PIRSA:20060023

Video URL

https://pirsa.org/20060023

Light Hidden Sectors and the Hubble Tension

Blinov, N. (2020). Light Hidden Sectors and the Hubble Tension. Perimeter Institute for Theoretical Physics. https://pirsa.org/20060023

Blinov, Nikita. Light Hidden Sectors and the Hubble Tension. Perimeter Institute for Theoretical Physics, Jun. 09, 2020, https://pirsa.org/20060023 

          @misc{ scivideos_PIRSA:20060023,
            doi = {10.48660/20060023},
            url = {https://pirsa.org/20060023},
            author = {Blinov, Nikita},
            keywords = {Particle Physics},
            language = {en},
            title = {Light Hidden Sectors and the Hubble Tension},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2020},
            month = {jun},
            note = {PIRSA:20060023 see, \url{https://scivideos.org/index.php/pirsa/20060023}}
          }

Nikita Blinov York University

Talk numberPIRSA:20060023
DOI10.48660/20060023
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

The inference of the present expansion rate from the Cosmic Microwave Background and other early-time probes (assuming standard
cosmology) is in significant tension with several direct measurements of the same quantity. If this discrepancy is not due to unresolved systematics, it could provide strong evidence for physics beyond the standard models of particle physics and cosmology. I will describe a few simple models that attempt to alleviate this Hubble tension. All of these scenarios contain additional energy density of new light particles at early times with interactions that modify the background cosmology and evolution of density perturbations in the early universe. First, I will motivate the existence of a decaying component of dark matter with a significant free-streaming length as a means of addressing this tension. Then I will consider models with self-interacting neutrino or dark radiation components. I will show that such scenarios face stringent cosmological and laboratory constraints. As a result, in these examples, the tension can be alleviated but not eliminated altogether.