Theory of Quasi‐Equilibrium Nucleosynthesis and Applications to Matter Expanding from High Temperature and Density
- 10 May 1998
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 498 (2) , 808-830
- https://doi.org/10.1086/305562
Abstract
No abstract availableThis publication has 12 references indexed in Scilit:
- Synthesis of the elements in stars: forty years of progressReviews of Modern Physics, 1997
- 48Ca Production in Matter Expanding from High Temperature and DensityThe Astrophysical Journal, 1996
- Silicon Burning. I. Neutronization and the Physics of Quasi-EquilibriumThe Astrophysical Journal, 1996
- The alpha-process and the r-processThe Astrophysical Journal, 1992
- Explosive nucleosynthesis in SN 1987A. II - Composition, radioactivities, and the neutron star massThe Astrophysical Journal, 1990
- Thermonuclear reaction rates VAtomic Data and Nuclear Data Tables, 1988
- Nucleosynthesis in neutron-rich supernova ejectaThe Astrophysical Journal, 1985
- The Explosive Burning of Oxygen and SiliconThe Astrophysical Journal Supplement Series, 1973
- Nuclear Quasi-Equilibrium during Silicon BurningThe Astrophysical Journal Supplement Series, 1968
- The Synthesis of the Elements from HydrogenMonthly Notices of the Royal Astronomical Society, 1946