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20242026
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astro-ph.GA2026

Learning the Universe at High Redshifts: Impact of Accretion Modeling on Early Black Hole Growth

Jonathan Kho, Aklant K. Bhowmick, Rainer Weinberger +8

JWST discoveries of the earliest () supermassive black holes (BHs, ) challenge the BH seeding and accretion models of most cosmol…

astro-ph.GA2026

Learning the Universe with PRFM-vol: Introducing a new subgrid model for star formation in cosmological simulations

Jan D. Burger, Volker Springel, Eve C. Ostriker +7

We introduce PRFM-vol, a new subgrid model for star formation in cosmological simulations that aims to increase the physical realism of cosmological simulations by leveraging resul…

astro-ph.GA2026

Blue Monsters and Dusty Descendants: Reconciling UV and IR Emission from Galaxies from z=7, up to z= 14

Laura Sommovigo, Lachlan Lancaster, Shyam H. Menon +3

Recent JWST observations reveal massive, UV-bright galaxies at with little apparent dust attenuation, whereas ALMA detections at show similarly massive system…

astro-ph.GA2026

Chemical Signatures of Population III Stars in Damped Lyman- Absorption Systems at

Eli Visbal, Greg L. Bryan, Zoltan Haiman

Recently, Sodini et al. (2024) presented a sample of OI damped Lyman- absorption system (DLA) analogs at that contain possible chemical signatures of Population III (P…

astro-ph.GA2025

LAP1-B is the First Observed System Consistent with Theoretical Predictions for Population III Stars

Eli Visbal, Ryan Hazlett, Greg L. Bryan

Recently, Nakajima et al. (2025) presented James Webb Space Telescope observations of the Population III (Pop III) candidate LAP1-B, which is gravitationally lensed by gala…

astro-ph.GA2025

Modeling Cosmic Rays at AGN Jet-Driven Shock Fronts

Kung-Yi Su, Greg L. Bryan, Philip F. Hopkins +4

Active Galactic Nuclei (AGN) feedback is a key physical mechanism proposed to regulate star formation, primarily in massive galaxies. In particular, cosmic rays associated with AGN…