{"title":"旋转轴对称结构和引力辐射的广义相对论代码:数值方法和试验","authors":"Richard F. Stark , Tsvi Piran","doi":"10.1016/0167-7977(87)90003-7","DOIUrl":null,"url":null,"abstract":"<div><p>We describe a fully general relativistic computer code for solving the complete coupled Einstein/hydrodynamic equations for rotating axisymmetric systems including their gravitational wave emission. We describe the formalism used; the form of the equations which are solved; and the numerical methods employed. The hydrodynamic and geometrical tests used to check the code are also documented.</p></div>","PeriodicalId":100318,"journal":{"name":"Computer Physics Reports","volume":"5 5","pages":"Pages 221-264"},"PeriodicalIF":0.0000,"publicationDate":"1987-09-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/0167-7977(87)90003-7","citationCount":"35","resultStr":"{\"title\":\"A general relativistic code for rotating axisymmetric configurations and gravitational radiation: Numerical methods and tests\",\"authors\":\"Richard F. Stark , Tsvi Piran\",\"doi\":\"10.1016/0167-7977(87)90003-7\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p>We describe a fully general relativistic computer code for solving the complete coupled Einstein/hydrodynamic equations for rotating axisymmetric systems including their gravitational wave emission. We describe the formalism used; the form of the equations which are solved; and the numerical methods employed. The hydrodynamic and geometrical tests used to check the code are also documented.</p></div>\",\"PeriodicalId\":100318,\"journal\":{\"name\":\"Computer Physics Reports\",\"volume\":\"5 5\",\"pages\":\"Pages 221-264\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"1987-09-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://sci-hub-pdf.com/10.1016/0167-7977(87)90003-7\",\"citationCount\":\"35\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Computer Physics Reports\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/0167797787900037\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Computer Physics Reports","FirstCategoryId":"1085","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/0167797787900037","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
A general relativistic code for rotating axisymmetric configurations and gravitational radiation: Numerical methods and tests
We describe a fully general relativistic computer code for solving the complete coupled Einstein/hydrodynamic equations for rotating axisymmetric systems including their gravitational wave emission. We describe the formalism used; the form of the equations which are solved; and the numerical methods employed. The hydrodynamic and geometrical tests used to check the code are also documented.
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