Dynamo action by differential rotation in a stably stratified stellar interior

Abstract

Magnetic fields can be created in stably stratified (non-convective) layers in a differentially rotating star. A magnetic instability in the toroidal field (wound up by differential rotation) replaces the role of convection in closing the field amplification loop. Tayler instability is likely to be the most relevant magnetic instability. A dynamo model is developed from these ingredients, and applied to the problem of angular momentum transport in stellar interiors. It produces a prodominantly horizontal field. This dynamo process might account for the observed pattern of rotation in the solar core.

Expanded version as accepted by Astron. Astrophys

Cited by in corpus (649)

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• The effects of surface fossil magnetic fields on massive star evolution: III. The case of $\tau$ Sco
• Evolution of a magnetic field in a differentially rotating radiative zone
• Rotation and magnetism in intermediate mass stars
• Spin and Magnetism of White Dwarfs
• Optical Multi-Channel Intensity Interferometry - or: How To Resolve O-Stars in the Magellanic Clouds
• Inverse Tides in Pulsating Binary Stars
• A Comparison of 2D Magnetohydrodynamic Supernova Simulations with the CoCoNuT-FMT and Aenus-Alcar Codes
• Detecting deep axisymmetric toroidal magnetic fields in stars. The traditional approximation of rotation for differentially rotating deep spherical shells with a general azimuthal magnetic field
• Critical angular momentum distributions in collapsars: quiescent periods from accretion state transitions in long gamma-ray bursts
• Polar confinement of the Sun's interior magnetic field by laminar magnetostrophic flow
• The spin rates and spin evolution of the O components in WR+O binaries
• On the Angular Momentum Transport Efficiency within the Star Constrained from Gravitational-wave Observations
• Phase-resolved spectroscopic analysis of the eclipsing black hole X-ray binary M33 X-7: System properties, accretion, and evolution
• Multi-site Observations of Pulsation in the Accreting White Dwarf SDSS J161033.64-010223.3 (V386 Ser)
• Effects of QCD phase transition on gravitational radiation from two-dimensional collapse and bounce of massive stars
• Evidence of active MHD instability in EULAG-MHD simulations of solar convection
• Differential rotation in rapidly rotating early-type stars. I. Motivations for combined spectroscopic and interferometric studies
• Magnetism in High-Mass Stars
• Simulations of a Magnetic Fluctuation Driven Large Scale Dynamo and Comparison with a Two-scale Model
• The GSF Instability and Turbulence do not Account for the Relatively Low Rotation Rate of Pulsars
• Soft coronal X-rays from β Pictoris
• Towards a unified model of stellar rotation II: Model-dependent characteristics of stellar populations
• Formation of low-spinning 100 Msun black holes
• Magnetic induction processes in Hot Jupiters, application to KELT-9b
• Angular momentum transport and element mixing in the stellar interior I. Application to the rotating Sun
• Resolving Black Hole Family Issues Among the Massive Ancestors of Very High-Spin Gravitational-Wave Events Like GW231123
• Numerical simulations of the Tayler-Spruit dynamo in proto-magnetars
• Helicity and dynamo action in magnetized stellar radiation zones
• Reverse Algols and hydrogen-rich Wolf-Rayet stars from very massive binaries
• Spins of black holes in coalescing compact binaries
• On the synchronizability of Tayler-Spruit and Babcock-Leighton type dynamos
• Testing angular momentum transport processes with asteroseismology of solar-type main-sequence stars
• The Effects of Magnetic Fields on the Dynamics of Radiation Pressure Dominated Massive Star Envelopes
• Hypercritical Accretion for Black Hole High Spin in Cygnus X-1
• Biases in estimates of black hole kicks from the spin distribution of binary black holes
• Magnetic field structure in single late-type giants: The effectively single giant V390 Aur
• Centrifugally Driven Mass Loss and Outbursts of Massive Stars
• Magnetic fields generated by r-modes in accreting millisecond pulsars
• Burn Out or Fade Away? On the X-ray and Magnetic Death of Intermediate Mass Stars
• The evolution of massive and very massive stars in clusters
• Wave mediated angular momentum transport in astrophysical boundary layers
• Magnetohydrodynamic Simulations of the Tayler Instability in Rotating Stellar Interiors
• On The Impact Of 22Ne On The Pulsation Periods Of Carbon-Oxygen White Dwarfs With Helium Dominated Atmospheres
• Models for Gamma-Ray Bursts and Diverse Transients
• Calibrating angular momentum transport in intermediate-mass stars from gravity-mode asteroseismology
• Ionizing photon production of Population III stars: effects of rotation, convection, and initial mass function
• Magnetohydrodynamic Shearing Waves
• Asteroseismology of evolved stars to constrain the internal transport of angular momentum. V. Efficiency of the transport on the red giant branch and in the red clump
• Magnetic field evolution in neutron stars
• Enhanced Rotational Mixing in the Radiative Zones of Massive Stars
• The mean electromotive force resulting from magnetic buoyancy instability
• Spinning up the Surface: Evidence for Planetary Engulfment or Unexpected Angular Momentum Transport?
• Differential Rotation in a 3D Simulation of Oxygen Shell Burning
• Common origin for black holes in both high mass X-ray binaries and gravitational-wave sources
• Large-scale ordered magnetic fields generated in mergers of helium white dwarfs
• A Common Envelope Binary Star Origin of Long Gamma-ray Bursts
• Asteroseismology of evolved stars to constrain the internal transport of angular momentum. VI. Testing a parametric formulation for the azimuthal magneto-rotational instability
• Helium and Nitrogen Enrichment in Massive Main Sequence Stars: Mechanisms and Implications for the Origin of WNL Stars
• Impact of Population III homogeneous stellar evolution on early cosmic reionisation
• Merging binary black holes formed through double-core evolution
• Backtracing the internal rotation history of the $\beta$ Cep star HD 129929
• Detection of Magnetic Massive Stars in the Open Cluster NGC 3766
• Solar models with new low-metal abundances
• Long-duration Gamma-ray Burst Progenitors and Magnetar Formation
• The Tayler Instability in the Anelastic Approximation
• Pre-explosion dynamo in the cores of massive stars
• Magneto-Rotational Transport in the Early Sun
• Some glimpses from helioseismology at the dynamics of the deep solar interior
• Gravitational Wave Astronomy
• The branching ratio of LIGO binary black holes
• On the dependence of X-ray burst rate on accretion and spin rate
• Revisiting Kepler-444. II. Rotational, orbital and high-energy fluxes evolution of the system
• Comparisons and Connections between Mean Field Dynamo Theory and Accretion Disc Theory
• Rapidly rotating neutron star progenitors
• Dynamical He Flashes in Double White Dwarf Binaries
• The spins of stripped B stars support magnetic internal angular momentum transport
• Exploring Supernova Gravitational Waves with Machine Learning
• Looking deep into the Cat's Eye: Structure and rotation in the fast wind of the PN central star of NGC6543
• On the Role of the $\Omega \Gamma$ Limit in the Formation of Population III Massive Stars
• Inefficient Angular Momentum Transport in Accretion Disk Boundary Layers: Angular Momentum Belt in the Boundary Layer
• Two types of axisymmetric helical magnetorotational instability in rotating flows with positive shear
• Populations of evolved massive binary stars in the Small Magellanic Cloud I: Predictions from detailed evolution models
• Rotation and Magnetism of Massive Stellar Cores
• Exploring the stellar rotation of early-type stars in the LAMOST Medium-Resolution Survey. II. Statistics
• Spectroscopic and evolutionary analyses of the binary system AzV 14 outline paths toward the WR stage at low metallicity
• Three-Dimensional Simulations of Massive Stars: II. Age Dependence
• The key impact of the host star's rotational history on the evolution of TOI-849b
• Evolution and Nucleosynthesis of Very Massive Stars
• Turbulent Mixing on Helium-Accreting White Dwarfs
• The Three-Dimensional Collapse of a Rapidly Rotating 16 $M_{\odot }$ Star
• Multidimensional Simulations of Core Convection
• Can very massive Population III stars produce a super-collapsar?
• Neutron stars formation and Core Collapse Supernovae
• Angular momentum transport in a contracting stellar radiative zone embedded in a large scale magnetic field
• Effects of Resistivity on Magnetized Core-Collapse Supernovae
• Asteroseismic sensitivity to internal rotation along the red-giant branch
• Four-frequency solution in a magnetohydrodynamic Couette flow as a consequence of azimuthal symmetry breaking
• Tayler-Spruit dynamo in stably stratified rotating fluids: Application to proto-magnetars
• Magnetized hot neutron matter: lowest order constrained variational calculations
• Can GW231123 have a stellar origin?
• Tracing the evolution of short-period binaries with super-synchronous fast rotators
• Unveiling complex magnetic field configurations in red giant stars
• Constraints on the properties of macroscopic transport in the Sun from combined lithium and beryllium depletion
• Angular momentum transport near convective-core boundaries of Gamma Doradus stars
• Tayler Instability Revisited
• Generating neutron-star magnetic fields: three dynamo phases
• A low-metallicity massive contact binary undergoing slow Case A mass transfer: A detailed spectroscopic and orbital analysis of SSN 7 in NGC 346 in the SMC
• An upper limit on the spins of merging binary black holes formed through binary evolution
• Kinematic Dynamo, Supersymmetry Breaking, and Chaos
• Black Hole Formation and Explosion from Rapidly Rotating Very Massive Stars
• Symmetry breaking in merging binary black holes from young massive clusters and isolated binaries
• Properties and applications of a predicted population of runaway He-sdO/B stars ejected from single degenerate He-donor SNe
• Linking 1D Evolutionary to 3D Hydrodynamical Simulations of Massive Stars
• Critical fields and growth rates of the Tayler instability as probed by a columnar gallium experiment
• Helioseismic inference of the solar radiative opacity
• Presupernova Structure of Massive Stars
• Be star discs: powered by a non-zero central torque
• Stability of toroidal magnetic fields in stellar interiors
• Small-Scale Dynamo in Stably Stratified Turbulence
• Structure and Skewness of the Effective Inspiral Spin Distribution of Binary Black Hole Mergers
• Searching for candidates of coalescing binary black holes formed through chemically homogeneous evolution in GWTC-3
• Stochastic Core Spin-Up in Massive Stars -- Implications of 3D Simulations of Oxygen Shell Burning
• Photometric White Dwarf Rotation
• Diving into the planetary system of Proxima with NIRPS -- Breaking the metre per second barrier in the infrared
• Baroclinic Instability in Stellar Radiation Zones
• Magnetohydrodynamic simulations of A-type stars: Long-term evolution of core dynamo cycles
• The shear-Hall instability in newborn neutron stars
• Decihertz gravitational waves from double white dwarf merger remnants
• Minute-cadence Observations of the LAMOST Fields with the TMTS: III. Statistic Study of the Flare Stars from the First Two Years
• On the multiplicity of the O-star Cyg OB2 #8A and its contribution to the gamma-ray source 3EG J2033+4118
• Coralie radial-velocity search for companions around evolved stars (CASCADES) III. A new Jupiter host-star: in-depth analysis of HD 29399 using TESS data
• The Betelgeuse Project III: Merger Characteristics
• On large-scale dynamos with stable stratification and the application to stellar radiative zones
• Rotational mixing in carbon-enhanced metal-poor stars with s-process enrichment
• Towards early-type eclipsing binaries as extragalactic milestones: II. NLTE spectral analysis and stellar parameters of the detached O-type system OGLE-LMC-ECL-06782 in the LMC
• Bringing Stellar Evolution & Feedback Together: Summary of proposals from the Lorentz Center Workshop, 2022
• Global simulations of Tayler instability in stellar interiors: a long-time multi-stage evolution of the magnetic field
• Tayler-Spruit dynamo in binary neutron star merger remnants
• Magnetic Archaeology of Early-Type Stellar Dynamos
• Analytic approximations for massive close post-mass transfer binary systems
• A model of anisotropic winds from rotating stars for evolutionary calculations
• Detectability of axisymmetric magnetic fields from the core to the surface of oscillating post-main sequence stars
• Magnetic Braking at work in binaries
• Discovery of magnetic fields in three He variable Bp stars with He and Si spots
• Effects of Rotationally-Induced Mixing in Compact Binary Systems with Low-Mass Secondaries and in Single Solar-Type Stars
• Formation of twin compact stars in low-mass X-ray binaries: Implications on eccentric and isolated millisecond pulsar populations
• Revising the evolutionary stage of HD 163899: the effects of convective overshooting and rotation
• Nonaxisymmetric linear instability of cylindrical magnetohydrodynamic Taylor-Couette flow
• Nonideal evolution of nonaxisymmetric, force-free magnetic fields in a magnetar
• Turning Points in the Evolution of Isolated Neutron Stars' Magnetic Fields
• Waves, Coriolis force and the dynamo effect
• Metal-enriched Pair-instability supernovae: Effects of rotation
• Maximal Jet Energy of Gamma-Ray Bursts through the Blandford-Znajek Mechanism
• The partial ionisation zone of heavy elements in F-stars: a study on how it correlates with rotation
• Nucleosynthesis from massive stars 50 years after B2FH
• On obliquely magnetized and differentially rotating stars
• A systematic route to subcritical dynamo branches
• Toroidal Field Reversals and the Axisymmetric Tayler Instability
• Storing magnetic fields in pre-collapse cores of massive stars
• Self-gravitating collapsing star and black hole spin-up in long gamma ray bursts
• Evolution of the surface magnetic field of rotating proto-neutron stars
• Impact of rotation on stellar models
• Formation of Wind-Fed Black Hole High-mass X-ray Binaries: The Role of Roche-lobe-Overflow Post Black-Hole Formation
• Signatures of a subpopulation of hierarchical mergers in the GWTC-4 gravitational-wave dataset
• Who Ordered That? Unequal-Mass Binary Black Hole Mergers Have Larger Effective Spins
• Rotating Supermassive Pop III Stars On The Main Sequence
• Rotation profiles of solar-like stars with magnetic fields
• Atmospheric heating and magnetism driven by ${}^{22}$Ne distillation in isolated white dwarfs
• A new long gamma-ray burst formation pathway at solar metallicity
• Towards a holistic magnetic braking model from the evolution of cataclysmic variables to stellar spin-down -- I: the spin-down of fully convective M-dwarfs
• Can massive Be/Oe stars be progenitors of long gamma ray bursts?
• Eddy viscosity and turbulent Schmidt number by kink-type instability of strong toroidal magnetic fields
• Differential Rotation in Convective Envelopes: Constraints from Eclipsing Binaries
• Flare Activity and Magnetic Feature Analysis of the Flare Stars II: Sub-Giant Branch
• Magnetic Webs in Stellar Radiative Zones
• X-ray emission from helium star+black hole binaries as probes of tidally induced spin-up of second-born black holes
• Massive stars, successes and challenges
• Angular momentum and lithium transport from main sequence to sub-giant and red giant low-mass stars
• Convective Differential Rotation in Stars and Planets II: Observational and Numerical Tests
• Weak magnetic fields of intermediate-mass stars
• Nonlinear internal waves breaking in stellar radiation zones. Parametrisation for the transport of angular momentum: bridging geophysical to stellar fluid dynamics
• Axisymmetric investigation of differential rotation in contracting stellar radiative zones
• Magnetic field generated by r-modes in accreting quark stars
• Asteroseismology of the young open cluster NGC 2516 II. Constraining cluster age using gravity-mode pulsators
• Evolution of Massive Stars along the Cosmic History
• Spindown of massive main sequence stars in the Milky Way
• On the possibility of helicity oscillations in the saturation of the Tayler instability
• Evolutionary status of the Of?p star HD148937 and of its surrounding nebula NGC6164/5
• Longitudinal drift of Tayler instability eigenmodes as a possible explanation for super-slowly rotating Ap stars
• Interior rotation modelling of the $\beta$ Cep pulsator HD 192575 including multiplet asymmetries
• Stability of toroidal magnetic fields in the solar tachocline and beneath
• The efficiency of mixed modes for angular momentum transport
• Standing torsional Alfvén waves as the source of the rotational period variation in magnetic early-type stars
• Analysis of 3D MHD Instability of Antisolar Latitudinal Differential Rotation in F, G and K stars
• The Initial Magnetic Field Distribution in AB Stars
• Exploring the internal rotation of the extremely low-mass He-core white dwarf GD 278 with TESS asteroseismology
• Asteroseismogyrometry of low-mass red giants I. The SOLA inversion method
• A mixed helium-oxygen shell in some core-collapse supernova progenitors
• The robustness of inferred envelope and core rotation rates of red-giant stars from asteroseismology
• Evolutionary models for the Very Massive Stars in the R136 cluster of 30 Doradus in the Large Magellanic Cloud
• Dynamism in the solar core
• The rotational shear in pre-collapse cores of massive stars
• Reassessing the Spin of Second-born Black Holes in Coalescing Binary Black Holes and Its Connection to the chi_eff-q Correlation
• Large-scale dynamo action of magnetized Taylor-Couette flows
• Westward hotspot offset explained by subcritical dynamo action in an ultra-hot Jupiter atmosphere
• Constraining differential rotation in gamma Doradus stars from inertial dips properties
• A closer look at supernovae as seeds for galactic magnetization
• Chemical evolution of close massive binaries -- tidally-enhanced or tidally-suppressed mixing?
• Shaping core dynamos in A-type stars: The role of dipolar fossil fields
• Evidence for Three Subpopulations of Merging Binary Black Holes at Different Primary Masses
• The evolutionary state of the chemically peculiar members of the open cluster NGC2516
• On the rotation properties of a post-explosion helium-star companion in Type Iax supernovae
• Discovery of new magnetic δ Scuti stars and impact of magnetism on pulsation excitation
• Magnetic field dynamos and magnetically triggered flow instabilities
• Ultrashort-period WD binaries are not undergoing strong tidal heating
• Magnetic dynamos powered by white dwarf superficial convection
• Magnetic amplification in premerger neutron stars through resonance-induced magnetorotational instabilities
• Numerical evolution of the resistive relativistic magnetohydrodynamic equations: a minimally implicit Runge-Kutta scheme
• Using Lithium and Beryllium to Study Structure and Evolution of Rotating Stars
• Evolution of stars with 60 and 200 Msun: predictions for WNh stars in the Milky Way
• Meridional Circulation Streamlined
• Modelling stellar coronal magnetic fields
• Towards a holistic magnetic braking model -- II: explaining several long-term internal- and surface-spin properties of solar-like stars and the Sun
• Exploring the probing power of gamma-Dor's inertial dip for core magnetism: case of a toroidal field
• Near-critical magnetic fields in Kepler red giants
• Very Massive Close Binaries and the Puzzling Temporal Evolution of 14N in the Solar Neighbourhood
• Breaking gyrochronology through the collapse of coronal winds
• Impact of near-degeneracy effects on linear rotational inversions for red-giant stars
• Probing the internal magnetism of stars using asymptotic magneto-asteroseismology
• Magneto-Archeology of White Dwarfs. Revisiting the fossil field scenario with observational constraints during the red giant branch
• A semi-analytic approach to angular momentum transport in stellar radiative interiors
• General relativistic magnetohydrodynamics simulations for binary neutron star mergers
• Impact of the Tayler magnetic instability on the surface abundance of boron in massive stars
• Spin-up and spin distribution of stellar black holes grown by gas accretion in proto-stellar clusters
• An apparent positive relation between spin and orbital angular momentum in X-ray binaries
• A study of the electrostatic properties of the interiors of low-mass stars: Possible implications for the observed rotational properties
• Resonance locking and tidal evolution in rotating γ-Doradus binaries
• Which black hole formed first? Mass-ratio reversal in massive binary stars from gravitational-wave data
• Distinguishing Dirac and Majorana Neutrinos: Resonant Spin-Flavor Precession of GeV-Scale Astrophysical Transients
• Impact of stellar rotation on type II supernova progenitor masses from pre-explosion imaging
• Viscous and centrifugal instabilities of massive stars
• Understanding hydrodynamical wave-driven shear mixing in stellar radiation zones. Looking in the mirror of the dyapicnal oceanic mixing
• Mixing of CNO-cycled matter in massive stars
• Extra-galactic distances with massive stars: the role of stellar variability in the case of M33
• Near-degeneracy effects in Quadrupolar Mixed Modes. From an Asymptotic Description to Data Fitting
• Confinement of the Solar Tachocline by Dynamo Action in the Radiative Interior
• Stable magnetic fields and changing starspots on Vega -- An ultra-deep decadal survey at Pic du Midi and OHP
• EP250108a/SN2025kg: A Magnetar-powered Gamma-Ray Burst Supernova Originating from a Close Helium-star Binary via Isolated Binary Evolution
• Impact of tides on non-coplanar orbits of progenitors of high-mass X-ray binaries
• Co-existence of Internal Gravity Waves and Tayler-Spruit Magnetic Fields in the Radiative Core of Low-mass Stars
• Toward a Comprehensive Grid of Cepheid Models with MESA. IV. Modest Effects of Rotation on Blue Loops
• Coronal and chromospheric emission in A-type stars