vice.yields.sneia.gronow21¶
Gronow et al. (2021a, b) Type Ia supernova (SN Ia) yields
Signature: from vice.yields.sneia import gronow21
New in version 1.3.0.
Importing this module will automatically set the SN Ia yield settings for all elements to the delay-time distribution integrated yields calculated with the Gronow et al. (2021a, b) [1] [2] yield tables under the M10_10_1 progenitor model. These studies reports yields for double detonations of sub-Chandrasekhar mass (1.4 \(M_\odot\)) white dwarfs at various progenitor metallicities, with the solar metallicity yields published in Gronow et al. (2021a) and those for remaining metallicities (\(Z / Z_\odot\) = 0.01, 0.1, and 3) in Gronow et al. (2021b).
We provide type Ia supernova yields from the Gronow et al. (2021a, b) studies under the following explosion models presented in their journal publications:
M08_03_001, M08_03_01, M08_03_1, M08_03_3
M08_05_001, M08_05_01, M08_05_1, M08_05_3
M08_10_001, M08_10_01, M08_10_1, M08_10_3
M09_03_001, M09_03_01, M09_03_1, M09_03_3
M09_05_001, M09_05_01, M09_05_1, M09_05_3
M09_10_001, M09_10_01, M09_10_1, M09_10_3
M10_02_001, M10_02_01, M10_02_1, M10_02_3
M10_03_001, M10_03_01, M10_03_1, M10_03_3
M10_05_001, M10_05_01, M10_05_1, M10_05_3
M10_10_001, M10_10_01, M10_10_1, M10_10_3
M11_05_001, M11_05_01, M11_05_1, M11_05_3
These models are named for the mass of the carbon-oxygen core, the mass of the helium shell, and the metallicity of the progenitor relative to solar, in that order. For example, the “M09_05_01” model refers to one with a 0.9 \(M_\odot\) carbon-oxygen core and a 0.05 \(M_\odot\) helium shell produced by a star that was initially at a metallicity of 0.1 \(Z_\odot\).
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.
Contents¶
- set_params<function>
Update the parameters with which the yields are calculated.