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MODULES FOR EXPERIMENTS IN STELLAR ASTROPHYSICS (MESA): BINARIES, PULSATIONS, AND EXPLOSIONS

  • Authors: Bill Paxton, Pablo Marchant, Josiah Schwab, Evan B. Bauer, Lars Bildsten, Matteo Cantiello, Luc Dessart, R. Farmer, H. Hu, N. Langer, R. H. D. Townsend, Dean M. Townsley, and F. X. Timmes

2015 The Astrophysical Journal Supplement Series 220 15.

  • Provider: AAS Journals

Caption: Figure 19.

Evolution of the composition for a one-zone burn at constant T = 9.6 × 109 K and ρ = 6.0 × 109 g cm−3 for 106 s starting with a pure 28Si composition. The calculation uses the mesa_204.net isotope listing (see Table 2), the most abundant isotopes are drawn with thick lines, and several isotopes are labeled. The initial composition is quickly erased as NSE for ﹩{Y}_{{\rm{e}}}\;\approx ﹩ 0.5 is established by ﹩\approx ﹩ 10−8 s. Several orders of magnitude in time pass before weak reactions drive a second period of rearrangement. By ﹩\approx 10﹩ s a second NSE quiescent period with ﹩{Y}_{{\rm{e}}}\;\approx ﹩ 0.403 is established.

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