{"title":"萨德伯里中微子天文台的太阳反中微子探测","authors":"A. Balantekin, F. Loreti","doi":"10.1063/1.41482","DOIUrl":null,"url":null,"abstract":"Antineutrinos can be produced in the sun by the spin‐flavor precession. The possibility of detecting such antineutrinos at the Sudbury Neutrino Observatory is examined.","PeriodicalId":316054,"journal":{"name":"Intersections between particle and nuclear physics","volume":"14 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2008-05-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":"{\"title\":\"Solar antineutrino detection at Sudbury Neutrino Observatory\",\"authors\":\"A. Balantekin, F. Loreti\",\"doi\":\"10.1063/1.41482\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Antineutrinos can be produced in the sun by the spin‐flavor precession. The possibility of detecting such antineutrinos at the Sudbury Neutrino Observatory is examined.\",\"PeriodicalId\":316054,\"journal\":{\"name\":\"Intersections between particle and nuclear physics\",\"volume\":\"14 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2008-05-29\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"1\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Intersections between particle and nuclear physics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1063/1.41482\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Intersections between particle and nuclear physics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1063/1.41482","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Solar antineutrino detection at Sudbury Neutrino Observatory
Antineutrinos can be produced in the sun by the spin‐flavor precession. The possibility of detecting such antineutrinos at the Sudbury Neutrino Observatory is examined.
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