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dc.contributor.author이명재-
dc.date.accessioned2019-12-08T03:02:29Z-
dc.date.available2019-12-08T03:02:29Z-
dc.date.issued2018-05-
dc.identifier.citationPHYSICS OF PLASMAS, v. 25, no. 5, Article no. 053704en_US
dc.identifier.issn1070-664X-
dc.identifier.issn1089-7674-
dc.identifier.urihttps://aip.scitation.org/doi/10.1063/1.5028290-
dc.identifier.urihttps://repository.hanyang.ac.kr/handle/20.500.11754/118685-
dc.description.abstractThe dispersion properties of surface dust ion-acoustic waves in a self-gravitating magnetized dusty plasma layer with the (r, q) distribution are investigated. The result shows that the wave frequency of the symmetric mode in the plasma layer decreases with an increase in the wave number. It is also shown that the wave frequency of the symmetric mode decreases with an increase in the spectral index r. However, the wave frequency of the anti-symmetric mode increases with an increase in the wave number. It is also found that the anti-symmetric mode wave frequency increases with an increase in the spectral index r. In addition, it is found that the influence of the self-gravitation on the symmetric mode wave frequency decreases with increasing scaled Jeans frequency. Moreover, it is found that the wave frequency of the symmetric mode increases with an increase in the dust charge; however, the anti-symmetric mode shows opposite behavior. Published by AIP Publishing.en_US
dc.description.sponsorshipOne of the authors (Y.-D.J.) gratefully acknowledges Dr. M. Rosenberg for useful discussions and warm hospitality while visiting the Department of Electrical and Computer Engineering at the University of California, San Diego. This research was initiated while one of the authors (Y.-D.J.) was affiliated with UC San Diego as a visiting professor. This work was supported by the National Research Foundation of Korea (NRF) grant funded by the Korean Government (MISP) (No. NRF-2016R1A2B4011356).en_US
dc.language.isoen_USen_US
dc.publisherAMER INST PHYSICSen_US
dc.subjectSLABen_US
dc.titlePropagation of symmetric and anti-symmetric surface waves in a self-gravitating magnetized dusty plasma layer with generalized (r, q) distributionen_US
dc.typeArticleen_US
dc.relation.no5-
dc.relation.volume25-
dc.identifier.doi10.1063/1.5028290-
dc.relation.page1-8-
dc.relation.journalPHYSICS OF PLASMAS-
dc.contributor.googleauthorLee, Myoung-Jae-
dc.contributor.googleauthorJung, Young-Dae-
dc.relation.code2018001843-
dc.sector.campusS-
dc.sector.daehakCOLLEGE OF NATURAL SCIENCES[S]-
dc.sector.departmentDEPARTMENT OF PHYSICS-
dc.identifier.pidmjlee-
dc.identifier.researcherIDE-2611-2017-
dc.identifier.orcidhttp://orcid.org/0000-0001-7814-4731-
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COLLEGE OF NATURAL SCIENCES[S](자연과학대학) > PHYSICS(물리학과) > Articles
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