Talk detail

MG13 - Talk detail

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 Participant

Demianski, Marek

Institution

Institute of Theoretical Physics, Faculty of Physics, University of Warsaw  - Hoza 69 - Warsaw - Poland - Poland

Session

OC3

Accepted

Order

Time

Talk

Oral abstract

Title

High redshift cosmography: new results and implications for dark energy
Co-authors

Abstract

We use all the available date on high redshift objects (Union2 Type Ia supernovae, GRBs and BAO) to derive constrains on the parameters of FRWL cosmological model without imposing any a priori assumptions about on the dynamical equations for gravity. These data sets allow us to put constrains on the cosmographic expansion up to the fifth order. To perform our analysis we use the Markov Chain Monte Carlo Method. To investigate the dark energy component we use different parametrizations of its equation of state. We show that the deceleration parameter clearly confirms the present acceleration phase of the Universe, there are hints that the dark energy equation of state is evolving and there are possible deviations from the LCDM model.

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