Matches in SemOpenAlex for { <https://semopenalex.org/work/W3021702671> ?p ?o ?g. }
Showing items 1 to 98 of
98
with 100 items per page.
- W3021702671 endingPage "31" @default.
- W3021702671 startingPage "1" @default.
- W3021702671 abstract "The origin of cosmic rays is one of the key questions in high-energy astrophysics. Supernovae have been always considered as the dominant sources of cosmic rays below the energy spectrum knee. Multi-wavelength observations indeed show that supernova remnants are capable for accelerating particles into sub-PeV (1015 eV) energies. Diffusive shock acceleration is considered as one of the most efficient acceleration mechanisms of astrophysical high-energy particles, which may just operate effectively in the large-scale shocks of supernova remnants. Recently, a series of high-precision ground and space experiments have greatly promoted the study of cosmic rays and supernova remnants. New observational features challenge the classical acceleration model by diffusive shock and the application to the scenario of supernova remnants for the origin of Galactic cosmic rays, and have deepened our understanding to the cosmic high-energy phenomena. In combination with the time evolution of radiation energy spectrum of supernova remnants, a time-dependent particle acceleration model is established, which can not only explain the anomalies in cosmic-ray distributions around 200 GV, but also naturally form the cosmic-ray spectrum knee, even extend the contribution of supernova particle acceleration to cosmic ray flux up to the spectrum ankle. This model predicts that the high-energy particle transport behavior is dominated by the turbulent convection, which needs to be verified by future observations and plasma numerical simulations relevant to the particle transport." @default.
- W3021702671 created "2020-05-13" @default.
- W3021702671 creator A5026433926 @default.
- W3021702671 creator A5045252910 @default.
- W3021702671 date "2020-01-01" @default.
- W3021702671 modified "2023-09-29" @default.
- W3021702671 title "The Origin of Cosmic Rays from Supernova Remnants" @default.
- W3021702671 cites W1642228177 @default.
- W3021702671 cites W1967985088 @default.
- W3021702671 cites W1992498614 @default.
- W3021702671 cites W2002973683 @default.
- W3021702671 cites W2005981582 @default.
- W3021702671 cites W2018586004 @default.
- W3021702671 cites W2032882333 @default.
- W3021702671 cites W2057751156 @default.
- W3021702671 cites W2067800544 @default.
- W3021702671 cites W2069414247 @default.
- W3021702671 cites W2073311682 @default.
- W3021702671 cites W2077772794 @default.
- W3021702671 cites W2087364146 @default.
- W3021702671 cites W2099903154 @default.
- W3021702671 cites W2105767155 @default.
- W3021702671 cites W2122658693 @default.
- W3021702671 cites W2123448902 @default.
- W3021702671 cites W2123645395 @default.
- W3021702671 cites W2133040363 @default.
- W3021702671 cites W2135523816 @default.
- W3021702671 cites W2156231369 @default.
- W3021702671 cites W2162832027 @default.
- W3021702671 cites W2171691780 @default.
- W3021702671 cites W2190641241 @default.
- W3021702671 cites W2584392057 @default.
- W3021702671 cites W2605208926 @default.
- W3021702671 cites W2732755937 @default.
- W3021702671 cites W2770270630 @default.
- W3021702671 cites W2790266757 @default.
- W3021702671 cites W2901755040 @default.
- W3021702671 cites W2902030104 @default.
- W3021702671 cites W2921415325 @default.
- W3021702671 cites W3098977317 @default.
- W3021702671 cites W3099047178 @default.
- W3021702671 cites W3101901670 @default.
- W3021702671 cites W3102190058 @default.
- W3021702671 cites W3102363668 @default.
- W3021702671 cites W3103273060 @default.
- W3021702671 cites W3104821600 @default.
- W3021702671 cites W3105235709 @default.
- W3021702671 cites W3105941745 @default.
- W3021702671 doi "https://doi.org/10.1016/j.chinastron.2020.04.001" @default.
- W3021702671 hasPublicationYear "2020" @default.
- W3021702671 type Work @default.
- W3021702671 sameAs 3021702671 @default.
- W3021702671 citedByCount "6" @default.
- W3021702671 countsByYear W30217026712021 @default.
- W3021702671 countsByYear W30217026712022 @default.
- W3021702671 countsByYear W30217026712023 @default.
- W3021702671 crossrefType "journal-article" @default.
- W3021702671 hasAuthorship W3021702671A5026433926 @default.
- W3021702671 hasAuthorship W3021702671A5045252910 @default.
- W3021702671 hasConcept C111309251 @default.
- W3021702671 hasConcept C117896860 @default.
- W3021702671 hasConcept C121332964 @default.
- W3021702671 hasConcept C127592171 @default.
- W3021702671 hasConcept C1276947 @default.
- W3021702671 hasConcept C135975100 @default.
- W3021702671 hasConcept C44870925 @default.
- W3021702671 hasConcept C74650414 @default.
- W3021702671 hasConcept C75183268 @default.
- W3021702671 hasConceptScore W3021702671C111309251 @default.
- W3021702671 hasConceptScore W3021702671C117896860 @default.
- W3021702671 hasConceptScore W3021702671C121332964 @default.
- W3021702671 hasConceptScore W3021702671C127592171 @default.
- W3021702671 hasConceptScore W3021702671C1276947 @default.
- W3021702671 hasConceptScore W3021702671C135975100 @default.
- W3021702671 hasConceptScore W3021702671C44870925 @default.
- W3021702671 hasConceptScore W3021702671C74650414 @default.
- W3021702671 hasConceptScore W3021702671C75183268 @default.
- W3021702671 hasIssue "1" @default.
- W3021702671 hasLocation W30217026711 @default.
- W3021702671 hasOpenAccess W3021702671 @default.
- W3021702671 hasPrimaryLocation W30217026711 @default.
- W3021702671 hasRelatedWork W118416873 @default.
- W3021702671 hasRelatedWork W1779282710 @default.
- W3021702671 hasRelatedWork W1979923063 @default.
- W3021702671 hasRelatedWork W2051667087 @default.
- W3021702671 hasRelatedWork W2260754674 @default.
- W3021702671 hasRelatedWork W2950050680 @default.
- W3021702671 hasRelatedWork W3105941745 @default.
- W3021702671 hasRelatedWork W4309135452 @default.
- W3021702671 hasRelatedWork W4313189457 @default.
- W3021702671 hasRelatedWork W2106152412 @default.
- W3021702671 hasVolume "44" @default.
- W3021702671 isParatext "false" @default.
- W3021702671 isRetracted "false" @default.
- W3021702671 magId "3021702671" @default.
- W3021702671 workType "article" @default.