Keagan Blanchette
Velocity-dependent J-factors for Milky Way dwarf spheroidal analogues in cosmological simulations
Blanchette, Keagan; Piccirillo, Erin; Bozorgnia, Nassim; Strigari, Louis E.; Fattahi, Azadeh; Frenk, Carlos S.; Navarro, Julio F.; Sawala, Till
Authors
Erin Piccirillo
Nassim Bozorgnia
Louis E. Strigari
Dr Azadeh Fattahi Savadjani azadeh.fattahi-savadjani@durham.ac.uk
Associate Professor
Professor Carlos Frenk c.s.frenk@durham.ac.uk
Professor
Julio F. Navarro
Till Sawala
Abstract
We study the impact of the dark matter velocity distribution modelling on signals from velocity-dependent dark matter annihilation in Milky Way dwarf spheroidal galaxies. Using the high resolution APOSTLE simulations, we identify analogues corresponding to Milky Way dwarf spheroidal galaxies, and from these directly determine the dark matter pair-wise relative velocity distribution, and compare to best-fitting Maxwell-Boltzmann distribution models. For three velocity-dependent annihilation models, p-wave, d-wave, and the Sommerfeld model, we quantify the errors introduced when using the Maxwell-Boltzmann parameterization. We extract a simple power-law relation between the maximum circular velocity of the dwarf spheroidal analogue and the peak speed of the Maxwell-Boltzmann distribution. We show that this relation can be used to accurately calculate the dark matter relative velocity distribution, and find that it allows us to estimate the dark matter annihilation signal without the need to directly calculate the relative velocity distribution for each galaxy. The scatter in the J-factors calculated from the analogues dominates the uncertainty obtained when compared to the J-factor as determined from the observational data for each dwarf spheroidal, with the largest scatter from d-wave models and the smallest from Sommerfeld models.
Citation
Blanchette, K., Piccirillo, E., Bozorgnia, N., Strigari, L. E., Fattahi, A., Frenk, C. S., …Sawala, T. (2023). Velocity-dependent J-factors for Milky Way dwarf spheroidal analogues in cosmological simulations. Journal of Cosmology and Astroparticle Physics, 2023(03), Article 021. https://doi.org/10.1088/1475-7516/2023/03/021
Journal Article Type | Article |
---|---|
Acceptance Date | Feb 9, 2023 |
Online Publication Date | Mar 8, 2023 |
Publication Date | 2023-03 |
Deposit Date | May 31, 2023 |
Publicly Available Date | Jun 2, 2023 |
Journal | Journal of Cosmology and Astroparticle Physics |
Publisher | IOP Publishing |
Peer Reviewed | Peer Reviewed |
Volume | 2023 |
Issue | 03 |
Article Number | 021 |
DOI | https://doi.org/10.1088/1475-7516/2023/03/021 |
Public URL | https://durham-repository.worktribe.com/output/1172265 |
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Copyright Statement
Published by IOP Publishing Ltd on behalf of Sissa Medialab. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
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