Traversable Wormhole Solutions in f (Q, Lm) Gravity
K. Suhasini, G. Ravi Kiran, N. S. Kavya, C. S. Varsha, and V. Venkatesha

TL;DR
This paper explores traversable wormhole solutions in a modified gravity theory with non-minimal matter-geometry coupling, analyzing specific shape functions, energy conditions, and geometric viability to demonstrate the theory's potential for supporting such exotic structures.
Contribution
It introduces new traversable wormhole solutions within $f( ext{Q}, ext{L}_m)$ gravity, analyzing their geometric properties and energy conditions, highlighting the role of non-minimal coupling.
Findings
Null energy condition is violated near the throat.
Traversability conditions are satisfied for chosen shape functions.
Non-minimal coupling influences wormhole geometry and matter distribution.
Abstract
We investigate traversable wormhole solutions within the framework of gravity, a symmetric teleparallel theory featuring non-minimal coupling between geometry and matter. Adopting a linear functional form , we derive the field equations for a static, spherically symmetric Morris-Thorne wormhole geometry with vanishing redshift function. Four distinct shape functions are considered: , (with ), and . The geometric viability of each configuration is verified through standard traversability conditions, including the flaring-out requirement and asymptotic flatness. We analyze the energy conditions and demonstrate that, consistent with known results in wormhole physics,…
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.
Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Noncommutative and Quantum Gravity Theories
