Search for high energy neutrinos from bright GRBs with ANTARES

被引：0

作者：

Sanguineti, M. ^{[1
,2
]}

Celli, S. ^{[3
,4
]}

Turpin, D. ^{[5
]}

机构：

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

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

[3] Gran Sasso Sci Inst, Viale Francesco Crispi 7, I-00167 Laquila, Italy

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

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

来源：

RICAP16, 6TH ROMA INTERNATIONAL CONFERENCE ON ASTROPARTICLE PHYSICS | 2017年 / 136卷

关键词：

GAMMA-RAY BURSTS;

D O I：

10.1051/epjconf/201713604004

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Gamma-ray bursts are a possible site of hadronic acceleration, thus neutrinos are expected in correspondence of a GRB event. The brightest GRB observed between 2008 and 2013 (GRB080916C, GRB110918A, GRB130427A and GRB130505A) have been investigated using the data of the ANTARES high energy neutrino telescope. In this paper two of most promising models of the GRB neutrino emission will be studied: the internal shock model and the photospheric model. No muons have been measured in space and time correlation with the selected GRBs and upper limits at 90% C.L. on the expected neutrino fluxes have been derived. This measure allows also setting constraints on some parameters used in the modeling of the neutrino flux: the bulk Lorentz factor of the jet Gamma and the baryon loading f(p).

引用

页数：4

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