ON silicon group elements ejected by supernovae type ia

Soma De, Francis Timmes, Edward F. Brown, Alan C. Calder, Dean M. Townsley, Themis Athanassiadou, David A. Chamulak, Wendy Hawley, Dennis Jack

Research output: Contribution to journalArticle

9 Citations (Scopus)

Abstract

There is evidence that the peak brightness of a Type Ia supernova is affected by the electron fraction Y e at the time of the explosion. The electron fraction is set by the aboriginal composition of the white dwarf and the reactions that occur during the pre-explosive convective burning. To date, determining the makeup of the white dwarf progenitor has relied on indirect proxies, such as the average metallicity of the host stellar population. In this paper, we present analytical calculations supporting the idea that the electron fraction of the progenitor systematically influences the nucleosynthesis of silicon group ejecta in Type Ia supernovae. In particular, we suggest the abundances generated in quasi-nuclear statistical equilibrium are preserved during the subsequent freeze-out. This allows potential recovery of Y e at explosion from the abundances recovered from an observed spectra. We show that measurement of 28Si, 32S, 40Ca, and 54Fe abundances can be used to construct Y e in the silicon-rich regions of the supernovae. If these four abundances are determined exactly, they are sufficient to recover Y e to 6%. This is because these isotopes dominate the composition of silicon-rich material and iron-rich material in quasi-nuclear statistical equilibrium. Analytical analysis shows the 28Si abundance is insensitive to Y e , the 32S abundance has a nearly linear trend with Y e , and the 40Ca abundance has a nearly quadratic trend with Y e . We verify these trends with post-processing of one-dimensional models and show that these trends are reflected in the model's synthetic spectra.

Original languageEnglish (US)
Article number149
JournalAstrophysical Journal
Volume787
Issue number2
DOIs
StatePublished - Jun 1 2014

Fingerprint

silicon
supernovae
trends
electron
explosions
explosion
electrons
ejecta
nuclear fusion
metallicity
explosive
brightness
isotopes
recovery
isotope
iron
trend

Keywords

  • nuclear reactions, nucleosynthesis, abundances
  • supernovae: general
  • white dwarfs

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

De, S., Timmes, F., Brown, E. F., Calder, A. C., Townsley, D. M., Athanassiadou, T., ... Jack, D. (2014). ON silicon group elements ejected by supernovae type ia. Astrophysical Journal, 787(2), [149]. https://doi.org/10.1088/0004-637X/787/2/149

ON silicon group elements ejected by supernovae type ia. / De, Soma; Timmes, Francis; Brown, Edward F.; Calder, Alan C.; Townsley, Dean M.; Athanassiadou, Themis; Chamulak, David A.; Hawley, Wendy; Jack, Dennis.

In: Astrophysical Journal, Vol. 787, No. 2, 149, 01.06.2014.

Research output: Contribution to journalArticle

De, S, Timmes, F, Brown, EF, Calder, AC, Townsley, DM, Athanassiadou, T, Chamulak, DA, Hawley, W & Jack, D 2014, 'ON silicon group elements ejected by supernovae type ia', Astrophysical Journal, vol. 787, no. 2, 149. https://doi.org/10.1088/0004-637X/787/2/149
De S, Timmes F, Brown EF, Calder AC, Townsley DM, Athanassiadou T et al. ON silicon group elements ejected by supernovae type ia. Astrophysical Journal. 2014 Jun 1;787(2). 149. https://doi.org/10.1088/0004-637X/787/2/149
De, Soma ; Timmes, Francis ; Brown, Edward F. ; Calder, Alan C. ; Townsley, Dean M. ; Athanassiadou, Themis ; Chamulak, David A. ; Hawley, Wendy ; Jack, Dennis. / ON silicon group elements ejected by supernovae type ia. In: Astrophysical Journal. 2014 ; Vol. 787, No. 2.
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