McGill.CA / Science / Department of Physics

HEP Theory Journal Club

A unifying description of dark energy

David Langlois

Laboratoire Astroparticules et Cosmologie
Université Paris Diderot

This talk will present an effective description of dark energy/modified gravity models involving a single scalar field. It is based on a 3+1 splitting of space-time with respect to uniform scalar field hypersurfaces. The advantage of this approach is that it can describe in the same language a vast number of existing models, including quintessence, F(R) gravity, Horndeski theories, as well as scalar-tensor theories "beyond" Horndeski, which I will also discuss. This approach provides a unified treatment of linear cosmological perturbations, generically characterized by a few time-dependent functions. This gives an economic and systematic way to confront theoretical models with cosmological observations.

Tuesday, February 7th 2017, 12:00
Ernest Rutherford Physics Building, room 326