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 \(M_\odot\).
We provide core collapse supernova yields for non-rotating progenitors as reported Nomoto, Kobayashi & Tominaga (2013) at metallicities relative to solar of \(\log_{10}(Z / Z_\odot)\) =
-inf
-1.15
-0.54
-0.24
0.15
0.55
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 calcualted.