Abstract
Having examined the application of quasi-equilibrium to hydrostatic silicon burning in Paper I of this series, we now turn our attention to explosive silicon burning. Previous authors have shown that for material that is heated to high temperature by a passing shock and then cooled by adiabatic expansion, the results can be divided into three broad categories, incomplete burning, normal freezeout, and α-rich freezeout, with the outcome depending on the temperature, density, and cooling timescale. In all three cases, we find that the important abundances obey quasi-equilibrium for temperatures greater than approximately 3 × 109 K, with relatively little nucleosynthesis occurring following the breakdown of quasi-equilibrium. We will show that quasi-equilibrium provides better abundance estimates than global nuclear statistical equilibrium, even for normal freezeout, and particularly for α-rich freezeout. We will also examine the accuracy with which the final nuclear abundances can be estimated from quasi-equilibrium.
Original language | English |
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Pages (from-to) | 862-875 |
Number of pages | 14 |
Journal | Astrophysical Journal |
Volume | 511 |
Issue number | 2 PART 1 |
DOIs | |
State | Published - Feb 1 1999 |
Keywords
- Nuclear reactions
- Stars: evolution
- Supernovae: general
- abundances
- nucleosynthesis