{"title":"SMBH relativistic mass and missing dark matter","authors":"Niko Gorjup, A. Šorli","doi":"10.12988/astp.2022.91963","DOIUrl":null,"url":null,"abstract":"The extremely high angular velocity of some SMBHs is the origin of their relativistic rotational energy that results in their relativistic mass. The relativistic mass of SMBHs increases their gravity, which is a partial answer to the missing dark matter.","PeriodicalId":127314,"journal":{"name":"Advanced Studies in Theoretical Physics","volume":"279 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1900-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"2","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Advanced Studies in Theoretical Physics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.12988/astp.2022.91963","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 2
Abstract
The extremely high angular velocity of some SMBHs is the origin of their relativistic rotational energy that results in their relativistic mass. The relativistic mass of SMBHs increases their gravity, which is a partial answer to the missing dark matter.
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