Towards a global model for planet formation in layered MHD wind-driven discs: A population synthesis approach to investigate the impact of low viscosity and accretion layer thickness
Fuente:
arXiv
Guardado en:
| Autores principales: | Weder, Jesse, Mordasini, Christoph |
|---|---|
| Formato: | Preprint |
| Publicado: |
2026
|
| Materias: | |
| Acceso en línea: | |
| Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
Ejemplares similares
Inferring the physics of protoplanetary disc evolution from the irradiated Cygnus OB2 region -- A comparison of viscous and MHD wind-driven scenarios
por: Weder, Jesse, et al.
Publicado: (2025)
por: Weder, Jesse, et al.
Publicado: (2025)
The importance of the dynamical corotation torque for the migration of low-mass planets -- 1D analytical prescriptions verified by 2D hydrodynamical simulations
por: Weder, Jesse, et al.
Publicado: (2025)
por: Weder, Jesse, et al.
Publicado: (2025)
An MHD-based model for wind-driven disc-planet interactions
por: Hammer, Michael, et al.
Publicado: (2025)
por: Hammer, Michael, et al.
Publicado: (2025)
The formation of planetary systems: physics, populations, and architectures
por: Kessler, Andrin, et al.
Publicado: (2026)
por: Kessler, Andrin, et al.
Publicado: (2026)
Planetary population synthesis
por: Burn, Remo, et al.
Publicado: (2024)
por: Burn, Remo, et al.
Publicado: (2024)
Convective mixing in distant and close-in giant planets -- Dependences on the initial composition, luminosity, bloating and semi-convection
por: Polman, Jesse, et al.
Publicado: (2024)
por: Polman, Jesse, et al.
Publicado: (2024)
Primordial planet spin driven by boundary layer effects in a decretion disc
por: Martin, Rebecca G., et al.
Publicado: (2025)
por: Martin, Rebecca G., et al.
Publicado: (2025)
Planetary formation tracks on the Hertzsprung-Russell diagram: Visualising the processes of giant planet growth
por: Gottstein, Benedikt, et al.
Publicado: (2026)
por: Gottstein, Benedikt, et al.
Publicado: (2026)
Semi-analytical model for the dynamical evolution of planetary system II: Application to systems formed by a planet formation model
por: Kimura, Tadahiro, et al.
Publicado: (2025)
por: Kimura, Tadahiro, et al.
Publicado: (2025)
The PAIRS project: a global formation model for planets in binaries. I. Effect of disc truncation on the growth of S-type planets
por: Venturini, Julia, et al.
Publicado: (2026)
por: Venturini, Julia, et al.
Publicado: (2026)
Similar-mass versus diverse-mass planetary systems in wind-driven accretion discs
por: Zhao, Yunpeng, et al.
Publicado: (2025)
por: Zhao, Yunpeng, et al.
Publicado: (2025)
Dust growth and planet formation by disc fragmentation
por: Lee, Hans, et al.
Publicado: (2025)
por: Lee, Hans, et al.
Publicado: (2025)
Constraints on PDS 70 b and c from the dust continuum emission of the circumplanetary discs considering in situ dust evolution
por: Shibaike, Yuhito, et al.
Publicado: (2024)
por: Shibaike, Yuhito, et al.
Publicado: (2024)
Coupled geophysical and thermal constraints link between Mars basal molten layer and the planet viscosity profile
por: Guinard, Alex, et al.
Publicado: (2024)
por: Guinard, Alex, et al.
Publicado: (2024)
The Solar System could have formed in a low-viscosity disc: A dynamical study from giant planet migration to the Nice model
por: Griveaud, Philippine, et al.
Publicado: (2024)
por: Griveaud, Philippine, et al.
Publicado: (2024)
Constraints on the formation history and composition of Kepler planets from their distribution of orbital period ratios
por: Chen, Di-Chang, et al.
Publicado: (2024)
por: Chen, Di-Chang, et al.
Publicado: (2024)
Sequential giant planet formation initiated by disc substructure
por: Lau, Tommy Chi Ho, et al.
Publicado: (2024)
por: Lau, Tommy Chi Ho, et al.
Publicado: (2024)
Pebble-driven migration of low-mass planets in the 2D regime of pebble accretion
por: Chrenko, O., et al.
Publicado: (2024)
por: Chrenko, O., et al.
Publicado: (2024)
Infall-driven gravitational instability in accretion discs
por: Longarini, Cristiano, et al.
Publicado: (2025)
por: Longarini, Cristiano, et al.
Publicado: (2025)
3D MHD simulations of planet migration in cavities and inner discs of magnetized stars
por: Romanova, M. M., et al.
Publicado: (2025)
por: Romanova, M. M., et al.
Publicado: (2025)
Protoplanetary disc population synthesis I. Constraining disc parameters to reproduce disc observations
por: Gomez, Jose L., et al.
Publicado: (2025)
por: Gomez, Jose L., et al.
Publicado: (2025)
The formation of transiting circumplanetary debris discs from the disruption of satellite systems during planet-planet scattering
por: Mustill, Alexander J., et al.
Publicado: (2024)
por: Mustill, Alexander J., et al.
Publicado: (2024)
Can the giant planets of the Solar System form via pebble accretion in a smooth protoplanetary disc?
por: Lau, Tommy Chi Ho, et al.
Publicado: (2024)
por: Lau, Tommy Chi Ho, et al.
Publicado: (2024)
Giant planet formation via pebble accretion across different stellar masses
por: Shibata, Sho, et al.
Publicado: (2025)
por: Shibata, Sho, et al.
Publicado: (2025)
The formation of circumbinary planets through disc fragmentation
por: Teasdale, Matthew, et al.
Publicado: (2026)
por: Teasdale, Matthew, et al.
Publicado: (2026)
Timescales diagnostics for saving viscous and MHD-driven dusty discs from external photoevaporation
por: Pichierri, Gabriele, et al.
Publicado: (2026)
por: Pichierri, Gabriele, et al.
Publicado: (2026)
The interplay between forming planets and photoevaporating discs II: Wind-driven gas redistribution
por: Weber, Michael L., et al.
Publicado: (2024)
por: Weber, Michael L., et al.
Publicado: (2024)
New migration patterns in high planet-star mass ratio systems in disks with low viscosity
por: Sánchez, Mariana, et al.
Publicado: (2025)
por: Sánchez, Mariana, et al.
Publicado: (2025)
Turning the knobs on dust evolution: Comparing codes, parameters and their effects on planet formation and disc observables
por: Eriksson, Linn E. J., et al.
Publicado: (2026)
por: Eriksson, Linn E. J., et al.
Publicado: (2026)
A formation pathway for giant planets in S-type discs of γ-Cephei-like compact binaries
por: Ronco, María Paula, et al.
Publicado: (2026)
por: Ronco, María Paula, et al.
Publicado: (2026)
Vapor equilibrium models of accreting rocky planets demonstrate direct core growth by pebble accretion
por: Steinmeyer, Marie-Luise, et al.
Publicado: (2024)
por: Steinmeyer, Marie-Luise, et al.
Publicado: (2024)
The impact of disc photoevaporation on the long-term evolution of giant planets in mean motion resonances
por: Greenfield, Emmanuel J., et al.
Publicado: (2026)
por: Greenfield, Emmanuel J., et al.
Publicado: (2026)
On the meaning of the dynamo radius in giant planets with stable layers
por: Wulff, Paula N., et al.
Publicado: (2025)
por: Wulff, Paula N., et al.
Publicado: (2025)
Eccentricity evolution during planet-disc interaction
por: Ragusa, Enrico, et al.
Publicado: (2017)
por: Ragusa, Enrico, et al.
Publicado: (2017)
How two-dimensional are planet--disc interactions? I. Locally isothermal discs
por: Cordwell, Amelia J., et al.
Publicado: (2025)
por: Cordwell, Amelia J., et al.
Publicado: (2025)
Stellar wind impact on early atmospheres around unmagnetized Earth-like planets
por: Canet, Ada, et al.
Publicado: (2024)
por: Canet, Ada, et al.
Publicado: (2024)
Non-linear spiral waves in accretion discs
por: Brown, Joshua J., et al.
Publicado: (2025)
por: Brown, Joshua J., et al.
Publicado: (2025)
Early stages of gap opening by planets in protoplanetary discs
por: Cordwell, Amelia J., et al.
Publicado: (2024)
por: Cordwell, Amelia J., et al.
Publicado: (2024)
Planet formation -- observational constraints, physical processes, and compositional patterns
por: Mordasini, Christoph, et al.
Publicado: (2024)
por: Mordasini, Christoph, et al.
Publicado: (2024)
Circumbinary accretion as a diagnostic for binary--disc misalignment
por: Smallwood, Jeremy L., et al.
Publicado: (2024)
por: Smallwood, Jeremy L., et al.
Publicado: (2024)
Ejemplares similares
-
Inferring the physics of protoplanetary disc evolution from the irradiated Cygnus OB2 region -- A comparison of viscous and MHD wind-driven scenarios
por: Weder, Jesse, et al.
Publicado: (2025) -
The importance of the dynamical corotation torque for the migration of low-mass planets -- 1D analytical prescriptions verified by 2D hydrodynamical simulations
por: Weder, Jesse, et al.
Publicado: (2025) -
An MHD-based model for wind-driven disc-planet interactions
por: Hammer, Michael, et al.
Publicado: (2025) -
The formation of planetary systems: physics, populations, and architectures
por: Kessler, Andrin, et al.
Publicado: (2026) -
Planetary population synthesis
por: Burn, Remo, et al.
Publicado: (2024)