Poster
Résumé
: A key
issue of contemporary cosmology is the
problem of currently accelerating
expansion of the Universe. The nature of
this phenomenon is one of the most
outstanding problems of physics and
astronomy today. Its origin may be
attributed to either unknown exotic
material component with negative pressure
- so called Dark Energy (DE), to infra red
modification of gravity at cosmological
scale or requires to relax the assumption
of homogeneity of the Universe. It should
be pointed out that the strength of modern
cosmology (which now enterd stage dubbed
the era of precision cosmology) lies in
consistency across independent pieces of
evidence rather than in single, crucial
experiment. We approach to this subject
from phenomenological point of view. In
this spirit we perform a cosmographic
analysis using several cosmological probes
such as Type Ia Supernovae (Union2
compilation), data from Cosmic Microwave
Background (WMAP7), Baryon Acoustic
Oscillation (BAO) and strongly
gravitationally lensed systems (combined
data sets from SLACS and LSD surveys) and
Gamma Ray Bursts. These tests falls into
two distinct cathegories. The first one
makes use of the angular diameter
distance, and refers to the so called
standard rulers. Here we have strong
lensing systems, shift parameter R from
CMB and BAO scales. The second uses the
luminosity distance and then we deal with
standard (or rather standarizable)
candles. Here we deal with SN Ia and GRB.
The two distance concepts, although
theoretically related to each other, in
practice have different systematic
uncertainties and different parameter
degeneracies.Hence their joint analysis is
more restrictive in the parameter space.
We considered several cosmological
scenarios of dark energy, widely discussed
in current literature. We also address the
question which model is the best with
information-theoretic criteria: the Akaike
Criterion (AIC) and Bayesian Information
Criterion (BIC). |
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