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/index.php/pirsa/07050032}}
}
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.
