Primordial non-Gaussianity from the large scale structure
Cosmology and Nongalactic Astrophysics
2015-05-18 v1 General Relativity and Quantum Cosmology
High Energy Physics - Phenomenology
Abstract
Primordial non-Gaussianity is a potentially powerful discriminant of the physical mechanisms that generated the cosmological fluctuations observed today. Any detection of non-Gaussianity would have profound implications for our understanding of cosmic structure formation. In this paper, we review past and current efforts in the search for primordial non-Gaussianity in the large scale structure of the Universe.
Keywords
Cite
@article{arxiv.1003.5020,
title = {Primordial non-Gaussianity from the large scale structure},
author = {Vincent Desjacques and Uros Seljak},
journal= {arXiv preprint arXiv:1003.5020},
year = {2015}
}
Comments
Invited review article for the CQG special issue on nonlinear cosmological perturbations.