Nucleosynthesis in Type II Supernovae
K. Nomoto, M. Hashimoto, T. Tsujimoto, F. -K. Thielemann, N. Kishimoto, Y. Kubo
Abstract
Presupernova evolution and explosive nucleosynthesis in massive stars for main-sequence masses from 13 M to 70 M are calculated. We examine the dependence of the supernova yields on the stellar mass, 12C(α, γ) 16O rate, and explosion energy. The supernova yields integrated over the initial mass function are compared with the solar abundances.
Create a lesson
Related papers
On binary pulsars and the force of gravity
Davor Palle
Tidal torques. A critical review of some techniques
Michael Efroimsky, James G. Williams
Dynamics of a Spherical Accretion Shock with Neutrino Heating and Alpha-Particle Recombination
Rodrigo Fernández, Christopher Thompson
Asymptotically FRW black holes
J. T. Firouzjaee, Reza Mansouri
Reaction of Accretion Disks to Abrupt Mass Loss During Binary Black Hole Merger
Sean M. O'Neill, M. Coleman Miller, Tamara Bogdanovic et al.
A Gamma-Ray Burst/Pulsar for Cosmic-Ray Positrons with a Dark Matter-like Spectrum
Kunihito Ioka