Fuzzy Dark Matter Less-complex Wormhole Structures in Higher-Order Curvature Gravity

TL;DR

This paper investigates fuzzy dark matter wormholes within higher-order curvature gravity, deriving their shape functions, analyzing stability, and highlighting their natural occurrence near galactic structures, emphasizing less complex geometries.

Contribution

It introduces new fuzzy wormhole solutions in higher-order curvature gravity and analyzes their stability and physical properties in galactic environments.

Findings

Fuzzy wormholes can be stable in higher-order curvature gravity.

Active gravitational mass varies inversely with radial distance.

Stable structures exist near dark matter halos and galactic bulges.

Abstract

Fuzzy dark matter wormhole solutions coupled with anisotropic matter distribution are explored in higher-order curvature gravity. We derive the shape function for fuzzy wormholes and explore their possible stability. We study the embedding diagrams of the active gravitational mass associated with fuzzy dark matter wormholes by taking a certain shape function. Aiming to highlight the role of higher-order curvature gravity in the modeling of less complex fuzzy wormhole structures, we evaluate the complexity factor, the conservation equation, and null energy conditions. Our study reinforces more importance of uniformly distributed pressure effects throughout the less complex region than the emergence of energy density homogeneity in the stability of fuzzy wormholes. It is shown that the active gravitational mass of the fuzzy wormhole structures varies inversely with the radial distance, thereby suggesting the breaching of energy conditions at some arena of the Einasto index. Furthermore, it is revealed that stable fuzzy dark matter wormhole structures exist in nature in the surroundings of cold dark matter halos and galactic bulges. The important physics understood from our analysis is that in higher-order curvature gravity, feasible geometries of fuzzy dark matter wormholes exist naturally in the environments of different galactic haloes.