Please use this identifier to cite or link to this item:
http://hdl.handle.net/2289/5578
Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Bhattacharjee, Pijushpani | - |
dc.contributor.author | Gupta, Nayantara | - |
dc.date.accessioned | 2013-05-15T08:51:01Z | - |
dc.date.available | 2013-05-15T08:51:01Z | - |
dc.date.issued | 2004-03 | - |
dc.identifier.citation | Pramana, 2004, Vol.62, p789 | en |
dc.identifier.issn | 0304-4289 | - |
dc.identifier.issn | 0973-7111(Online) | - |
dc.identifier.uri | http://hdl.handle.net/2289/5578 | - |
dc.description | Open Access. | en |
dc.description.abstract | Gamma ray bursts (GRBs) have been proposed as one possible class of sources of the ultrahigh energy cosmic ray (UHECR) events observed up to energies gtrsim 10^{20} eV. The synchrotron radiation of the highest energy protons accelerated within the GRB source should produce gamma rays up to TeV energies. Here we briefly discuss the implications on the energetics of the GRB from the point of view of the detectability of the prompt TeV gamma-rays of proton-synchrotron origin in GRBs in the up-coming ICECUBE muon detector in the south pole. | en |
dc.language.iso | en | en |
dc.publisher | Springer Verlag | en |
dc.relation.uri | http://adsabs.harvard.edu/abs/2004Prama..62..789B | en |
dc.relation.uri | http://arxiv.org/abs/astro-ph/0305185 | en |
dc.relation.uri | http://dx.doi.org/10.1007/BF02705371 | en |
dc.rights | 2004 Springer Verlag | en |
dc.title | Ultra-high energy cosmic rays and prompt TeV gamma rays from gamma ray bursts | en |
dc.type | Article | en |
Appears in Collections: | Research Papers (A&A) |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
2004_Pramana_Vol.62_p789.pdf Restricted Access | Open Access | 129.91 kB | Adobe PDF | View/Open Request a copy |
Items in RRI Digital Repository are protected by copyright, with all rights reserved, unless otherwise indicated.