Simon May

Simon May portrait
Perimeter Institute for Theoretical Physics
Areas of research:
  • Dome, T., May, S., Laguë, A., Marsh, D. J. E., Johnston, S., Bose, S., . . . Fialkov, A. (2024). Improved Halo Model Calibrations for Mixed Dark Matter Models of Ultralight Axions. arxiv:2409.11469v1
  • Krolewski, A., May, S., Smith, K., & Hopkins, H. (2024). No evidence for parity violation in BOSS. Journal of Cosmology and Astroparticle Physics, 2024(08), 044. doi:10.1088/1475-7516/2024/08/044
  • Krolewski, A., May, S., Smith, K., & Hopkins, H. (2024). No evidence for parity violation in BOSS. arxiv:2407.03397v1
  • Luu, H. N., Mocz, P., Vogelsberger, M., May, S., Borrow, J., Tye, S. -H. H., & Broadhurst, T. (2023). Nested solitons in two-field fuzzy dark matter. Monthly Notices of the Royal Astronomical Society, 527(2), 4162-4172. doi:10.1093/mnras/stad3482
  • May, S., & Springel, V. (2023). The halo mass function and filaments in full cosmological simulations with fuzzy dark matter. Monthly Notices of the Royal Astronomical Society, 524(3), 4256-4274. doi:10.1093/mnras/stad2031
  • Powell, D. M., Vegetti, S., McKean, J. P., White, S. D. M., Ferreira, E. G. M., May, S., & Spingola, C. (2023). A lensed radio jet at milli-arcsecond resolution – II. Constraints on fuzzy dark matter from an extended gravitational arc. Monthly Notices of the Royal Astronomical Society: Letters, 524(1), l84-l88. doi:10.1093/mnrasl/slad074
  • Chan, H. Y. J., Ferreira, E. G. M., May, S., Hayashi, K., & Chiba, M. (2022). The diversity of core–halo structure in the fuzzy dark matter model. Monthly Notices of the Royal Astronomical Society, 511(1), 943-952. doi:10.1093/mnras/stac063
  • May, S., & Springel, V. (2021). Structure formation in large-volume cosmological simulations of fuzzy dark matter: impact of the non-linear dynamics. Monthly Notices of the Royal Astronomical Society, 506(2), 2603-2618. doi:10.1093/mnras/stab1764
  • May, S. (2021). minimal-lagrangians: Generating and studying dark matter model Lagrangians with just the particle content. Computer Physics Communications, 261, 107773. doi:10.1016/j.cpc.2020.107773
  • Cosmic filaments and fuzzy dark matter, What Matter(s) Around Galaxies 2024, 2024/06/19
  • Simulations of cosmic structure formation with fuzzy dark matter, Dark Matter 2023: From the Smallest to the Largest Scales, Instituto de Física de Cantabria, Santander, Spain, 2023/05/30
  • Session 2 - Simon May, POSTDOC WELCOME 2022, 2022/10/24, PIRSA:22100118
  • Simulations of cosmic structure formation with fuzzy dark matter - Simon May, Max Planck Institute of Astrophysics, Cosmology and Gravitation, 2022/02/01, PIRSA:22020050