School of Mathematical Sciences

Machine Learning and Gravitational Wave Astronomy

Project description

I am looking to supervise PhD students interested in either gravitational physics / general relativity, or machine learning applied to scientific problems. Projects will be in the area of gravitational-wave (GW) astronomy, with focus on modeling and/or data analysis for gravitational systems such as black hole binaries. We aim to develop fast and accurate models and inference techniques, which we will then use to analyze real data from the LIGO-Virgo GW observatories and to make predictions for future detectors (LISA, ET). We can thereby precisely characterize sources, derive constraints on alternative gravity theories, and map out the GW universe.

To this end, my main research has been in developing probabilistic deep-learning techniques for Bayesian inference with GW data. This trains neural networks to analyze data in a fraction of the time of classical methods, with comparable levels of accuracy. Example projects could be either on the machine-learning side (developing faster and more accurate techniques, which could in principle be applied more broadly in science) or on applications (to future detectors, to new sources, and to populations of sources). On the theory side, I am interested primarily in modeling nonlinear effects using black hole perturbation theory, to study the behavior of black holes as they equilibrate following a merger, but I am happy to supervise interesting projects more broadly in general relativity.

Supervisor contacts

 

Related research centre or theme

Computational Statistics and Machine Learning

Gravity

 
 

 

 

Project published references

M. Dax, S. R. Green, J. Gair, J. H. Macke, A. Buonanno, and B. Schölkopf, “Real-Time Gravitational Wave Science with Neural Posterior Estimation”, Phys. Rev. Lett. 127, 241103 (2021), arXiv:2106.12594 [gr-qc].

L. Sberna, P. Bosch, W. E. East, S. R. Green, and L. Lehner, “Nonlinear effects in the black hole ringdown: Absorption-induced mode excitation”, Phys. Rev. D 105, 064046 (2022), arXiv:2112.11168 [gr-qc].

S. R. Green, S. Hollands, L. Sberna, V. Toomani, and P. Zimmerman, “Conserved currents for Kerr and orthogonality of quasinormal modes”, (2022), arXiv:2210.15935 [gr-qc].

More information

Full details of our Maths PhD

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School of Mathematical Sciences

The University of Nottingham
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Nottingham, NG7 2RD

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