s ( E ) = S(E) e –2 ph E -1
LUNA, the Sun and the other stars. Stellar Energy+Nucleosynthesis. Hydrogen Burning. s (E star ) with E star << E Coulomb. Carlo Broggini, INFN-Padova. s ( E ) = S(E) e –2 ph E -1. m = m 1 m 2 / ( m 1 + m 2 ). 2 ph = 31.29 Z 1 Z 2 m/E. . Reaction Rate(star) . F (E) s (E) dE.
222 views • 13 slides