vice.yields.ccsne.CL04

Chieffi & Limongi (2014), ApJ, 608, 405 core collapse supernova (CCSN) yields

Signature: from vice.yields.ccsne import CL04

Importing this module will automatically set the CCSN yield settings for all elements to the IMF-averaged yields calculated with the Chieffi & Limongi (2004) yield table for [M/H] = 0.15 stars. This will adopt an upper mass limit of 35 \(M_\odot\).

We provide core collapse supernova yields for non-rotating progenitors as reported by Chieffi & Limongi (2004) at metallicities relative to solar of \(\log_{10}(Z / Z_\odot)\) =

  • -inf

  • -4

  • -2

  • -1

  • -0.37

  • 0.15

assuming \(Z_\odot\) = 0.014 according to Asplund et al. (2009) 1.

Tip

By importing this module, the user does not sacrifice the ability to specify their yield settings directly.

Note

This module is not imported with a simple import vice statement.

Note

When this module is imported, the yields will be updated with a maximum of 10^5 bins in quadrature to decrease computational overhead. For some elements, the yield calculation may not converge. To rerun the yield calculation with higher numerical precision, simply call set_params with a new value for the keyword Nmax (see below).

Contents

set_params<function>

Update the parameters with which the yields are calculated.

1

Asplund et al. (2009), ARA&A, 47, 481