Limits on Neutrino Emission from Gamma-Ray Bursts with the 40 String IceCube Detector

Show simple item record

dc.contributor.author Santander, Marcos
dc.date.accessioned 2019-07-02T21:22:11Z
dc.date.available 2019-07-02T21:22:11Z
dc.date.issued 2011-04-07
dc.identifier.citation Abbasi, R., et al. (2011): Limits on Neutrino Emission from Gamma-Ray Bursts with the 40 String IceCube Detector. Physical Review Letters, 106(14). DOI: http://dx.doi.org/10.1103/PhysRevLett.106.141101 en_US
dc.identifier.uri http://ir.ua.edu/handle/123456789/5881
dc.description.abstract IceCube has become the first neutrino telescope with a sensitivity below the TeV neutrino flux predicted from gamma-ray bursts if gamma-ray bursts are responsible for the observed cosmic-ray flux above 10¹⁸ eV. Two separate analyses using the half-complete IceCube detector, one a dedicated search for neutrinos from pγ interactions in the prompt phase of the gamma-ray burst fireball and the other a generic search for any neutrino emission from these sources over a wide range of energies and emission times, produced no evidence for neutrino emission, excluding prevailing models at 90% confidence. en_US
dc.format.mimetype application/pdf en_US
dc.language English en_US
dc.subject γ-ray sources; γ-ray bursts en_US
dc.subject Neutrino, muon, pion, and other elementary particles; cosmic rays en_US
dc.subject Cosmic rays (including sources, origin, acceleration, and interactions) en_US
dc.title Limits on Neutrino Emission from Gamma-Ray Bursts with the 40 String IceCube Detector en_US
dc.type text en_US


Files in this item

This item appears in the following Collection(s)

Show simple item record

Search DSpace


Browse

My Account