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Nuclear Reactions in Stars & in the Laboratory

Nuclear Reactions in Stars & in the Laboratory

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Stellar reaction rates<br />

r<br />

1<br />

= YT<br />

Ypρ<br />

2 2<br />

NA<br />

< σv<br />

1+<br />

δ<br />

pT<br />

><br />

reactions per s and cm 3<br />

1<br />

λ = Y p<br />

ρ NA<br />

< σv<br />

1+<br />

δ<br />

pT<br />

><br />

reactions per s &<br />

Target nucleus<br />

this is usually referred to<br />

as <strong>the</strong> stellar reaction rate<br />

units of stellar reaction rate N A<br />

: usually cm 3 /s/mole<br />

n<br />

T<br />

X<br />

T<br />

= ρ ⋅ N<br />

A<br />

⋅ = ρ ⋅<br />

AT<br />

N<br />

A<br />

⋅Y<br />

T<br />

X T ; mass fraction<br />

Y T : abundance

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