The quasi-equilibrium-reduced α-network

W. Raphael Hix, Alexei M. Khokhlov, J. Craig Wheeler, Friedrich Karl Thielemann

Research output: Contribution to journalArticlepeer-review

33 Scopus citations

Abstract

An examination of the process of silicon burning, the burning stage that leads to the production of the iron peak nuclei, reveals that the nuclear evolution is dominated by large groups of nuclei in mutual equilibrium. These quasi-equilibrium (QSE) groups form well in advance of the global nuclear statistical equilibrium (NSE). We present an improved "minimal" nuclear network, which takes advantage of QSE in order to calculate the nuclear evolution and energy generation while further reducing the computational cost compared with a conventional α-chain network. During silicon burning the resultant QSE-rcduced α-network is twice as fast as the full α-network it replaces and requires the tracking of only half as many abundance variables, without significant loss of accuracy. When the QSE-reduced α-network is used in combination with a conventional a-network stretching from He to Si, the combined network, which we call the α7 network, provides an accurate approximation for all of the burning stages from He burning to NSE, while tracking only seven abundances. These reductions in computational cost and the number of species evolved make the α7 network well suited for inclusion within hydrodynamic simulations, particularly those in multidimension.

Original languageEnglish
Pages (from-to)332-343
Number of pages12
JournalAstrophysical Journal
Volume503
Issue number1 PART I
DOIs
StatePublished - 1998

Keywords

  • Methods: numerical
  • Nuclear reactions, nucleosynthesis, abundances stars: evolution
  • Supernovae: general

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