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
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