Clustering in interacting dark energy cosmologies
APA
Pettorino, V. (2008). Clustering in interacting dark energy cosmologies. Perimeter Institute. https://pirsa.org/08110038
MLA
Pettorino, Valeria. Clustering in interacting dark energy cosmologies. Perimeter Institute, Nov. 14, 2008, https://pirsa.org/08110038
BibTex
@misc{ pirsa_PIRSA:08110038, doi = {10.48660/08110038}, url = {https://pirsa.org/08110038}, author = {Pettorino, Valeria}, keywords = {Cosmology}, language = {en}, title = {Clustering in interacting dark energy cosmologies}, publisher = {Perimeter Institute}, year = {2008}, month = {nov}, note = {PIRSA:08110038 see, \url{https://pirsa.org}} }
Universität Heidelberg
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Abstract
I will illustrate the case of interacting dark Energy, that is to say cosmologies in which the dark energy scalar field interacts with other things in the universe (gravity, cold dark matter or neutrinos). After briefly presenting the status of our work for the first two classes of models, regarding both linear perturbations and Nbody simulations, I will in particular focus on the case of \'growing neutrinos\': in these models, neutrinos with a mass increasing with time might be driven to cluster at very large scales, due to a new interaction stronger than gravity and mediated by the dark energy scalar field.