Dark Energy and Neutrino Mass
APA
Franca, U. (2007). Dark Energy and Neutrino Mass. Perimeter Institute. https://pirsa.org/07050032
MLA
Franca, Urbano. Dark Energy and Neutrino Mass. Perimeter Institute, May. 18, 2007, https://pirsa.org/07050032
BibTex
@misc{ pirsa_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}, year = {2007}, month = {may}, note = {PIRSA:07050032 see, \url{https://pirsa.org}} }
Harvard University
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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.