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Energy Sources in Stars (§10.3)

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Proton-Proton Cha<strong>in</strong>S<strong>in</strong>ce the Sun’s s mass consists mostly of H and He, we anticipatenuclear reactions <strong>in</strong>volv<strong>in</strong>g these two elementsegp + + p + → 2 Hep + + 4 He → 5 Li4 He + 4 He → 8 BeBut there is a problem here - what is it?All these reactions produce unstable particlesegp + + p + → 2 He → p + + p +p + + 4 He → 5 Li → p + + 4 He4 He + 4 He → 8 Be → 4 He + 4 HeSo among light elements there are no two-particle exothermicreactions produc<strong>in</strong>g stable particles. We have to look tomore peculiar reactions or those <strong>in</strong>volv<strong>in</strong>g rarer particles

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