FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3103188632> ?p ?o ?g. }

• W3103188632 endingPage "338" @default.
• W3103188632 startingPage "325" @default.
• W3103188632 abstract "We report the results of one-dimensional particle-in-cell simulations of magnetized ultrarelativistic shock waves in proton-electron-positron plasmas. Relativistic cyclotron instability, as the incoming particles encounter the increasing magnetic field within the shock front provides the basic plasma heating mechanism. The major new results come from simulations with mass ratio mp/m± = 100. When the protons provide a sufficiently large fraction of the upstream flow energy density (including particle kinetic energy and Poynting flux), a substantial fraction of the shock heating goes into the formation of suprathermal power-law spectra of e-e+. Cyclotron absorption by the pairs of the high harmonic ion cyclotron waves, emitted by the protons, provides the nonthermal acceleration mechanism. When the proton fraction is small (pair plasma almost charge-symmetric), the e- and e+ have approximately equal amounts of nonthermal heating. At the lower range of our simulations with mass ratio 100, when the ions contribute 56% of the upstream flow energy flux, the pairs' nonthermal acceleration efficiency by energy is about 1%, increasing to 5% as the ions' energy fraction increases to 72%. When the fraction of upstream flow energy in the ions rises to 84%, the efficiency of nonthermal acceleration of the pairs reaches 30%: the e+ receive most of the nonthermal power and the nonthermal spectra harden. We suggest that the varying power-law spectra observed in synchrotron sources that may be powered by magnetized winds and jets might reflect the correlation of the proton-to-pair content enforced by the underlying electrodynamics of these sources' outflows, and that the observed correlation between the X-ray spectra of rotation-powered pulsars with the X-ray spectra of their nebulae might reflect the same correlation." @default.
• W3103188632 created "2020-11-23" @default.
• W3103188632 creator A5008829697 @default.
• W3103188632 creator A5021435483 @default.
• W3103188632 date "2006-12-10" @default.
• W3103188632 modified "2023-09-23" @default.
• W3103188632 title "Heating and Nonthermal Particle Acceleration in Relativistic, Transverse Magnetosonic Shock Waves in Proton‐Electron‐Positron Plasmas" @default.
• W3103188632 cites W1970453854 @default.
• W3103188632 cites W1982670431 @default.
• W3103188632 cites W1986002430 @default.
• W3103188632 cites W1992338820 @default.
• W3103188632 cites W1992768712 @default.
• W3103188632 cites W1998718175 @default.
• W3103188632 cites W2004697089 @default.
• W3103188632 cites W2018829983 @default.
• W3103188632 cites W2029677436 @default.
• W3103188632 cites W2034727108 @default.
• W3103188632 cites W2044261325 @default.
• W3103188632 cites W2046814797 @default.
• W3103188632 cites W2055339120 @default.
• W3103188632 cites W2069062146 @default.
• W3103188632 cites W2072276097 @default.
• W3103188632 cites W2080109131 @default.
• W3103188632 cites W2086318762 @default.
• W3103188632 cites W2089280567 @default.
• W3103188632 cites W2124648171 @default.
• W3103188632 cites W2990950665 @default.
• W3103188632 cites W3100980057 @default.
• W3103188632 cites W3101851053 @default.
• W3103188632 cites W3103515358 @default.
• W3103188632 cites W3103582265 @default.
• W3103188632 cites W3105957717 @default.
• W3103188632 cites W3105969607 @default.
• W3103188632 cites W4246652625 @default.
• W3103188632 doi "https://doi.org/10.1086/508050" @default.
• W3103188632 hasPublicationYear "2006" @default.
• W3103188632 type Work @default.
• W3103188632 sameAs 3103188632 @default.
• W3103188632 citedByCount "94" @default.
• W3103188632 countsByYear W31031886322012 @default.
• W3103188632 countsByYear W31031886322013 @default.
• W3103188632 countsByYear W31031886322014 @default.
• W3103188632 countsByYear W31031886322015 @default.
• W3103188632 countsByYear W31031886322016 @default.
• W3103188632 countsByYear W31031886322017 @default.
• W3103188632 countsByYear W31031886322018 @default.
• W3103188632 countsByYear W31031886322019 @default.
• W3103188632 countsByYear W31031886322020 @default.
• W3103188632 countsByYear W31031886322021 @default.
• W3103188632 countsByYear W31031886322022 @default.
• W3103188632 countsByYear W31031886322023 @default.
• W3103188632 crossrefType "journal-article" @default.
• W3103188632 hasAuthorship W3103188632A5008829697 @default.
• W3103188632 hasAuthorship W3103188632A5021435483 @default.
• W3103188632 hasBestOaLocation W31031886321 @default.
• W3103188632 hasConcept C115260700 @default.
• W3103188632 hasConcept C121332964 @default.
• W3103188632 hasConcept C135889238 @default.
• W3103188632 hasConcept C147120987 @default.
• W3103188632 hasConcept C184779094 @default.
• W3103188632 hasConcept C185544564 @default.
• W3103188632 hasConcept C30475298 @default.
• W3103188632 hasConcept C39527238 @default.
• W3103188632 hasConcept C54516573 @default.
• W3103188632 hasConcept C62520636 @default.
• W3103188632 hasConcept C70477161 @default.
• W3103188632 hasConcept C75183268 @default.
• W3103188632 hasConcept C82706917 @default.
• W3103188632 hasConcept C97355855 @default.
• W3103188632 hasConceptScore W3103188632C115260700 @default.
• W3103188632 hasConceptScore W3103188632C121332964 @default.
• W3103188632 hasConceptScore W3103188632C135889238 @default.
• W3103188632 hasConceptScore W3103188632C147120987 @default.
• W3103188632 hasConceptScore W3103188632C184779094 @default.
• W3103188632 hasConceptScore W3103188632C185544564 @default.
• W3103188632 hasConceptScore W3103188632C30475298 @default.
• W3103188632 hasConceptScore W3103188632C39527238 @default.
• W3103188632 hasConceptScore W3103188632C54516573 @default.
• W3103188632 hasConceptScore W3103188632C62520636 @default.
• W3103188632 hasConceptScore W3103188632C70477161 @default.
• W3103188632 hasConceptScore W3103188632C75183268 @default.
• W3103188632 hasConceptScore W3103188632C82706917 @default.
• W3103188632 hasConceptScore W3103188632C97355855 @default.
• W3103188632 hasIssue "1" @default.
• W3103188632 hasLocation W31031886321 @default.
• W3103188632 hasLocation W31031886322 @default.
• W3103188632 hasOpenAccess W3103188632 @default.
• W3103188632 hasPrimaryLocation W31031886321 @default.
• W3103188632 hasRelatedWork W1573921104 @default.
• W3103188632 hasRelatedWork W2021472480 @default.
• W3103188632 hasRelatedWork W2053241837 @default.
• W3103188632 hasRelatedWork W2153986253 @default.
• W3103188632 hasRelatedWork W2334620464 @default.
• W3103188632 hasRelatedWork W2793869639 @default.
• W3103188632 hasRelatedWork W3104083206 @default.
• W3103188632 hasRelatedWork W4246904474 @default.
• W3103188632 hasRelatedWork W4376122885 @default.
• W3103188632 hasRelatedWork W4382458573 @default.

• next