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Seeds Don't Sink: Even Massive Black Hole "Seeds" Cannot Migrate to Galaxy Centers Efficiently

, , , , , and . (2021)cite arxiv:2101.02727Comment: submitted to MNRAS, comments welcomed.

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Local positive feedback in the overall negative: the impact of quasar winds on star formation in the FIRE cosmological simulations, , , , , , , , , and 3 other author(s). (2023)cite arxiv:2301.01784Comment: 17 pages, 12 figures. Accepted for publication in MNRAS.Seeds Don't Sink: Even Massive Black Hole "Seeds" Cannot Migrate to Galaxy Centers Efficiently, , , , , and . (2021)cite arxiv:2101.02727Comment: submitted to MNRAS, comments welcomed.Breaking baryon-cosmology degeneracy with the electron density power spectrum, , , , , , , , , and 1 other author(s). (2022)cite arxiv:2201.04142Comment: 31 pages, 10 figures, to be submitted to JCAP.Reionization with Simba: How much does astrophysics matter in modeling cosmic reionization?, , , , , , , and . (2021)cite arxiv:2109.03840Comment: 13 pages, 7figures, submitted to ApJ.The Origin and Evolution of Lyman-alpha Blobs in Cosmological Galaxy Formation Simulations, , , , , , , , , and . (2020)cite arxiv:2004.08397Comment: Submitted to ApJ; comments welcome. 23 pages, 21 figures.Percent-level constraints on baryonic feedback with spectral distortion measurements, , , , , , , , , and . (2022)cite arxiv:2201.01663Comment: 10+5 pages, 7 figures.Weighing the Milky Way and Andromeda with Artificial Intelligence, , , , , , , , and . (2021)cite arxiv:2111.14874Comment: 2 figures, 2 tables, 7 pages. Code publicly available at https://github.com/PabloVD/HaloGraphNet.The black hole population in low-mass galaxies in large-scale cosmological simulations, , , , , , , , , and 1 other author(s). (2022)cite arxiv:2201.09888Comment: Submitted to MNRAS, 21 pages, 11 figures, 1 table.Exploring supermassive black hole physics and galaxy quenching across halo mass in FIRE cosmological zoom simulations, , , , , , , , , and . (2022)cite arxiv:2203.06201Comment: 18 pages, 9 figures. Submitted to MNRAS, comments welcome.The SZ flux-mass (Y-M) relation at low halo masses: improvements with symbolic regression and strong constraints on baryonic feedback., , , , , , , , , and 1 other author(s). CoRR, (2022)