Astroseminar Series - Xinyi Chen - IN PERSON

Wednesday, November 22, 2023 11:30 am - 12:30 pm EST (GMT -05:00)

Astroseminar - Xinyi Chen - IN PERSON

Xinyi Chen

Xinyi Chen is a graduate student at Yale University, working on large-scale structure cosmology with Prof. Nikhil Padmanabhan. Her research combines machine learning, statistics and theoretical modeling to probe the nature of dark energy and inflation via large galaxy surveys such as Dark Energy Spectroscopic Instrument (DESI). In particular, she develops high-fidelity initial condition reconstruction algorithms, and applies them to optimally extract cosmological information from the data and constrain the physics of inflation through the measurement of primordial non-Gaussianity. She is also involved in DESI Y1 baryon acoustic oscillation (BAO) analysis. Previously, she completed her Bachelor's degree at the University of Michigan.

Title: Probing primordial non-Gaussianity by reconstructing the initial conditions with machine learning

Abstract: Inflation remains one of the enigmas in fundamental physics. While it is difficult to distinguish different inflation models, information contained in primordial non-Gaussianity (PNG) offers a route to break the degeneracy. In galaxy surveys, the local type PNG is usually probed by measuring the scale-dependent bias in the galaxy power spectrum on large scales, where cosmic variance and systematics are also large. Other types of PNG need bispectrum, which is computationally challenging and is contaminated by gravity. I will introduce a new approach to measuring PNG by using the reconstructed density field, a density field reversed to the initial conditions from late time. With the reconstructed density field, we can fit a new template at the field level, or compute a near optimal bispectrum estimator, to constrain PNG. By reconstructing the initial conditions, we remove the nonlinearity induced by gravity, which is a source of confusion when measuring PNG. Near optimal bispectrum estimator mitigates computational challenges. This new approach shows strong constraining power, offers an alternative way to the existing method with different systematics, and also follows organically the procedure of baryon acoustic oscillation (BAO) analysis in large galaxy surveys. I will present a reconstruction method using convolutional neural networks that significantly improves the performance of traditional reconstruction algorithms in the matter density field, which is crucial for more effectively probing PNG. This pipeline can enable new observational constraints on PNG from the ongoing Dark Energy Spectroscopic Instrument (DESI) and Euclid surveys, as well as from upcoming surveys, such as that of the Nancy Grace Roman Space Telescope.