{"title":"修正重力下具有线性变减速参数的Kaluza-Klein FRW型完美流体宇宙学模型","authors":"D. Reddy, Y. Aditya","doi":"10.18689/IJPSR-1000105","DOIUrl":null,"url":null,"abstract":"Here, we investigate cosmological models with perfect fluid source in the framework of KaluzaKlein FRW space time in a modified theory of gravity known as f (R, T) gravity (Harko et al. 2011) where R is the Ricci scalar and T is the trace of the stress energy tensor of the perfect fluid. By solving the field equations, we have found an exact solution of the field equations using a linearly varying deceleration parameter which can be considered as a five dimensional FRW type cosmological model in f (R, T) gravity. We have determined the spatial volume and average Hubble parameter of the model. We have also determined and discussed the physical parameters, pressure and density for dust, radiation and stiff matter dominated eras.","PeriodicalId":319356,"journal":{"name":"International Journal of Physics: Study and Research","volume":"88 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2018-06-28","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"2","resultStr":"{\"title\":\"Kaluza-Klein FRW type Perfect Fluid Cosmological Models with Linearly varying Deceleration Parameter in a Modified Gravity\",\"authors\":\"D. Reddy, Y. Aditya\",\"doi\":\"10.18689/IJPSR-1000105\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Here, we investigate cosmological models with perfect fluid source in the framework of KaluzaKlein FRW space time in a modified theory of gravity known as f (R, T) gravity (Harko et al. 2011) where R is the Ricci scalar and T is the trace of the stress energy tensor of the perfect fluid. By solving the field equations, we have found an exact solution of the field equations using a linearly varying deceleration parameter which can be considered as a five dimensional FRW type cosmological model in f (R, T) gravity. We have determined the spatial volume and average Hubble parameter of the model. We have also determined and discussed the physical parameters, pressure and density for dust, radiation and stiff matter dominated eras.\",\"PeriodicalId\":319356,\"journal\":{\"name\":\"International Journal of Physics: Study and Research\",\"volume\":\"88 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2018-06-28\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"2\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"International Journal of Physics: Study and Research\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.18689/IJPSR-1000105\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"International Journal of Physics: Study and Research","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.18689/IJPSR-1000105","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 2
摘要
在这里,我们研究了KaluzaKlein FRW时空框架下具有完美流体源的宇宙学模型,该模型采用了一种被称为f (R, T)引力的修正引力理论(Harko et al. 2011),其中R是里奇标量,T是完美流体的应力能量张量的迹线。通过对场方程的求解,我们得到了在f (R, T)引力作用下使用线性变化的减速参数的场方程的精确解,可以看作是一个五维FRW型宇宙学模型。我们已经确定了该模型的空间体积和平均哈勃参数。我们还确定并讨论了尘埃、辐射和硬物质主导时代的物理参数、压力和密度。
Kaluza-Klein FRW type Perfect Fluid Cosmological Models with Linearly varying Deceleration Parameter in a Modified Gravity
Here, we investigate cosmological models with perfect fluid source in the framework of KaluzaKlein FRW space time in a modified theory of gravity known as f (R, T) gravity (Harko et al. 2011) where R is the Ricci scalar and T is the trace of the stress energy tensor of the perfect fluid. By solving the field equations, we have found an exact solution of the field equations using a linearly varying deceleration parameter which can be considered as a five dimensional FRW type cosmological model in f (R, T) gravity. We have determined the spatial volume and average Hubble parameter of the model. We have also determined and discussed the physical parameters, pressure and density for dust, radiation and stiff matter dominated eras.