par  Aartsen, M. G.;Aguilar Sanchez, Juan Antonio  ;Hanson, Kael
;Hanson, Kael  ;Heereman von Zuydtwyck, David
;Heereman von Zuydtwyck, David  ;Meures, Thomas
;Meures, Thomas  ;O'Murchadha, Aongus
;O'Murchadha, Aongus  ;Pinat, Elisa
;Pinat, Elisa  ; [et al.]
; [et al.]
Référence The astrophysical journal. Letters, 805, 1, L5
Publication Publié, 2015-05
           ;Hanson, Kael
;Hanson, Kael  ;Heereman von Zuydtwyck, David
;Heereman von Zuydtwyck, David  ;Meures, Thomas
;Meures, Thomas  ;O'Murchadha, Aongus
;O'Murchadha, Aongus  ;Pinat, Elisa
;Pinat, Elisa  ; [et al.]
; [et al.]Référence The astrophysical journal. Letters, 805, 1, L5
Publication Publié, 2015-05
                                                                                                       
			Article révisé par les pairs
                                                  
        | Résumé : | We present constraints derived from a search of four years of IceCube data for a prompt neutrino flux from gamma-ray bursts (GRBs). A single low-significance neutrino, compatible with the atmospheric neutrino background, was found in coincidence with one of the 506 observed bursts. Although GRBs have been proposed as candidate sources for ultra-high-energy cosmic rays, our limits on the neutrino flux disfavor much of the parameter space for the latest models. We also find that no more than ∼1% of the recently observed astrophysical neutrino flux consists of prompt emission from GRBs that are potentially observable by existing satellites. | 



