Statistics – Computation
Scientific paper
Dec 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.253..599c&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 253, Dec. 15, 1991, p. 599-604. Research supported by D
Statistics
Computation
27
Astronomical Models, Autocorrelation, Probability Density Functions, Relic Radiation, Temperature Distribution, Anisotropy, Baryons, Computational Astrophysics, Dark Matter
Scientific paper
The probability density function of the temperature autocorrelation is given in a semi-analytical form for the case of Gaussian temperature fluctuations. Based on this result we obtain confidence intervals for the anisotropies expected in several cosmological scenarios dominated by baryonic (B), hot dark matter (HDM) and cold dark matter (CDM) with adiabatic fluctuations. We also confront these expectations with the upper limits given by the present experiments at large angular scales.
Cayón Laura
Luis Sanz José
Martinez-Gonzalez Enrique
No associations
LandOfFree
The probability density function of the temperature autocorrelation of the cosmic microwave background for a Gaussian cosmological model 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 The probability density function of the temperature autocorrelation of the cosmic microwave background for a Gaussian cosmological model, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The probability density function of the temperature autocorrelation of the cosmic microwave background for a Gaussian cosmological model will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1541309