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The MillenniumTNG Project: The hydrodynamical full physics simulation and a first look at its galaxy clusters

, , , , , , , , , , , , , , and . (2022)cite arxiv:2210.10060Comment: 17 pages, 14 figures, submitted to MNRAS, comments welcome.

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ETHOS -- an effective theory of structure formation: Predictions for the high-redshift Universe -- abundance of galaxies and reionization, , , , , , , , and . (2017)cite arxiv:1711.10497Comment: 15 pages, 8 figures, to be submitted to MNRAS. Please contact lovell@hi.is with any comments.Cosmic rays and non-thermal emission in simulated galaxies: III. probing cosmic ray calorimetry with radio spectra and the FIR-radio correlation, , and . (2021)cite arxiv:2105.12134Comment: 24 pages, 15 figures, submitted to MNRAS, comments are welcome.Importance of Resolving the Spectral Support of Beam-plasma Instabilities in Simulations, , , , , and . The Astrophysical Journal, 848 (2): 81 (October 2017)Turbulence and Particle Acceleration in Giant Radio Halos: the Origin of Seed Electrons, , and . (Mar 26, 2015)The Linear Instability of Dilute Ultrarelativistic \$e^\pm\$ Pair Beams, , , , , , and . (Oct 6, 2016)Giant radio relics in galaxy clusters: reacceleration of fossil relativistic electrons?, , and . (Jan 23, 2013)A new cosmic ray-driven instability, , and . (2020)cite arxiv:2010.11197Comment: 16 pages, 13 figures, 2 tables, submitted to ApJ. Comments are welcome.Galactic winds driven by isotropic and anisotropic cosmic ray diffusion in disk galaxies, , , and . (2016)cite arxiv:1605.00643Comment: 6 pages, 5 figures, submitted to ApJL, comments welcome.The Lyman-alpha forest in a blazar-heated Universe, , , , and . (2011)cite arxiv:1107.3837Comment: 15 pages, 13 figures, submitted to MNRAS.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.