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bad_bursters [2014/06/09 10:33] lauer |
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Link to Code on GitHub: [[https://github.com/brownjustinmichael/VH1|External Link]] | Link to Code on GitHub: [[https://github.com/brownjustinmichael/VH1|External Link]] | ||
- | Parameter sources | + | |
+ | =====RESULTS===== | ||
+ | 1D on a solid surface was successful so the 2D case was the bulk of the project work. The solid case was unstable and resulted in an non-physical explosion. Both the infall and reflective cases were attempted, we found the [] to be optimal. We were able to model a non-viscous and viscous case using hydronamic force and energy equation. Terms for the extremely large B field (10^7-8 T) were not included. Both accreted around the central mass with a large high pressure/empty barrier for the non-viscous case, as the angular momentum is not dissipated. The viscous case correctly accreted on to the surface. | ||
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+ | [[https://docmgmt.nscl.msu.edu/share/proxy/alfresco/api/node/content/workspace/SpacesStore/8e4a7857-347b-4603-9f64-bf2422ff5e7e/Simulating%20Accretion%20on%20Degenerate%20Matter%20to%20Model%20Surface.pdf|Presentation PDF]] | ||
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+ | [[|video of non viscous ac | ||
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+ | References: | ||
*Accretion Power in Astrophysics - Frank, King, Raine | *Accretion Power in Astrophysics - Frank, King, Raine | ||
*Accretion Disk for Beginners : [[http://www.astronomy.ohio-state.edu/~ryden/ast825/ | External Link]] (Notes PDF) | *Accretion Disk for Beginners : [[http://www.astronomy.ohio-state.edu/~ryden/ast825/ | External Link]] (Notes PDF) | ||
- | RESULTS: | ||
- | [[https://docmgmt.nscl.msu.edu/share/proxy/alfresco/api/node/content/workspace/SpacesStore/8e4a7857-347b-4603-9f64-bf2422ff5e7e/Simulating%20Accretion%20on%20Degenerate%20Matter%20to%20Model%20Surface.pdf|Presentation PDF]] | + | |
~~DISCUSSION|Comments~~ | ~~DISCUSSION|Comments~~ |