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Interacting Dark Energy

Bruno J. Barros


It will be presented a model of dark energy described by a single canonical scalar field interacting with one cold dark matter component. The background will be fixed as LCDM and the theory will still be distinguishable at the perturbative level where differences arise. We also compare the observables against redshift space distortion data. Finally it will be proposed a new, non-canonical, generalized coupled dark energy model by briefly introducing the main background cosmology equations.

2017 October 03, 09:30

Faculdade de Ciências da Universidade de Lisboa (C8.2.12)
Campo Grande, 1749-016 Lisboa

Faculdade de Ciências da Universidade de Lisboa Universidade do Porto Faculdade de Ciências e Tecnologia da Universidade de Coimbra
Fundação para a Ciência e a Tecnologia COMPETE 2020 PORTUGAL 2020 União Europeia