Global dynamics of the Horava-Lifshitz cosmological model in a non-flat universe with non-zero cosmological constant

TL;DR

This paper investigates the global behavior of a non-flat universe within Horava-Lifshitz gravity when a non-zero cosmological constant is present, using qualitative differential equations analysis.

Contribution

It provides a novel qualitative analysis of the cosmological dynamics in Horava-Lifshitz gravity with non-zero cosmological constant and spatial curvature.

Findings

Characterizes the global dynamics of the model

Identifies critical points and stability conditions

Explores the impact of non-zero cosmological constant

Abstract

When the cosmological constant is non-zero the dynamics of the cosmological model based on Horava-Lifshitz gravity in a non-flat universe is characterized by using the qualitative theory of differential equations.