The impact of the Hall effect during cloud core collapse:implications for circumstellar disk evolution

Abstract

We perform three-dimensional radiation non-ideal magnetohydrodynamics simulations and investigate the impact of the Hall effect on the angular momentum evolution in the collapsing cloud cores in which the magnetic field $\magB$ and angular momentum $\angJ$ are misaligned with each other. We find that the Hall effect notably changes the magnetic torques in the pseudo-disk, and strengthens and weakens the magnetic braking in cores with an acute and obtuse relative angles between $\magB$ and $\angJ$, respectively. This suggests that the bimodal evolution of the disk size may occur in early disk evolutionary phase even if $\magB$ and $\angJ$ are randomly distributed. We show that a counter-rotating envelope form in the upper envelope of the pseudo-disk in cloud cores with obtuse relative angles. We also find that a counter-rotating region forms at the midplane of the pseudo-disk in cloud cores with acute relative angles. The former and latter types of counter-rotating envelopes may be associated with the YSOs with a large ($r\sim 100$ AU) and small ($r\lesssim 10$ AU) disks, respectively.

22 pages, 20 figures, accepted by PASJ. several discussions are added. Comments are welcome

References in corpus (73)

• Low Temperature Opacities
• Gas- and dust evolution in protoplanetary disks
• Rosseland and Planck Mean Opacities for Protoplanetary Discs
• Wind-driven Accretion in Protoplanetary Disks. I: Suppression of the Magnetorotational Instability and Launching of the Magnetocentrifugal Wind
• Magnetic processes in a collapsing dense core. I Accretion and Ejection
• Protostellar disk formation and transport of angular momentum during magnetized core collapse
• Global simulations of protoplanetary disks with ohmic resistivity and ambipolar diffusion
• Collapse of Magnetized Singular Isothermal Toroids: II. Rotation and Magnetic Braking
• A 0.2 solar mass protostar with a Keplerian disk in the very young L1527 IRS system
• Magnetic Braking and Protostellar Disk Formation: The Ideal MHD Limit
• The impact of magnetic fields on single and binary star formation
• TADPOL: A 1.3 mm Survey of Dust Polarization in Star-forming Cores and Regions
• Electric charging of dust aggregates and its effect on dust coagulation in protoplanetary disks
• Radiation Magnetohydrodynamic Simulations of Protostellar Collapse: Protostellar Core Formation
• A Keplerian disk around a Class 0 source: ALMA observations of VLA1623A
• Disk formation during collapse of magnetized protostellar cores
• Mechanism of Magnetic Flux Loss in Molecular Clouds
• Ambipolar diffusion in low-mass star formation. I. General comparison with the ideal MHD case
• Collapse of Rotating Magnetized Molecular Cloud Cores and Mass Outflows
• Formation of a Keplerian disk in the infalling envelope around L1527 IRS: transformation from infalling motions to Kepler motions
• Radiation Magnetohydrodynamic Simulations of Protostellar Collapse: Non-Ideal Magnetohydrodynamic Effects and Early Formation of Circumstellar Disks
• Nonideal MHD Effects and Magnetic Braking Catastrophe in Protostellar Disk Formation
• Global Simulations of the Inner Regions of Protoplanetary Disks with Comprehensive Disk Microphysics
• Misalignment of Magnetic Fields and Outflows in Protostellar Cores
• Formation Process of the Circumstellar Disk: Long-term Simulations in the Main Accretion Phase of Star Formation
• Effect of Magnetic Braking on the Circumstellar Disk Formation in a Strongly Magnetized Cloud
• Signs of Early-Stage Disk Growth Revealed with ALMA
• Can non-ideal magnetohydrodynamics solve the magnetic braking catastrophe?
• Protostellar collapse: radiative and magnetic feedbacks on small scale fragmentation
• Recurrent Planet Formation and Intermittent Protostellar Outflows Induced by Episodic Mass Accretion
• Magnetic Fields and Rotations of Protostars
• Directions of Outflows, Disks, Magnetic Fields, and Rotation of YSOs in Collapsing Molecular Cloud Cores
• Effects of Ohmic and ambipolar diffusion on the formation and evolution of the first cores, protostars and circumstellar discs
• Conditions for Circumstellar Disk Formation: Effects of Initial Conditions and Sink Treatment
• Does Magnetic Field-Rotation Misalignment Solve the Magnetic Braking Catastrophe in Protostellar Disk Formation?
• Bridging the gap: disk formation in the Class 0 phase with ambipolar diffusion and Ohmic dissipation
• Bimodality of circumstellar disk evolution induced by Hall current
• Emergence of Protoplanetary Disks and Successive Formation of Gaseous Planets by Gravitational Instability
• ALMA Observations of the Transition from Infall Motion to Keplerian Rotation around the Late-phase Protostar TMC-1A
• The Origin and Formation of the Circumstellar Disk
• Hall diffusion and the magnetorotational instability in protoplanetary discs
• A faster algorithm for smoothed particle hydrodynamics with radiative transfer in the flux-limited diffusion approximation
• The Turbulent Magnetic Prandtl Number of MHD Turbulence in Disks
• Star Formation and the Hall Effect
• Turbulent resistivity driven by the magnetorotational instability
• Grand Design Spiral Arms in A Young Forming Circumstellar Disk
• Disk Formation in Magnetized Clouds Enabled by the Hall Effect
• First MHD Simulation of Collapse and Fragmentation of Magnetized Molecular Cloud Cores
• Hall-effect Mediated Magnetic Flux Transport in Protoplanetary Disks
• Smoothed particle hydrodynamics with radiative transfer in the flux-limited diffusion approximation
• A chemical solver to compute molecule and grain abundances and non-ideal MHD resistivities in prestellar core collapse calculations
• No Keplerian Disk >10 AU around the Protostar B335: Magnetic Braking or Young Age?
• Effects of radiation transfer on the structure of self-gravitating disks, their fragmentation and evolution of the fragments
• Transition from the Infalling Envelope to the Keplerian Disk around L1551 IRS 5
• The Hall effect in star formation
• Smoothed particle magnetohydrodynamics with a Riemann solver and the method of characteristics
• Apparent disk-mass reduction and planetesimal formation in gravitationally unstable disks in Class 0/I YSOs
• The effect of magnetic fields on the formation of circumstellar discs around young stars
• Simulations of protostellar collapse using multigroup radiation hydrodynamics. I. The first collapse
• Ambipolar diffusion in smoothed particle magnetohydrodynamics
• NICIL: A stand alone library to self-consistently calculate non-ideal magnetohydrodynamic coefficients in molecular cloud cores
• A grid of 1D low-mass star formation collapse models
• The Hall effect in accretion flows
• Formation, orbital and thermal evolution, and survival of planetary-mass clumps in the early phase of circumstellar disk evolution
• Formation and Early Evolution of Circumstellar Disks in Turbulent Molecular Cloud Cores
• An explicit scheme for ohmic dissipation with smoothed particle magneto-hydrodynamics
• The dependence of protostar formation on the geometry and strength of the initial magnetic field
• The magnetic diffusivities in 3D radiative chemo-hydrodynamic simulations of protostellar collapse
• Dissipation of magnetic fields in star-forming clouds with different metallicities
• Magnetic field and early evolution of circumstellar disks
• Evidence for Infalling Gas of Low Angular Momentum towards the L1551 NE Keplerian Circumbinary Disk
• The effect of external environment on the evolution of protostellar disks
• An alternative model for the origin of gaps in circumstellar disks

Cited by in corpus (53)

• Interferometric observations of magnetic fields in forming stars
• Protostellar birth with ambipolar and ohmic diffusion
• The role of magnetic fields in the formation of protostellar discs
• There is no magnetic braking catastrophe: Low-mass star cluster and protostellar disc formation with non-ideal magnetohydrodynamics
• What determines the formation and characteristics of protoplanetary discs?
• Global Hydromagnetic Simulations of Protoplanetary Disks with Stellar Irradiation and Simplified Thermochemistry
• The collapse of a molecular cloud core to stellar densities using radiation non-ideal magnetohydrodynamics
• Angular momentum profiles of Class 0 protostellar envelopes
• The Effect of Misalignment between Rotation Axis and Magnetic Field on Circumstellar Disk
• Magnetic field amplification in accretion discs around the first stars: implications for the primordial IMF
• The Origin of the Stellar Mass Distribution and Multiplicity
• Disk structure around the Class I protostar L1489 IRS revealed by ALMA: a warped disk system
• Impact of the Hall effect in star formation and the issue of angular momentum conservation
• Does misalignment between magnetic field and angular momentum enhance or suppress circumstellar disk formation?
• The Co-evolution of Disk and Star in Embedded Stages: The Case of the Very Low-mass Protostar
• Hall Effect in Protostellar Disc Formation and Evolution
• Non-ideal magnetohydrodynamics vs turbulence I: Which is the dominant process in protostellar disc formation?
• The impact of non-ideal magnetohydrodynamic processes on discs, outflows, counter-rotation and magnetic walls during the early stages of star formation
• Hall effect-driven formation of gravitationally unstable discs in magnetized molecular cloud cores
• The JCMT BISTRO survey: alignment between outflows and magnetic fields in dense cores/clumps
• On the origin of magnetic fields in stars
• The effect of extreme ionisation rates during the initial collapse of a molecular cloud core
• The Interplay between Ambipolar Diffusion and Hall Effect on Magnetic Field Decoupling and Protostellar Disc Formation
• Early evolution of disk, outflow, and magnetic field of young stellar objects: Impact of dust model
• Star-disk alignment in the protoplanetary disks: SPH simulation of the collapse of turbulent molecular cloud cores
• Substructures in the Disk-Forming Region of the Class 0 Low-Mass Protostellar Source IRAS 16293-2422 Source A on a 10 au Scale
• Dependence of Hall Coefficient on Grain Size and Cosmic Ray Rate and Implication for Circumstellar Disk Formation
• Non-ideal magnetohydrodynamics vs turbulence II: Which is the dominant process in stellar core formation?
• Do we need non-ideal magnetohydrodynamics to model protostellar discs?
• On the origin of magnetic fields in stars II: The effect of numerical resolution
• Impact of the Hall effect in star formation : improving the angular momentum conservation
• Conditions for justifying single-fluid approximation for charged and neutral dust fluids and a smoothed particle magnetohydrodynamics method for dust-gas mixture
• Protostellar disk formation by a non-rotating, non-axisymmetric collapsing cloud: model and comparison with observations
• Different Modes of Star Formation II: Gas Accretion Phase of Initially Subcritical Star-Forming Clouds
• Protostellar Evolution in Serpens Main: Possible Origin of Disk-Size Diversity
• Ionization degree and magnetic diffusivity in the primordial star-forming clouds
• Possible Counter Rotation between the Disk and Protostellar Envelope around the Class I Protostar IRAS 04169+2702
• Non-ideal magnetohydrodynamic simulations of the first star formation: the effect of ambipolar diffusion
• Transition from ordered pinched to warped magnetic field on a 100 au scale in the Class 0 protostar B335
• ALMA Observations toward the S-shaped Outflow and the Envelope around NGC1333 IRAS 4A2
• Ambipolar diffusion and the molecular abundances in prestellar cores
• FERIA: Flat Envelope Model with Rotation and Infall under Angular Momentum Conservation
• The Distinct Evolutionary Nature of two Class 0 Protostars in Serpens Main SMM4
• Driving Conditions of Protostellar Outflows in Different Star-Forming Environments
• Time Evolution of 3D Disk Formation with Misaligned Magnetic Field and Rotation Axes
• A misaligned protostellar disk fed by gas streamers in a barred spiral-like massive dense core
• Discovery of Asymmetric Spike-like Structures of the 10 au Disk around the Very Low-luminosity Protostar Embedded in the Taurus Dense Core MC 27/L1521F with ALMA
• Simulations of the isothermal collapse of magnetic rotating protostellar clouds
• Star-forming environments in smoothed particle magnetohydrodynamics simulations I: Clump extraction and properties
• Dust enrichment and growth in the earliest stages of protoplanetary disk formation
• Co-evolution of dust grains and protoplanetary disks II: structure and evolution of protoplanetary disks; an analytical approach
• The VLA/ALMA Nascent Disk and Multiplicity (VANDAM) Survey of Orion Protostars VI. Insights from Radiative Transfer Modeling
• Special Relativistic Smoothed Particle Hydrodynamics Based on Riemann Solver