Silicon Burning. II. Quasi‐Equilibrium and Explosive Burning
Author(s) -
W. R. Hix,
F.K. Thielemann
Publication year - 1999
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/306692
Subject(s) - explosive material , hydrostatic equilibrium , adiabatic process , silicon , thermodynamic equilibrium , chemical equilibrium , physics , nucleosynthesis , abundance (ecology) , thermodynamics , nuclear physics , nuclear reaction , chemistry , optoelectronics , organic chemistry , fishery , biology , quantum mechanics
Having examined the application of quasi-equilibrium to hydrostatic siliconburning in Paper I of this series, Hix & Thielemann (1996), we now turn ourattention to explosive silicon burning. Previous authors have shown that formaterial which is heated to high temperature by a passing shock and then cooledby adiabatic expansion, the results can be divided into three broad categories;\emph{incomplete burning}, \emph{normal freezeout} and \emph{$\alpha$-richfreezeout}, with the outcome depending on the temperature, density and coolingtimescale. In all three cases, we find that the important abundances obeyquasi-equilibrium for temperatures greater than approximately 3 GK, withrelatively little nucleosynthesis occurring following the breakdown ofquasi-equilibrium. We will show that quasi-equilibrium provides betterabundance estimates than global nuclear statistical equilibrium, even fornormal freezeout and particularly for $\alpha$-rich freezeout. We will alsoexamine the accuracy with which the final nuclear abundances can be estimatedfrom quasi-equilibrium.Comment: 27 pages, including 15 inline figures. LaTeX 2e with aaspp4 and graphicx packages. Accepted to Ap
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