Fundamental fields, General Relativity and black holes

Lead Research Organisation: University of Sheffield
Department Name: Mathematics and Statistics

Abstract

In the first year, the project concerns the scattering, absorption and emission of an electromagnetic field by a rotating (Kerr) black hole. The student will use the Debye/Hertz potential approach of Cohen & Kegeles (1974), to reconstruct the Faraday tensor on a Kerr black hole background by acting on a single complex scalar quantity with differential operators. The complex scalar is governed by a second-order PDE that is separable. By constructing a sum over the modes, the student will examine aspects such as planar wave scattering (via scattering cross sections); quasi-normal modes and Regge pole spectra; and electromagnetic self-force.

Publications

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Macedo C (2018) Spectral lines of extreme compact objects in Physical Review D

Studentship Projects

Project Reference Relationship Related To Start End Student Name
EP/N509735/1 01/10/2016 30/09/2021
1798678 Studentship EP/N509735/1 01/10/2016 31/03/2020 Thomas Stratton
 
Description We have developed the theory of scattering by compact bodies. More specifically, we have examined scattering of waves by compact stars, such as a neutron star.
The waves correspond to perturbations (disturbances) of the gravitational field (gravitational waves) or the electromagnetic field (light).
We have discovered that one might expect to see a diffraction phenomenan in scattering by compact bodies, known as rainbow scattering. This is analogous to the everday atmospheric effect. There is an intense `bow' and chromatic seperation (of frequencies). There are additional effects associated with the helicity or spin of the field.
Scattering by black holes has been studied extensively and we have compared and constrasted with these results.
We have developed compex angular momentum techniques used in classical and nuclear scattering studies.
Also, in collaborations we have investigated scattering and absorption by so called black hole `mimickers'. This is part of the ongoing effort to distinguish black holes from possible alternatives.
Exploitation Route We think our findings could be tested by analogue systems such as bathtub experiments. For example, there is the group at Nottingham University led by Dr Silke Weinfurtner who construct black hole analogue experiments (https://www.gravitylaboratory.com/) who we have had discussions with. This could be relatively easy to implement and possibly take to a wider audience including school children. It would be an inspiring sight for budding scientists to "see" gravitational waves scattered by a neutron star.
Sectors Education

URL https://journals.aps.org/prd/abstract/10.1103/PhysRevD.95.124055
 
Description University of Sheffield and Federal University of Para 
Organisation Federal University of ParĂ¡
Country Brazil 
Sector Academic/University 
PI Contribution Myself and Dr Sam Dolan participated in a collaboration with two researchers from the Federal University of Pará (UFPA). We contributed to a project researching the absorptive properties of exotic compact objects. This resulted in the output of a paper together entitled: "Spectral lines of extreme compact objects" We are still working on some research into scattering by compact bodies with researchers at UFPA.
Collaborator Contribution Our partners led the research project into scattering and absorption by exotic compact objects, partly inspired by our previous work.
Impact Article in Physical Review D DOI: https://doi.org/10.1103/PhysRevD.98.104034
Start Year 2018