High-redshift Galaxy Formation with Self-consistently Modeled Stars and Massive Black Holes: Stellar Feedback and Quasar Growth

Kim, Ji-hoon; Wise, John H.; Abel, Tom; Jo, Yongseok; Primack, Joel R.; Hopkins, Philip F.

doi:10.3847/1538-4357/ab510b

Title: High-redshift Galaxy Formation with Self-consistently Modeled Stars and Massive Black Holes: Stellar Feedback and Quasar Growth

Journal Article · 15 December 2019 · The Astrophysical Journal (Online)

DOI: https://doi.org/10.3847/1538-4357/ab510b · OSTI ID:1604568

^[1];

^[2]; Abel, Tom ^[3]; Jo, Yongseok ^[1];

^[4];

^[5]

Seoul National Univ., Seoul (Korea). Center for Theoretical Physics, Dept. of Physics and Astronomy
Georgia Inst. of Technology, Atlanta, GA (United States)
SLAC National Accelerator Lab., Menlo Park, CA (United States); Stanford Univ., CA (United States)
Univ. of California, Santa Cruz, CA (United States)
California Institute of Technology (CalTech), Pasadena, CA (United States)

As computational resolution of modern cosmological simulations come closer to resolving individual star-forming clumps in a galaxy, the need for "resolution-appropriate" physics for a galaxy-scale simulation has never been greater. To this end, we introduce a self-consistent numerical framework that includes explicit treatments of feedback from star-forming molecular clouds (SFMCs) and massive black holes (MBHs). In addition to the thermal supernovae feedback from SFMC particles, photoionizing radiation from both SFMCs and MBHs is tracked through full three-dimensional ray tracing. A mechanical feedback channel from MBHs is also considered. Using our framework, we perform a state-of-the-art cosmological simulation of a quasar-host galaxy at z ~ 7.5 for ~25 Myr with all relevant galactic components, such as dark matter, gas, SFMCs, and an embedded MBH seed of ≳ 10⁶ M_⊙. We find that feedback from SFMCs and an accreting MBH suppresses runaway star formation locally in the galactic core region. Newly included radiation feedback from SFMCs, combined with feedback from the MBH, helps the MBH grow faster by retaining gas that eventually accretes on to the MBH. Our experiment demonstrates that previously undiscussed types of interplay between gas, SFMCs, and a MBH may hold important clues about the growth and feedback of quasars and their host galaxies in the high-redshift universe.

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Research Organization:: SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)

Sponsoring Organization:: USDOE Office of Science (SC)

Grant/Contract Number:: AC02-76SF00515

OSTI ID:: 1604568

Journal Information:: The Astrophysical Journal (Online), Journal Name: The Astrophysical Journal (Online) Journal Issue: 2 Vol. 887; ISSN 1538-4357

Publisher:: Institute of Physics (IOP)Copyright Statement

Country of Publication:: United States

Language:: English

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Galaxy Formation with Self-Consistently Modeled Stars and Massive Black Holes. I: Feedback-Regulated Star Formation and Black Hole Growth

Journal Article · 2011 · Astrophys.J.738:54,2011 · OSTI ID:1028672

Kim, Ji-hoon; Wise, John H; Alvarez, Marcelo A; +1 more

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79 ASTRONOMY AND ASTROPHYSICS
galaxies: formation
galaxies: evolution
galaxies: kinematics and dynamics
galaxies: star formation
galaxies: nuclei
ISM: structure
stars: formation
quasars: supermassive black holes
methods: numerical

Title: High-redshift Galaxy Formation with Self-consistently Modeled Stars and Massive Black Holes: Stellar Feedback and Quasar Growth

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