Noncommutative Wormhole Solutions in Einstein Gauss-Bonnet Gravity
Shamaila Rani, Abdul Jawad

TL;DR
This paper investigates static spherically symmetric wormhole solutions within Einstein Gauss-Bonnet gravity in higher dimensions, focusing on energy condition satisfaction using non-commutative geometries and analyzing their stability.
Contribution
It presents novel wormhole solutions in higher-dimensional Einstein Gauss-Bonnet gravity that satisfy energy conditions, including stable fifth-dimensional solutions.
Findings
Fifth-dimensional stable wormholes satisfy energy conditions.
Solutions are derived using Gaussian and Lorentzian non-commutative geometries.
Both positive and negative Gauss-Bonnet coefficients are considered.
Abstract
In this paper, we explore static spherically symmetric wormhole solutions in the framework of -dimensional Einstein Gauss-Bonnet gravity. Our objective is to find out wormhole solutions that satisfy energy conditions. For this purpose, we consider two frameworks such as Gaussian distributed and Lorentzian distributed non-commutative geometry. Taking into account constant redshift function, we obtain solutions in the form of shape function. The fifth and sixth dimensional solutions with positive as well as negative Gauss-Bonnet coefficient are discussed. Also, we check the equilibrium condition for the wormhole solutions with the help of generalized Tolman-Oppenheimer-Volkov equation. It is interesting to mention here that we obtain fifth dimensional stable wormhole solutions in both distributions that satisfy the energy conditions.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Geometric Analysis and Curvature Flows
