How two-dimensional are planet-disc interactions? II. Radiation hydrodynamics and suitable cooling prescriptions
arXiv:2509.20464 · doi:10.1051/0004-6361/202557399
Abstract
The ring and gap structures found in observed protoplanetary disks are often attributed to embedded gap-opening planets and typically modeled with simplified thermodynamics in the 2D, thin disk approximation. However, it has been shown that radiative cooling and meridional processes play key roles in planet-disk interaction, though their computational cost has limited their exploration. We investigate the differences between 2D and 3D models of gap-opening planets while also comparing thermodynamical frameworks ranging from locally isothermal to fully radiative. We also compare simplified cooling recipes to fully radiative models in an effort to motivate the inclusion of radiative effects in future modeling even in a parametrized manner. We perform hydrodynamical simulations in both 2D and 3D, and then compare the angular momentum deposition by planetary spirals to assess gap opening efficiency. We repeat comparisons with different thermodynamical treatments: locally isothermal, adiabatic, local beta cooling, and fully radiative including radiative diffusion. We find that 2D models are able to capture the essential physics of gap opening with remarkable accuracy, even when including full radiation transport in both cases. Simple cooling prescriptions can capture the trends found in fully radiative models, albeit slightly overestimating gap opening efficiency near the planet. Inherently 3D effects such as vertical flows that cannot be captured in 2D can explain the differences between the two approaches, but do not impact gap opening significantly. Our findings encourage the use of models that include radiative processes in the study of planet-disk interaction, even with simplified yet physically motivated cooling prescriptions in lieu of full radiation transport. This is particularly important in the context of substructure-inducing planets in the ALMA-sensitive disk regions (>10 au).
12 pages, 9 figures. Accepted in A&A
References in corpus (75)
- PLUTO: a Numerical Code for Computational Astrophysics
- The Disk Substructures at High Angular Resolution Project (DSHARP): I. Motivation, Sample, Calibration, and Overview
- A simple model for the evolution of the dust population in protoplanetary disks
- Discovery of a planetary-mass companion within the gap of the transition disk around PDS 70
- Rossby Wave Instability of Keplerian Accretion Disks
- FARGO: a fast eulerian transport algorithm for differentially rotating disks
- Rosseland and Planck Mean Opacities for Protoplanetary Discs
- Two accreting protoplanets around the young star PDS 70
- Protoplanetary Disk Turbulence Driven by the Streaming Instability: Non-Linear Saturation and Particle Concentration
- Linear and nonlinear evolution of the vertical shear instability in accretion discs
- The Disk Substructures at High Angular Resolution Project (DSHARP): VII. The Planet-Disk Interactions Interpretation
- Consistent dust and gas models for protoplanetary disks. I. Disk shape, dust settling, opacities, and PAHs
- The Disk Substructures at High Angular Resolution Project (DSHARP): V. Interpreting ALMA maps of protoplanetary disks in terms of a dust model
- Planetary Torques as the Viscosity of Protoplanetary Disks
- Protoplanetary Disk Turbulence Driven by the Streaming Instability: Linear Evolution and Numerical Methods
- FARGO3D: A new GPU-oriented MHD code
- Mocassin: A fully three-dimensional Monte Carlo photoionization code
- Mass Estimates of a Giant Planet in a Protoplanetary Disk from the Gap Structures
- Planet migration and gap formation by tidally-induced shocks
- Nonlinear propagation of planet-generated tidal waves
- On the wake generated by a planet in a disc
- Cooling Requirements for the Vertical Shear Instability in Protoplanetary Disks
- Convective Overstability in radially stratified accretion disks under thermal relaxation
- Low-Mass Proto-Planet Migration in T-Tauri Alpha-Disks
- Meridional circulation of gas into gaps opened by giant planets in three-dimensional low-viscosity disks
- 3D-radiation hydro simulations of disk-planet interactions: I. Numerical algorithm and test cases
- Molecules with ALMA at Planet-forming Scales (MAPS) IV: Emission Surfaces and Vertical Distribution of Molecules
- Treating gravity in thin disk simulations
- An Overview of the 2014 ALMA Long Baseline Campaign
- Dust growth and evolution in protoplanetary disks
- Zombie Vortex Instability I: A Purely Hydrodynamic Instability to Resurrect the Dead Zones of Protoplanetary Disks
- Migration of Earth-size planets in 3D radiative discs
- 3D Radiation Non-ideal Magnetohydrodynamical Simulations Of The Inner Rim In Protoplanetary Disks
- Convective overstability in accretion disks: 3D linear analysis and nonlinear saturation
- Gap Opening in 3D: Single Planet Gaps
- Vortex migration in protoplanetary disks
- Including Dust Coagulation in Hydrodynamic Models of Protoplanetary Disks: Dust Evolution in the Vicinity of a Jupiter-mass Planet
- The initial conditions for planet formation: Turbulence driven by hydrodynamical instabilities in disks around young stars
- A conservative orbital advection scheme for simulations of magnetized shear flows with the PLUTO code
- DustPy: A Python Package for Dust Evolution in Protoplanetary Disks
- Mapping the Conditions for Hydrodynamic Instability on Steady State Accretion Models of Protoplanetary Disks
- Planet-disk interaction in disks with cooling: basic theory
- Predicting the observational signature of migrating Neptune-sized planets in low-viscosity disks
- The effects of disk self-gravity and radiative cooling on the formation of gaps and spirals by young planets
- Observational Signatures of Tightly Wound Spirals Driven by Buoyancy Resonances in Protoplanetary Disks
- The Sandwich Mode for Vertical Shear Instability in Protoplanetary Disks
- Gaps and Rings in Protoplanetary Disks with Realistic Thermodynamics: The Critical Role of In-Plane Radiation Transport
- On shocks driven by high-mass planets in radiatively inefficient disks. II. Three-dimensional global disk simulations
- Planet-Disk interaction in 3D: the importance of buoyancy waves
- Razor-thin dust layers in protoplanetary disks: Limits on the vertical shear instability
- The impact of planet wakes on the location and shape of the water iceline in a protoplanetary disk
- Puffed up Edges of Planet-opened Gaps in Protoplanetary Disks. I. hydrodynamic simulations
- Migration of Jupiter mass planets in low viscosity discs
- An empirically-derived formula for the shape of planet-induced gaps in protoplanetary disks
- exoALMA V: Gaseous Emission Surfaces and Temperature Structures
- IDEFIX: a versatile performance-portable Godunov code for astrophysical flows
- Zombie Vortex Instability. II. Thresholds to Trigger Instability and the Properties of Zombie Turbulence in the Dead Zones of Protoplanetary Disks
- exoALMA XII: Weighing and sizing exoALMA disks with rotation curve modelling
- Low-mass planet migration in three dimensional wind-driven inviscid discs: a negative corotation torque
- The ALMA Survey of Gas Evolution of PROtoplanetary Disks (AGE-PRO): I. Program Overview and Summary of First Results
- Importance of radiative effects in gap opening by planets in protoplanetary disks
- WIde Separation Planets In Time (WISPIT): A Gap-clearing Planet in a Multi-ringed Disk around the Young Solar-type Star WISPIT 2
- Planet migration, resonant locking and accretion streams in PDS70: Comparing models and data
- Self-Destructing Spiral Waves: Global Simulations of a Spiral Wave Instability in Accretion Disks
- The Spiral Wave Instability Induced by a Giant Planet: I. Particle Stirring in the Inner Regions of Protoplanetary Disks
- Modeling planet-induced gaps and rings in ALMA disks: the role of in-plane radiative diffusion
- Planet-disc interaction in laminar and turbulent discs
- Gap-opening Planets Make Dust Rings Wider
- Three-Dimensional Dust Stirring by a Giant Planet Embedded in a Protoplanetary Disk
- Effects of Radiative Diffusion on the Dynamical Corotation Torque in Three-Dimensional Protoplanetary Disks
- Hydrodynamic turbulence in disks with embedded planets
- Can gap-edge illumination excite spirals in protoplanetary disks? Three-temperature radiation hydrodynamics and NIR image modelling
- How to form compact & other longer-lived planet-induced vortices: VSI, planet migration, or re-triggers, but not feedback
- Gravito-turbulence in local disk simulations with an adaptive moving mesh
- How two-dimensional are planet--disc interactions? I. Locally isothermal discs