October 13, 2023
2:30PM
-
3:30PM
PRB 1080 & Zoom
Add to Calendar
2023-10-13 13:30:00
2023-10-13 14:30:00
CCAPP Seminar: Dragan Huterer (Michigan)
Speaker: Dragan Huterer (Michigan)
Evidence for the suppression of structure growth in the standard cosmological model
I will first review the status of the theory/data interface in cosmology, focusing in particular on the Hubble tension as well as recent results from large cosmological surveys. I will then review recent work where we found a~4-sigma evidence for the suppression of growth of structure in the standard cosmological model. I will end by reviewing expected forthcoming measurements that will shed light on cosmological tensions, including those from the DESI experiment.
For Zoom information, please contact the seminar coordinators.
PRB 1080 & Zoom
OSU ASC Drupal 8
ascwebservices@osu.edu
America/New_York
public
Date Range
2023-10-13 14:30:00
2023-10-13 15:30:00
CCAPP Seminar: Dragan Huterer (Michigan)
Speaker: Dragan Huterer (Michigan)
Evidence for the suppression of structure growth in the standard cosmological model
I will first review the status of the theory/data interface in cosmology, focusing in particular on the Hubble tension as well as recent results from large cosmological surveys. I will then review recent work where we found a~4-sigma evidence for the suppression of growth of structure in the standard cosmological model. I will end by reviewing expected forthcoming measurements that will shed light on cosmological tensions, including those from the DESI experiment.
For Zoom information, please contact the seminar coordinators.
PRB 1080 & Zoom
America/New_York
public
Speaker: Dragan Huterer (Michigan)
Evidence for the suppression of structure growth in the standard cosmological model
I will first review the status of the theory/data interface in cosmology, focusing in particular on the Hubble tension as well as recent results from large cosmological surveys. I will then review recent work where we found a~4-sigma evidence for the suppression of growth of structure in the standard cosmological model. I will end by reviewing expected forthcoming measurements that will shed light on cosmological tensions, including those from the DESI experiment.
For Zoom information, please contact the seminar coordinators.