FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1994504013> ?p ?o ?g. }

• W1994504013 endingPage "29" @default.
• W1994504013 startingPage "19" @default.
• W1994504013 abstract "We calculate the flux of neutrinos generated by the propagation of ultra-high energy iron over cosmological distances and show that even if ultra-high energy cosmic rays are composed of heavy nuclei, a significant flux of high-energy neutrinos should be present throughout the universe. The resulting neutrino flux has a new peak at ∼1014 eV generated by neutron decay and reproduces the double peak structure due to photopion production at higher energies (∼1018 eV). Depending on the maximum energy and cosmological evolution of extremely high energy cosmic accelerators the generated neutrino flux can be detected by future experiments." @default.
• W1994504013 created "2016-06-24" @default.
• W1994504013 creator A5002454518 @default.
• W1994504013 creator A5026999404 @default.
• W1994504013 creator A5053874234 @default.
• W1994504013 creator A5065816081 @default.
• W1994504013 creator A5080982135 @default.
• W1994504013 date "2005-02-01" @default.
• W1994504013 modified "2023-10-03" @default.
• W1994504013 title "Cosmogenic neutrinos from ultra-high energy nuclei" @default.
• W1994504013 cites W1570459158 @default.
• W1994504013 cites W1647766962 @default.
• W1994504013 cites W1971013739 @default.
• W1994504013 cites W1986014666 @default.
• W1994504013 cites W1987808862 @default.
• W1994504013 cites W1998174391 @default.
• W1994504013 cites W2008787083 @default.
• W1994504013 cites W2015169265 @default.
• W1994504013 cites W2020834529 @default.
• W1994504013 cites W2025229797 @default.
• W1994504013 cites W2030501080 @default.
• W1994504013 cites W2044612502 @default.
• W1994504013 cites W2049899114 @default.
• W1994504013 cites W2054246448 @default.
• W1994504013 cites W2057751156 @default.
• W1994504013 cites W2067136643 @default.
• W1994504013 cites W2077722377 @default.
• W1994504013 cites W2080223834 @default.
• W1994504013 cites W2085023683 @default.
• W1994504013 cites W2088664089 @default.
• W1994504013 cites W2104948382 @default.
• W1994504013 cites W2116429900 @default.
• W1994504013 cites W2118265220 @default.
• W1994504013 cites W2126588894 @default.
• W1994504013 cites W2132636807 @default.
• W1994504013 cites W2136501176 @default.
• W1994504013 cites W2140537989 @default.
• W1994504013 cites W2140887005 @default.
• W1994504013 cites W3102293548 @default.
• W1994504013 cites W3103273060 @default.
• W1994504013 cites W3123491491 @default.
• W1994504013 doi "https://doi.org/10.1016/j.astropartphys.2004.11.001" @default.
• W1994504013 hasPublicationYear "2005" @default.
• W1994504013 type Work @default.
• W1994504013 sameAs 1994504013 @default.
• W1994504013 citedByCount "103" @default.
• W1994504013 countsByYear W19945040132012 @default.
• W1994504013 countsByYear W19945040132013 @default.
• W1994504013 countsByYear W19945040132014 @default.
• W1994504013 countsByYear W19945040132015 @default.
• W1994504013 countsByYear W19945040132016 @default.
• W1994504013 countsByYear W19945040132017 @default.
• W1994504013 countsByYear W19945040132018 @default.
• W1994504013 countsByYear W19945040132019 @default.
• W1994504013 countsByYear W19945040132020 @default.
• W1994504013 countsByYear W19945040132021 @default.
• W1994504013 countsByYear W19945040132022 @default.
• W1994504013 countsByYear W19945040132023 @default.
• W1994504013 crossrefType "journal-article" @default.
• W1994504013 hasAuthorship W1994504013A5002454518 @default.
• W1994504013 hasAuthorship W1994504013A5026999404 @default.
• W1994504013 hasAuthorship W1994504013A5053874234 @default.
• W1994504013 hasAuthorship W1994504013A5065816081 @default.
• W1994504013 hasAuthorship W1994504013A5080982135 @default.
• W1994504013 hasBestOaLocation W19945040132 @default.
• W1994504013 hasConcept C107966497 @default.
• W1994504013 hasConcept C109214941 @default.
• W1994504013 hasConcept C111309251 @default.
• W1994504013 hasConcept C121332964 @default.
• W1994504013 hasConcept C132221716 @default.
• W1994504013 hasConcept C152568617 @default.
• W1994504013 hasConcept C185544564 @default.
• W1994504013 hasConcept C186453547 @default.
• W1994504013 hasConcept C187379410 @default.
• W1994504013 hasConcept C191897082 @default.
• W1994504013 hasConcept C192562407 @default.
• W1994504013 hasConcept C2985973956 @default.
• W1994504013 hasConcept C44870925 @default.
• W1994504013 hasConcept C68709404 @default.
• W1994504013 hasConcept C84999194 @default.
• W1994504013 hasConceptScore W1994504013C107966497 @default.
• W1994504013 hasConceptScore W1994504013C109214941 @default.
• W1994504013 hasConceptScore W1994504013C111309251 @default.
• W1994504013 hasConceptScore W1994504013C121332964 @default.
• W1994504013 hasConceptScore W1994504013C132221716 @default.
• W1994504013 hasConceptScore W1994504013C152568617 @default.
• W1994504013 hasConceptScore W1994504013C185544564 @default.
• W1994504013 hasConceptScore W1994504013C186453547 @default.
• W1994504013 hasConceptScore W1994504013C187379410 @default.
• W1994504013 hasConceptScore W1994504013C191897082 @default.
• W1994504013 hasConceptScore W1994504013C192562407 @default.
• W1994504013 hasConceptScore W1994504013C2985973956 @default.
• W1994504013 hasConceptScore W1994504013C44870925 @default.
• W1994504013 hasConceptScore W1994504013C68709404 @default.
• W1994504013 hasConceptScore W1994504013C84999194 @default.
• W1994504013 hasIssue "1" @default.
• W1994504013 hasLocation W19945040131 @default.
• W1994504013 hasLocation W19945040132 @default.

• next