{"title":"广义相对论中椭圆星系或恒星附近光的偏转","authors":"Bijan Nikouravan, J. Rawal","doi":"10.12988/ASTP.2013.3993","DOIUrl":null,"url":null,"abstract":"We study the evaluation of bending of light ray passing near a massive elliptical galaxy or star. To obtain this solution we used two dierent, Einsteinian and Lagrangian method. In doing this, we consider and compare the dierence deection angle between spherical and elliptical shape objects which led to appear a small but not negligible coecient as oblateness independent of mass but depend on shape and geometry of object.","PeriodicalId":127314,"journal":{"name":"Advanced Studies in Theoretical Physics","volume":"29 5","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2013-10-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"3","resultStr":"{\"title\":\"Deflection of light near elliptical galaxies or stars in general relativity\",\"authors\":\"Bijan Nikouravan, J. Rawal\",\"doi\":\"10.12988/ASTP.2013.3993\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"We study the evaluation of bending of light ray passing near a massive elliptical galaxy or star. To obtain this solution we used two dierent, Einsteinian and Lagrangian method. In doing this, we consider and compare the dierence deection angle between spherical and elliptical shape objects which led to appear a small but not negligible coecient as oblateness independent of mass but depend on shape and geometry of object.\",\"PeriodicalId\":127314,\"journal\":{\"name\":\"Advanced Studies in Theoretical Physics\",\"volume\":\"29 5\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2013-10-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"3\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Advanced Studies in Theoretical Physics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.12988/ASTP.2013.3993\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Advanced Studies in Theoretical Physics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.12988/ASTP.2013.3993","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Deflection of light near elliptical galaxies or stars in general relativity
We study the evaluation of bending of light ray passing near a massive elliptical galaxy or star. To obtain this solution we used two dierent, Einsteinian and Lagrangian method. In doing this, we consider and compare the dierence deection angle between spherical and elliptical shape objects which led to appear a small but not negligible coecient as oblateness independent of mass but depend on shape and geometry of object.
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