Test of the cosmic evolution using Gaussian processes

Much focus was on the possible slowing down of cosmic acceleration under the dark energy parametrization. In the present paper, we investigate this subject using the Gaussian processes (GP), without resorting to a particular template of dark energy. The reconstruction is carried out by abundant data...

Full description

Saved in:
Bibliographic Details
Published inJournal of cosmology and astroparticle physics Vol. 2016; no. 12; p. 5
Main Authors Zhang, Ming-Jian, Xia, Jun-Qing
Format Journal Article
LanguageEnglish
Published United States 05.12.2016
Subjects
ACCELERATION
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
COMPARATIVE EVALUATIONS
COSMIC GAMMA BURSTS
DISTANCE
EXPANSION
GALACTIC EVOLUTION
GAMMA RADIATION
GAUSSIAN PROCESSES
LUMINOSITY
NONLUMINOUS MATTER
STAR EVOLUTION
Online AccessGet full text

Cover

More Information
Summary:Much focus was on the possible slowing down of cosmic acceleration under the dark energy parametrization. In the present paper, we investigate this subject using the Gaussian processes (GP), without resorting to a particular template of dark energy. The reconstruction is carried out by abundant data including luminosity distance from Union2, Union2.1 compilation and gamma-ray burst, and dynamical Hubble parameter. It suggests that slowing down of cosmic acceleration cannot be presented within 95% C.L., in considering the influence of spatial curvature and Hubble constant. In order to reveal the reason of tension between our reconstruction and previous parametrization constraint for Union2 data, we compare them and find that slowing down of acceleration in some parametrization is only a ''mirage'. Although these parameterizations fits well with the observational data, their tension can be revealed by high order derivative of distance D. Instead, GP method is able to faithfully model the cosmic expansion history.
ISSN:1475-7516
1475-7516
DOI:10.1088/1475-7516/2016/12/005