Trans-Fe elements from Type Ia Supernovae. I. Heavy element nucleosynthesis during the formation of near-Chandrasekhar white dwarfs

Heavy element nucleosynthesis during the formation of near-Chandrasekhar white dwarfs Skip to main content We gratefully acknowledge support from the Simons Foundation, member institutions , and all contributors.
Heavy element nucleosynthesis during the formation of near-Chandrasekhar white dwarfs, by Umberto Battino and 10 other authors View PDF Abstract: Type Ia supernovae (SNIa) are thermonuclear explosions of white dwarfs in binary systems.
In this work, we present a grid of five models detailing the evolution and nucleosynthesis of slowly merging carbon-oxygen white dwarfs approaching the Chandrasekhar mass.
Connected Papers Toggle Connected Papers ( What is Connected Papers? )
Links to Code Toggle Papers with Code ( What is Papers with Code? )