{"title":"具有完美流体分布的f (R,T)理论中的高维Bianchi V模型","authors":"Kirti Khurdiya, Ajeet Singh","doi":"10.22147/jusps-a/350601","DOIUrl":null,"url":null,"abstract":"In this paper we have studied five-dimensional Bianchi type-V spacetime in the f (R,T) theory. To solve Einstein’s field equations, we have assumed that the Hubble parameter is inversely proportional toݎ ℎݐ power of the scale factor alpha i.e. H alpha 1/alphar. We have obtained a singular model for r >0, non-singular model for r=0. The physical behavior of the models has also been discussed using some physical parameters.","PeriodicalId":200922,"journal":{"name":"Journal of Ultra Scientist of Physical Sciences Section A","volume":"15 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2023-08-03","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Higher Dimensional Bianchi V Models in f (R,T) Theory with Perfect Fluid Distribution\",\"authors\":\"Kirti Khurdiya, Ajeet Singh\",\"doi\":\"10.22147/jusps-a/350601\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"In this paper we have studied five-dimensional Bianchi type-V spacetime in the f (R,T) theory. To solve Einstein’s field equations, we have assumed that the Hubble parameter is inversely proportional toݎ ℎݐ power of the scale factor alpha i.e. H alpha 1/alphar. We have obtained a singular model for r >0, non-singular model for r=0. The physical behavior of the models has also been discussed using some physical parameters.\",\"PeriodicalId\":200922,\"journal\":{\"name\":\"Journal of Ultra Scientist of Physical Sciences Section A\",\"volume\":\"15 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2023-08-03\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Journal of Ultra Scientist of Physical Sciences Section A\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.22147/jusps-a/350601\",\"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 Ultra Scientist of Physical Sciences Section A","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.22147/jusps-a/350601","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Higher Dimensional Bianchi V Models in f (R,T) Theory with Perfect Fluid Distribution
In this paper we have studied five-dimensional Bianchi type-V spacetime in the f (R,T) theory. To solve Einstein’s field equations, we have assumed that the Hubble parameter is inversely proportional toݎ ℎݐ power of the scale factor alpha i.e. H alpha 1/alphar. We have obtained a singular model for r >0, non-singular model for r=0. The physical behavior of the models has also been discussed using some physical parameters.
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