{"title":"用牛顿引力理论计算太阳系中光的偏转和广义相对论中光运动的轨道极","authors":"Mei Xiaochun","doi":"10.54647/physics14417","DOIUrl":null,"url":null,"abstract":"","PeriodicalId":194720,"journal":{"name":"SCIREA Journal of Physics","volume":"23 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2022-03-24","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":"{\"title\":\"Using the Newton’s Theory of Gravity to Calculate the Deflection of Light in the Solar System and the Orbital Poles of Light’s Motion of General Relativity\",\"authors\":\"Mei Xiaochun\",\"doi\":\"10.54647/physics14417\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"\",\"PeriodicalId\":194720,\"journal\":{\"name\":\"SCIREA Journal of Physics\",\"volume\":\"23 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2022-03-24\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"1\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"SCIREA Journal of Physics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.54647/physics14417\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"SCIREA Journal of Physics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.54647/physics14417","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Using the Newton’s Theory of Gravity to Calculate the Deflection of Light in the Solar System and the Orbital Poles of Light’s Motion of General Relativity