Tension in the Hubble Constant: Is There a Crisis in Cosmology?
APA
Freedman, W. (2021). Tension in the Hubble Constant: Is There a Crisis in Cosmology?. Perimeter Institute. https://pirsa.org/21020006
MLA
Freedman, Wendy. Tension in the Hubble Constant: Is There a Crisis in Cosmology?. Perimeter Institute, Feb. 24, 2021, https://pirsa.org/21020006
BibTex
@misc{ pirsa_PIRSA:21020006, doi = {10.48660/21020006}, url = {https://pirsa.org/21020006}, author = {Freedman, Wendy}, keywords = {Other}, language = {en}, title = {Tension in the Hubble Constant: Is There a Crisis in Cosmology?}, publisher = {Perimeter Institute}, year = {2021}, month = {feb}, note = {PIRSA:21020006 see, \url{https://pirsa.org}} }
An important and unresolved question in cosmology today is whether there is new physics that is missing from our current standard Lambda Cold Dark Matter (LCDM) model. A current discrepancy in the measurement of the Hubble constant could be signaling a new physical property of the universe or, more mundanely, unrecognized measurement uncertainties. I will discuss two of our most precise methods for measuring distances in the local universe: Cepheids and the Tip of the Red Giant Branch (TRGB). I will present new results from the Carnegie-Chicago Hubble Program (CCHP), the goal of which is to independently measure a value of the Hubble constant to a precision and accuracy of 2%. Using the Hubble Space Telescope Advanced Camera for Surveys, we are using the TRGB to calibrate Type Ia supernovae. I will address the uncertainties, discuss the current tension in Ho, and whether there is need for additional physics beyond the standard LCDM model.