Microwave Anisotropies from Random Sources
Astrophysics
2016-08-30 v1
Abstract
I report on recent developments in the theory of cosmic background radiation perturbations. I describe ways of modeling alternatives to the canonical Gaussian theories within the standard framework of cosmological perturbation theory. Some comments are made on using these techniques to resolve the uncertainties in theories of structure formation with topological defects. (To appear in the proceedings of the XXXIth Moriond meeting, ``Microwave Background Anisotropies'')
Cite
@article{arxiv.astro-ph/9606068,
title = {Microwave Anisotropies from Random Sources},
author = {Pedro G. Ferreira},
journal= {arXiv preprint arXiv:astro-ph/9606068},
year = {2016}
}
Comments
6 pages,uses cmb.sty and has 5 figs