Search for high energy neutrinos from bright GRBs with ANTARES

被引：0

作者：

Celli, S. ^{[1
,2
]}

Sanguineti, M. ^{[3
,4
]}

Turpin, D. ^{[5
]}

机构：

[1] Gran Sasso Sci Inst, Viale Francesco Crispi 7, I-67100 Laquila, Italy

[2] INFN, Sez Roma, Ple Aldo Moro 2, I-00185 Rome, Italy

[3] Univ Genoa, Dipartimento Fis, Via Dodecaneso 33, I-16146 Genoa, Italy

[4] INFN, Sez Genova, Via Dodecaneso 33, I-16146 Genoa, Italy

[5] Aix Marseille Univ, CNRS, IN2P3, CPPM,UMR 7346, F-13288 Marseille, France

来源：

XXVII INTERNATIONAL CONFERENCE ON NEUTRINO PHYSICS AND ASTROPHYSICS (NEUTRINO2016) | 2017年 / 888卷

关键词：

D O I：

10.1088/1742-6596/888/1/012100

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Gamma-ray bursts are thought to be cosmic-ray accelerators, thus neutrinos are expected from the decay of charged mesons, produced in p gamma interactions. The search for high-energy neutrinos from astrophysical sources is one of the main goals of the ANTARES scientific project. The methods and the results of a search for neutrinos from the brightest GRBs observed between 2008 and 2013 are presented. Two scenarios of the fireball model have been investigated: the internal shock and the photospheric case. Since no events have been detected in time and space coincidence with any of these bursts, upper limits at 90% C.L. on the expected neutrino fluxes are derived, as well as constraints on some parameters used in the modeling of the neutrino yield, as the bulk Lorentz factor Gamma of the jet and the baryon loading f(p).

引用

页数：3

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