Nuclear Astrophysics - Nuclear Physics
Nuclear Astrophysics - Nuclear Physics
Nuclear Astrophysics - Nuclear Physics
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Example:<br />
3 He + 3 He → 4 He + 2p<br />
T ~ 15x10 6 K (e.g. our Sun) ⇒ kT ~ 1 keV<br />
E 0 ~ 20 KeV<br />
σ ( E)<br />
=<br />
1<br />
E<br />
e<br />
−2πη<br />
S(<br />
E)<br />