In f(R, L_m) gravity, charged wormholes satisfy radial NEC for wide E ranges but tangential NEC only for 0.1 ≤ E ≤ 0.6, with violations linked to throat formation and distinct matter profiles versus compact objects.
Sofue, Rotation curve and mass distribution in the galactic cen- ter—from black hole to entire galaxy—, Publications of the Astronomi- cal Society of Japan 65 (6) (2013) 118
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Energy Conditions and Stability of Charged Wormholes in $f(R, \mathscr{L}_m)$ Gravity: A Comparative Analysis with Compact Objects
In f(R, L_m) gravity, charged wormholes satisfy radial NEC for wide E ranges but tangential NEC only for 0.1 ≤ E ≤ 0.6, with violations linked to throat formation and distinct matter profiles versus compact objects.