Galaxy imaging surveys as spin-sensitive detector for cosmological colliders

Galaxy imaging surveys provide us with information on both the galaxy distribution and their shapes. In this paper, we systematically investigate the sensitivity of galaxy shapes to new physics in the initial conditions. For this purpose, we decompose the galaxy shape function into spin components, and compute the contributions to each spin component from both intrinsic alignment and weak lensing. We then consider the angular-dependent primordial non-Gaussianity, which is generated by a non-zero integer spin particle when active during inflation, and show that a galaxy imaging survey essentially functions as a spin-sensitive detector of such particles in the early universe. We also perform a forecast of the PNG generated from a higher spin particle, considering a Rubin Observatory LSST-like galaxy survey.

Automated summary

This study systematically investigates the sensitivity of galaxy shapes to new physics in the initial conditions by decomposing the galaxy shape function into spin components and computing their contributions. It demonstrates that a galaxy imaging survey essentially functions as a spin-sensitive detector of such particles in the early universe, providing valuable insights into the primordial non-Gaussianity generated from higher spin particles.