Embedded class one analysis of wormhole configurations in 4𝒟 Einstein–Gauss–Bonnet gravity with logarithmic redshift functions

dc.contributor.author	Kumar, Jitendra
dc.date.accessioned	2026-03-11T06:49:25Z
dc.date.available	2026-03-11T06:49:25Z
dc.date.issued	2025
dc.description.abstract	This work delves into the characteristics of wormhole solutions in the context of 4𝒟 Einstein–Gauss–Bonnet gravity. The redshift function, 𝜒(𝑟), and the shape function, 𝜑(𝑟), are key components of the metric and play acrucial role in modeling wormholes. Our exploration reveals the influence of 4𝒟 Einstein–Gauss–Bonnet gravity attributes, providing valuable insights into the formation of wormholes. Additionally, we analyze energy conditions and fundamental features of wormhole configurations. The Gauss–Bonnet coupling constant, 𝛶, is shown to significantly affect the stability of wormhole geometries, especially when the throats are supported by exotic matter. Stability analysis using the Tolman–Oppenheimer–Volkoff equation confirms that these solutions meet equilibrium conditions. Moreover, the deflection angle increases near the throat, where the gravitational field is strongest, and approaches zero at larger distances, indicating minimal light bending in weak
dc.identifier.uri	http://cuh.ndl.gov.in/handle/123456789/1751
dc.language.iso	en
dc.title	Embedded class one analysis of wormhole configurations in 4𝒟 Einstein–Gauss–Bonnet gravity with logarithmic redshift functions

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