Dynamics Near the Inner Dead-Zone Edges in a Proprotoplanetary Disk
Kazunari Iwasaki, Kengo Tomida, Shinsuke Takasao, Satoshi Okuzumi,, Takeru K. Suzuki

TL;DR
This study uses advanced 3D non-ideal MHD simulations to reveal complex magnetic and flow structures near the inner dead-zone edge in protoplanetary disks, highlighting a transition zone with distinct properties affecting accretion.
Contribution
It introduces a detailed simulation-based analysis of the inner dead-zone edge, identifying a new transition zone with unique physical properties and magnetic flux behavior.
Findings
The dead zone splits into transition and coherent zones with different properties.
The transition zone inhibits mass and magnetic flux transport between zones.
Mass accumulates at the edges of the transition zone due to supply from adjacent zones.
Abstract
We perform three-dimensional global non-ideal magnetohydrodynamic simulations of a protoplanetary disk containing the inner dead-zone edge. We take into account realistic diffusion coefficients of the Ohmic resistivity and ambipolar diffusion based on detailed chemical reactions with single-size dust grains. We found that the conventional dead zone identified by the Els\"asser numbers of the Ohmic resistivity and ambipolar diffusion is divided into two regions: "the transition zone" and "the coherent zone". The coherent zone has the same properties as the conventional dead zone, and extends outside of the transition zone in the radial direction. Between the active and coherent zones, we discover the transition zone, the inner edge of which is identical to that of the conventional dead zone. The transition zone extends out over the regions where thermal ionization determines diffusion…
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Taxonomy
TopicsAstrophysics and Star Formation Studies · Astro and Planetary Science · Stellar, planetary, and galactic studies
