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• W3098086871 abstract "If axions exist, they are copiously produced in hot and dense plasmas, carrying away energy directly from the interior of stars. Various astronomical observables constrain the operation of such anomalous stellar energy-loss channels and thus provide a restrictive limits on the axion interactions with photons, nucleons, and electrons. In typical axion models a limit ma⪅10−2eV is implied. The main arguments leading to this result are explained, including more recent work on the important supernova 1987A constraint." @default.
• W3098086871 created "2020-11-23" @default.
• W3098086871 creator A5019081841 @default.
• W3098086871 date "1999-03-01" @default.
• W3098086871 modified "2023-09-26" @default.
• W3098086871 title "Stellar-evolution limits on axion properties" @default.
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• W3098086871 doi "https://doi.org/10.1016/s0920-5632(98)00501-5" @default.
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