Probing Parity in the Cosmic Microwave Background (CMB)
APA
(2024). Probing Parity in the Cosmic Microwave Background (CMB). Perimeter Institute. https://pirsa.org/24110083
MLA
Probing Parity in the Cosmic Microwave Background (CMB). Perimeter Institute, Nov. 26, 2024, https://pirsa.org/24110083
BibTex
@misc{ pirsa_PIRSA:24110083, doi = {10.48660/24110083}, url = {https://pirsa.org/24110083}, author = {}, keywords = {Cosmology}, language = {en}, title = {Probing Parity in the Cosmic Microwave Background (CMB)}, publisher = {Perimeter Institute}, year = {2024}, month = {nov}, note = {PIRSA:24110083 see, \url{https://pirsa.org}} }
Deviations from a parity-symmetric Universe would strongly signal the presence of new physics beyond the Standard Model. The lowest-order scalar observable sensitive to parity in a homogeneous and isotropic Universe is the connected four-point function of a given cosmological field. Geometrically, this function is described by a suitable average of this field over many tetrahedral configurations. As the CMB represents a spherical projection of three-dimensional curvature fluctuations, its four-point function serves as a unique, but potentially limited, probe of this fundamental symmetry. In this talk, I will discuss progress in rigorously understanding the CMB’s sensitivity to parity-violating physics from both early- and late-time sources.