6–8 May 2024
Building 50
US/Pacific timezone

An Effective Cosmological Collider

7 May 2024, 11:40
10m
Auditorium (Building 50)

Auditorium

Building 50

Speaker

Amara McCune (UC Santa Barbara)

Description

An upcoming suite of cosmological probes of large-scale structure poses a unique opportunity to search for physics beyond the Standard Model. Particles with masses of order Hubble during inflation create a distinct, oscillatory signal in the squeezed limit of the bispectrum. Fully leveraging this property to uncover new physics, a pursuit known as the “cosmological collider”, necessitates a comprehensive understanding of contributing opreators and their effects. In this talk, I’ll introduce our work that initiaties a systematic study of operator redundancies in inflationary spacetime. We establish a minimal operator basis for an archetypal example, an abelian gauge-Higgs theory that couples to the inflaton. Working up to dimension 9, we show that certain lower-dimensional operators are entirely redundant and identify new non-redundant operators with potentially interesting cosmological collider signatures. We expect particular reliance on 21 cm probes to distinguish them.

Primary author

Amara McCune (UC Santa Barbara)

Presentation materials