{"title":"带标量场的弗里德曼宇宙论的精确解","authors":"I. Fomin","doi":"10.17238/issn2226-8812.2018.1.21-30","DOIUrl":null,"url":null,"abstract":"The method of exact analysis of cosmological dynamics at the early inflation stage of the evolution of the Friedman Universe, which is determined by the dynamics of the scalar field for the case of minimal and nonminimal interaction of the field and curvature is considered in this work. The basis of the method is to reduce the equations of dynamics to the same form for all models. The proposed approach allows us to compare models based on the different theories of gravity.","PeriodicalId":445582,"journal":{"name":"SPACE, TIME AND FUNDAMENTAL INTERACTIONS","volume":"25 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2018-06-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"2","resultStr":"{\"title\":\"EXACT SOLUTIONS IN FRIEDMANN COSMOLOGY WITH SCALAR FIELDS\",\"authors\":\"I. Fomin\",\"doi\":\"10.17238/issn2226-8812.2018.1.21-30\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The method of exact analysis of cosmological dynamics at the early inflation stage of the evolution of the Friedman Universe, which is determined by the dynamics of the scalar field for the case of minimal and nonminimal interaction of the field and curvature is considered in this work. The basis of the method is to reduce the equations of dynamics to the same form for all models. The proposed approach allows us to compare models based on the different theories of gravity.\",\"PeriodicalId\":445582,\"journal\":{\"name\":\"SPACE, TIME AND FUNDAMENTAL INTERACTIONS\",\"volume\":\"25 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2018-06-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"2\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"SPACE, TIME AND FUNDAMENTAL INTERACTIONS\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.17238/issn2226-8812.2018.1.21-30\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"SPACE, TIME AND FUNDAMENTAL INTERACTIONS","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.17238/issn2226-8812.2018.1.21-30","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
EXACT SOLUTIONS IN FRIEDMANN COSMOLOGY WITH SCALAR FIELDS
The method of exact analysis of cosmological dynamics at the early inflation stage of the evolution of the Friedman Universe, which is determined by the dynamics of the scalar field for the case of minimal and nonminimal interaction of the field and curvature is considered in this work. The basis of the method is to reduce the equations of dynamics to the same form for all models. The proposed approach allows us to compare models based on the different theories of gravity.
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