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Kogai, Kazuhiro; Akitsu, Kazuyuki; Schmidt, Fabian; Urakawa, Yuko

Galaxy imaging surveys as spin-sensitive detector for cosmological colliders. (English) Zbl 1484.85015

J. Cosmol. Astropart. Phys. 2021, No. 3, Paper No. 60, 50 p. (2021).
Summary: 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.

Cited in 17 Documents

MSC:

85A15 Galactic and stellar structure
83F05 Relativistic cosmology
35B20 Perturbations in context of PDEs
83E50 Supergravity
78A45 Diffraction, scattering
58J47 Propagation of singularities; initial value problems on manifolds
81T11 Higher spin theories

Keywords:

inflation; cosmological perturbation theory; galaxy surveys; gravitational lensing

Software:

CAMB
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Full Text: DOI arXiv

References:

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