| dc.rights.license | CC-BY-NC-ND | |
| dc.contributor.advisor | Hinderer, T.P. | |
| dc.contributor.author | Imbens, Frank | |
| dc.date.accessioned | 2023-03-15T01:01:14Z | |
| dc.date.available | 2023-03-15T01:01:14Z | |
| dc.date.issued | 2023 | |
| dc.identifier.uri | https://studenttheses.uu.nl/handle/20.500.12932/43653 | |
| dc.description.sponsorship | Utrecht University | |
| dc.language.iso | EN | |
| dc.subject | Black holes and other compact objects are powerful tools to observationally test Einsteins field equations.
We explored the symplectic structure of the geodesics phase space of various solutions to Einsteins field
equations in a vaccuum, using the tools provided by Riemannian geometry. The symplectic structure
gives deeper insight into the geodesics around, and especially close to the black hole. This becomes a very
difficult analytical problem for more complex spacetimes, and so we turned to nu | |
| dc.title | Black holes and Symplectic Geometry | |
| dc.type.content | Master Thesis | |
| dc.rights.accessrights | Open Access | |
| dc.subject.keywords | black holes; symplectic geometry | |
| dc.subject.courseuu | Theoretical Physics | |
| dc.thesis.id | 14936 | |
