{"title":"空间均匀和各向异性两种形式的暗能量宇宙学模型","authors":"Y. Solanke, V. Dagwal, D. D. Pawar","doi":"10.47974/jdsgt-21-1-p05","DOIUrl":null,"url":null,"abstract":"We have examined spatially homogeneous and anisotropic cosmological models in the presence of two forms of dark energy (DE). We have calculated the exact solutions of the Einsteins field equations by assuming a special law of variation of Hubbles parameter [3] . Some physical parameters of the model are determined. From the point of kinematical behaviour we have also extended our work by deriving the analytic expressions for the look back time.","PeriodicalId":252169,"journal":{"name":"Journal of Dynamical Systems & Geometric Theories","volume":"10 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1900-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"SPATIALLY HOMOGENEOUS AND ANISOTROPIC TWO FORMS DARK ENERGY COSMOLOGICAL MODEL\",\"authors\":\"Y. Solanke, V. Dagwal, D. D. Pawar\",\"doi\":\"10.47974/jdsgt-21-1-p05\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"We have examined spatially homogeneous and anisotropic cosmological models in the presence of two forms of dark energy (DE). We have calculated the exact solutions of the Einsteins field equations by assuming a special law of variation of Hubbles parameter [3] . Some physical parameters of the model are determined. From the point of kinematical behaviour we have also extended our work by deriving the analytic expressions for the look back time.\",\"PeriodicalId\":252169,\"journal\":{\"name\":\"Journal of Dynamical Systems & Geometric Theories\",\"volume\":\"10 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"1900-01-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Journal of Dynamical Systems & Geometric Theories\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.47974/jdsgt-21-1-p05\",\"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 Dynamical Systems & Geometric Theories","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.47974/jdsgt-21-1-p05","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
SPATIALLY HOMOGENEOUS AND ANISOTROPIC TWO FORMS DARK ENERGY COSMOLOGICAL MODEL
We have examined spatially homogeneous and anisotropic cosmological models in the presence of two forms of dark energy (DE). We have calculated the exact solutions of the Einsteins field equations by assuming a special law of variation of Hubbles parameter [3] . Some physical parameters of the model are determined. From the point of kinematical behaviour we have also extended our work by deriving the analytic expressions for the look back time.
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