Denys Wilkinson Building, Department of Physics, University of Oxford, Keble Road, Oxford OX1 3RH
Oliver Philcox (Columbia University)
Abstract:
Spectroscopic surveys are generally used to constrain cosmology through the Baryon Acoustic Oscillation signature, often in combination with the CMB. However, their utility extends far further: thanks to recent theoretical developments, we can now place direct constraints on cosmological models (both in ΛCDM and beyond) using the full-shape of the galaxy power spectrum, bispectrum and beyond. Such analyses become increasingly useful as the volume of survey data increases; by the end of the decade, spectroscopic surveys will give the tightest constraints on many fundamental parameters.
In this talk, I will present the current status of the field, discussing a number of recent constraints obtained from the analysis of SDSS data in conjunction with a robust model, rooted in Effective Field Theory. In particular, I will show BOSS constraints on ΛCDM parameters, as well as direct measurements of primordial non-Gaussianity from the galaxy bispectrum. Finally, I will comment on recent claims of cosmological parity-violation and their implications for the primordial Universe.