Please use this identifier to cite or link to this item:
https://hdl.handle.net/2440/76715
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Full metadata record
DC Field | Value | Language |
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dc.contributor.author | Abbasi, R. | - |
dc.contributor.author | Hill, G. | - |
dc.date.issued | 2011 | - |
dc.identifier.citation | Physical Review Letters, 2011; 14(7):1-5 | - |
dc.identifier.issn | 0031-9007 | - |
dc.identifier.issn | 1079-7114 | - |
dc.identifier.uri | http://hdl.handle.net/2440/76715 | - |
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. | - |
dc.description.statementofresponsibility | R. Abbasi ... G. C. Hill ... et al. (IceCube Collaboration) | - |
dc.language.iso | en | - |
dc.publisher | American Physical Soc | - |
dc.rights | © 2011 American Physical Society | - |
dc.source.uri | http://dx.doi.org/10.1103/physrevlett.106.141101 | - |
dc.subject | IceCube Collaboration | - |
dc.title | Limits on Neutrino emission from gamma-ray bursts with the 40 string IceCube detector | - |
dc.type | Journal article | - |
dc.identifier.doi | 10.1103/PhysRevLett.106.141101 | - |
pubs.publication-status | Published | - |
Appears in Collections: | Aurora harvest 4 Chemistry and Physics publications |
Files in This Item:
File | Description | Size | Format | |
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hdl_76715.pdf | Published version | 443.96 kB | Adobe PDF | View/Open |
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