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Nuclear Astrophysics - Nuclear Physics

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Nucleosynthesis beyond Fe<br />

process<br />

conditions<br />

timescale<br />

site<br />

s-process<br />

(n,γ)<br />

β-decay<br />

...<br />

T~ 0.1 GK<br />

τ n ~ 1-1000 yr, n n ~10 7-8 /cm 3<br />

10 2 yr<br />

10 5-6 yrs<br />

Massive stars (weak)<br />

Low-mass AGB stars (main)<br />

r-process<br />

(n,γ)<br />

β-decay<br />

β-delayed n-emission<br />

fission<br />

...<br />

T~1-2 GK<br />

τ n ~ μs, n n ~10 24 /cm 3<br />

< 1s<br />

Type II Supernovae ?<br />

Neutron Star Mergers ?<br />

www.cyc.ucl.ac.be/CARINA<br />

a mengoni for CARINA

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