Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995apj...449..404g&link_type=abstract
Astrophysical Journal v.449, p.404
Astronomy and Astrophysics
Astronomy
4
Cosmology: Cosmic Microwave Background, Cosmology: Theory, Methods: Statistical
Scientific paper
We propose a set of statistics for detecting non-Gaussianity in one-dimensional cosmic microwave background radiation (CMBR) anisotropy data sets. These statistics are both simple and, according to calculations over a space of linear combinations of three-point functions, nearly optimal at detecting certain types of nonGaussian features. We use this statistic to analyze the anisotropy detected by the UCSB SP91 experiment. According to this statistic the mean of the four frequency channels is significantly non-Gaussian. If this signal represents primordial CMBR fluctuations, it would be highly unlikely in a Gaussian theory with a small coherence angle, such as "standard" (n = 1,Ωb = 0.05, h = 0.5, Δ = 0) inflation. We cannot tell whether the observed non-Gaussian signal is cosmological in origin, but if we assume it due instead to foreground emission, and remove the points responsible for the non-Gaussian behavior, the rms of the remaining fluctuations is improbably low for the "standard" inflation theory. Further data are clearly needed before any definitive conclusions may be drawn. We also generalize the ideas behind this statistic to non-Gaussian features that might be detected in other experimental schemes.
Graham Paul
Lubin Phil M.
Schuster Jeff A.
Turok Neil
No associations
LandOfFree
A Simple Test for Non-Gaussianity in Cosmic Microwave Background Radiation Measurements does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with A Simple Test for Non-Gaussianity in Cosmic Microwave Background Radiation Measurements, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Simple Test for Non-Gaussianity in Cosmic Microwave Background Radiation Measurements will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1269240