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Dynamics of protoplanetary disks
Protoplanetary disks are quasi-steady structures whose evolution and dispersal determine
the environment for planet formation. I review the theory of protoplanetary disk evolution and …
the environment for planet formation. I review the theory of protoplanetary disk evolution and …
Wind-driven accretion in protoplanetary disks. I. Suppression of the magnetorotational instability and launching of the magnetocentrifugal wind
We perform local, vertically stratified shearing-box MHD simulations of protoplanetary disks
(PPDs) at a fiducial radius of 1 AU that take into account the effects of both Ohmic resistivity …
(PPDs) at a fiducial radius of 1 AU that take into account the effects of both Ohmic resistivity …
[HTML][HTML] Global simulations of protoplanetary disks with net magnetic flux-i. non-ideal mhd case
Context. The planet-forming region of protoplanetary disks is cold, dense, and therefore
weakly ionized. For this reason, magnetohydrodynamic (MHD) turbulence is thought to be …
weakly ionized. For this reason, magnetohydrodynamic (MHD) turbulence is thought to be …
Global simulations of the inner regions of protoplanetary disks with comprehensive disk microphysics
The gas dynamics of weakly ionized protoplanetary disks (PPDs) are largely governed by
the coupling between gas and magnetic fields, described by three non-ideal …
the coupling between gas and magnetic fields, described by three non-ideal …
Thanatology in protoplanetary discs-The combined influence of Ohmic, Hall, and ambipolar diffusion on dead zones
Protoplanetary discs are poorly ionised due to their low temperatures and high column
densities and are therefore subject to three “non-ideal” magnetohydrodynamic (MHD) …
densities and are therefore subject to three “non-ideal” magnetohydrodynamic (MHD) …
Transport and accretion in planet-forming disks
Planets appear to form in environments shaped by the gas flowing through protostellar disks
to the central young stars. The flows in turn are governed by orbital angular momentum …
to the central young stars. The flows in turn are governed by orbital angular momentum …
Resonant drag instabilities in protoplanetary discs: the streaming instability and new, faster growing instabilities
We identify and study a number of new, rapidly growing instabilities of dust grains in
protoplanetary discs, which may be important for planetesimal formation. The study is based …
protoplanetary discs, which may be important for planetesimal formation. The study is based …
Hall effect controlled gas dynamics in protoplanetary disks. II. Full 3D simulations toward the outer disk
We perform three-dimensional stratified shearing-box magnetohydrodynamic (MHD)
simulations on the gas dynamics of protoplanetary disks with a net vertical magnetic flux of B …
simulations on the gas dynamics of protoplanetary disks with a net vertical magnetic flux of B …
Effect of ambipolar diffusion on the nonlinear evolution of magnetorotational instability in weakly ionized disks
We study the role of ambipolar diffusion (AD) on the nonlinear evolution of the
magnetorotational instability (MRI) in protoplanetary disks using the strong coupling limit …
magnetorotational instability (MRI) in protoplanetary disks using the strong coupling limit …
Ring formation and dust dynamics in wind-driven protoplanetary discs: global simulations
Large-scale vertical magnetic fields are believed to play a key role in the evolution of
protoplanetary discs. Associated with non-ideal effects, such as ambipolar diffusion, they are …
protoplanetary discs. Associated with non-ideal effects, such as ambipolar diffusion, they are …