Abstract: KEPLER is a general purpose stellar evolution/explosion code that incorporates implicit hydrodynamics and a detailed treatment of nuclear burning processes. It has been used to study the complete evolution of massive and supermassive stars, all major classes of supernovae, hydrostatic and explosive nucleosynthesis, and x- and gamma-ray bursts on neutron stars and white dwarfs.
Credit: Weaver, T.A.; Zimmerman, G.B.; Woosley, S.E.
Preferred citation method: http://adsabs.harvard.edu/abs/1978ApJ...225.1021W