vice.yields.ccsne.NKT13

Nomoto, Kobayashi & Tominaga (2013), ARA&A, 51, 457 core collapse supernova yields

Signature: from vice.yields.ccsne import NKT13

New in version 1.2.0.

Importing this module will automatically set the CCSN yield settings for all elements to the IMF-averaged yields calculated with the Nomoto, Kobayashi & Tominaga (2013) yield table for [M/H] = 0.15 stars. This will adopt an upper mass limit of 40 \(M_\odot\).

Tip

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

Note

[M/H] = 0.15 corresponds to Z = 0.02 if the solar abundance is Z = 0.014 (Asplund et al. 2009) 1.

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 calcualted.

1

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

• vice.yields.ccsne.NKT13.set_params