Dark Energy and Neutrino Mass

APA

Franca, U. (2007). Dark Energy and Neutrino Mass. Perimeter Institute for Theoretical Physics. https://pirsa.org/07050032

MLA

Franca, Urbano. Dark Energy and Neutrino Mass. Perimeter Institute for Theoretical Physics, May. 18, 2007, https://pirsa.org/07050032

BibTex

          @misc{ scivideos_PIRSA:07050032,
            doi = {10.48660/07050032},
            url = {https://pirsa.org/07050032},
            author = {Franca, Urbano},
            keywords = {Cosmology},
            language = {en},
            title = {Dark Energy and Neutrino Mass},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2007},
            month = {may},
            note = {PIRSA:07050032 see, \url{https://scivideos.org/pirsa/07050032}}
          }
          

Urbano Franca Harvard University

Source Repository PIRSA
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Subject

Abstract

One of the possible explanations for the current acceleration of the universe comes from a coupling between the Dark Energy and the Neutrino sectors. This coupling causes the neutrino mass to vary with cosmic time, what opens a new window to constrain this dark energy candidate. In this work, we analyze the mass-varying neutrino scenario in a model independent way, focusing on its effects for the Cosmic Microwave Background and Large Scale Structure.