Non-ideal MHD simulation of HL Tau disk: formation of rings

Abstract

Recent high resolution observations unveil ring structures in circumstellar disks. The origin of these rings has been widely investigated under various theoretical scenarios. In this work we perform global 3D non-ideal MHD simulations including effects from both Ohmic resistivity and ambipolar diffusion (AD) to model the HL Tau disk. The non-ideal MHD diffusion profiles are calculated based on the global dust evolution calculation including sintering effects. Disk ionization structure changes dramatically across the snow line due to the change of dust size distribution close to snow line of major volatiles. We find that accretion is mainly driven by disk wind. Gaps and rings can be quickly produced from different accretion rates across snow line. Furthermore, ambipolar diffusion (AD) leads to highly preferential accretion at midplane, followed by magnetic reconnection. This results a local zone of decretion that drains of mass in the field reconnection area, which leaves a gap and an adjacent ring just outside it. Overall, under the favorable condition, both snow lines and non-ideal MHD effects can lead to gaseous gaps and rings in protoplanetary disks.

arXiv comment13 pages, 10 figures, published on ApJ

References in corpus (45)

• First Results from High Angular Resolution ALMA Observations Toward the HL Tau Region
• Gaps and Rings in an ALMA Survey of Disks in the Taurus Star-forming Region
• Wind-driven Accretion in Protoplanetary Disks. I: Suppression of the Magnetorotational Instability and Launching of the Magnetocentrifugal Wind
• The Disk Substructures at High Angular Resolution Project (DSHARP): II. Characteristics of Annular Substructures
• Linear and nonlinear evolution of the vertical shear instability in accretion discs
• Dust Filtration by Planet-Induced Gap Edges: Implications for Transitional Disks
• Zonal Flows and Long-Lived Axisymmetric Pressure Bumps in Magnetorotational Turbulence
• The Disk Substructures at High Angular Resolution Project (DSHARP): VII. The Planet-Disk Interactions Interpretation
• Gaps, Rings, and Non-Axisymmetric Structures in Protoplanetary Disks - From Simulations to ALMA Observations
• Radiation-Hydrodynamic Models of X-Ray & EUV Photoevaporating Protoplanetary Discs
• Linear Analysis of the Hall Effect in Protostellar Disks
• Evidence of fast pebble growth near condensation fronts in the HL Tau protoplanetary disk
• A Kinematical Detection of Two Embedded Jupiter Mass Planets in HD 163296
• Sintering-induced Dust Ring Formation in Protoplanetary Disks: Application to the HL Tau Disk
• Observational Signatures of Planets in Protoplanetary Disks I: Gaps Opened by Single and Multiple Young Planets in Disks
• On planet formation in HL Tau
• Magnetic fields in protoplanetary disks
• Electric charging of dust aggregates and its effect on dust coagulation in protoplanetary disks
• MHD simulations of jet acceleration from Keplerian accretion disks: the effects of disk resistivity
• Heat and Dust in Active Layers of Protostellar Disks
• Global Simulations of the Inner Regions of Protoplanetary Disks with Comprehensive Disk Microphysics
• Global Evolution of an Accretion Disk with Net Vertical Field: Coronal Accretion, Flux Transport, and Disk Winds
• Protoplanetary disk rings and gaps across ages and luminosities
• Wind-driven Accretion in Protoplanetary Disks --- II: Radial Dependence and Global Picture
• Magnetic Flux Concentration and Zonal Flows in Magnetorotational Instability Turbulence
• The formation of rings and gaps in magnetically coupled disk-wind systems: ambipolar diffusion and reconnection
• Self-induced dust traps: overcoming planet formation barriers
• Global Simulations of Protoplanetary Disk Outflows with Coupled Non-ideal Magnetohydrodynamics and Consistent Thermochemistry
• Hall-effect Mediated Magnetic Flux Transport in Protoplanetary Disks
• An Origin of Multiple Ring Structure and Hidden Planets in HL Tau: A Unified Picture by Secular Gravitational Instability
• CN rings in full protoplanetary disks around young stars as probes of disk structure
• Hydrodynamic Photoevaporation of Protoplanetary Disks with Consistent Thermochemistry
• Nonsticky Ice at the Origin of the Uniformly Polarized Submillimeter Emission from the HL Tau Disk
• The formation of rings and gaps in wind-launching non-ideal MHD disks: three-dimensional simulations
• Stringent limits on the magnetic field strength in the disc of TW Hya: ALMA observations of CN polarisation
• Diverse protoplanetary disk morphology produced by a Jupiter-mass planet
• Radial Transport of Large-Scale Magnetic Fields in Accretion Disks. I. Steady Solutions and an Upper Limit on the Vertical Field Strength
• Resolving Protoplanetary Disks at Millimeter Wavelengths by CARMA
• The Role of Tiny Grains on the Accretion Process in Protoplanetary Disks
• Rings and gaps produced by variable magnetic disk winds and avalanche accretion streams: I. Axisymmetric resistive MHD simulations
• Magnetically Induced Disk Winds and Transport in the HL Tau Disk
• Self-organisation in protoplanetary disks: global, non-stratified Hall-MHD simulations
• Inside-Out Planet Formation. III. Planet-disk interaction at the dead zone inner boundary
• Magnetorotational instability in protoplanetary discs: The effect of dust grains
• On the Origin of Banded Structure in Dusty Protoplanetary Discs: HL Tau and TW Hya

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• Three-dimensional Global Simulations of Type-II Planet-disk Interaction with a Magnetized Disk Wind: I. Magnetic Flux Concentration and Gap Properties
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• Super-resolution trends in the ALMA Taurus survey: Structured inner discs and compact discs
• Constraining Protoplanetary Disk Accretion and Young Planets Using ALMA Kinematic Observations
• The maximum accretion rate of a protoplanet: how fast can runaway be?
• Formation of Dust Rings and Gaps in Non-ideal MHD Disks Through Meridional Gas Flows
• Ring formation by coagulation of dust aggregates in early phase of disk evolution around a protostar
• Gravitoviscous Protoplanetary Discs with a Dust Component. IV. Disc Outer Edges, Spectral Indices, and Opacity Gaps
• Self-consistent ring model in protoplanetary disks: temperature dips and substructure formation
• Growth of Magnetorotational Instability in Circumstellar Disks around Class 0 Protostars
• Architecture of planetary systems predicted from protoplanetary disks observed with ALMA I: mass of the possible planets embedded in the dust gap
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• The steady-state hydrodynamics of a long-lived disc: planetary system architecture and prospects of observing a circumplanetary disc shadow in V4046Sgr
• Dust rings as a footprint of planet formation in a protoplanetary disk
• A Tale of Two Grains: impact of grain size on ring formation via nonideal MHD processes
• Nonlinear evolution of streaming instabilities in accreting protoplanetary disks
• Gap Opening in Protoplanetary Disks: Gas Dynamics from Global Non-ideal MHD Simulations with Consistent Thermochemistry
• Architecture of three-planet systems predicted from the observed protoplanetary disk of HL Tau
• DBNets2.0: simulation-based inference for planet-induced dust substructures in protoplanetary discs
• Unlocking planetesimal magnetic field histories: a refined, versatile model for thermal evolution and dynamo generation
• On the origin of transition disk cavities: Pebble-accreting protoplanets vs Super-Jupiters
• Confirmation of a ring structure in the disk around MP Mus (PDS 66) with ALMA Band 7 observations
• exoALMA XXIII. Estimating Disk and Planet Properties from Dust Morphologies with DBNets2.0
• Magnetic reconnection in partially ionized plasmas
• History of the Solar Nebula from Meteorite Paleomagnetism