PYCNONUCLEAR REACTIONS in dense stellar matter
PYCNONUCLEAR REACTIONS in dense stellar matter
PYCNONUCLEAR REACTIONS in dense stellar matter
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THERMONUCLEAR <strong>REACTIONS</strong><br />
Z<br />
1<br />
+ Z2<br />
→ Zc<br />
→<br />
...<br />
Reaction rate:<br />
n1n2<br />
R =<br />
1+<br />
δ<br />
12<br />
vσ<br />
reactions<br />
cm<br />
3<br />
s<br />
Z 1 Z 2<br />
∞<br />
∫<br />
0<br />
dv<br />
v<br />
3<br />
e<br />
−E / T<br />
σ<br />
( E)<br />
S(<br />
E)<br />
P(<br />
E)<br />
σ −η<br />
E<br />
( E) = , P(<br />
E)<br />
= exp( )<br />
a<br />
2 Z1Z<br />
η ( E)<br />
= 2 dr<br />
p(<br />
r)<br />
π<br />
h<br />
∫ =<br />
hv<br />
b<br />
2<br />
e<br />
2