Halting Type I planet migration in non-isothermal disks

Abstract

Aims: We investigate the effect of including a proper energy balance on the interaction of a low-mass planet with a protoplanetary disk. Methods: We use a three-dimensional version of the RODEO method to perform hydrodynamical simulations including the energy equation. Radiation is included in the flux-limited diffusion approach. Results: The sign of the torque depends sensitively on the ability of the disk to radiate away the energy generated in the immediate surroundings of the planet. In the case of high opacity, corresponding to the dense inner regions of protoplanetary disks, migration is directed \emph{outward}, instead of the usual inward migration that was found in locally isothermal disks. For low values of the opacity we recover inward migration, and we show that torques originating in the coorbital region are responsible for the change in migration direction.

4 pages, 5 figures, accepted for A&A letters

References in corpus (17)

• Using FU Orionis Outbursts to Constrain Self-Regulated Protostellar Disk Models
• Dust coagulation in protoplanetary disks: a rapid depletion of small grains
• Runaway migration and the formation of hot Jupiters
• Three-dimensional Calculations of High and Low-mass Planets Embedded in Protoplanetary Discs
• Orbital Migration and Mass Accretion of Protoplanets in 3D Global Computations with Nested Grids
• The interaction of planets with a disc with MHD turbulence IV: Migration rates of embedded protoplanets
• Nested-grid calculations of disk-planet interaction
• Planet migration and gap formation by tidally-induced shocks
• The co-orbital corotation torque in a viscous disk: numerical simulations
• Low-Mass Proto-Planet Migration in T-Tauri Alpha-Disks
• 3D-radiation hydro simulations of disk-planet interactions: I. Numerical algorithm and test cases
• Saturation of the corotation resonance in a gaseous disk
• Stopping inward planetary migration by a toroidal magnetic field
• On the coorbital corotation torque in a viscous disk and its impact on planetary migration
• Type I Migration in a Non-Isothermal Protoplanetary Disk
• Halting Planet Migration in the Evacuated Centers of Protoplanetary Disks
• RODEO: a new method for planet-disk interaction

Cited by in corpus (203)

• A low mass for Mars from Jupiter's early gas-driven migration
• Planet-disk interaction and orbital evolution
• Origins of Hot Jupiters
• Extrasolar planet population synthesis I: Method, formation tracks and mass-distance distribution
• A torque formula for non-isothermal Type I planetary migration - II. Effects of diffusion
• Assisted Inspirals of Stellar Mass Black Holes Embedded in AGN Disks: Solving the "Final AU Problem"
• A torque formula for non-isothermal Type I planetary migration - I. Unsaturated horseshoe drag
• Breaking the Chains: Hot Super-Earth systems from migration and disruption of compact resonant chains
• Migration and the formation of systems of hot super-Earths and Neptunes
• Pebble isolation mass --- scaling law and implications for the formation of super-Earths and gas giants
• New Horizons for Fundamental Physics with LISA
• Formation of the Terrestrial Planets from a Narrow Annulus
• Migration then assembly: Formation of Neptune mass planets inside 1 AU
• The structure of protoplanetary discs around evolving young stars
• Unveiling the Structure of Pre-Transitional Disks
• Characterization of exoplanets from their formation II: The planetary mass-radius relationship
• The great dichotomy of the Solar System: small terrestrial embryos and massive giant planet cores
• The Quest for Dual and Binary Supermassive Black Holes: A Multi-Messenger View
• Testing In Situ Assembly with the Kepler Planet Candidate Sample
• On the corotation torque in a radiatively inefficient disk
• Three-dimensional simulations of multiple protoplanets embedded in a protostellar disc
• Migration Traps in Disks Around Supermassive Black Holes
• Inside-Out Planet Formation
• Dynamics of pebbles in the vicinity of a growing planetary embryo: hydro-dynamical simulations
• Fossilized condensation lines in the Solar System protoplanetary disk
• The isotropic diffusion source approximation for supernova neutrino transport
• Orbital Migration of Interacting Stellar Mass Black Holes in Disks around Supermassive Black Holes
• Planet migration in three-dimensional radiative discs
• Formation of planetary systems by pebble accretion and migration: Growth of gas giants
• The Migration of Gap-Opening Planets is not Locked to Viscous Disk Evolution
• Migration of Protoplanets in Radiative Disks
• Observable Consequences of Planet Formation Models in Systems with Close-in Terrestrial Planets
• Orbital migration of low-mass planets in evolutionary radiative models: Avoiding catastrophic infall
• Challenges in Planet Formation
• Imprint of Accretion Disk-Induced Migration on Gravitational Waves from Extreme Mass Ratio Inspirals
• Stellar irradiated discs and implications on migration of embedded planets I: equilibrium discs
• On corotation torques, horseshoe drag and the possibility of sustained stalled or outward protoplanetary migration
• Type I planetary migration in a self-gravitating disk
• Orbital evolution of eccentric planets in radiative discs
• On disc protoplanet interactions in a non-barotropic disc with thermal diffusion
• On the evolution of eccentric and inclined protoplanets embedded in protoplanetary disks
• Hot super-Earths and giant planet cores from different migration histories
• On the orbital evolution of supermassive black hole binaries with circumbinary accretion discs
• Gas accretion onto planetary cores: three-dimensional self-gravitating radiation hydrodynamical calculations
• Dynamical corotation torques on low-mass planets
• Type I Planet Migration in Nearly Laminar Disks
• Migration of Earth-size planets in 3D radiative discs
• Dusty gas with one fluid
• Impacts of planet migration models on planetary populations. Effects of saturation, cooling and stellar irradiation
• A reassessment of the in situ formation of close-in super-Earths
• Stellar irradiated discs and implications on migration of embedded planets II: accreting-discs
• On the corotation torque for low-mass eccentric planets
• The Origin of Planetary System Architectures. I. Multiple Planet Traps in Gaseous Discs
• Evolution of gas disc-embedded intermediate mass ratio inspirals in the LISA band
• Density Waves Excited by Low-Mass Planets in Protoplanetary Disks II: High-Resolution Simulations of the Nonlinear Regime
• Saturated torque formula for planetary migration in viscous disks with thermal diffusion: recipe for protoplanet population synthesis
• Protoplanetary migration in turbulent isothermal disks
• On the formation of hot Neptunes and super-Earths
• Three-Dimensional Radiation-Hydrodynamics Calculations of the Envelopes of Young Planets Embedded in Protoplanetary Disks
• Growing and moving low-mass planets in non-isothermal disks
• Turbulent Torques on Protoplanets in a Dead Zone
• Type I planet migration in nearly laminar disks - long term behavior
• Planet gaps in the dust layer of 3D protoplanetary disks: I. Hydrodynamical simulations of T Tauri disks
• Orbital Migration of Interacting Stellar Mass Black Holes in Disks around Supermassive Black Holes II. Spins and Incoming Objects
• Gas pile-up, gap overflow, and Type 1.5 migration in circumbinary disks: application to supermassive black hole binaries
• Global magnetohydrodynamical models of turbulence in protoplanetary disks I. A cylindrical potential on a Cartesian grid and transport of solids
• Probing gas disc physics with LISA: simulations of an intermediate mass ratio inspiral in an accretion disc
• Migration of Gas Giant Planets in Gravitationally Unstable Disks
• Accretion of Uranus and Neptune from inward-migrating planetary embryos blocked by Jupiter and Saturn
• Range of outward migration and influence of the disc's mass on the migration of giant planet cores
• On the horseshoe drag of a low-mass planet. II Migration in adiabatic disks
• Orbital migration of interacting low-mass planets in evolutionary radiative turbulent models
• Formation of planetary cores at Type I migration traps
• The fate of planetesimals in turbulent disks with dead zones. II. Limits on the viability of runaway accretion
• Numerical simulations of type III planetary migration: III. Outward migration of massive planets
• Tidal interactions in multi-planet systems
• On the Interaction between a Protoplanetary Disk and a Planet in an Eccentric Orbit: Application of Dynamical Friction
• Migration of planets embedded in a circumstellar disk
• On the width and shape of the corotation region for low-mass planets
• The dynamical role of the circumplanetary disc in planetary migration
• Building Giant-Planet Cores at a Planet Trap
• Minimum Mass Solar Nebulae and Planetary Migration
• The Kepler Dichotomy in Planetary Disks: Linking Kepler Observables to Simulations of Late-Stage Planet Formation
• Terrestrial Planet Formation in the Presence of Migrating Super-earths
• Efficiency of thermal relaxation by radiative processes in protoplanetary discs: constraints on hydrodynamic turbulence
• Global Calculations of Density Waves and Gap Formation in Protoplanetary Disks using a Moving Mesh
• Interactions Between Moderate- and Long-Period Giant Planets: Scattering Experiments for Systems in Isolation and with Stellar Flybys
• New Worlds on the Horizon: Earth-Sized Planets Close to Other Stars
• Evolution of inclined planets in three-dimensional radiative discs
• Gas Accretion onto a Protoplanet and Formation of a Gas Giant Planet
• Type I planet migration in weakly magnetised laminar discs
• Migration rates of planets due to scattering of planetesimals
• On the dynamics of multiple systems of hot super-Earths and Neptunes: Tidal circularization, resonance and the HD 40307 system
• Bulk composition of the transiting hot Neptune around GJ 436
• Torques Induced by Scattered Pebble-flow in Protoplanetary Disks
• Supernova explosions in active galactic nuclear discs
• The effect of type I migration on the formation of terrestrial planets in hot-Jupiter systems
• The formation of systems with closely spaced low-mass planets and the application to Kepler-36
• Time evolution of snow regions and planet traps in an evolving protoplanetary disk
• Early Dynamical Instabilities in the Giant Planet Systems
• Outward migration of a super-Earth in a disc with outward propagating density waves excited by a giant planet
• DUSTYBOX and DUSTYWAVE: Two test problems for numerical simulations of two fluid astrophysical dust-gas mixtures
• Gas pile-up, gap overflow, and Type 1.5 migration in circumbinary disks: general theory
• Stellar irradiated discs and implications on migration of embedded planets III: viscosity transitions
• Pebbles versus planetesimals: the outcomes of population synthesis models
• Influence of the water content in protoplanetary discs on planet migration and formation
• Numerical simulations of the type III migration:I. Disc model and convergence tests
• Is the ring inside or outside the planet?: The effect of planet migration on dust rings
• Planet migration: self-gravitating radiation hydrodynamical models of protoplanets with surfaces
• Planetesimal and Protoplanet Dynamics in a Turbulent Protoplanetary Disk: Ideal Unstratified Disks
• Influence of viscosity and the adiabatic index on planetary migration
• Convergence zones for Type I migration: an inward shift for multiple planet systems
• The Effect of Thermal Torques on AGN Disc Migration Traps and Gravitational Wave Populations
• Quiescent and active galactic nuclei as factories of merging compact objects in the era of gravitational-wave astronomy
• Thermal torque effects on the migration of growing low-mass planets
• General Analysis of Type I Planetary Migration with Stochastic Perturbations
• Runaway gas accretion and gap opening versus type~I migration
• Numerical simulations of type III planetary migration: II. Inward migration of massive planets
• Recent developments in planet migration theory
• Planet-Disk interaction in 3D: the importance of buoyancy waves
• Photoevaporation as a Truncation Mechanism for Circumplanetary Disks
• Trapping of giant-planet cores - I. Vortex aided trapping at the outer dead zone edge
• On the horseshoe drag of a low-mass planet. I - Migration in isothermal disks
• Planet formation via pebble accretion in externally photoevaporating discs
• pAGN: the one-stop solution for AGN disc modeling
• Outwards migration for planets in stellar irradiated 3D discs
• Migration and Growth of Protoplanetary Embryos I: Convergence of Embryos in Protoplanetary Disks
• Migration of Extrasolar Planets: Effects from X-Wind Accretion Disks
• Planet Shadows in Protoplanetary Disks. I: Temperature Perturbations
• Setting the Stage: Planet formation and Volatile Delivery
• Dead Zones as Thermal Barriers to Rapid Planetary Migration in Protoplanetary Disks
• The effect of a strong pressure bump in the Sun's natal disk: Terrestrial planet formation via planetesimal accretion rather than pebble accretion
• Terrestrial planet formation: Dynamical shake-up and the low mass of Mars
• Inner Super-Earths, Outer Gas Giants: How Pebble Isolation and Migration Feedback Keep Jupiters Cold
• Two-Dimensional Study of the Propagation of Planetary Wake and the Indication to Gap Opening in an Inviscid Protoplanetary Disk
• Three body resonances in close orbiting planetary systems: Tidal dissipation and orbital evolution
• 3D Simulations of Planet Trapping at Disc-Cavity Boundaries
• Dust Settling and Rapid Planetary Migration
• Considerations on the accretion of Uranus and Neptune by mutual collisions of planetary embryos in the vicinity of Jupiter and Saturn
• Stirring up the dust: A dynamical model for halo-like dust clouds in transitional disks
• The effects of a magnetic field on planetary migration in laminar and turbulent discs
• On the formation of the Kepler-10 planetary system
• The role of the initial surface density profiles of the disc on giant planet formation: comparing with observations
• Dynamics and Eccentricity Formation of Planets in OGLE-06-109L System
• Trapping planets in an evolving protoplanetary disk: preferred time, locations and planet mass
• Forming Habitable Planets around Dwarf Stars: Application to OGLE-06-109L
• From Dust to Planets I: Planetesimal and Embryo Formation
• Type I Migration in Radiatively Efficient Discs
• Dusty disc-planet interaction with dust-free simulations
• Inner rocky super-Earth formation: distinguishing the formation pathways in viscously heated and passive discs
• Influence of migration models and thermal torque on planetary growth in the pebble accretion scenario
• Formation of Terrestrial Planets
• Impact of thermal effects on the evolution of eccentricity and inclination of low-mass planets
• How the presence of a gas giant affects the formation of mean-motion resonances between two low-mass planets in a locally isothermal gaseous disc
• Brightest Group Galaxies: Stellar Mass and Star Formation Rate (paper I)
• The Vertical Structure of Planet-induced Gaps in Proto-Planetary Discs
• Proximity of exoplanets to first-order mean-motion resonances
• Oscillatory migration of accreting protoplanets driven by a 3D distortion of the gas flow
• Torques felt by solid accreting planets
• Chondrule Formation via Impact Jetting Triggered by Planetary Accretion
• Radiatively heated, protoplanetary discs with dead zones. I. Dust settling and thermal structure of discs around M stars
• Global N-body simulations of circumbinary planet formation around Kepler-16 and -34 analogues I: Exploring the pebble accretion scenario
• Migrating Low-Mass Planets in Inviscid Dusty Protoplanetary Discs
• Planetary Migration in Protoplanetary Disks
• A recipe for orbital eccentricity damping in the type-I regime for low viscosity 2D-discs
• Dead Zones In Circumplanetary Discs as Formation Sites For Regular Satellites
• A Super-Earth caught in a trap
• Consequences of tidal interaction between disks and orbiting protoplanets for the evolution of multi-planet systems with architecture resembling that of Kepler 444
• Disruption of co-orbital (1:1) planetary resonances during gas-driven orbital migration
• Migrating Planets into Ultra-Short-Period Orbits during Episodic Accretion Events
• Planetary core formation via multi-species pebble accretion
• Super-Earths as Failed Cores in Orbital Migration Traps
• Migration of protoplanets with surfaces through discs with steep temperature gradients
• The growth of super-Earths: the importance of a self-consistent treatment of disc structures and pebble accretion
• 3D Adiabatic Simulations of Binary Black Hole Formation in AGN
• Local Linear Analysis of Interaction between a Planet and Viscous Disk and an Implication on Type I Planetary Migration
• Migration of gap-opening planets in 3D stellar-irradiated accretion disks
• What Determines the Maximum Mass of AGN-assisted Black Hole Mergers?
• Modeling Planetary System Formation with N-Body Simulations: Role of Gas Disk and Statistics Comparing to Observations
• How the planetary eccentricity influences the pebble isolation mass
• Accreting luminous low-mass planets escape from migration traps at pressure bumps
• The role of density perturbation on planet formation by pebble accretion
• Meridional Circulation driven by Planetary Spiral Wakes in Radiative and Magnetized Protoplanetary Discs
• Migration of Accreting Planets and Black Holes in Disks
• Calibrated Gas Accretion and Orbital Migration of Protoplanets in 1D Disc Models
• Disc-planet interactions in sub-keplerian discs
• Hidden under a warm blanket: If planets existed in protostellar disks, they would hardly produce observable substructures
• Gravitational Collapse and Disk Formation in Magnetized Cores
• Observable Signatures of EMRI Black Hole Binaries Embedded in Thin Accretion Disks
• Type I migration in optically thick accretion discs
• On the formation of planetary systems in photoevaporating transition discs
• The late formation of chondrites as a consequence of Jupiter-induced gaps and rings
• DIPSY: A new Disc Instability Population SYnthesis, I. Modeling, evolution of individual systems, and tests
• Resurgence of CO in a warm bubble around accreting protoplanets and its observability
• Protoplanets with core masses below the critical mass fill in their Roche lobe
• Occurrence of the 2:1 commensurability in a gas giant-Super-Earth system
• Planet migration in wind-fed accretion disks in binaries
• Origin of compact exoplanetary systems during disk infall
• Callisto's Nonresonant Orbit as an Outcome of Circum-Jovian Disk Substructure
• Single Fluid vs. Multifluid: Comparison between single fluid and multifluid dust models for disc planet interactions
• Planetary migration in wind-fed non-stationary accretion disks in binary systems
• Dirty waveforms: multiband harmonic content of gas-embedded gravitational wave sources
• Modelling the evolution of planets in disks