Leptophilic ALPs with m_a > f_a can explain the electron anomalous magnetic moment tension over a large parameter space and are testable via μ→e conversion.
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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.
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Crossing into the $m_a > f_a$ Region for Leptophilic ALPs
Leptophilic ALPs with m_a > f_a can explain the electron anomalous magnetic moment tension over a large parameter space and are testable via μ→e conversion.
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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.