Wormhole solutions in $f(Q,T)$ gravity with a radial dependent B parameter
Moreshwar Tayde, Joao R. L. Santos, Julia N. Araujo, P.K. Sahoo

TL;DR
This paper explores new traversable wormhole solutions within $f(Q,T)$ gravity, demonstrating their viability with exotic strange matter and satisfying key energy conditions, thus expanding the landscape of alternative gravity models.
Contribution
It introduces novel wormhole solutions in $f(Q,T)$ gravity with a radial dependent parameter, incorporating strange matter and analyzing energy conditions.
Findings
Wormhole solutions satisfy SEC and WEC energy conditions.
Traversable wormholes are viable in $f(Q,T)$ gravity with strange matter.
New scenarios confirm the existence of stable wormholes in the modified gravity context.
Abstract
A possible astrophysical object to be found in General Relativity is the wormhole. This special solution describes a topological bridge connecting points in two distinguished universes or two different points in the same universe. Despite it was never observed so far, is desired to find traversable wormholes, i.e. wormholes which have a throat at which there is no horizon. However, the traversable wormhole constraints yield solutions that violate all the energy conditions in General Relativity. In the last few years, several models to describe gravity beyond CDM have been proposed. Then, it is relevant to look for wormhole solutions for these new theories. In this study, we are going to unveil new wormhole solutions for the so-called gravity. This theory of gravity is based on the non-metricity scalar , which is responsible for the gravitational interaction together…
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Geophysics and Gravity Measurements
