TRAPPING OF NEUTRINOS IN EXTREMELY COMPACT STARS AND THE INFLUENCE OF BRANE TENSION ON THIS PROCESS

We present estimates on the efficiency of neutrino trapping in brany extremely compact stars, using the simplest model with uniform distribution of energy density, assuming massless neutrinos and uniform distribution of neutrino emissivity. Computation have been done for two different uniform-density stellar solution in the Randall–Sundrum II