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  1. Turning the knobs on dust evolution: Comparing codes, parameters and their effects on planet formation and disc observables

    Publication
    Protoplanetary discs contain a wide range of dust sizes that influence their thermal structure and planet formation processes such as planetesimal formation and pebble accretion. Dust evolution models …

  2. Fragmentation-limited Dust Filtration in 2D Simulations of Planet-Disk Systems with Dust Coagulation: Parameter Study and Implications for the Inner Disk's Dust Mass Budget and Composition

    Publication
    Superthermal gas giant planets or their progenitor cores are known to open deep gaps in protoplanetary disks, which stop large, drifting dust particles on their way to the …

  3. TriPoDPy: 1D Tri-Population size distributions forDust evolution in protoplanetary disks

    Publication
    TriPoDPy is a code simulating the dust evolution, including dust growth and dynamics in protoplanetary disks using the parametric dust model presented in (Pfeil et al., 2024). The …

  4. TriPoD: Tri-Population size distributions for Dust evolution: Coagulation in vertically integrated hydrodynamic simulations of protoplanetary disks

    Publication
    Context. Dust coagulation and fragmentation impact the structure and evolution of protoplanetary disks and set the initial conditions for planet formation. Dust grains dominate the opacities, they determine …

  5. Vertical shear instability with dust evolution and consistent cooling times. On the importance of the initial dust distribution

    Publication
    … atmosphere, where they can cool the gas. Whether the instability can emerge for a specific stratification depends on the initial dust grain sizes and the initial dust …