The dynamics of background evolution and structure formation in phase space: a semi-cosmographic reconstruction
Pankaj Chavan, Tapomoy Guha Sarkar, Anjan A Sen

TL;DR
This paper introduces a semi-cosmographic method to analyze background evolution and structure formation in phase space, fitting observational data without assuming a specific dark energy model, revealing deviations from Lambda-CDM at low redshifts.
Contribution
It develops a novel semi-cosmographic framework that reconstructs cosmological functions and phase trajectories directly from data, avoiding predefined dark energy models.
Findings
Detected deviations from Lambda-CDM at low redshifts.
Identified key redshifts for future observational focus.
Reconstructed phase space trajectories consistent with current data.
Abstract
The Baryon Acoustic Oscillation (BAO) feature, imprinted in the transverse and radial clustering of dark matter tracers, enables the simultaneous measurement of the angular diameter distance and the Hubble parameter at a given redshift. Further, measuring the redshift space anisotropy (RSD) allows us to measure the combination . Motivated by this, we simultaneously study the dynamics of background evolution and structure formation in an abstract phase space of dynamical quantities: , , and . We adopt a semi-cosmographic approach, whereby we do not pre-assume any specific dark energy model to integrate the dynamical system. The Luminosity distance is expanded as a Pad\'e rational approximation in the variable . The dynamical system is solved by using a semi-cosmographic equation of state, which…
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Taxonomy
TopicsAstro and Planetary Science · Planetary Science and Exploration
