R. Muharlyamov, T. Pankratyeva, Shehabaldeen O. A. Bashir
{"title":"Isotropization of the magnetic universe in the Horndeski theory with $G_3(X,\\phi)$ and $G_5(X)$","authors":"R. Muharlyamov, T. Pankratyeva, Shehabaldeen O. A. Bashir","doi":"10.1088/1674-1137/ad65de","DOIUrl":null,"url":null,"abstract":"\n We study the isotropization process of Bianchi-I space-times in the Horndeski theory with $G_3(X,\\phi)\\neq 0$ and $G_5=\\text{const}/X$. A global unidirectional electromagnetic field interacts with a scalar field according to the law $f^2(\\phi)F_{\\mu\\nu}F^{\\mu\\nu}$. In the Horndeski theory, the anisotropy can develop in different ways. The proposed reconstruction method allowed us to build models with acceptable the anisotropy behavior. To analyze space-time anisotropy, we used the relations $a_i/a$ ($i=1,2,3$), where $a_i$ are metric functions and $a\\equiv(a_1a_2a_3)^{1/3}$.","PeriodicalId":504778,"journal":{"name":"Chinese Physics C","volume":"3 6","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-07-22","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Chinese Physics C","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1088/1674-1137/ad65de","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
We study the isotropization process of Bianchi-I space-times in the Horndeski theory with $G_3(X,\phi)\neq 0$ and $G_5=\text{const}/X$. A global unidirectional electromagnetic field interacts with a scalar field according to the law $f^2(\phi)F_{\mu\nu}F^{\mu\nu}$. In the Horndeski theory, the anisotropy can develop in different ways. The proposed reconstruction method allowed us to build models with acceptable the anisotropy behavior. To analyze space-time anisotropy, we used the relations $a_i/a$ ($i=1,2,3$), where $a_i$ are metric functions and $a\equiv(a_1a_2a_3)^{1/3}$.