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1
Introduction
2
Dust included simulation
3
circumplanetary disks
4
planetary disks
5
black hole discs
6
low ionization
7
opacity
8
opacity gradient
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lessons from planet formation
10
shocks matter
11
gravitational potential
12
viscosity
13
torques
14
gaps
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gap profile
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threedimensionality
17
vertical slice
18
envelope
19
observational predictions
20
imaging
21
pds70c
22
scds
23
line predictions
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summary
25
migration maps
Description:
Explore accretion processes within circumplanetary disks and their similarities to black hole mini-disks in this 29-minute conference talk by Judit Szulagyi from ETH Zurich. Delve into dust-included simulations, examining the roles of opacity, shocks, gravitational potential, and viscosity in shaping these systems. Investigate gap profiles, three-dimensionality, and observational predictions for both planetary and black hole disks. Gain insights from planet formation studies and their applications to broader astrophysical contexts, including migration patterns and imaging techniques. Part of the "Building Bridges" conference at the Kavli Institute for Theoretical Physics, this talk bridges stellar and black hole binary accretion research, offering a unified perspective on these diverse astrophysical phenomena.

Accretion Inside Circumplanetary Disks, the Equivalents of BH Mini-Disks - Judit Szulagyi

Kavli Institute for Theoretical Physics
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