Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4460
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dc.contributor.authorGupta, Nayantara-
dc.date.accessioned2012-05-07T10:36:11Z-
dc.date.available2012-05-07T10:36:11Z-
dc.date.issued2002-06-
dc.identifier.citationPhysical Review D, 2002, Vol.65, p113005en
dc.identifier.issn1550-7998-
dc.identifier.issn1550-2368 (Online)-
dc.identifier.urihttp://hdl.handle.net/2289/4460-
dc.descriptionRestricted Access. An open-access version is available at arXiv.org (one of the alternative locations)en
dc.description.abstractThe number of neutrino induced upward going muons from a single gamma ray burst (GRB) expected to be detected by the proposed kilometer scale IceCube detector at the South Pole is calculated. The effects of the Lorentz factor, total energy of the GRB emitted in neutrinos and its distance from the observer (redshift) on the number of neutrino events from that GRB are examined. The present investigation reveals that there is the possibility of exploring the physical processes of the early universe with the proposed kilometer scale IceCube neutrino telescope.en
dc.language.isoenen
dc.publisherAmerican Physical Societyen
dc.relation.urihttp://adsabs.harvard.edu/abs/2002PhRvD..65k3005Gen
dc.relation.urihttp://arxiv.org/abs/astro-ph/0201509en
dc.relation.urihttp://dx.doi.org/10.1103/PhysRevD.65.113005en
dc.rights2002 The American Physical Societyen
dc.subjectgamma-ray sourcesen
dc.subjectgamma-ray burstsen
dc.subjectCosmic raysen
dc.titleNeutrino induced upward going muons from a gamma ray burst in a neutrino telescope of km2 areaen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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