Dust Dynamics in Hall-effected Protoplanetary Disks. I. Background Drift Hall Instability

Recent studies have shown that the large-scale gas dynamics of protoplanetary disks (PPDs) are controlled by nonideal magnetohydrodynamics (MHD), but how this influences dust dynamics is not fully understood. To this end, we investigate the stability of dusty, magnetized disks subject to the Hall ef...

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Main Authors: Yinhao Wu, Min-Kai Lin, Can Cui, Leonardo Krapp, Yueh-Ning Lee, Andrew N. Youdin
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/ad15fe
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author Yinhao Wu
Min-Kai Lin
Can Cui
Leonardo Krapp
Yueh-Ning Lee
Andrew N. Youdin
author_facet Yinhao Wu
Min-Kai Lin
Can Cui
Leonardo Krapp
Yueh-Ning Lee
Andrew N. Youdin
author_sort Yinhao Wu
collection DOAJ
description Recent studies have shown that the large-scale gas dynamics of protoplanetary disks (PPDs) are controlled by nonideal magnetohydrodynamics (MHD), but how this influences dust dynamics is not fully understood. To this end, we investigate the stability of dusty, magnetized disks subject to the Hall effect, which applies to planet-forming regions of PPDs. We find a novel background drift Hall instability (BDHI) that may facilitate planetesimal formation in Hall-effected disk regions. Through a combination of linear analysis and nonlinear simulations, we demonstrate the viability and characteristics of BDHI. We find it can potentially dominate over the classical streaming instability (SI) and standard MHD instabilities at low dust-to-gas ratios and weak magnetic fields. We also identify magnetized versions of the classic SI, but these are usually subdominant. We highlight the complex interplay between magnetic fields and dust-gas dynamics in PPDs, underscoring the need to consider nonideal MHD like the Hall effect in the broader narrative of planet formation.
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spelling doaj.art-fca5f9ce91b94e44ad13dbb0148c8ae72024-02-19T10:37:14ZengIOP PublishingThe Astrophysical Journal1538-43572024-01-01962217310.3847/1538-4357/ad15feDust Dynamics in Hall-effected Protoplanetary Disks. I. Background Drift Hall InstabilityYinhao Wu0https://orcid.org/0000-0003-3728-8231Min-Kai Lin1https://orcid.org/0000-0002-8597-4386Can Cui2https://orcid.org/0000-0003-3180-0038Leonardo Krapp3https://orcid.org/0000-0001-7671-9992Yueh-Ning Lee4https://orcid.org/0000-0003-3497-2329Andrew N. Youdin5https://orcid.org/0000-0002-3644-8726School of Physics and Astronomy, University of Leicester , Leicester LE1 7RH, UK ; yw505@leicester.ac.uk; Institute of Astronomy and Astrophysics , Academia Sinica, Taipei 10617, Taiwan, R.O.C. ; mklin@asiaa.sinica.edu.twInstitute of Astronomy and Astrophysics , Academia Sinica, Taipei 10617, Taiwan, R.O.C. ; mklin@asiaa.sinica.edu.tw; Physics Division, National Center for Theoretical Sciences , Taipei 10617, Taiwan, R.O.C.Department of Astronomy and Astrophysics, University of Toronto , Toronto, ON M5S 3H4, Canada; DAMTP, University of Cambridge , Wilberforce Road, Cambridge CB3 0WA, UKDepartment of Astronomy and Steward Observatory, University of Arizona , Tucson, AZ 85721, USAPhysics Division, National Center for Theoretical Sciences , Taipei 10617, Taiwan, R.O.C.; Department of Earth Sciences, National Taiwan Normal University , Taipei 116059, Taiwan, R.O.C.; Center of Astronomy and Gravitation, National Taiwan Normal University , Taipei 116059, Taiwan, R.O.C.Department of Astronomy and Steward Observatory, University of Arizona , Tucson, AZ 85721, USA; The Lunar and Planetary Laboratory, University of Arizona , Tucson, AZ 85721, USARecent studies have shown that the large-scale gas dynamics of protoplanetary disks (PPDs) are controlled by nonideal magnetohydrodynamics (MHD), but how this influences dust dynamics is not fully understood. To this end, we investigate the stability of dusty, magnetized disks subject to the Hall effect, which applies to planet-forming regions of PPDs. We find a novel background drift Hall instability (BDHI) that may facilitate planetesimal formation in Hall-effected disk regions. Through a combination of linear analysis and nonlinear simulations, we demonstrate the viability and characteristics of BDHI. We find it can potentially dominate over the classical streaming instability (SI) and standard MHD instabilities at low dust-to-gas ratios and weak magnetic fields. We also identify magnetized versions of the classic SI, but these are usually subdominant. We highlight the complex interplay between magnetic fields and dust-gas dynamics in PPDs, underscoring the need to consider nonideal MHD like the Hall effect in the broader narrative of planet formation.https://doi.org/10.3847/1538-4357/ad15feProtoplanetary disksPlanet formationPlanetesimalsHydrodynamicsMagnetohydrodynamicsAstrophysical fluid dynamics
spellingShingle Yinhao Wu
Min-Kai Lin
Can Cui
Leonardo Krapp
Yueh-Ning Lee
Andrew N. Youdin
Dust Dynamics in Hall-effected Protoplanetary Disks. I. Background Drift Hall Instability
The Astrophysical Journal
Protoplanetary disks
Planet formation
Planetesimals
Hydrodynamics
Magnetohydrodynamics
Astrophysical fluid dynamics
title Dust Dynamics in Hall-effected Protoplanetary Disks. I. Background Drift Hall Instability
title_full Dust Dynamics in Hall-effected Protoplanetary Disks. I. Background Drift Hall Instability
title_fullStr Dust Dynamics in Hall-effected Protoplanetary Disks. I. Background Drift Hall Instability
title_full_unstemmed Dust Dynamics in Hall-effected Protoplanetary Disks. I. Background Drift Hall Instability
title_short Dust Dynamics in Hall-effected Protoplanetary Disks. I. Background Drift Hall Instability
title_sort dust dynamics in hall effected protoplanetary disks i background drift hall instability
topic Protoplanetary disks
Planet formation
Planetesimals
Hydrodynamics
Magnetohydrodynamics
Astrophysical fluid dynamics
url https://doi.org/10.3847/1538-4357/ad15fe
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