Matches in SemOpenAlex for { <https://semopenalex.org/work/W2001995222> ?p ?o ?g. }
- W2001995222 abstract "In this article we examine the hypothesis that the highest energy cosmic rays are complex nuclei from extragalactic sources. Under reasonable physical assumptions, we show that the nearby metally rich starburst galaxies (M82 and NGC 253) can produce all the events observed above the ankle. This requires diffusion of particles below $10^{20}$ eV in extragalactic magnetic fields $B approx 15$ nG. Above $10^{19}$ eV, the model predicts the presence of significant fluxes of medium mass and heavy nuclei with small rate of change of composition. Notwithstanding, the most salient feature of the starburst-hypothesis is a slight anisotropy induced by iron debris just before the spectrum-cutoff." @default.
- W2001995222 created "2016-06-24" @default.
- W2001995222 creator A5056332130 @default.
- W2001995222 creator A5065873945 @default.
- W2001995222 creator A5066495992 @default.
- W2001995222 creator A5070861259 @default.
- W2001995222 date "2001-11-26" @default.
- W2001995222 modified "2023-09-25" @default.
- W2001995222 title "Extragalactic sources for ultrahigh energy cosmic ray nuclei" @default.
- W2001995222 cites W1570459158 @default.
- W2001995222 cites W1964306313 @default.
- W2001995222 cites W1984436283 @default.
- W2001995222 cites W1986014666 @default.
- W2001995222 cites W1989815304 @default.
- W2001995222 cites W1990694915 @default.
- W2001995222 cites W1993167844 @default.
- W2001995222 cites W1993608814 @default.
- W2001995222 cites W1994794528 @default.
- W2001995222 cites W1996713538 @default.
- W2001995222 cites W1998174391 @default.
- W2001995222 cites W2004310296 @default.
- W2001995222 cites W2006206882 @default.
- W2001995222 cites W2007199474 @default.
- W2001995222 cites W2011354505 @default.
- W2001995222 cites W2020212004 @default.
- W2001995222 cites W2033643370 @default.
- W2001995222 cites W2038158971 @default.
- W2001995222 cites W2045603145 @default.
- W2001995222 cites W2051233944 @default.
- W2001995222 cites W2052276106 @default.
- W2001995222 cites W2055541941 @default.
- W2001995222 cites W2057751156 @default.
- W2001995222 cites W2064221922 @default.
- W2001995222 cites W2070433795 @default.
- W2001995222 cites W2071572174 @default.
- W2001995222 cites W2072201065 @default.
- W2001995222 cites W2075051312 @default.
- W2001995222 cites W2088841343 @default.
- W2001995222 cites W2098745975 @default.
- W2001995222 cites W2102597554 @default.
- W2001995222 cites W2116429900 @default.
- W2001995222 cites W2136501176 @default.
- W2001995222 cites W2138310146 @default.
- W2001995222 cites W2141775111 @default.
- W2001995222 cites W2155391059 @default.
- W2001995222 cites W2171691780 @default.
- W2001995222 cites W2949507200 @default.
- W2001995222 cites W3098450652 @default.
- W2001995222 cites W3102293548 @default.
- W2001995222 cites W3103088100 @default.
- W2001995222 cites W3103273060 @default.
- W2001995222 cites W3104120054 @default.
- W2001995222 cites W3104679153 @default.
- W2001995222 cites W3105220337 @default.
- W2001995222 cites W3124862688 @default.
- W2001995222 doi "https://doi.org/10.1103/physrevd.64.123004" @default.
- W2001995222 hasPublicationYear "2001" @default.
- W2001995222 type Work @default.
- W2001995222 sameAs 2001995222 @default.
- W2001995222 citedByCount "14" @default.
- W2001995222 countsByYear W20019952222016 @default.
- W2001995222 countsByYear W20019952222018 @default.
- W2001995222 countsByYear W20019952222022 @default.
- W2001995222 crossrefType "journal-article" @default.
- W2001995222 hasAuthorship W2001995222A5056332130 @default.
- W2001995222 hasAuthorship W2001995222A5065873945 @default.
- W2001995222 hasAuthorship W2001995222A5066495992 @default.
- W2001995222 hasAuthorship W2001995222A5070861259 @default.
- W2001995222 hasBestOaLocation W20019952222 @default.
- W2001995222 hasConcept C111309251 @default.
- W2001995222 hasConcept C121332964 @default.
- W2001995222 hasConcept C1276947 @default.
- W2001995222 hasConcept C2778217198 @default.
- W2001995222 hasConcept C44870925 @default.
- W2001995222 hasConcept C62520636 @default.
- W2001995222 hasConcept C85725439 @default.
- W2001995222 hasConcept C98444146 @default.
- W2001995222 hasConceptScore W2001995222C111309251 @default.
- W2001995222 hasConceptScore W2001995222C121332964 @default.
- W2001995222 hasConceptScore W2001995222C1276947 @default.
- W2001995222 hasConceptScore W2001995222C2778217198 @default.
- W2001995222 hasConceptScore W2001995222C44870925 @default.
- W2001995222 hasConceptScore W2001995222C62520636 @default.
- W2001995222 hasConceptScore W2001995222C85725439 @default.
- W2001995222 hasConceptScore W2001995222C98444146 @default.
- W2001995222 hasIssue "12" @default.
- W2001995222 hasLocation W20019952221 @default.
- W2001995222 hasLocation W20019952222 @default.
- W2001995222 hasOpenAccess W2001995222 @default.
- W2001995222 hasPrimaryLocation W20019952221 @default.
- W2001995222 hasRelatedWork W1641631973 @default.
- W2001995222 hasRelatedWork W1690707023 @default.
- W2001995222 hasRelatedWork W2037983614 @default.
- W2001995222 hasRelatedWork W2101070158 @default.
- W2001995222 hasRelatedWork W2144397903 @default.
- W2001995222 hasRelatedWork W2963316917 @default.
- W2001995222 hasRelatedWork W3102549633 @default.
- W2001995222 hasRelatedWork W3102816282 @default.
- W2001995222 hasRelatedWork W4308191026 @default.
- W2001995222 hasRelatedWork W4313591799 @default.