Award Date
May 2023
Degree Type
Thesis
Degree Name
Master of Science (MS)
Department
Physics and Astronomy
First Committee Member
Zhaohuan Zhu
Second Committee Member
Rebecca Martin
Third Committee Member
Daniel Proga
Fourth Committee Member
Pengtao Sun
Number of Pages
82
Abstract
Rings are one of the most ubiquitous substructures observed in protoplanetary disks. They are known to be a robust site for planetesimal formation; thus we look for mechanisms that can originate stable rings. From chemical modelling of snow lines, we expect a bump in the Ambipolar Diffusion (AD) Elssaser number (Am) in the radial direction. We use the Athena++ code to model the non-ideal Magentohydrodynamics (MHD) behavior of an Am bump. We explore a parameter space of Gaussian bumps with Am = 5, 1, 0.5 peak strength and σ = 0.25, 1, 5. The Gaussian profile is inserted into the local shearing box MHD model originally run by Hawley et al. (1995). We run both positive and inverted profile cases to 100 orbits, in an 8H × 8H × 1H box. A variety of Am profiles are capable of concentrating gas up to 2.5 × ρ0 (initial density), beyond zonal flows. We note magnetic flux is concentrated in areas of low gas density. σ = 0.25 Gaussians are inconsistent and can exhibit ideal MHD. In the case of a weak overall magnitude of AD, but a non-flat profile, zonal flows are disrupted. The gas density bumps driven by AD are sufficient to trap particles, and therefore an Am bump can trigger ring formation. We also suggest that zonal flows may be fragile to non-flat Am. The Am − ρ relationship in Bai & Stone (2011) is shown to be accurate to within 30% for all but the σ = 0.25 runs, but could be improved upon.
Keywords
Ambipolar Diffusion; Athena++; Magnetohydrodynamics; Non-Ideal MHD; Proto-Planetary Disks
Disciplines
Astrophysics and Astronomy | Other Physics | Physics
File Format
Degree Grantor
University of Nevada, Las Vegas
Language
English
Repository Citation
Mohov, Aleksey S., "Simulating Radial Ring Structure with an Ambipolar Elsasser (Am) Bump in Non-Ideal Magnetohydrodynamics of Protoplanetary Disks" (2023). UNLV Theses, Dissertations, Professional Papers, and Capstones. 4740.
http://dx.doi.org/10.34917/36114765
Rights
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