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…
s(E) = S(E) e–2ph E-1 2ph = 31.29 Z1Z2 m/E m = m1m2 / (m1+m2) Reaction Rate(star) F(E) s(E) dE Gamow Peak s Maxwell Boltzmann Extrap. Meas. s Carlo Broggini…
s(E) = S(E) e–2ph E-1 2ph = 31.29 Z1Z2 m/E m = m1m2 / (m1+m2) Reaction Rate(star) F(E) s(E) dE Gamow Peak s Maxwell Boltzmann Extrap. Meas. s Carlo Broggini,…