Although beta decay is not directly part of nuclear fission, the beta-day lifetimes are sometimes so short that the additional beta-decay energy released can be counted as part of the total energy release in the total fission fragmentation process. There are many neutron-rich fission products with half-lives in the millisecond range.
When I referred to (anti) neutrinos carrying away "un-recoverable" energy, I did not mean that the energy is lost. The neutrinos end up in some other galaxy in a few thousand light-years, and release their energy there, but the energy is never really "lost". Energy is always conserved in some form, of which the lowest forms (when there are no constraints) are photons or phonons; gammas, X-rays. UV, light, IR, etc. With one exception (that I can think of), neutrinos are always released in a continuous spectrum up to a fixed-energy end point (Curie point), and never in a discrete energy line, like the 661-KeV Cs-137 gamma ray line for example.
When two equal-energy photons collide and create a matter-antimatter pair, the energy of the two photons adds to produce E
CM, or total energy in the center of mass. But the two photons do not literally couple to produce a single photon of twice the energy (e.g., "frequency doubling", like in lasers). Look up two-photon physics.
http://en.wikipedia.org/wiki/Two-photon_physics
Bob S