July 28, 2025 to August 1, 2025
Perimeter Institute for Theoretical Physics
America/Toronto timezone

Probing baryonic feedback and cosmology with patchy screening in the FLAMINGO Simulations.

Jul 28, 2025, 4:10 p.m.
10m
PI/1-100 - Theatre (Perimeter Institute for Theoretical Physics)

PI/1-100 - Theatre

Perimeter Institute for Theoretical Physics

190
Contributed Talk

Speaker

Mr Jonah Conley (Astrophysics Research Institute - Liverpool John Moores Universtiy)

Description

Understanding the impact of baryonic feedback across different cosmic environments is crucial for accurate interpretation of large-scale structure in Stage-IV cosmological surveys. Hydrodynamical simulations offer a valuable tool for capturing how gas is redistributed by energetic processes, such as AGN feedback, and for predicting how this redistribution alters observable tracers of structure formation. Traditionally, feedback models have been constrained through X-ray and Sunyaev-Zel’dovich measurements of galaxy groups and clusters. However, new observational tracers are emerging that open up alternative windows into the baryonic content of the cosmic web.

One such tracer is the patchy screening effect, a subtle CMB anisotropy arising from excess Thomson scattering along the line of sight to groups/clusters due to their higher electron optical depths. This effect is sensitive to the diffuse baryons in the outer regions of the gas profile of the halo, tracing the structure of the cosmic web. It is complementary to the kinetic Sunyaev-Zel’dovich effect, as it probes optical depth without dependence on velocity.

In this talk, we present predictions of the patchy screening signal from the FLAMINGO suite of large-volume cosmological hydrodynamical simulations. By generating mock patchy screened CMB maps and cross-correlating them with simulated galaxy populations, we explore how feedback and cosmology shape the optical depth field. Our goal is to assess the sensitivity of this signal to the cosmology and baryonic physics, and to evaluate its potential as a new probe of the gas distribution within the anisotropic structure of the cosmic web.

Primary Theme Small to large scales
Secondary Theme Past feedback processes to present-day observations
Presenter's Name Jonah T Conley
Presenter's Email Address [email protected]
Keywords patchy screening, weak lensing, simulations, feedback, CMB
Recording Permission YES
Virtual Audience Permission YES
Photography Permission YES
If your talk is not accepted for a contributed talk, would you be interested in presenting a fireslide/lightning talk? Yes
If your fireslide/lighting talk is not accepted, would you be interested in presenting a poster? Yes

Author

Mr Jonah Conley (Astrophysics Research Institute - Liverpool John Moores Universtiy)

Presentation materials

There are no materials yet.

External references