{"title":"黑弦的隧穿辐射","authors":"Guqiang Li","doi":"10.1088/0305-4470/39/38/014","DOIUrl":null,"url":null,"abstract":"We use the Parikh–Wilczek method to study the tunnelling radiation from the event of the black string, which is asymptotically anti-de Sitter and possesses cylindrical symmetry. We show that higher corrections to the semi-classical rate which are caused by energy conservation and angular momentum conservation exist and the emission rate has completely the same functional form as that for spherically symmetric or axisymmetric black holes.","PeriodicalId":87442,"journal":{"name":"Journal of physics A: Mathematical and general","volume":null,"pages":null},"PeriodicalIF":0.0000,"publicationDate":"2006-09-05","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"12","resultStr":"{\"title\":\"Black string's tunnelling radiation\",\"authors\":\"Guqiang Li\",\"doi\":\"10.1088/0305-4470/39/38/014\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"We use the Parikh–Wilczek method to study the tunnelling radiation from the event of the black string, which is asymptotically anti-de Sitter and possesses cylindrical symmetry. We show that higher corrections to the semi-classical rate which are caused by energy conservation and angular momentum conservation exist and the emission rate has completely the same functional form as that for spherically symmetric or axisymmetric black holes.\",\"PeriodicalId\":87442,\"journal\":{\"name\":\"Journal of physics A: Mathematical and general\",\"volume\":null,\"pages\":null},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2006-09-05\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"12\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Journal of physics A: Mathematical and general\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1088/0305-4470/39/38/014\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of physics A: Mathematical and general","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1088/0305-4470/39/38/014","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
We use the Parikh–Wilczek method to study the tunnelling radiation from the event of the black string, which is asymptotically anti-de Sitter and possesses cylindrical symmetry. We show that higher corrections to the semi-classical rate which are caused by energy conservation and angular momentum conservation exist and the emission rate has completely the same functional form as that for spherically symmetric or axisymmetric black holes.