Matches in SemOpenAlex for { <https://semopenalex.org/work/W4367333085> ?p ?o ?g. }
- W4367333085 endingPage "04001" @default.
- W4367333085 startingPage "04001" @default.
- W4367333085 abstract "Understanding the acceleration of Ultra High Energy Cosmic Rays is one of the great challenges of contemporary astrophysics. In this short review, we summarize the general observational constraints on their composition, spectrum and isotropy which indicate that nuclei heavier than single protons dominate their spectra above $sim 5,{rm EeV}$, that they are strongly suppressed above energies $sim50,{rm EeV}$, and that the only significant departure from isotropy is a dipole. Constraints based upon photopion and photodisintegration losses allow their ranges and luminosity density to be estimated. Three general classes of source model are discussed - magnetospheric models (including neutron stars and black holes), jet models (including Gamma Ray Bursts, Active Galactic Nuclei and Tidal Disruption Events) and Diffusive Shock Acceleration models (involving large accretion shocks around rich clusters of galaxies). The value of constructing larger and more capable arrays to measure individual masses at the highest energies and probably identifying their sources is emphasized." @default.
- W4367333085 created "2023-04-30" @default.
- W4367333085 creator A5035206337 @default.
- W4367333085 creator A5035555064 @default.
- W4367333085 date "2023-01-01" @default.
- W4367333085 modified "2023-09-26" @default.
- W4367333085 title "Ultra High Energy Cosmic Ray Source Models: Successes, Challenges and General Predictions" @default.
- W4367333085 cites W1480366033 @default.
- W4367333085 cites W1567969845 @default.
- W4367333085 cites W1793559938 @default.
- W4367333085 cites W1974226674 @default.
- W4367333085 cites W1983072771 @default.
- W4367333085 cites W1992960149 @default.
- W4367333085 cites W1998174391 @default.
- W4367333085 cites W2008748006 @default.
- W4367333085 cites W2015750713 @default.
- W4367333085 cites W2026078995 @default.
- W4367333085 cites W2063712348 @default.
- W4367333085 cites W2086411872 @default.
- W4367333085 cites W2089918076 @default.
- W4367333085 cites W2138672762 @default.
- W4367333085 cites W2148111402 @default.
- W4367333085 cites W2161657246 @default.
- W4367333085 cites W2165331371 @default.
- W4367333085 cites W2340649795 @default.
- W4367333085 cites W2461160318 @default.
- W4367333085 cites W2757328851 @default.
- W4367333085 cites W2898932633 @default.
- W4367333085 cites W2910952808 @default.
- W4367333085 cites W2929611936 @default.
- W4367333085 cites W2963926945 @default.
- W4367333085 cites W3041248047 @default.
- W4367333085 cites W3049510596 @default.
- W4367333085 cites W3087847054 @default.
- W4367333085 cites W3099386252 @default.
- W4367333085 cites W3100703165 @default.
- W4367333085 cites W3101327116 @default.
- W4367333085 cites W3103048770 @default.
- W4367333085 cites W3103704815 @default.
- W4367333085 cites W3103716838 @default.
- W4367333085 cites W3103840321 @default.
- W4367333085 cites W3104767921 @default.
- W4367333085 cites W3105676301 @default.
- W4367333085 cites W3106334214 @default.
- W4367333085 cites W3120223812 @default.
- W4367333085 cites W3122948819 @default.
- W4367333085 cites W3159665842 @default.
- W4367333085 cites W3163747086 @default.
- W4367333085 cites W4206830195 @default.
- W4367333085 cites W4214925878 @default.
- W4367333085 cites W4225425525 @default.
- W4367333085 cites W4280521069 @default.
- W4367333085 cites W4283794440 @default.
- W4367333085 cites W4291000122 @default.
- W4367333085 cites W4310438556 @default.
- W4367333085 doi "https://doi.org/10.1051/epjconf/202328304001" @default.
- W4367333085 hasPublicationYear "2023" @default.
- W4367333085 type Work @default.
- W4367333085 citedByCount "0" @default.
- W4367333085 crossrefType "journal-article" @default.
- W4367333085 hasAuthorship W4367333085A5035206337 @default.
- W4367333085 hasAuthorship W4367333085A5035555064 @default.
- W4367333085 hasBestOaLocation W43673330851 @default.
- W4367333085 hasConcept C111309251 @default.
- W4367333085 hasConcept C121332964 @default.
- W4367333085 hasConcept C12287442 @default.
- W4367333085 hasConcept C1276947 @default.
- W4367333085 hasConcept C152568617 @default.
- W4367333085 hasConcept C185544564 @default.
- W4367333085 hasConcept C192887742 @default.
- W4367333085 hasConcept C26001627 @default.
- W4367333085 hasConcept C2776401274 @default.
- W4367333085 hasConcept C44870925 @default.
- W4367333085 hasConcept C91752515 @default.
- W4367333085 hasConcept C98444146 @default.
- W4367333085 hasConceptScore W4367333085C111309251 @default.
- W4367333085 hasConceptScore W4367333085C121332964 @default.
- W4367333085 hasConceptScore W4367333085C12287442 @default.
- W4367333085 hasConceptScore W4367333085C1276947 @default.
- W4367333085 hasConceptScore W4367333085C152568617 @default.
- W4367333085 hasConceptScore W4367333085C185544564 @default.
- W4367333085 hasConceptScore W4367333085C192887742 @default.
- W4367333085 hasConceptScore W4367333085C26001627 @default.
- W4367333085 hasConceptScore W4367333085C2776401274 @default.
- W4367333085 hasConceptScore W4367333085C44870925 @default.
- W4367333085 hasConceptScore W4367333085C91752515 @default.
- W4367333085 hasConceptScore W4367333085C98444146 @default.
- W4367333085 hasLocation W43673330851 @default.
- W4367333085 hasLocation W43673330852 @default.
- W4367333085 hasLocation W43673330853 @default.
- W4367333085 hasLocation W43673330854 @default.
- W4367333085 hasOpenAccess W4367333085 @default.
- W4367333085 hasPrimaryLocation W43673330851 @default.
- W4367333085 hasRelatedWork W1864702457 @default.
- W4367333085 hasRelatedWork W2018460911 @default.
- W4367333085 hasRelatedWork W2963621444 @default.
- W4367333085 hasRelatedWork W3084104036 @default.
- W4367333085 hasRelatedWork W3098997918 @default.