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Prompt cusps and the dark matter annihilation signal

, and . (2022)cite arxiv:2209.11237Comment: 19 pages, 10 figures; submitted.

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The host galaxies of active galactic nuclei, , , , , , , , , and 3 other author(s). Monthly Notices of the Royal Astronomical Society, 346 (4): 1055--1077 (2003)A Universal Density Profile from Hierarchical Clustering, , and . (1996)cite arxiv:astro-ph/9611107 Comment: typos in eqs A5 and A14 corrected. In press in the ApJ, Dec 1, 1997. Full PS file with figures can be obtained from http://penedes.as.arizona.edu/~jfn/preprints/dprof.ps.gz.The Origin of Disks and Spheroids in Simulated Galaxies, , , , , , , and . (2011)cite arxiv:1112.2220Comment: 11 pages, 8 figures. Submitted to MNRAS.Universality in the structure of dark matter haloes over twenty orders of magnitude in halo mass, , , , , , and . (2019)cite arxiv:1911.09720Comment: 35 pages, 8 figures, submitted.The MillenniumTNG Project: The hydrodynamical full physics simulation and a first look at its galaxy clusters, , , , , , , , , and 5 other author(s). (2022)cite arxiv:2210.10060Comment: 17 pages, 14 figures, submitted to MNRAS, comments welcome.Baryonic effects on the detectability of annihilation radiation from dark matter subhaloes around the Milky Way, and . (2020)cite arxiv:2012.07846Comment: submitted to MNRAS.Simulating the universe., , , , , , , and . PDP, page 234-239. IEEE Computer Society, (1997)Satellite abundances around bright isolated galaxies, and . (2012)cite arxiv:1203.0009 Comment: Submitted to MNRAS, 29 pages, 24 figures.Idealized models for galactic disk formation and evolution in 'realistic' LambdaCDM haloes, and . (2012)cite arxiv:1203.1190Comment: 24 pages, 20 figures, submitted to MNRAS.Local Group galaxies emerge from the dark, , , , , , , , , and 6 other author(s). (2014)cite arxiv:1412.2748Comment: 14 pages, 4 figures.