Documents Carlo Broggini, INFN-Padova Nuclear Burning in Stars (E star ) ( E ) = S(E) e –2 E -1 2 cm m m m m...

Slide 1Carlo Broggini, INFN-Padova Nuclear Burning in Stars (E star ) ( E ) = S(E) e –2 E -1 2 cm m m m m Astrophysical Factor Gamow Factor Reaction Rate(star) (E) (E)…

Documents Carlo Broggini, INFN-Padova Nuclear Burning in Stars (E star ) ( E ) = S(E) e –2 E -1 2 ....

Slide 1Carlo Broggini, INFN-Padova Nuclear Burning in Stars  (E star )  ( E ) = S(E) e –2   E -1 2     …

Documents Carlo Broggini, INFN-Padova

Carlo Broggini, INFN-Padova Nuclear Burning in Stars s(Estar) s(E) = S(E) e–2ph E-1 2ph = 31.29 Z1Z2 m/Ecm m = m1m2 / (m1+m2) Astrophysical Factor Gamow Factor Reaction…

Documents Carlo Broggini, INFN-Padova

Carlo Broggini, INFN-Padova Nuclear Burning in Stars s(Estar) s(E) = S(E) e–2ph E-1 Reaction Rate(star)   F(E) s(E) dE Gamow Peak s Maxwell Boltzmann Extrap. Meas.…