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Non-thermal shielding effects on the Compton scattering power in astrophysical plasmas

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dc.contributor.authorShin, Dong-Soo-
dc.contributor.authorJung, Young-Dae-
dc.date.accessioned2021-06-22T19:03:20Z-
dc.date.available2021-06-22T19:03:20Z-
dc.date.created2021-01-21-
dc.date.issued2015-10-
dc.identifier.issn0927-6505-
dc.identifier.urihttps://scholarworks.bwise.kr/erica/handle/2021.sw.erica/17012-
dc.description.abstractThe non-thermal shielding effects on the inverse Compton scattering are investigated in astrophysical non-thermal Lorentzian plasmas. The inverse Compton power is obtained by the modified Compton scattering cross section in Lorentzian plasmas with the blackbody photon distribution. The total Compton power is also obtained by the Lorentzan distribution of plasmas. It is found that the influence of non-thermal character of the plasma suppresses the inverse Compton power in astrophysical Lorentzian plasmas. It is also found that the non-thermal effect on the inverse Compton power decreases with an increase of the temperature. In addition, the non-thermal effect on the total Compton power with Lorentzan plasmas increases in low-temperature photons and, however, decreases in intermediate-temperature photons with increasing Debye length. The variation of the total Compton power is also discussed. (C) 2015 Elsevier B.V. All rights reserved.-
dc.language영어-
dc.language.isoen-
dc.publisherElsevier BV-
dc.titleNon-thermal shielding effects on the Compton scattering power in astrophysical plasmas-
dc.typeArticle-
dc.contributor.affiliatedAuthorShin, Dong-Soo-
dc.contributor.affiliatedAuthorJung, Young-Dae-
dc.identifier.doi10.1016/j.astropartphys.2015.03.012-
dc.identifier.scopusid2-s2.0-84929096243-
dc.identifier.wosid000356755400003-
dc.identifier.bibliographicCitationAstroparticle Physics, v.70, pp.27 - 32-
dc.relation.isPartOfAstroparticle Physics-
dc.citation.titleAstroparticle Physics-
dc.citation.volume70-
dc.citation.startPage27-
dc.citation.endPage32-
dc.type.rimsART-
dc.type.docTypeArticle-
dc.description.journalClass1-
dc.description.isOpenAccessN-
dc.description.journalRegisteredClassscie-
dc.description.journalRegisteredClassscopus-
dc.relation.journalResearchAreaAstronomy & Astrophysics-
dc.relation.journalResearchAreaPhysics-
dc.relation.journalWebOfScienceCategoryAstronomy & Astrophysics-
dc.relation.journalWebOfScienceCategoryPhysics, Particles & Fields-
dc.subject.keywordPlusTHOMSON SCATTERING-
dc.subject.keywordPlusFLUCTUATIONS-
dc.subject.keywordPlusTEMPERATURE-
dc.subject.keywordPlusEXCITATIONS-
dc.subject.keywordPlusRADIATION-
dc.subject.keywordPlusELECTRONS-
dc.subject.keywordAuthorAtomic processes-
dc.subject.keywordAuthorCompton scattering-
dc.subject.keywordAuthorAstrophysical plasmas-
dc.identifier.urlhttps://www.sciencedirect.com/science/article/pii/S0927650515000651?via%3Dihub-
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COLLEGE OF SCIENCE AND CONVERGENCE TECHNOLOGY > DEPARTMENT OF APPLIED PHYSICS > 1. Journal Articles
COLLEGE OF SCIENCE AND CONVERGENCE TECHNOLOGY > DEPARTMENT OF PHOTONICS AND NANOELECTRONICS > 1. Journal Articles

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