51ΑΤΖζΘλΏΪ

Skip to main content
Department Of Physics text logo
  • Research
    • Our research
    • Our research groups
    • Our research in action
    • Research funding support
    • Summer internships for undergraduates
  • 51ΑΤΖζΘλΏΪ
    • Undergraduates
    • Postgraduates
  • Engage
    • For alumni
    • For business
    • For schools
    • For the public
  • Support
Menu
Black Hole

Lensing of space time around a black hole. At Oxford 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

Optimal Inflationary Potentials

(2023)

Authors:

TomΓ‘s Sousa, Deaglan J Bartlett, Harry Desmond, Pedro G Ferreira

Marginalised Normal Regression: Unbiased curve fitting in the presence of x-errors

ArXiv 2309.00948 (2023)

Authors:

Deaglan Bartlett, Harry Desmond

Constraints on dark matter and astrophysics from tomographic $\gamma$-ray cross-correlations

(2023)

Authors:

Anya Paopiamsap, David Alonso, Deaglan J Bartlett, Maciej Bilicki

Priors for symbolic regression

GECCO '23 Companion: Proceedings of the Companion Conference on Genetic and Evolutionary Computation Association for Computing Machinery (2023) 2402-2411

Authors:

Deaglan Bartlett, Harry Desmond, Pedro Ferreira

Abstract:

When choosing between competing symbolic models for a data set, a human will naturally prefer the β€œsimpler” expression or the one which more closely resembles equations previously seen in a similar context. This suggests a non-uniform prior on functions, which is, however, rarely considered within a symbolic regression (SR) framework. In this paper we develop methods to incorporate detailed prior information on both functions and their parameters into SR. Our prior on the structure of a function is based on a ngram language model, which is sensitive to the arrangement of operators relative to one another in addition to the frequency of occurrence of each operator. We also develop a formalism based on the Fractional Bayes Factor to treat numerical parameter priors in such a way that models may be fairly compared though the Bayesian evidence, and explicitly compare Bayesian, Minimum Description Length and heuristic methods for model selection. We demonstrate the performance of our priors relative to literature standards on benchmarks and a real-world dataset from the field of cosmology.

Modeling and Testing Screening Mechanisms in the Laboratory and in Space

Universe MDPI 9:7 (2023) ARTN 340

Authors:

Valeri Vardanyan, Deaglan J Bartlett

Abstract:

<jats:p>The non-linear dynamics of scalar fields coupled to matter and gravity can lead to remarkable density-dependent screening effects. In this short review, we present the main classes of screening mechanisms, and discuss their tests in laboratory and astrophysical systems. We particularly focused on reviewing numerical and technical aspects involved in modeling the non-linear dynamics of screening and on tests using laboratory experiments and astrophysical systems, such as stars, galaxies, and dark matter halos.</jats:p>

Pagination

  • First page First
  • Previous page Prev
  • …
  • Page 4
  • Page 5
  • Page 6
  • Page 7
  • Current page 8
  • Page 9
  • Page 10
  • Page 11
  • Page 12
  • Next page Next
  • Last page Last

Footer Menu

  • Contact us
  • Giving to the Dept of Physics
  • Work with us
  • Media

User account menu

  • Log in

Follow us

FIND US

Clarendon Laboratory,

Parks Road,

Oxford,

OX1 3PU

CONTACT US

Tel: +44(0)1865272200

Department Of Physics text logo

Β© University of Oxford - Department of Physics

Cookies | Privacy policy | Accessibility statement

  • Home
  • Research
  • 51ΑΤΖζΘλΏΪ
  • Engage
  • Our people
  • News & Comment
  • Events
  • Our facilities & services
  • 51ΑΤΖζΘλΏΪ
  • Giving to Physics