{"title":"Cosmological Nucleosynthesis","authors":"","doi":"10.2307/j.ctv173f2k2.10","DOIUrl":null,"url":null,"abstract":"O In the discussion of the thermal history of the early universe form temperatures 10 11 • K down to about 10 6 • K we were neglecting the tiny contribution of relict nucleons which were not completely annihilated in particle-antiparticle annihilation.","PeriodicalId":445387,"journal":{"name":"Supernovae and Nucleosynthesis","volume":"28 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2020-11-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Supernovae and Nucleosynthesis","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.2307/j.ctv173f2k2.10","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
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Abstract
O In the discussion of the thermal history of the early universe form temperatures 10 11 • K down to about 10 6 • K we were neglecting the tiny contribution of relict nucleons which were not completely annihilated in particle-antiparticle annihilation.
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