Please use this identifier to cite or link to this item:
http://hdl.handle.net/11375/23984
Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.advisor | Wadsley, James | - |
dc.contributor.advisor | Couchman, Hugh | - |
dc.contributor.author | Mudway, Thomas | - |
dc.date.accessioned | 2019-03-08T20:57:51Z | - |
dc.date.available | 2019-03-08T20:57:51Z | - |
dc.date.issued | 2018 | - |
dc.identifier.uri | http://hdl.handle.net/11375/23984 | - |
dc.description.abstract | We describe the implementation and testing of the TREVR (Tree-based REVerse Ray-tracing) radiative transfer algorithm in the ChaNGa (Charm N-body Gravity solver) code. We calculated the optimal values for the source walk opening angle and ray trace walk refinement parameter of θ = 0.5 and τ = 0.01 respectively. We then studied the effects of the merging of sources on the accuracy of the calculated flux in absorbing regions, noting a systematic negative error and an angular dependence across all optical depths. We dubbed this the “Complex Sources Problem” and provide suggestions to mitigate its effects | en_US |
dc.language.iso | en | en_US |
dc.subject | Physics | en_US |
dc.subject | Astrophysics | en_US |
dc.subject | Radiation | en_US |
dc.subject | Radiative Transfer | en_US |
dc.title | The Efficient Simulation of Complex Radiation Sources | en_US |
dc.type | Thesis | en_US |
dc.contributor.department | Mathematics and Statistics | en_US |
dc.description.degreetype | Thesis | en_US |
dc.description.degree | Master of Science (MSc) | en_US |
Appears in Collections: | Open Access Dissertations and Theses |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
Mudway_Thomas_W_FinalSubmission2018Sept_CSE.pdf | 2.47 MB | Adobe PDF | View/Open |
Items in MacSphere are protected by copyright, with all rights reserved, unless otherwise indicated.