Count response model for the CMB spots
Cosmology and Nongalactic Astrophysics
2010-10-29 v1 General Relativity and Quantum Cosmology
High Energy Physics - Phenomenology
Abstract
The statistics of the curvature quanta generated during a stage of inflationary expansion is used to derive a count response model for the large-scale phonons determining, in the concordance lore, the warmer and the cooler spots of the large-scale temperature inhomogeneities. The multiplicity distributions for the counting statistics are shown to be generically overdispersed in comparison with conventional Poissonian regressions. The generalized count response model deduced hereunder accommodates an excess of correlations in the regime of high multiplicities and prompts dedicated analyses with forthcoming data collected by instruments of high angular resolution and high sensitivity to temperature variations per pixel.
Cite
@article{arxiv.1010.5972,
title = {Count response model for the CMB spots},
author = {Massimo Giovannini},
journal= {arXiv preprint arXiv:1010.5972},
year = {2010}
}
Comments
9 pages