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.