{"title":"引力参数G在宇宙学中的决定性作用","authors":"Vladimir S. Netchitailo","doi":"10.4236/jhepgc.2023.93051","DOIUrl":null,"url":null,"abstract":"In 1937, P. Dirac proposed the Large Number Hypothesis and the Hypothesis of the variable gravitational “constant,” and later added the notion of continuous creation of Matter in the World. The Hypersphere World-Universe Model (WUM) follows these ideas, albeit introducing a different mechanism of Matter creation. In this paper we show that Gravitational parameter G that can be measured directly makes measurable all Cosmological parameters, which cannot be measured directly.","PeriodicalId":59175,"journal":{"name":"高能物理(英文)","volume":null,"pages":null},"PeriodicalIF":0.0000,"publicationDate":"2023-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"4","resultStr":"{\"title\":\"Decisive Role of Gravitational Parameter <i>G</i> in Cosmology\",\"authors\":\"Vladimir S. Netchitailo\",\"doi\":\"10.4236/jhepgc.2023.93051\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"In 1937, P. Dirac proposed the Large Number Hypothesis and the Hypothesis of the variable gravitational “constant,” and later added the notion of continuous creation of Matter in the World. The Hypersphere World-Universe Model (WUM) follows these ideas, albeit introducing a different mechanism of Matter creation. In this paper we show that Gravitational parameter G that can be measured directly makes measurable all Cosmological parameters, which cannot be measured directly.\",\"PeriodicalId\":59175,\"journal\":{\"name\":\"高能物理(英文)\",\"volume\":null,\"pages\":null},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2023-01-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"4\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"高能物理(英文)\",\"FirstCategoryId\":\"1089\",\"ListUrlMain\":\"https://doi.org/10.4236/jhepgc.2023.93051\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"高能物理(英文)","FirstCategoryId":"1089","ListUrlMain":"https://doi.org/10.4236/jhepgc.2023.93051","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Decisive Role of Gravitational Parameter G in Cosmology
In 1937, P. Dirac proposed the Large Number Hypothesis and the Hypothesis of the variable gravitational “constant,” and later added the notion of continuous creation of Matter in the World. The Hypersphere World-Universe Model (WUM) follows these ideas, albeit introducing a different mechanism of Matter creation. In this paper we show that Gravitational parameter G that can be measured directly makes measurable all Cosmological parameters, which cannot be measured directly.