Approaches to tests of gravity on cosmological scales
APA
Silvestri, A. (2015). Approaches to tests of gravity on cosmological scales. Perimeter Institute. https://pirsa.org/15030103
MLA
Silvestri, Alessandra. Approaches to tests of gravity on cosmological scales. Perimeter Institute, Mar. 31, 2015, https://pirsa.org/15030103
BibTex
@misc{ pirsa_PIRSA:15030103, doi = {10.48660/15030103}, url = {https://pirsa.org/15030103}, author = {Silvestri, Alessandra}, keywords = {Cosmology}, language = {en}, title = {Approaches to tests of gravity on cosmological scales}, publisher = {Perimeter Institute}, year = {2015}, month = {mar}, note = {PIRSA:15030103 see, \url{https://pirsa.org}} }
More than a decade after its discovery, cosmic acceleration still
poses a puzzle for modern cosmology and a plethora of models of dark energy
or modified gravity, able to reproduce the observed expansion history, have
been proposed as alternatives to the cosmological standard model. In recent
years it has become increasingly evident that probes of the expansion his-
tory are not sufficient to distinguish among the candidate models, and that
it is necessary to combine those with observations that probe the dynamics
of inhomogeneities. Future cosmological surveys will map the evolution of
inhomogeneities to high accuracy, allowing us to test the relationships be-
tween matter overdensities, local curvature, and the Newtonian potential on
cosmological scales.
I will discuss theoretical issues involved in finding an optimal framework to
study deviations from General Relativity on cosmological scales, giving an
overview of recent progress, with a focus on model-independent, parametrized
approaches. I will summarize where we stand and what are the next steps
we should take.