We propose an oscillation mechanism for meson mixing that causes charg
e symmetry breaking in nucleon-nucleon interactions. The mixing probab
ilities of the rho meson component in the omega meson and vice versa a
re estimated in a nuclear medium by using the data of the branching ra
tio B(omega-->2 pi) and proton-proton (p-p) and neutron-neutron (n-n)
scattering lengths. It is shown that the mixing probability depends on
the nuclear density and is very small at normal density. In a nuclear
medium, rho-omega mixing is larger in the p-p interaction than in the
n-n interaction because of Coulomb repulsion.