Skip navigation
Please use this identifier to cite or link to this item: http://arks.princeton.edu/ark:/88435/dsp01n296x160r
Full metadata record
DC FieldValueLanguage
dc.contributor.advisorStone, James M.-
dc.contributor.authorWhite, Christopher-
dc.contributor.otherAstrophysical Sciences Department-
dc.date.accessioned2016-09-27T15:47:44Z-
dc.date.available2016-09-27T15:47:44Z-
dc.date.issued2016-
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/dsp01n296x160r-
dc.description.abstractWe describe the implementation of sophisticated numerical techniques for general-relativistic magnetohydrodynamics simulations in the Athena++ code framework. Improvements over many existing codes include the use of advanced Riemann solvers and of staggered-mesh constrained transport. Combined with considerations for computational performance and parallel scalability, these allow us to investigate black hole accretion flows with unprecedented accuracy. The capability of the code is demonstrated by exploring magnetically arrested disks.-
dc.language.isoen-
dc.publisherPrinceton, NJ : Princeton University-
dc.relation.isformatofThe Mudd Manuscript Library retains one bound copy of each dissertation. Search for these copies in the library's main catalog: <a href=http://catalog.princeton.edu> catalog.princeton.edu </a>-
dc.subjectaccretion-
dc.subjectblack hole-
dc.subjectgeneral relativity-
dc.subjectmagnetohydrodynamics-
dc.subjectsimulation-
dc.subject.classificationAstrophysics-
dc.titleDevelopment and Application of Numerical Techniques for General-Relativistic Magnetohydrodynamics Simulations of Black Hole Accretion-
dc.typeAcademic dissertations (Ph.D.)-
pu.projectgrantnumber690-2143-
Appears in Collections:Astrophysical Sciences

Files in This Item:
File Description SizeFormat 
White_princeton_0181D_11905.pdf9.19 MBAdobe PDFView/Download


Items in Dataspace are protected by copyright, with all rights reserved, unless otherwise indicated.