Neutrinos from pulsar wind bubbles as precursors to gamma-ray bursts

Jonathan Granot; Dafne Guetta

doi:10.1103/PhysRevLett.90.191102

Neutrinos from pulsar wind bubbles as precursors to gamma-ray bursts

Jonathan Granot
, Dafne Guetta

פרסום מחקרי: פרסום בכתב עת › מאמר › ביקורת עמיתים

18 ציטוטים ‏(Scopus)

תקציר

Neutrino production in the pulsar wind bubble (PWB) was considered in the context of the supranova model for gamma-ray bursts (GRBs). It was found that the ∼10 TeV neutrino fluence from a PWB at z∼0.1-1 implies ∼0.1-10 upward moving mouns in a km² detector.

שפה מקורית	אנגלית
מספר המאמר	191102
עמודים (מ-עד)	191102/1-191102/4
כתב עת	Physical Review Letters
כרך	90
מספר גיליון	19
מזהי עצם דיגיטלי (DOIs)	https://doi.org/10.1103/PhysRevLett.90.191102
סטטוס פרסום	פורסם - 16 מאי 2003
פורסם באופן חיצוני	כן

גישה למסמך

10.1103/PhysRevLett.90.191102

קבצים וקישורים אחרים

Link to publication in Scopus

פורמט ציטוט ביבליוגרפי

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title = "Neutrinos from pulsar wind bubbles as precursors to gamma-ray bursts",

abstract = "Neutrino production in the pulsar wind bubble (PWB) was considered in the context of the supranova model for gamma-ray bursts (GRBs). It was found that the ∼10 TeV neutrino fluence from a PWB at z∼0.1-1 implies ∼0.1-10 upward moving mouns in a km2 detector.",

author = "Jonathan Granot and Dafne Guetta",

note = "Funding Information: We thank P. Goldreich, A. K{\"o}nigl, E. Waxman, ?>A. Loeb, P. M{\'e}sz{\'a}ros, and C. Pe{\~n}a-Garay for useful discussions. J. G. is supported by the Institute for Advanced Study, funds for natural sciences. D. G. thanks the IAS in Princeton, for the hospitality and the nice working atmosphere during the course of this work.",

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AU - Granot, Jonathan

AU - Guetta, Dafne

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PY - 2003/5/16

Y1 - 2003/5/16

N2 - Neutrino production in the pulsar wind bubble (PWB) was considered in the context of the supranova model for gamma-ray bursts (GRBs). It was found that the ∼10 TeV neutrino fluence from a PWB at z∼0.1-1 implies ∼0.1-10 upward moving mouns in a km2 detector.

AB - Neutrino production in the pulsar wind bubble (PWB) was considered in the context of the supranova model for gamma-ray bursts (GRBs). It was found that the ∼10 TeV neutrino fluence from a PWB at z∼0.1-1 implies ∼0.1-10 upward moving mouns in a km2 detector.

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Neutrinos from pulsar wind bubbles as precursors to gamma-ray bursts

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