The Roles of Dust Growth in the Temperature Evolution and Snow Line Migration in Magnetically Accreting Protoplanetary Disks

The temperature structure of protoplanetary disks provides an important constraint on where in the disks rocky planets like our own form. Recent nonideal magnetohydrodynamical (MHD) simulations have shown that the internal Joule heating associated with magnetically driven disk accretion is inefficie...

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Veröffentlicht in:	arXiv.org 2023-03
Hauptverfasser:	Kondo, Katsushi, Okuzumi, Satoshi, Mori, Shoji
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion disks Dust Gas ionization Grain growth Grain size Magnetohydrodynamics Ohmic dissipation Opacity Physics - Earth and Planetary Astrophysics Physics - Solar and Stellar Astrophysics Planet formation Planetary evolution Protoplanetary disks Resistance heating Snow Terrestrial planets Vertical distribution
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