English

Lecture Notes: WISPs in gamma-ray astrophysics

High Energy Astrophysical Phenomena 2025-05-20 v1 High Energy Physics - Phenomenology

Abstract

These lecture notes provide an overview of high-energy astrophysical processes involving axions, axion-like particles (ALPs), and other weakly interacting slim particles (WISPs) focusing on their potential observational signatures in astrophysical environments. After introducing key concepts in high-energy astrophysics, we present the fundamental properties of WISPs, emphasizing their phenomenological implications. Particular attention is given to ALP-photon conversion in strong magnetic fields and the possible decay signatures of ALPs in sources such as active galactic nuclei, galaxy clusters, and cosmic-ray accelerators. These effects can lead to distinctive modifications in astrophysical spectra, spatial distributions, and polarization patterns, providing unique probes of physics beyond the Standard Model. We discuss their role in dark matter scenarios and their potential impact on high-energy observations. The lecture series is supplemented by hands-on tutorials, including exercises on axion electrodynamics and an analysis of gamma-ray data from NGC 1275 to search for ALP-photon conversion signatures.

Keywords

Cite

@article{arxiv.2505.12905,
  title  = {Lecture Notes: WISPs in gamma-ray astrophysics},
  author = {Francesca Calore and Christopher Eckner},
  journal= {arXiv preprint arXiv:2505.12905},
  year   = {2025}
}

Comments

Lectures Notes of the 2nd Training School of the COST Action COSMIC WISPers (CA21106). To be published in Proceedings of Science. Comments are welcome!

R2 v1 2026-07-01T02:21:21.442Z