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Nuclear Reactions in Stars & in the Laboratory

Nuclear Reactions in Stars & in the Laboratory

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Reaction rates for <strong>in</strong>verse Processes<br />

Detailed balance between<br />

forward & <strong>in</strong>verse reaction.<br />

A(a,b)B<br />

The reaction rate ratio<br />

between <strong>the</strong> forward &<br />

<strong>the</strong> <strong>in</strong>verse reaction<br />

depends on <strong>the</strong> Q-value<br />

and <strong>the</strong> temperature T!<br />

kT=T[GK]/11.605<br />

μ=m 1·m 2<br />

/(m 1<br />

+m 2<br />

)

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