A Novel Approach to Constraining Baryonic Feedback: Coherent Field-Level Inference of Lensing and Electron Pressure

Information

  • NSF Award
  • 2406551
Owner
  • Award Id
    2406551
  • Award Effective Date
    9/1/2024 - 4 months ago
  • Award Expiration Date
    8/31/2027 - 2 years from now
  • Award Amount
    $ 457,976.00
  • Award Instrument
    Standard Grant

A Novel Approach to Constraining Baryonic Feedback: Coherent Field-Level Inference of Lensing and Electron Pressure

One key challenge in constraining cosmology using galaxy weak lensing measurements is developing an accurate model of how gas is distributed in the universe. The mismodeling of the gas distribution could potentially explain one of the outstanding issues seen in cosmology today. This research team will apply a novel framework based on numerical simulations to the latest data from cosmic microwave background (CMB) and galaxy surveys to gain insights on this topic. This work will bridge a gap between the technical development that has taken off due to the recent advances in artificial intelligence (AI) and machine learning (ML) tools, and the deep knowledge that has been gained over the last 10 years in working with large galaxy and CMB survey data sets. This award will additionally support development of an AI/ML curriculum as well as new collaborations with the Adler Planetarium on visualizations of the universe. <br/><br/>Accurately modeling how baryons are distributed in the universe is challenging. The mismodeling of baryonic distribution could potentially explain the S8 tension between galaxy weak lensing surveys and CMB experiments. The investigators will apply a novel field-level inference framework based on differentiable simulations to the latest data from CMB and galaxy surveys to gain insights on this topic. They envision a three-step process building up to a final analysis using galaxy weak lensing data from the Dark Energy Survey (DES) and the thermal Sunyaev-Zeldovich (tSZ) effect map from the deepest 100 sq. degree data from the South Pole Telescope (SPT-3G). First, the team will build on their prototype pipeline and scale up the volume and resolution of the weak lensing portion to what would be required to analyze the data. Second, the team will implement the tSZ effect into their field-level simulations. Finally, they will incorporate further observational effects into the simulations and apply the framework to the DES and SPT-3G datasets.<br/><br/>This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.

  • Program Officer
    ANDREAS BERLINDaberlind@nsf.gov7032925387
  • Min Amd Letter Date
    8/29/2024 - 4 months ago
  • Max Amd Letter Date
    8/29/2024 - 4 months ago
  • ARRA Amount

Institutions

  • Name
    University of Chicago
  • City
    CHICAGO
  • State
    IL
  • Country
    United States
  • Address
    5801 S ELLIS AVE
  • Postal Code
    606375418
  • Phone Number
    7737028669

Investigators

  • First Name
    Chihway
  • Last Name
    Chang
  • Email Address
    chihway@kicp.uchicago.edu
  • Start Date
    8/29/2024 12:00:00 AM

Program Element

  • Text
    EXTRAGALACTIC ASTRON & COSMOLO
  • Code
    121700

Program Reference

  • Text
    OBSERVATIONAL ASTRONOMY
  • Code
    1207