PIRSA:22080001

Video URL

https://pirsa.org/22080001

Probing the String Axiverse with Galaxy Surveys

Lague, A. (2022). Probing the String Axiverse with Galaxy Surveys. Perimeter Institute for Theoretical Physics. https://pirsa.org/22080001

Lague, Alex. Probing the String Axiverse with Galaxy Surveys. Perimeter Institute for Theoretical Physics, Aug. 02, 2022, https://pirsa.org/22080001 

          @misc{ scivideos_PIRSA:22080001,
            doi = {10.48660/22080001},
            url = {https://pirsa.org/22080001},
            author = {Lague, Alex},
            keywords = {Cosmology},
            language = {en},
            title = {Probing the String Axiverse with Galaxy Surveys},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2022},
            month = {aug},
            note = {PIRSA:22080001 see, \url{https://scivideos.org/pirsa/22080001}}
          }

Alex Lague University of Toronto

Talk numberPIRSA:22080001
DOI10.48660/22080001
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

String theory suggests the existence of multiple axion species forming what is known as an “axiverse”. The axions in this model are thought to have logarithmically-distributed masses extending far below 10^{-21} eV, leading to the presence of ultralight axions. The latter have astrophysical de Broglie wavelength and affect the cosmic structures in which they cluster by erasing small-scale features. In contrast to other ultralight or fuzzy dark matter models, the string axiverse allows for a mixed dark sector with a subdominant ultralight component. Trace amounts of ultralight axions have been shown alleviate some observational discrepancies in cosmology such as the missing satellite problem and the Hubble-S8 tensions. Using an effective field theory approach and data from the Baryon Oscillation Spectroscopic Survey, we reach the strongest constraints on the axion relic density for axions with masses below 10^{-25} eV. To study heavier axions, we develop a new algorithm capable of simulating the formation of large-scale structure in the presence of more than one axion species. Making use of this code, we isolate new observational features in the cosmic web which may help us detect the presence of a plenitude of axions with weak lensing surveys.

Zoom Link: https://pitp.zoom.us/j/95089179013?pwd=NTBIeitScFRhYnBBSnlrcnoyVEhydz09