Stress-energy tensor of quantized massive scalar fields in thermal states on zero-tidal wormholes satisfies Morris-Thorne conditions only for bounded masses and temperatures below a mass-dependent critical value.
The particle problem in the general theory of relativity
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Numerical non-perturbative stationary vacuum ring wormhole solutions invariant under throat reflections, with slow-rotation M ~ J^2, fast-rotation J = M^2, and limits mimicking extremal Kerr.
A 3-neck wormhole metric obtained via spherical inversion of a 3-torus is asserted to be an exact non-vacuum solution of Einstein's field equations with diagonal Ricci and stress-energy tensors.
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.
citing papers explorer
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Stress-energy tensor of quantized scalar fields in thermal states on a zero-tidal wormhole
Stress-energy tensor of quantized massive scalar fields in thermal states on zero-tidal wormholes satisfies Morris-Thorne conditions only for bounded masses and temperatures below a mass-dependent critical value.
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Stationary generalizations for the vacuum ring wormhole
Numerical non-perturbative stationary vacuum ring wormhole solutions invariant under throat reflections, with slow-rotation M ~ J^2, fast-rotation J = M^2, and limits mimicking extremal Kerr.
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Spacetime triple wormhole
A 3-neck wormhole metric obtained via spherical inversion of a 3-torus is asserted to be an exact non-vacuum solution of Einstein's field equations with diagonal Ricci and stress-energy tensors.
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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.