ASCL.net

Astrophysics Source Code Library

Making codes discoverable since 1999

ASCL Code Record

[ascl:1807.023] DAMOCLES: Monte Carlo line radiative transfer code

The Monte Carlo code DAMOCLES models the effects of dust, composed of any combination of species and grain size distributions, on optical and NIR emission lines emitted from the expanding ejecta of a late-time (> 1 yr) supernova. The emissivity and dust distributions follow smooth radial power-law distributions; any arbitrary distribution can be specified by providing the appropriate grid. DAMOCLES treats a variety of clumping structures as specified by a clumped dust mass fraction, volume filling factor, clump size and clump power-law distribution, and the emissivity distribution may also initially be clumped. The code has a large number of variable parameters ranging from 5 dimensions in the simplest models to > 20 in the most complex cases.

Code site:
https://github.com/damocles-code/damocles
Appears in:
http://adsabs.harvard.edu/abs/2016MNRAS.456.1269B http://adsabs.harvard.edu/abs/2018arXiv180310241B
Bibcode:
2018ascl.soft07023B

Views: 293

ascl:1807.023
Add this shield to your page
Copy the above HTML to add this shield to your code's website.