Electric Heating and Angular Momentum Transport in Laminar Models of Protoplanetary Disks

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• William Bethune (University of Tuebingen)
• Tuesday 27 April 2021, 13:00-14:00
• ONLINE - Details to be sent by email.

If you have a question about this talk, please contact Dr Can Cui.

Observations point toward weak levels of turbulence in protoplanetary disks, and theoretical studies now focus on magneto-thermal winds rather than MRI turbulence as the main driver of mass accretion. Although MHD turbulence might be quenched, large-scale magnetic structures may still transport angular momentum and induce substantial accretion heating inside the disk. Using steady-state radiative MHD models, I examine how much stress and heat can thus be obtained in the weakly ionized parts of protoplanetary disks under the assumption of a purely laminar flow.

This talk is part of the Exoplanet Seminars series.

This talk is included in these lists:

• Cambridge Astronomy Talks
• Combined External Astrophysics Talks DAMTP
• Cosmology, Astrophysics and General Relativity
• Exoplanet Seminars
• Institute of Astronomy Talk Lists
• LCLU Departmental Talks
• ONLINE - Details to be sent by email

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