{"title":"克尔空间中不存在封闭的时间似大地线","authors":"Giulio Sanzeni","doi":"arxiv-2409.09094","DOIUrl":null,"url":null,"abstract":"The Kerr-star spacetime is the extension over the horizons and in the\nnegative radial region of the Kerr spacetime. Despite the presence of closed\ntimelike curves below the inner horizon, we prove that the timelike geodesics\ncannot be closed in the Kerr-star spacetime. Since the existence of closed null\ngeodesics was ruled out by the author in Sanzeni [arXiv:2308.09631v3 (2024)],\nthis result shows the absence of closed causal geodesics in the Kerr-star\nspacetime.","PeriodicalId":501113,"journal":{"name":"arXiv - MATH - Differential Geometry","volume":"53 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-09-12","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Nonexistence of closed timelike geodesics in Kerr spacetimes\",\"authors\":\"Giulio Sanzeni\",\"doi\":\"arxiv-2409.09094\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The Kerr-star spacetime is the extension over the horizons and in the\\nnegative radial region of the Kerr spacetime. Despite the presence of closed\\ntimelike curves below the inner horizon, we prove that the timelike geodesics\\ncannot be closed in the Kerr-star spacetime. Since the existence of closed null\\ngeodesics was ruled out by the author in Sanzeni [arXiv:2308.09631v3 (2024)],\\nthis result shows the absence of closed causal geodesics in the Kerr-star\\nspacetime.\",\"PeriodicalId\":501113,\"journal\":{\"name\":\"arXiv - MATH - Differential Geometry\",\"volume\":\"53 1\",\"pages\":\"\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2024-09-12\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"arXiv - MATH - Differential Geometry\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/arxiv-2409.09094\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - MATH - Differential Geometry","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2409.09094","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Nonexistence of closed timelike geodesics in Kerr spacetimes
The Kerr-star spacetime is the extension over the horizons and in the
negative radial region of the Kerr spacetime. Despite the presence of closed
timelike curves below the inner horizon, we prove that the timelike geodesics
cannot be closed in the Kerr-star spacetime. Since the existence of closed null
geodesics was ruled out by the author in Sanzeni [arXiv:2308.09631v3 (2024)],
this result shows the absence of closed causal geodesics in the Kerr-star
spacetime.