Quasi-Bernoulli statistics of string-induced fluctuations of cosmic microwave background radiation

Details Quasi-Bernoulli statistics of string-induced fluctuations of cosmic microwave background radiation Quasi-Bernoulli statistics of string-induced fluctuations of cosmic microwave background radiation

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998phrvd..58l7301b&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 58, Issue 12, 15 December 1998, id. 127301

Statistics

4

Particle-Theory And Field-Theory Models Of The Early Universe, Background Radiations

Scientific paper

A new kind of statistical distribution, a quasi-Bernoulli distribution, is suggested to describe the non-Gaussian string-induced perturbations of the cosmic microwave background radiation. Good agreement between predictions based on this statistics and data of numerical and laboratory simulations using some simplified models is established, and a possible relation of this statistic to a large-scale galaxy distribution is briefly discussed.

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