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Bibliographische Detailangaben
Hauptverfasser:	Ziampras, Alexandros, Cordwell, Amelia J., Rafikov, Roman R., Nelson, Richard P.
Format:	Preprint
Veröffentlicht:	2025
Schlagworte:	Earth and Planetary Astrophysics
Online-Zugang:	https://arxiv.org/abs/2509.20464
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!

Ähnliche Einträge

How two-dimensional are planet--disc interactions? I. Locally isothermal discs
von: Cordwell, Amelia J., et al.
Veröffentlicht: (2025)

Early stages of gap opening by planets in protoplanetary discs
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$αβq_\mathrm{th}$-mapping of planet-induced density wave damping in protoplanetary discs
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Eccentric planet-disc interactions: orbital migration and eccentricity evolution
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Indirect forces in disc-planet interaction
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Buoyancy torques prevent low-mass planets from stalling in low-turbulence radiative disks
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Migration of low-mass planets in inviscid disks: the effect of radiation transport on the dynamical corotation torque
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Substructure in externally irradiated protoplanetary disks, I. spirals and rings in two-dimensional radiation hydrodynamics
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Sculpting protoplanetary discs -- modelling circumbinary cavities at observable scales with radiation hydrodynamics
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Conservation laws in non-inertial frames and non-conservation of energy of relative motion in two-body problem
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Halting the migration of super-Earths by efficient gap opening in radiative, low viscosity disks
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Spirals, rings, and vortices shaped by shadows in protoplanetary disks: from radiative hydrodynamical simulations to observable signatures
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Dusty substructures induced by planets in ALMA disks: how dust growth and dynamics changes the picture
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Overstability of the 2:1 mean motion resonance: Exploring disc parameters with hydrodynamic simulations
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Starlight-driven flared-staircase geometry in radiation hydrodynamic models of protoplanetary disks
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Thermal structure of circumbinary discs: Circumbinary planets should be icy not rocky
von: Pierens, Arnaud, et al.
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Eccentricity evolution during planet-disc interaction
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Introducing two improved methods for approximating radiative cooling in hydrodynamical simulations of accretion discs
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The role of detailed gas and dust opacities in shaping the evolution of the inner disc edge subject to episodic accretion
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Dust growth and planet formation by disc fragmentation
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An MHD-based model for wind-driven disc-planet interactions
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Pushing the limits of eccentricity in planet-disc interactions
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Veröffentlicht: (2025)

Damping of planet-driven density waves in discs: The relative importance of cooling, viscosity and non-linearity (DATASET)
von: Cordwell, Amelia, et al.
Veröffentlicht: (2026)

Eccentric discs as a gateway to giant planets outward migration
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Veröffentlicht: (2025)

How disc initial conditions sculpt the atmospheric composition of giant planets
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Veröffentlicht: (2026)

The stochastic nature of migration of disc instability protoplanets in three-dimensional hydrodynamical and MHD simulations of fragmenting discs
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Veröffentlicht: (2025)

The importance of the dynamical corotation torque for the migration of low-mass planets -- 1D analytical prescriptions verified by 2D hydrodynamical simulations
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Viscous circumbinary protoplanetary discs -- II. Disc effects on the binary orbit
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Planet formation at the inner edge of the dead zone -- I. the interplay between accretion outbursts and dust growth
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The interplay between forming planets and photoevaporating discs II: Wind-driven gas redistribution
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Veröffentlicht: (2024)

The Circumbinary Disc of HD 34700A II. Analysis of a strong dust asymmetry
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Sequential giant planet formation initiated by disc substructure
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Veröffentlicht: (2024)

Effect of irradiation model on 2D hydrodynamic simulations of self-gravitating protoplanetary discs
von: Leedham, Caitriona S., et al.
Veröffentlicht: (2025)

How external photo-evaporation changes the chemical composition of the inner disc
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Veröffentlicht: (2024)

The formation of transiting circumplanetary debris discs from the disruption of satellite systems during planet-planet scattering
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Veröffentlicht: (2024)

Mass-radius relationships and contraction of condensed planets by cooling or despinning
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Viscous circumbinary protoplanetary discs -- I. Structure of the inner cavity
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The formation of circumbinary planets through disc fragmentation
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Veröffentlicht: (2026)

3D MHD simulations of planet migration in cavities and inner discs of magnetized stars
von: Romanova, M. M., et al.
Veröffentlicht: (2025)

Direct imaging characterization of cool gaseous planets
von: Min, Michiel, et al.
Veröffentlicht: (2025)

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