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An absence of neutrinos associated with cosmic-ray acceleration in γ-ray bursts

Abstract:

Very energetic astrophysical events are required to accelerate cosmic rays to above 1018 electronvolts. GRBs (γ-ray bursts) have been proposed as possible candidate sources1,2,3. In the GRB ‘fireball’ model, cosmic-ray acceleration should be accompanied by neutrinos produced in the decay of charged pions created in interactions between the high-energy cosmic-ray protons and γ-rays4. Previous searches for such neutrinos found no...

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Publication status:
Published
Peer review status:
Peer reviewed

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Files:
Publisher copy:
10.1038/nature11068

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Publisher:
Springer Nature Publisher's website
Journal:
Nature Journal website
Volume:
484
Issue:
7394
Pages:
351-354
Publication date:
2012-04-18
Acceptance date:
2012-03-08
DOI:
EISSN:
1476-4687
ISSN:
0028-0836
Source identifiers:
325257
Keywords:
Pubs id:
pubs:325257
UUID:
uuid:41e141f1-c824-4a0a-bc5a-f268ede8c331
Local pid:
pubs:325257
Deposit date:
2017-08-16

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