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Statistics of thermal gas pressure as a probe of cosmology and galaxy formation

Chen, Ziyang; Jamieson, Drew; Komatsu, Eiichiro; Bose, Sownak; Dolag, Klaus; Hadzhiyska, Boryana; Hernández-Aguayo, César; Hernquist, Lars; Kannan, Rahul; Pakmor, Rüdiger; Springel, Volker

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Authors

Ziyang Chen

Drew Jamieson

Eiichiro Komatsu

Klaus Dolag

Boryana Hadzhiyska

César Hernández-Aguayo

Lars Hernquist

Rahul Kannan

Rüdiger Pakmor

Volker Springel



Abstract

The statistics of thermal gas pressure are a new and promising probe of cosmology and astrophysics. The large-scale cross-correlation between galaxies and the thermal Sunyaev-Zeldovich effect gives the bias-weighted mean electron pressure, ⟨bhPe⟩. In this paper, we show that ⟨bhPe⟩ is sensitive to the amplitude of fluctuations in matter density, for example ⟨bhPe⟩∝(σ8Ωm0.81h0.67)3.14 at redshift z=0. We find that at z<0.5 the observed ⟨bhPe⟩ is smaller than that predicted by the state-of-the-art hydrodynamical simulations of galaxy formation, MillenniumTNG, by a factor of 0.93. This can be explained by a lower value of σ8 and Ωm, similar to the so-called “S8 tension” seen in the gravitational lensing effect, although the influence of astrophysics cannot be completely excluded. The difference between and MillenniumTNG at z<2 is small, indicating that the difference in the galaxy formation models used by these simulations has little impact on ⟨bhPe⟩ at this redshift range. At higher z, we find that both simulations are in a modest tension with the existing upper bounds on ⟨bhPe⟩. We also find a significant difference between these simulations there, which we attribute to a larger sensitivity to the galaxy formation models in the high redshift regime. Therefore, more precise measurements of ⟨bhPe⟩ at all redshifts will provide a new test of our understanding of cosmology and galaxy formation. Published by the American Physical Society 2024

Citation

Chen, Z., Jamieson, D., Komatsu, E., Bose, S., Dolag, K., Hadzhiyska, B., Hernández-Aguayo, C., Hernquist, L., Kannan, R., Pakmor, R., & Springel, V. (2024). Statistics of thermal gas pressure as a probe of cosmology and galaxy formation. Physical Review D, 109(6), Article 063513. https://doi.org/10.1103/physrevd.109.063513

Journal Article Type Article
Acceptance Date Feb 2, 2024
Online Publication Date Mar 8, 2024
Publication Date Mar 8, 2024
Deposit Date May 16, 2024
Publicly Available Date May 16, 2024
Journal Physical Review D
Print ISSN 2470-0010
Electronic ISSN 2470-0029
Publisher American Physical Society
Peer Reviewed Peer Reviewed
Volume 109
Issue 6
Article Number 063513
DOI https://doi.org/10.1103/physrevd.109.063513
Public URL https://durham-repository.worktribe.com/output/2442642

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http://creativecommons.org/licenses/by/4.0/

Publisher Licence URL
http://creativecommons.org/licenses/by/4.0/

Copyright Statement
Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Open access publication funded by the Max Planck Society.






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