Self-gravitating disks with Radiative Transfer: Their role in Giant Planet Formation

Details Self-gravitating disks with Radiative Transfer: Their role in Giant Planet Formation Self-gravitating disks with Radiative Transfer: Their role in Giant Planet Formation

Aug 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1158..139m&link_type=abstract

EXOPLANETS AND DISKS: THEIR FORMATION AND DIVERSITY: Proceedings of the International Conference. AIP Conference Proceedings, V

Physics

Radiative Transfer, Scattering, Accretion And Accretion Disks, Thermodynamic Processes, Conduction, Convection, Equations Of State

Scientific paper

We present preliminary results on the ability of self-gravitating disks to cool in response to their internal heating. These disks are modelled using a smoothed particle hydrodynamics (SPH) code with radiative transfer [1], and we investigate the ability of these disks to maintain a state of thermal equilibrium with their boundaries as an indication of their likelihood to fragment.

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