Planet migration with gravitationally unstable gaps
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If you have a question about this talk, please contact Henrik Latter.
I present numerical simulations of disc-planet interactions where the
planet opens a gravitationally unstable gap in an otherwise gravitationally
stable disc. In our disc models, as the gap becomes more unstable the
planet migrates outwards more rapidly. Our results suggest that standard
type II migration, applicable to giant planets in non-self-gravitating
viscous discs, is likely to be significantly modified in massive discs when
gravitational instabilities associated with the gap occur. I will also
present recent 3D simulations on gap stability.
This talk is part of the DAMTP Astrophysics Seminars series.
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