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Stellar proton cycle

The first major set of nuclear reactions in stellar evolution involves hydrogenburning through the pp chains and the CN cycle or CNO bi-cycle, which liberate 6.68 MeV of energy per proton minus neutrino losses (2 neutrinos are emitted for each 4He nucleus synthesized). The first two reactions of the pp chains are... [Pg.167]

See other pages where Stellar proton cycle is mentioned: [Pg.872]    [Pg.174]    [Pg.3]    [Pg.144]    [Pg.298]    [Pg.432]    [Pg.39]    [Pg.46]    [Pg.71]    [Pg.72]    [Pg.77]    [Pg.11]    [Pg.222]    [Pg.233]    [Pg.62]    [Pg.573]    [Pg.642]   
See also in sourсe #XX -- [ Pg.22 ]



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