Isotopic distributions for light particles and intermediate mass fragments
have been measured for Sn-112+Sn-112, Sn-112+Sn-124, Sn-124+Sn-112 and Sn-1
24+Sn-124 collisions at E/A=50 MeV. Isotope, isotone and isobar yield ratio
techniques are utilized to obtain an estimate of the relative abundance of
free neutrons and protons at breakup. Consistent with the predictions of s
tatistical models, which include two components in the liquid gas phase tra
nsition, neutrons and protons are not uniformly distributed at breakup. Ins
tead, the neutron excess is amplified in the light charged particles.