The Effects of Active Galactic Nuclei Feedback on the Lyα Forest Flux Power Spectrum

The Effects of Active Galactic Nuclei Feedback on the Lyα Forest Flux Power Spectrum

We study the effects of active galactic nuclei (AGN) feedback on the Ly α forest 1D flux power spectrum (P1D). Using the Simba cosmological-hydrodynamic simulations, we examine the impact that adding different AGN feedback modes has on the predicted P1D. We find that, for Simba , the impact of AGN f...

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Bibliographic Details
Main Authors: Megan Taylor Tillman, Blakesley Burkhart, Stephanie Tonnesen, Simeon Bird, Greg L. Bryan
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Cosmology
Extragalactic astronomy
Intergalactic medium
Lyα forest
Active galactic nuclei
Supermassive black holes
Online Access:https://doi.org/10.3847/1538-4357/ada5f7
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Summary:We study the effects of active galactic nuclei (AGN) feedback on the Ly α forest 1D flux power spectrum (P1D). Using the Simba cosmological-hydrodynamic simulations, we examine the impact that adding different AGN feedback modes has on the predicted P1D. We find that, for Simba , the impact of AGN feedback is most dramatic at lower redshifts ( z  < 1) and that AGN jet feedback plays the most significant role in altering the P1D. The effects of AGN feedback can be seen across a large range of wavenumbers (1.5 × 10 ^−3  <  k  < 10 ^−1 s km ^−1 ) changing the ionization state of hydrogen in the IGM through heating. AGN feedback can also alter the thermal evolution of the IGM and thermally broaden individual Ly α absorbers. For the Simba model, these effects become observable at z  ≲ 1.0. At higher redshifts ( z  > 2.0), AGN feedback has a 2% effect on the P1D for k  < 5 × 10 ^−2 s km ^−1 and an 8% effect for k  > 5 × 10 ^−2 s km ^−1 . We show that the small-scale effect is reduced when normalizing the simulation to the observed mean flux. On large scales, the effect of AGN feedback appears via a change in the IGM temperature and is thus unlikely to bias cosmological parameters. The strong AGN jets in the Simba simulation can reproduce the z  > 2 Ly α forest. We stress that analyses comparing different AGN feedback models to future higher precision data will be necessary to determine the full extent of this effect.
ISSN:1538-4357

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