, J.; Celli, S.; Chiarusi, T.; Circella, M.; Coelho, J. A. B.; Coleiro, A.; Coniglione, R.; Costantini, H.; Coyle, P.; Creusot, A.; Deschamps, A.; Bonis, G. De; Distefano, C.; Palma, I. Di; Donzaud, C.; Dornic, D.; Drouhin, D.; Eberl, T.; Bojaddaini, I. El; Elsässer, Dominik; Enzenhöfer, A.; Fusco, L.; Galatà, S.; Geißelsöder, S.; Geyer, K.; Giordano, V.; Gleixner, A.; Glotin, Hervé; Grégoire, T.; Gracia-Ruiz, R.; Graf, Κ.; Hallmann, S.; Haren, Hans van; Heijboer, A.; Hello, Y.; Hernández-Rey, J. J.; Hößl, J.; Hofestädt, J.; Hugon, C.; Illuminati, G.; James, C. W.; Jong, M. de; Jongen, M.; Kadler, M.; Kalekin, O.; Katz, U.; Kießling, D.; Kouchner, A.; Kreter, M.; Kreykenbohm, I.; Kulikovskiy, V.; Lachaud, C.; Lahmann, R.; Lefèvre, D.; Leonora, E.; Lotze, Martín; Loucatos, S.; Marcelin, M.; Margiotta, A.; Marinelli, A.; Martínez-Mora, J. A.; Mathieu, A.; Mele, R.; Melis, K.; Michael, T.; Migliozzi, P.; Moussa, A.; Mueller, C. L.; Nezri, E.; Păvălaş, G. E.; Pellegrino, C.; Perrina, C.; Piattelli, P.; Popa, V.; Pradier, T.; Quinn, L.; Racca, C.; Riccobene, G.; Roensch, K.; Sánchez-Losa, A.; Saldaña, M.; Salvadori, I.; Samtleben, D. F. E.; Sanguineti, M.; Sapienza, P.; Schnabel, J.; Schüßler, F.; Seitz, T.; Sieger, C.; Spurio, M.; Stolarczyk, Th.; Taiuti, M.; Tayalati, Y.; Trovato, A.; Tselengidou, M.; Turpin, D.; Tönnis, Christoph; Vallage, B.; Vallée, C.; Elewyck, V. Van; Vivolo, D.; Vizzocca, A.; Wagner, S. J.; Wilms, J.; Zornoza, J.D.; Zúñiga, J.

doi:10.1093/mnras/stx902

Cited by 37 publications

(34 citation statements)

References 42 publications

Supporting

Mentioning

Contrasting

Order By: Relevance

“…For this search, the four brightest GRBs have been selected, and a dedicated optimization of the event selection criteria has been used. No neutrinos have been found in coincidence with the four bright gamma ray bursts, and upper limits have been derived [22].…”

Section: Latest Antares Resultsmentioning

confidence: 95%

ANTARES and KM3NeT: The Latest Results of the Neutrino Telescopes in the Mediterranean

Sanguineti¹

2019

Universe

View full text Add to dashboard Cite

The measurement of cosmic neutrinos is a new and unique method to observe the Universe. Neutrinos are chargeless, weakly-interacting particles that can provide information about the interior of an astrophysical object for cosmological distances. Indeed, they are a complementary probe with respect to other messengers such as multi-wavelength light and charged cosmic rays, allowing the observation of the far Universe and providing information on the production mechanism. Here, the neutrino telescopes in the Mediterranean Sea that are operating or in progress will be reviewed. The ANTARES (Astronomy with a Neutrino Telescope and Abyss environmental RESearch) detector is the largest neutrino telescope currently in operation in the Mediterranean Sea and the first operating in sea water. Some of the ANTARES results will be summarized, including diffuse, point-like, and multi-messenger source searches. Finally, the future km 3 -scale telescope KM3NeT (Cubic Kilometre Neutrino Telescope) will be described focusing on the expected performances and sensitivities.

show abstract

Section: Latest Antares Resultsmentioning

confidence: 95%

ANTARES and KM3NeT: The Latest Results of the Neutrino Telescopes in the Mediterranean

Sanguineti¹

2019

Universe

View full text Add to dashboard Cite

show abstract

“…From theoretical models, the timescale of the neutrino emission depends dramatically upon the type of sources. The hypothesis that the gamma ray burst are associated to a prompt neutrino emission (lasting a few hours or less) has been tested: the non-detection of coincident events between neutrinos and GRBs with IceCube [121,122] and ANTARES [123] data has led to important constraints on cosmic-ray acceleration in GRBs. Other episodic events of intense neutrino emission could at least in principle occur in AGN, and be associated, for example, also to accretion phenomena.…”

Section: Discussion and Prospectsmentioning

confidence: 99%

Neutrino Telescopes and High-Energy Cosmic Neutrinos

2020

View full text Add to dashboard Cite

In this review paper, we present the main aspects of high-energy cosmic neutrino astrophysics. We begin by describing the generic expectations for cosmic neutrinos, including the effects of propagation from their sources to the detectors. Then we introduce the operating principles of current neutrino telescopes, and examine the main features (topologies) of the observable events. After a discussion of the main background processes, due to the concomitant presence of secondary particles produced in the terrestrial atmosphere by cosmic rays, we summarize the current status of the observations with astrophysical relevance that have been greatly contributed by IceCube detector. Then, we examine various interpretations of these findings, trying to assess the best candidate sources of cosmic neutrinos. We conclude with a brief perspective on how the field could evolve within a few years.

show abstract

“…A search of neutrinos from four of the brightest GRBs visible by ANTARES between 2008 and 2013 (GRB080916C, GRB110918A, GRB130427A and GRB130505A) was also done [32] yielding to constrains of the internal shock and photospheric GRB model neutrino emissions.…”

Section: Off-line Analysesmentioning

confidence: 99%

Latest results on high-energy cosmic neutrino searches with the ANTARES neutrino telescope

Losa

2019

EPJ Web Conf.

View full text Add to dashboard Cite

The ANTARES detector is currently the largest undersea neutrino telescope. Located in the Mediterranean Sea at a depth of 2.5 km, 40 km off the Southern coast of France, it has been looking for cosmic neutrinos for more than 10 years. High-energy cosmic neutrino production is strongly linked with cosmic ray production. The latest results from IceCube Collaboration represent a step forward towards the confirmation of a highenergy cosmic ray source. The ANTARES location in the Northern Hemisphere is optimal for the observation of most of the Galactic Plane, including the Galactic Center. It has constrained the IceCube neutrino excess reports as well as, more recently, the flux from the source identified in the Blazar TXS 0506+056. The latest results of ANTARES on such analyses, including point-like and extended sources, diffuse fluxes, transient phenomena and multi-messenger studies, are presented.

show abstract

Search for high-energy neutrinos from bright GRBs with ANTARES

Cited by 37 publications

References 42 publications

ANTARES and KM3NeT: The Latest Results of the Neutrino Telescopes in the Mediterranean

ANTARES and KM3NeT: The Latest Results of the Neutrino Telescopes in the Mediterranean

Neutrino Telescopes and High-Energy Cosmic Neutrinos

Latest results on high-energy cosmic neutrino searches with the ANTARES neutrino telescope

Contact Info

Product

Resources

About