Primordial gravity waves from tidal imprints in large-scale structure
APA
Masui, K. (2017). Primordial gravity waves from tidal imprints in large-scale structure. Perimeter Institute. https://pirsa.org/17100081
MLA
Masui, Kiyoshi. Primordial gravity waves from tidal imprints in large-scale structure. Perimeter Institute, Oct. 17, 2017, https://pirsa.org/17100081
BibTex
@misc{ pirsa_PIRSA:17100081, doi = {10.48660/17100081}, url = {https://pirsa.org/17100081}, author = {Masui, Kiyoshi}, keywords = {Cosmology}, language = {en}, title = {Primordial gravity waves from tidal imprints in large-scale structure}, publisher = {Perimeter Institute}, year = {2017}, month = {oct}, note = {PIRSA:17100081 see, \url{https://pirsa.org}} }
I will describe a tidal effect whereby the decay of primordial gravity waves leaves a permanent shear in the large-scale structure of the Universe. Future large-scale structure surveys - especially radio surveys of high-redshift hydrogen gas - could measure this shear and its spatial dependence to form a map of the initial gravity-wave field. The three dimensional nature of this probe makes it sensitive to the helicity of the gravity waves, allowing for searches for early-Universe gravitational parity violation. Due to the large number of measurable modes in the high-redshift large-scale structure, these tidal imprints could ultimately be more sensitive than searches for CMB B-modes.