Galactic Center Excess in a New Light: Disentangling the γ-Ray Sky with Bayesian Graph Convolutional Neural Networks

Florian List, Nicholas L. Rodd, Geraint F. Lewis, and Ishaan Bhat
Phys. Rev. Lett. 125, 241102 – Published 10 December 2020
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Abstract

A fundamental question regarding the Galactic Center excess (GCE) is whether the underlying structure is pointlike or smooth, often framed in terms of a millisecond pulsar or annihilating dark matter (DM) origin for the emission. We show that Bayesian neural networks (NNs) have the potential to resolve this debate. In simulated data, the method is able to predict the flux fractions from inner Galaxy emission components to on average 0.5%. When applied to the Fermi photon-count map, the NN identifies a smooth GCE in the data, suggestive of the presence of DM, with the estimates for the background templates being consistent with existing results.

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  • Received 29 June 2020
  • Revised 24 September 2020
  • Accepted 26 October 2020

DOI:https://doi.org/10.1103/PhysRevLett.125.241102

© 2020 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & Astrophysics

Authors & Affiliations

Florian List1,*, Nicholas L. Rodd2,3, Geraint F. Lewis1, and Ishaan Bhat4

  • 1Sydney Institute for Astronomy, School of Physics, A28, The University of Sydney, New South Wales 2006, Australia
  • 2Berkeley Center for Theoretical Physics, University of California, Berkeley, California 94720, USA
  • 3Theoretical Physics Group, Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA
  • 4UMC Utrecht, Image Sciences Institute, 3508 GA Utrecht, The Netherlands

  • *florian.list@sydney.edu.au

See Also

Extracting the Galactic Center excess’ source-count distribution with neural nets

Florian List, Nicholas L. Rodd, and Geraint F. Lewis
Phys. Rev. D 104, 123022 (2021)

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Vol. 125, Iss. 24 — 11 December 2020

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