{"title":"宇宙核合成","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":"{\"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}","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}
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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