{"title":"f(R, T)引力理论中含夸克和奇异夸克物质的各向异性宇宙学模型","authors":"S. Ram, Surendra K. Singh, M. K. Verma","doi":"10.22606/NHMP.2018.23001","DOIUrl":null,"url":null,"abstract":"Einstein’s field equations in f(R, T ) gravity theory in the presence of quark and strange quark matter are considered for a plane symmetric space-time. We have obtained exact solutions of the field equations by assuming a special form of Hubble parameter that yield a time-varying deceleration parameter. The physical behaviors of the cosmological model are discussed.","PeriodicalId":355259,"journal":{"name":"New Horizons in Mathematical Physics","volume":"1 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2018-09-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Anisotropic Cosmological Model with Quark and Strange Quark Matter in f(R, T ) Gravity Theory\",\"authors\":\"S. Ram, Surendra K. Singh, M. K. Verma\",\"doi\":\"10.22606/NHMP.2018.23001\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Einstein’s field equations in f(R, T ) gravity theory in the presence of quark and strange quark matter are considered for a plane symmetric space-time. We have obtained exact solutions of the field equations by assuming a special form of Hubble parameter that yield a time-varying deceleration parameter. The physical behaviors of the cosmological model are discussed.\",\"PeriodicalId\":355259,\"journal\":{\"name\":\"New Horizons in Mathematical Physics\",\"volume\":\"1 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2018-09-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"New Horizons in Mathematical Physics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.22606/NHMP.2018.23001\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"New Horizons in Mathematical Physics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.22606/NHMP.2018.23001","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Anisotropic Cosmological Model with Quark and Strange Quark Matter in f(R, T ) Gravity Theory
Einstein’s field equations in f(R, T ) gravity theory in the presence of quark and strange quark matter are considered for a plane symmetric space-time. We have obtained exact solutions of the field equations by assuming a special form of Hubble parameter that yield a time-varying deceleration parameter. The physical behaviors of the cosmological model are discussed.