Static traversable wormhole solutions in $f(R,L_m)$ gravity

Abstract

In this study, we explore the new wormhole solutions in the framework of new modified $f(R,L_m)$ gravity. To obtain a characteristic wormhole solution, we use anisotropic matter distribution and a specific form of energy density. As second adopt the isotropic case with a linear EoS relation as a general technique for the system and discuss several physical attributes of the system under the wormhole geometry. Detailed analytical and graphical discussion about the matter contents via energy conditions is discussed. In both cases, the shape function of wormhole geometry satisfies the required conditions. Several interesting points have evolved from the entire investigation along with the features of the exotic matter within the wormhole geometry. Finally, we have concluding remarks.

arXiv commentChinese Journal of Physics accepted version

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• Investigating the dark energy phenomenon in $f(R,L_m)$ cosmological models with observational constraints
• Impact of dark matter galactic halo models on wormhole geometry within $f(Q,T)$ gravity
• Exploring wormhole solutions in curvature-matter coupling gravity supported by noncommutative geometry and conformal symmetry
• $f(Q,L_m)$ gravity, and its cosmological implications
• Moment of inertia and compactness of quark stars within the context of $f(R,T,L_m)$ gravity
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• Conformally symmetric wormhole solutions supported by non-commutative geometry in $f(Q,T)$ gravity
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• Evolving Wormholes in a Cosmological Background
• Energy Conditions and Stability of Charged Wormholes in $f(R,{\mathcal{L}}_m)$ Gravity: A Comparative Analysis with Compact Objects