Stellar Nucleosynthesis

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Elemental Abundances in the Solar SystemSynthesized in the Big BangWe need to consider the creation of all the other elementsin stars.
Abundances of nuclei3Slide: Stephen Smartt
Page 1: Stellar NucleosynthesisThey Might b
Page 5 and 6: Review: Binding Energy of Nuclei
Page 7 and 8: Rate of Reactions
Page 9 and 10: Occurrence of fusion reactionsNow w
Page 11 and 12: The Gamow peakSchematically this is
Page 13 and 14: ResonancesResonanceC 12 + P => N 13
Page 15 and 16: Relative importance of PPIand PPII
Page 17 and 18: When does a given P-P chain dominat
Page 19 and 20: The CNO CycleAt birth stars contain
Page 21 and 22: Temperature dependence of PP chain
Page 23 and 24: Changes in Elemental Abundances Dur
Page 25 and 26: Helium Burning: the triple-α react
Page 27 and 28: Carbon and oxygen burningCarbon bur
Page 29 and 30: Major nuclear burning processesComm
Page 31 and 32: In the process two types of reactio
Page 33: 1.We described the basic accounting

Stellar Nucleosynthesis

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