Traversable Wormholes and Energy Conditions with Two Different Shape Functions in $f(R)$ Gravity
Nisha Godani, Gauranga C. Samanta

TL;DR
This paper investigates traversable wormholes in $f(R)$ gravity using two different shape functions, analyzing their energy conditions and supporting the existence of wormholes with phantom fluid characteristics.
Contribution
It introduces a new shape function and studies wormholes with two shape functions in $f(R)$ gravity, analyzing energy conditions and cosmic expansion implications.
Findings
Energy density is positive in studied models.
All energy conditions are violated, supporting wormhole existence.
Equation of state indicates phantom fluid presence.
Abstract
Traversable wormholes, tunnel like structures introduced by Morris \& Thorne \cite{morris1}, have a significant role in connection of two different space-times or two different parts of the same space-time. The characteristics of these wormholes depend upon the redshift and shape functions which are defined in terms of radial coordinate. In literature, several shape functions are defined and wormholes are studied in gravity with respect to these shape functions \cite{lobo, saiedi, baha}. In this paper, two shape functions (i) and (ii) , are considered. The first shape function is newly defined, however the second one is collected from the literature\cite{cataldo}. The wormholes are investigated for each type of shape function in gravity with , where…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
