Exploring Traversable Wormholes in $f(Q)$ gravity: Shadows and Quasinormal modes
General Relativity and Quantum Cosmology
2025-04-29 v1
Abstract
The present work deals with some WH solutions in gravity theory for non-constant red-shift function subject to a power law model of , being the non-metricity scalar. Important properties of a WH configuration like the asymptotic flatness, traversability, flairing out condition and energy conditions have been checked for the obtained solutions. Shadows for these WHs have been determined and effect of non-metricity has been discussed. Finally, the paper gives an essence of Quasinormal modes and grey body factors for traversable WHs in general and wormholes in particular indicating a distinct signature of non-metricity influencing these observational tools.
Keywords
Cite
@article{arxiv.2504.19282,
title = {Exploring Traversable Wormholes in $f(Q)$ gravity: Shadows and Quasinormal modes},
author = {Madhukrishna Chakraborty and Subenoy Chakraborty},
journal= {arXiv preprint arXiv:2504.19282},
year = {2025}
}
Comments
23 pages, 10 figures