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[ascl:2010.005] GRAPUS: GRAvitational instability PopUlation Synthesis

GRAPUS (GRAvitational instability PopUlation Synthesis) executes population synthesis modeling of self-gravitating disc fragmentation and tidal downsizing in protostellar discs. It reads in pre-run 1D viscous disc models of self-gravitating discs and computes where fragmentation will occur and the initial fragment mass. GRAPUS then allows these fragment embryos to evolve under various forces, including quasistatic collapse of the embryo, growth and sedimentation of the dust inside the embryo, and the formation of solid cores. The software also evolves migration due to embryo-disc interactions and tidal disruption of the embryo, and can optionally determine gravitational interactions with neighboring embryos.

Code site:
https://github.com/dh4gan/grapus
Described in:
https://ui.adsabs.harvard.edu/abs/2013MNRAS.432.3168F https://ui.adsabs.harvard.edu/abs/2018MNRAS.474.5036F
Bibcode:
2020ascl.soft10005F
Preferred citation method:

Please see citation information here: https://github.com/dh4gan/grapus#grapus---gravitational-instability-population-synthesis


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ascl:2010.005
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