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Thesis

Reflections upon black hole accretion discs: advanced x-ray modelling and novel timing methods

Abstract:

The regions close to black holes (BHs) have the most extreme gravitational fields; therefore we are able to probe Einstein’s theory of gravity by studying how matter accretes onto these objects. The best data we have of black hole accretion comes from X-ray binaries (XRBs) within the Milky Way, which shine brightly in X-rays. The accretion discs are very small and therefore are unresolved in observations, so we have to study the properties of the X-ray point source in great detail to und...

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Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Oxford college:
St Hugh's College
Role:
Author
ORCID:
0000-0002-9633-9193

Contributors

Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Role:
Supervisor
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Role:
Supervisor
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Role:
Examiner
Role:
Examiner
More from this funder
Funder identifier:
http://dx.doi.org/10.13039/501100000288
Grant:
RGF\R1\180077
Type of award:
DPhil
Level of award:
Doctoral
Awarding institution:
University of Oxford

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