vice.yields.ccsne

Core Collapse Supernovae (CCSNe) Nucleosynthetic Yield Tools

Calculate IMF-averaged yields and modify yield settings for use in simulations. This package provides tables from the following nucleosynthetic yield studies:

  • Limongi & Chieffi (2018) [1]

  • Sukhbold et al. (2016) [2]

  • Chieffi & Limongi (2013) [3]

  • Nomoto, Kobayashi & Tominaga (2013) [4]

  • Chieffi & Limongi (2004) [5]

  • Woosley & Weaver (1995) [6]

Contents

fractional<function>

Calculate an IMF-averaged yield for a given element.

table<function>

Obtain the table of mass yields and progenitor masses for a given element from a given study.

settingsdataframe

Stores current settings for these yields.

enginesmodule

Models for massive star explodability as a function of progenitor mass for use in yield calculations.

LC18module

Sets yields according to the Limongi & Chieffi (2018) study.

S16module

Sets the yields according to one of the explosion engines in the Sukhbold et al. (2016) study.

CL13module

Sets yields according to the Chieffi & Limongi (2013) study.

NKT13module

Sets yields according to the Nomoto, Kobayashi & Tominaga (2013) study.

CL04module

Sets yields according to the Chieffi & Limongi (2004) study.

WW95module

Sets yields according to the Woosley & Weaver (1995) study.

Notes

The yield tables built into this module reflect a post-processing treatment for two radioactive nuclides. For the Limongi & Chieffi (2018), Sukhbold et al. (2016), and Chieffi & Limongi (2013) tables, we add the nickel-56 yield to the iron yields and the aluminum-26 yield to the magnesium yields. We also add the aluminum-26 yield to the magnesium yields for the Woosley & Weaver (1995) study. Otherwise, the data are included as published. The Chieffi & Limongi (2013) and Nomoto, Kobayashi & Tominaga (2013) yields report yields after radioactive isotopes have been decayed, so no further treatment is necessary.