Overview
In this section, we summarize the treatment for each dust process in CosmicGrain.
Here is a list of the primary research sources for the dust physics:
- DUST CREATION
- Todini & Ferrara 2001 — SN dust yields
- Ferrarotti & Gail 2006 — AGB dust yields
- Nozawa et al. 2003 — Dust condensation in SN ejecta *
- GRAIN GROWTH (accretion)
- Hirashita & Kuo 2011 (HK11) — Subgrid accretion timescales
- Asano et al. 2013 — Accretion + coagulation framework *
- THERMAL SPUTTERING
- Draine & Salpeter 1979 — Thermal sputtering physics
- McKinnon et al. 2017 — Sputtering timescale formula (Eq. 2)
- Tsai & Mathews 1995 — Sputtering in hot gas *
- SHOCK DESTRUCTION
- McKee & Ostriker 1977 — SN energetics (10^51 erg standard)
- Sedov 1959 — Self-similar blast wave solution
- Jones et al. 1994, 1996 — Grain shattering threshold (~50 km/s)
- Bocchio et al. 2014 — Grain destruction efficiencies (Table 6) *
- DRAG COUPLING
- McKinnon et al. 2018 — Epstein drag (eqs. 8–9) *
- GRAIN TEMPERATURE
- Hollenbach & McKee 1979 — Gas-grain collisional coupling
- Draine & Lee 1984 — Modified blackbody Q_abs opacity law
- Mathis et al. 1983 — ISRF parametrisation
- Draine & Li 2007 — Grain opacity and composition *
- RADIATION PRESSURE
- Draine & Lee 1984 — Q_pr radiation pressure efficiency
- Draine & Li 2007 — Grain opacity and composition treatment *
- GENERAL FRAMEWORK
- Dwek 1998 — Dust evolution in the ISM
- McKinnon et al. 2016 — Dust in cosmological simulations