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91̽»¨
Black Hole

Lensing of space time around a black hole. At 91̽»¨ we study black holes observationally and theoretically on all size and time scales - it is some of our core work.

Credit: ALAIN RIAZUELO, IAP/UPMC/CNRS. CLICK HERE TO VIEW MORE IMAGES.

Dr Deaglan Bartlett

Eric and Wendy Schmidt AI in Science Postdoctoral Fellow

Research theme

  • Astronomy and astrophysics
  • Particle astrophysics & cosmology

Sub department

  • Astrophysics

Research groups

  • Beecroft Institute for Particle Astrophysics and Cosmology
  • Cosmology
  • Galaxy formation and evolution
deaglan.bartlett@physics.ox.ac.uk
Denys Wilkinson Building, room 532G
  • About
  • Publications

CHARM: Creating Halos with Auto-Regressive Multi-stage networks

ArXiv 2409.09124 (2024)

Authors:

Shivam Pandey, Chirag Modi, Benjamin D Wandelt, Deaglan J Bartlett, Adrian E Bayer, Greg L Bryan, Matthew Ho, Guilhem Lavaux, T Lucas Makinen, Francisco Villaescusa-Navarro

COmoving Computer Acceleration (COCA): $N$-body simulations in an emulated frame of reference

ArXiv 2409.02154 (2024)

Authors:

Deaglan J Bartlett, Marco Chiarenza, Ludvig Doeser, Florent Leclercq

Statistical Patterns in the Equations of Physics and the Emergence of a Meta-Law of Nature

(2024)

Authors:

Andrei Constantin, Deaglan Bartlett, Harry Desmond, Pedro G Ferreira

LtU-ILI: An All-in-One Framework for Implicit Inference in Astrophysics and Cosmology

The Open Journal of Astrophysics Maynooth University 7 (2024)

Authors:

Matthew Ho, Deaglan J Bartlett, Nicolas Chartier, Carolina Cuesta-Lazaro, Simon Ding, Axel Lapel, Pablo Lemos, Christopher C Lovell, T Lucas Makinen, Chirag Modi, Viraj Pandya, Shivam Pandey, Lucia A Perez, Benjamin Wandelt, Greg L Bryan

Abstract:

<jats:p>This paper presents the Learning the Universe Implicit Likelihood Inference (LtU-ILI) pipeline, a codebase for rapid, user-friendly, and cutting-edge machine learning (ML) inference in astrophysics and cosmology. The pipeline includes software for implementing various neural architectures, training schema, priors, and density estimators in a manner easily adaptable to any research workflow. It includes comprehensive validation metrics to assess posterior estimate coverage, enhancing the reliability of inferred results. Additionally, the pipeline is easily parallelizable, designed for efficient exploration of modeling hyperparameters. To demonstrate its capabilities, we present real applications across a range of astrophysics and cosmology problems, such as: estimating galaxy cluster masses from X-ray photometry; inferring cosmology from matter power spectra and halo point clouds; characterising progenitors in gravitational wave signals; capturing physical dust parameters from galaxy colors and luminosities; and establishing properties of semi-analytic models of galaxy formation. We also include exhaustive benchmarking and comparisons of all implemented methods as well as discussions about the challenges and pitfalls of ML inference in astronomical sciences. All code and examples are made publicly available at https://github.com/maho3/ltu-ili.</jats:p>

A precise symbolic emulator of the linear matter power spectrum

Astronomy and Astrophysics EDP Sciences 686 (2024) a209

Authors:

Deaglan J Bartlett, Lukas Kammerer, Gabriel Kronberger, Harry Desmond, Pedro G Ferreira, Benjamin D Wandelt, Bogdan Burlacu, David Alonso, Matteo Zennaro

Abstract:

Context. Computing the matter power spectrum, P(k), as a function of cosmological parameters can be prohibitively slow in cosmological analyses, hence emulating this calculation is desirable. Previous analytic approximations are insufficiently accurate for modern applications, so black-box, uninterpretable emulators are often used.

Aims. We aim to construct an efficient, differentiable, interpretable, symbolic emulator for the redshift zero linear matter power spectrum which achieves sub-percent level accuracy. We also wish to obtain a simple analytic expression to convert As to σ8 given the other cosmological parameters.

Methods. We utilise an efficient genetic programming based symbolic regression framework to explore the space of potential mathematical expressions which can approximate the power spectrum and σ8. We learn the ratio between an existing low-accuracy fitting function for P(k) and that obtained by solving the Boltzmann equations and thus still incorporate the physics which motivated this earlier approximation.

Results. We obtain an analytic approximation to the linear power spectrum with a root mean squared fractional error of 0.2% between k = 9 &³Ù¾±³¾±ð²õ; 10−3 &³¾¾±²Ô³Ü²õ; 9 h M±è³¦−1 and across a wide range of cosmological parameters, and we provide physical interpretations for various terms in the expression. Our analytic approximation is 950 times faster to evaluate than CAMB and 36 times faster than the neural network based matter power spectrum emulator BACCO. We also provide a simple analytic approximation for σ8 with a similar accuracy, with a root mean squared fractional error of just 0.1% when evaluated across the same range of cosmologies. This function is easily invertible to obtain As as a function of σ8 and the other cosmological parameters, if preferred.

Conclusions. It is possible to obtain symbolic approximations to a seemingly complex function at a precision required for current and future cosmological analyses without resorting to deep-learning techniques, thus avoiding their black-box nature and large number of parameters. Our emulator will be usable long after the codes on which numerical approximations are built become outdated.

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