Modeling and Simulation of Circumstellar Disks with the Next Generation of Hydrodynamic Solvers

DSpace/Manakin Repository

Modeling and Simulation of Circumstellar Disks with the Next Generation of Hydrodynamic Solvers

Citable link to this page

 

 
Title: Modeling and Simulation of Circumstellar Disks with the Next Generation of Hydrodynamic Solvers
Author: Munoz, Diego Jose
Citation: Munoz, Diego Jose. 2013. Modeling and Simulation of Circumstellar Disks with the Next Generation of Hydrodynamic Solvers. Doctoral dissertation, Harvard University.
Full Text & Related Files:
Abstract: This thesis is a computational study of circumstellar gas disks, with a special focus on modeling techniques and on numerical methods not only as scientific tools but also as a target of study. In particular, in-depth discussions are included on the main numerical strategy used, namely the moving-mesh method for astrophysical hydrodynamics. In this work, the moving-mesh approach is used to simulate circumstellar disks for the first time.
Terms of Use: This article is made available under the terms and conditions applicable to Other Posted Material, as set forth at http://nrs.harvard.edu/urn-3:HUL.InstRepos:dash.current.terms-of-use#LAA
Citable link to this page: http://nrs.harvard.edu/urn-3:HUL.InstRepos:11181673
Downloads of this work:

Show full Dublin Core record

This item appears in the following Collection(s)

 
 

Search DASH


Advanced Search
 
 

Submitters