PIRSA:14030095

Cosmology Results from the Pan-STARRs Supernova Survey

APA

Scolnic, D. (2014). Cosmology Results from the Pan-STARRs Supernova Survey. Perimeter Institute for Theoretical Physics. https://pirsa.org/14030095

MLA

Scolnic, Daniel. Cosmology Results from the Pan-STARRs Supernova Survey. Perimeter Institute for Theoretical Physics, Mar. 04, 2014, https://pirsa.org/14030095

BibTex

          @misc{ scivideos_PIRSA:14030095,
            doi = {10.48660/14030095},
            url = {https://pirsa.org/14030095},
            author = {Scolnic, Daniel},
            keywords = {Cosmology},
            language = {en},
            title = {Cosmology Results from the Pan-STARRs Supernova Survey},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2014},
            month = {mar},
            note = {PIRSA:14030095 see, \url{https://scivideos.org/index.php/pirsa/14030095}}
          }
          

Danial Scolnic Johns Hopkins University

Talk numberPIRSA:14030095
Source RepositoryPIRSA
Talk Type Scientific Series
Subject

Abstract

The Pan-STARRs supernova survey has discovered one of the largest samples of Type Ia supernovae. Measurements of the distances to these supernovae allow us to probe some of the most fundamental questions about the properties of the universe like what is dark energy. When combining measurements from various astrophysical probes, we find hints of interesting tension with the Lambda-CDM model. I discuss the various combinations of astrophysical probes and the source of this tension. It is possible that this tension is due to systematic uncertainties in the various measurements, and I show how we analyze these uncertainties in the Pan-STARRs sample.