Condensed body mass accretion with DBI-essence dark energy and its reconstruction with f(Q) gravity

TL;DR

This paper reconstructs a DBI-essence dark energy model within f(Q) gravity, analyzing black hole and wormhole mass accretion, thermodynamic conditions, and effects of singularity resolutions.

Contribution

It introduces a novel reconstruction of the DBI-essence dark energy model using f(Q) gravity and examines its implications on black hole and wormhole mass accretion.

Findings

Black hole and wormhole masses are affected by reconstructed dark energy.

Thermodynamic energy conditions are validated within the model.

Singularity resolutions influence mass accretion dynamics.

Abstract

We have studied the reconstruction formalism of the DBI-essence dark energy scalar field model with the help of non-metricity of gravity or f(Q) gravity. The critical analysis has been done on the reconstructed model. The Black hole and Wormhole mass accretions have been studied with this reconstructed model. We have analyzed the validities of thermodynamic energy conditions. In our reconstructed model, we have assumed four types of singularity resolutions of scale factor and investigated the black hole and wormhole masses due to accretion of reconstructed dark energy. Diagrammatically, we have analyzed the nature of physical quantities with the kinetic and potential energies as well as the mass due to accretion in the reconstructed DBI-essence dark energy in the background of f(Q) gravity.