@article{PAR00016180,
  title = {{S}earch for high-energy neutrinos from bright {GRB}s with {ANTARES}},
  author = {{A}lbert, {A}. and {A}ndre, {M}. and {A}nghinolfi, {M}. and {A}nton, {G}. and {A}rdid, {M}. and {A}ubert, {J}. {J}. and {A}vgitas, {T}. and {B}aret, {B}. and {B}arrios-{M}arti, {J}. and {B}asa, {S}. and {B}ertin, {V}. and {B}iagi, {S}. and {B}ormuth, {R}. and {B}ourret, {S}. and {B}ouwhuis, {M}. {C}. and {B}ruijn, {R}. and {B}runner, {J}. and {B}usto, {J}. and {C}apone, {A}. and {C}aramete, {L}. and {C}arr, {J}. and {C}elli, {S}. and {C}hiarusi, {T}. and {C}ircella, {M}. and {C}oelho, {J}. {A}. {B}. and {C}oleiro, {A}. and {C}oniglione, {R}. and {C}ostantini, {H}. and {C}oyle, {P}. and {C}reusot, {A}. and {D}eschamps, {A}. and {D}e {B}onis, {G}. and {D}istefano, {C}. and {D}i {P}alma, {I}. and {D}onzaud, {C}. and {D}ornic, {D}. and {D}rouhin, {D}. and {E}berl, {T}. and {E}l {B}ojaddaini, {I}. and {E}lsasser, {D}. and {E}nzenhofer, {A}. and {F}elis, {I}. and {F}usco, {L}. {A}. and {G}alata, {S}. and {G}ay, {P}. and {G}eisseloder, {S}. and {G}eyer, {K}. and {G}iordano, {V}. and {G}leixner, {A}. and {G}lotin, {H}. and {G}regoire, {T}. and {G}racia-{R}uiz, {R}. and {G}raf, {K}. and {H}allmann, {S}. and van {H}aren, {H}. and {H}eijboer, {A}. {J}. and {H}ello, {Y}ann and et al.},
  editor = {},
  language = {{ENG}},
  abstract = {{G}amma-ray bursts are thought to be sites of hadronic acceleration, thus neutrinos are expected from the decay of charged particles, produced in p gamma interactions. {T}he methods and results of a search for muon neutrinos in the data of the {ANTARES} neutrino telescope from four bright {GRB}s ({GRB} 080916{C}, {GRB} 110918{A}, {GRB} 130427{A} and {GRB} 130505{A}) observed between 2008 and 2013 are presented. {T}wo scenarios of the fireball model have been investigated: the internal shock scenario, leading to the production of neutrinos with energies mainly above 100 {T}e{V}, and the photospheric scenario, characterized by a low-energy component in neutrino spectra due to the assumption of neutrino production closer to the central engine. {S}ince no neutrino events have been detected in temporal and spatial coincidence with these bursts, upper limits at 90 per cent confidence level on the expected neutrino fluxes are derived. {T}he non-detection allows for directly constraining the bulk {L}orentz factor of the jet {G}amma and the baryon loading f(p).},
  keywords = {acceleration of particles ; neutrinos ; gamma-ray burst: individual: {GRB} ; 080916{C} ; gamma-ray burst: individual: {GRB} 110918{A} ; gamma-ray burst: ; individual: {GRB} 130427{A} ; gamma-ray burst: individual: {GRB} 130505{A}},
  booktitle = {},
  journal = {{M}onthly {N}otices of the {R}oyal {A}stronomical {S}ociety},
  volume = {469},
  numero = {1},
  pages = {906--915},
  ISSN = {0035-8711},
  year = {2017},
  DOI = {10.1093/mnras/stx902},
  URL = {https://www.documentation.ird.fr/hor/{PAR}00016180},
}