Gravitational radiation of charged rotating body하전된 회전체의 중력복사

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dc.contributor.advisorCho, Byung-Ha-
dc.contributor.advisor조병하-
dc.contributor.authorCho, Yoon-Hyoung-
dc.contributor.author조윤형-
dc.date.accessioned2011-12-14T07:49:04Z-
dc.date.available2011-12-14T07:49:04Z-
dc.date.issued1985-
dc.identifier.urihttp://library.kaist.ac.kr/search/detail/view.do?bibCtrlNo=64468&flag=dissertation-
dc.identifier.urihttp://hdl.handle.net/10203/48108-
dc.description학위논문(석사) - 한국과학기술원 : 물리학과, 1985.2, [ [ii], 41, [3] p. ]-
dc.description.abstractThe Newman-Penrose spin coefficient formalism is applied to nonstationary charged rotating body. The spin coefficients, tetrad components of trace free Ricci tensor and Weyl components are obtained. The energy-momentum tensor consists of a radiating field and a residual one. Asymptotically the charge contribution term fade out more promptly than the geometrical optics term which can be interpreted as a source free Maxwell field.eng
dc.languageeng-
dc.publisher한국과학기술원-
dc.titleGravitational radiation of charged rotating body-
dc.title.alternative하전된 회전체의 중력복사-
dc.typeThesis(Master)-
dc.identifier.CNRN64468/325007-
dc.description.department한국과학기술원 : 물리학과, -
dc.identifier.uid000831390-
dc.contributor.localauthorCho, Yoon-Hyoung-
dc.contributor.localauthor조윤형-
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PH-Theses_Master(석사논문)
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