FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2127312972> ?p ?o ?g. }

• W2127312972 endingPage "74" @default.
• W2127312972 startingPage "62" @default.
• W2127312972 abstract "We study the radiation yield of the synchrotron self-Compton (SSC) process in the framework of the relativistic collision front model proposed by Pohl & Schlickeiser. In that model, the decay of neutral pions is a prominent process, in particular concerning the TeV-scale � -ray emission. The SSC process must occur at some level in all blazars, however, on account of the strong radiation field in the jet provided by the synchrotron cooling of the simultaneously produced secondary electrons and positrons from charged pion decay. We investigate the influence of the parameters of the relativistic collision front and the ambient matter on the spectral evolution of the blazar emission, and we present multiwavelength spectra, light curves, and flux ratios for a few characteristic situations. We also consider the effects on the temporal evolution of the multiband spectra of AGNs caused by the additional cooling high-energy electrons due to the SSC emission. Our results indicate that the SSC radiation provides the decisive contribution to the GeV range of AGN emission spectra, whereas the � 0 decay provides � -rays at the highest energies in the TeV band. The synchrotron radiation at keVenergies, the SSC emission in the GeV range, and the� 0 decay component in the TeV band can vary on the same short timescales on account of small-scale structure in the interstellar medium of the AGN host galaxies and hence rapid fluctuations in the injection rate of relativistic protons. This behavior would be very difficult to explain in a purely leptonic SSC model. When the light curves are smoothed over small to medium timescales, the GeV-to-keVand the TeV-to-keV flux ratios show a characteristic longterm evolution that depends on the jet aspect angle and the initial jet Lorentz factor. Our results emphasize the need for AGN observations at GeV energies, e.g., by the upcoming GLAST mission, to complement the ongoing blazar monitoring by satellite X-ray detectors and ground-based Cerenkov telescopes that cover the TeV band. Subject headingg gamma rays: theory — quasars: general — radiation mechanisms: nonthermal" @default.
• W2127312972 created "2016-06-24" @default.
• W2127312972 creator A5014924834 @default.
• W2127312972 creator A5035724494 @default.
• W2127312972 creator A5057580739 @default.
• W2127312972 date "2005-07-01" @default.
• W2127312972 modified "2023-09-27" @default.
• W2127312972 title "Synchrotron Self‐Comptonization in a Relativistic Collision Front Model" @default.
• W2127312972 cites W1548209730 @default.
• W2127312972 cites W1627220256 @default.
• W2127312972 cites W1966892777 @default.
• W2127312972 cites W1974671362 @default.
• W2127312972 cites W1978059554 @default.
• W2127312972 cites W1980801366 @default.
• W2127312972 cites W1983354252 @default.
• W2127312972 cites W2002976439 @default.
• W2127312972 cites W2003313311 @default.
• W2127312972 cites W2008852708 @default.
• W2127312972 cites W2019252893 @default.
• W2127312972 cites W2019646688 @default.
• W2127312972 cites W2034798742 @default.
• W2127312972 cites W2038367995 @default.
• W2127312972 cites W2044992101 @default.
• W2127312972 cites W2049177115 @default.
• W2127312972 cites W2052553505 @default.
• W2127312972 cites W2054923548 @default.
• W2127312972 cites W2061333692 @default.
• W2127312972 cites W2067045760 @default.
• W2127312972 cites W2072235101 @default.
• W2127312972 cites W2083595252 @default.
• W2127312972 cites W2090118635 @default.
• W2127312972 cites W2107208483 @default.
• W2127312972 cites W2108484121 @default.
• W2127312972 cites W2124633616 @default.
• W2127312972 cites W2127586797 @default.
• W2127312972 cites W2152242740 @default.
• W2127312972 cites W2152822092 @default.
• W2127312972 cites W2949130100 @default.
• W2127312972 cites W3098003348 @default.
• W2127312972 cites W3098117879 @default.
• W2127312972 cites W3098395009 @default.
• W2127312972 cites W3098604333 @default.
• W2127312972 cites W3099319445 @default.
• W2127312972 cites W3100063856 @default.
• W2127312972 cites W3102821076 @default.
• W2127312972 doi "https://doi.org/10.1086/430118" @default.
• W2127312972 hasPublicationYear "2005" @default.
• W2127312972 type Work @default.
• W2127312972 sameAs 2127312972 @default.
• W2127312972 citedByCount "16" @default.
• W2127312972 countsByYear W21273129722012 @default.
• W2127312972 countsByYear W21273129722018 @default.
• W2127312972 countsByYear W21273129722019 @default.
• W2127312972 countsByYear W21273129722021 @default.
• W2127312972 countsByYear W21273129722022 @default.
• W2127312972 countsByYear W21273129722023 @default.
• W2127312972 crossrefType "journal-article" @default.
• W2127312972 hasAuthorship W2127312972A5014924834 @default.
• W2127312972 hasAuthorship W2127312972A5035724494 @default.
• W2127312972 hasAuthorship W2127312972A5057580739 @default.
• W2127312972 hasConcept C121332964 @default.
• W2127312972 hasConcept C121704057 @default.
• W2127312972 hasConcept C1276947 @default.
• W2127312972 hasConcept C145472833 @default.
• W2127312972 hasConcept C147120987 @default.
• W2127312972 hasConcept C153294291 @default.
• W2127312972 hasConcept C163862864 @default.
• W2127312972 hasConcept C168997771 @default.
• W2127312972 hasConcept C185544564 @default.
• W2127312972 hasConcept C21368211 @default.
• W2127312972 hasConcept C2777551076 @default.
• W2127312972 hasConcept C38652104 @default.
• W2127312972 hasConcept C41008148 @default.
• W2127312972 hasConcept C43481613 @default.
• W2127312972 hasConcept C44870925 @default.
• W2127312972 hasConcept C98444146 @default.
• W2127312972 hasConceptScore W2127312972C121332964 @default.
• W2127312972 hasConceptScore W2127312972C121704057 @default.
• W2127312972 hasConceptScore W2127312972C1276947 @default.
• W2127312972 hasConceptScore W2127312972C145472833 @default.
• W2127312972 hasConceptScore W2127312972C147120987 @default.
• W2127312972 hasConceptScore W2127312972C153294291 @default.
• W2127312972 hasConceptScore W2127312972C163862864 @default.
• W2127312972 hasConceptScore W2127312972C168997771 @default.
• W2127312972 hasConceptScore W2127312972C185544564 @default.
• W2127312972 hasConceptScore W2127312972C21368211 @default.
• W2127312972 hasConceptScore W2127312972C2777551076 @default.
• W2127312972 hasConceptScore W2127312972C38652104 @default.
• W2127312972 hasConceptScore W2127312972C41008148 @default.
• W2127312972 hasConceptScore W2127312972C43481613 @default.
• W2127312972 hasConceptScore W2127312972C44870925 @default.
• W2127312972 hasConceptScore W2127312972C98444146 @default.
• W2127312972 hasIssue "1" @default.
• W2127312972 hasLocation W21273129721 @default.
• W2127312972 hasOpenAccess W2127312972 @default.
• W2127312972 hasPrimaryLocation W21273129721 @default.
• W2127312972 hasRelatedWork W2008571261 @default.
• W2127312972 hasRelatedWork W2072179120 @default.

• next