Dynamical system analysis in teleparallel gravity with boundary term
S. A. Kadam, Ninaad P. Thakkar, B. Mishra

TL;DR
This paper performs a dynamical system analysis of extended teleparallel gravity models, identifying critical points and stability across different cosmic epochs, and demonstrating the models' ability to produce an accelerating universe consistent with observations.
Contribution
It introduces a novel dynamical system framework for $f(T, B)$ gravity, analyzing critical points and stability in two specific models involving boundary terms.
Findings
Critical points correspond to radiation, matter, and de-Sitter phases.
Both models exhibit stable critical points leading to cosmic acceleration.
Density parameters and equation of state parameters align with observed universe behavior.
Abstract
In this paper, we perform the dynamical system analysis of the cosmological models framed in the extended teleparallel gravity, the gravity. We use the mapping, -+, and define the dynamical variables to form the autonomous dynamical system. The critical points are obtained in two well-motivated forms of , one that involves the logarithmic form of the boundary term B, and the other one is the non-linear form of the boundary term. The position of critical points is shown in the different evolutionary phases of the Universe such as radiation, matter, and de-Sitter phase. The stability condition of each of the critical points of both the models is derived and the behavior of each point has been obtained mathematically and through the phase portrait. The evolution of standard density parameters such as radiation (),…
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Geophysics and Gravity Measurements
