000293258 001__ 293258
000293258 005__ 20250730113847.0
000293258 0247_ $$2doi$$a10.1038/ncomms7783
000293258 0247_ $$2WOS$$aWOS:000353702500023
000293258 0247_ $$2pmid$$apmid:25858274
000293258 0247_ $$2altmetric$$aaltmetric:3896662
000293258 0247_ $$2inspire$$ainspire:1315770
000293258 0247_ $$2arXiv$$aarXiv:1409.2874
000293258 0247_ $$2openalex$$aopenalex:W1976228239
000293258 037__ $$aPUBDB-2016-00413
000293258 082__ $$a500
000293258 088__ $$2arXiv$$aarXiv:1409.2874
000293258 1001_ $$0P:(DE-HGF)0$$aBustamante, Mauricio$$b0$$eCorresponding author
000293258 245__ $$aNeutrino and cosmic-ray emission from multiple internal shocks in gamma-ray bursts
000293258 260__ $$aLondon$$bNature Publishing Group$$c2015
000293258 3367_ $$2DRIVER$$aarticle
000293258 3367_ $$2DataCite$$aOutput Types/Journal article
000293258 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$bjournal$$mjournal$$s1598607954_15993
000293258 3367_ $$2BibTeX$$aARTICLE
000293258 3367_ $$2ORCID$$aJOURNAL_ARTICLE
000293258 3367_ $$00$$2EndNote$$aJournal Article
000293258 500__ $$aOA
000293258 520__ $$aGamma-ray bursts (GRBs) are short-lived, luminous explosions at cosmological distances, thought to originate from relativistic jets launched at the deaths of massive stars. They are among the prime candidates to produce the observed cosmic rays at the highest energies. Recent neutrino data have, however, started to constrain this possibility in the simplest models with only one emission zone. In the classical theory of GRBs, it is expected that particles are accelerated at mildly relativistic shocks generated by the collisions of material ejected from a central engine. Here we consider neutrino and cosmic-ray emission from multiple emission regions since these internal collisions must occur at very different radii, from below the photosphere all the way out to the circumburst medium, as a consequence of the efficient dissipation of kinetic energy. We demonstrate that the different messengers originate from different collision radii, which means that multi-messenger observations open windows for revealing the evolving GRB outflows.
000293258 536__ $$0G:(DE-HGF)POF2-523$$a523 - High-energy gamma ray astronomy (POF2-523)$$cPOF2-523$$fPOF II$$x0
000293258 588__ $$aDataset connected to CrossRef
000293258 693__ $$0EXP:(DE-MLZ)NOSPEC-20140101$$5EXP:(DE-MLZ)NOSPEC-20140101$$eNo specific instrument$$x0
000293258 7001_ $$aBaerwald, Philipp$$b1
000293258 7001_ $$aMurase, Kohta$$b2
000293258 7001_ $$0P:(DE-H253)PIP1021242$$aWinter, Walter$$b3
000293258 773__ $$0PERI:(DE-600)2553671-0$$a10.1038/ncomms7783$$gVol. 6, p. 6783 -$$p6783 -$$tNature Communications$$v6$$x2041-1723$$y2015
000293258 7870_ $$0PUBDB-2015-00416$$aBustamante, Mauricio et.al.$$d2014$$iIsParent$$rarXiv:1409.2874$$tNeutrino and Cosmic-Ray Emission from Multiple Internal Shocks in Gamma-Ray Bursts
000293258 8564_ $$uhttps://bib-pubdb1.desy.de/record/293258/files/ncomms7783.pdf$$yOpenAccess
000293258 8564_ $$uhttps://bib-pubdb1.desy.de/record/293258/files/ncomms7783.gif?subformat=icon$$xicon$$yOpenAccess
000293258 8564_ $$uhttps://bib-pubdb1.desy.de/record/293258/files/ncomms7783.jpg?subformat=icon-1440$$xicon-1440$$yOpenAccess
000293258 8564_ $$uhttps://bib-pubdb1.desy.de/record/293258/files/ncomms7783.jpg?subformat=icon-180$$xicon-180$$yOpenAccess
000293258 8564_ $$uhttps://bib-pubdb1.desy.de/record/293258/files/ncomms7783.jpg?subformat=icon-640$$xicon-640$$yOpenAccess
000293258 8564_ $$uhttps://bib-pubdb1.desy.de/record/293258/files/ncomms7783.pdf?subformat=pdfa$$xpdfa$$yOpenAccess
000293258 909CO $$ooai:bib-pubdb1.desy.de:293258$$pdnbdelivery$$pdriver$$pVDB$$popen_access$$popenaire
000293258 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-HGF)0$$aDeutsches Elektronen-Synchrotron$$b0$$kDESY
000293258 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1021242$$aDeutsches Elektronen-Synchrotron$$b3$$kDESY
000293258 9132_ $$0G:(DE-HGF)POF3-613$$1G:(DE-HGF)POF3-610$$2G:(DE-HGF)POF3-600$$aDE-HGF$$bForschungsbereich Materie$$lMaterie und Universum$$vMatter and Radiation from the Universe$$x0
000293258 9131_ $$0G:(DE-HGF)POF2-523$$1G:(DE-HGF)POF2-520$$2G:(DE-HGF)POF2-500$$3G:(DE-HGF)POF2$$4G:(DE-HGF)POF$$aDE-HGF$$bStruktur der Materie$$lAstroteilchenphysik$$vHigh-energy gamma ray astronomy$$x1
000293258 9141_ $$y2015
000293258 915__ $$0StatID:(DE-HGF)0200$$2StatID$$aDBCoverage$$bSCOPUS
000293258 915__ $$0StatID:(DE-HGF)1030$$2StatID$$aDBCoverage$$bCurrent Contents - Life Sciences
000293258 915__ $$0LIC:(DE-HGF)CCBY4$$2V:(DE-HGF)$$aCreative Commons Attribution CC BY 4
000293258 915__ $$0StatID:(DE-HGF)1040$$2StatID$$aDBCoverage$$bZoological Record
000293258 915__ $$0StatID:(DE-HGF)0100$$2StatID$$aJCR$$bNAT COMMUN : 2014
000293258 915__ $$0StatID:(DE-HGF)9910$$2StatID$$aIF >= 10$$bNAT COMMUN : 2014
000293258 915__ $$0StatID:(DE-HGF)1150$$2StatID$$aDBCoverage$$bCurrent Contents - Physical, Chemical and Earth Sciences
000293258 915__ $$0StatID:(DE-HGF)0150$$2StatID$$aDBCoverage$$bWeb of Science Core Collection
000293258 915__ $$0StatID:(DE-HGF)0110$$2StatID$$aWoS$$bScience Citation Index
000293258 915__ $$0StatID:(DE-HGF)0111$$2StatID$$aWoS$$bScience Citation Index Expanded
000293258 915__ $$0StatID:(DE-HGF)0510$$2StatID$$aOpenAccess
000293258 915__ $$0StatID:(DE-HGF)0500$$2StatID$$aOpenAccess
000293258 915__ $$0StatID:(DE-HGF)1060$$2StatID$$aDBCoverage$$bCurrent Contents - Agriculture, Biology and Environmental Sciences
000293258 915__ $$0StatID:(DE-HGF)0310$$2StatID$$aDBCoverage$$bNCBI Molecular Biology Database
000293258 915__ $$0StatID:(DE-HGF)1050$$2StatID$$aDBCoverage$$bBIOSIS Previews
000293258 915__ $$0StatID:(DE-HGF)0300$$2StatID$$aDBCoverage$$bMedline
000293258 915__ $$0StatID:(DE-HGF)0560$$2StatID$$aOpenAccess / APC funded
000293258 915__ $$0StatID:(DE-HGF)0199$$2StatID$$aDBCoverage$$bThomson Reuters Master Journal List
000293258 9201_ $$0I:(DE-H253)Z_THAT-20210408$$kZ_THAT$$lTheoretische Astroteilchenphysik$$x0
000293258 980__ $$ajournal
000293258 980__ $$aVDB
000293258 980__ $$aUNRESTRICTED
000293258 980__ $$aI:(DE-H253)Z_THAT-20210408
000293258 9801_ $$aUNRESTRICTED
000293258 9801_ $$aFullTexts