2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/179545The reaction rates of neutron capture reactions on light nuclei are important for reliably simulating nucleosynthesis in a variety of stellar scenarios. Neutron capture reaction rates on neutron-rich C-, N-, and O-isotopes are calculated in the framework of a hybrid compound and direct capture model. The results are tabulated and compared with the results of previous calculations as well as with experimental results.33 pages (uses revtex) and 9 postscript figures, accepted for publication in Phys. Rev. CNuclear TheoryAstrophysicsNuclear Experimenttext