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Gamma ray heating and neutrino cooling rates due to weak interaction processes on s d $sd$ -shell nuclei in stellar cores

Crossref DOI link: https://doi.org/10.1007/s10509-017-3112-1

Published Online: 2017-06-26

Published Print: 2017-07

Update policy: https://doi.org/10.1007/springer_crossmark_policy