Supersymmetry alone does not ensure time-reversal invariance in Model A; an additional condition is required, but effective TRI emerges at large scales per FRG analysis, which also recovers Ising magnetization distributions.
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Derives closed 5D partial-wave Raman scattering amplitude via NS functions and computes non-vanishing dynamical ℓ=0 and static ℓ=1 scalar tidal Love numbers with RG running up to O(G²) for STBH.
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Supersymmetry Without Time-Reversal Invariance in Model A: A FRG perspective
Supersymmetry alone does not ensure time-reversal invariance in Model A; an additional condition is required, but effective TRI emerges at large scales per FRG analysis, which also recovers Ising magnetization distributions.
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5-Dimensional Gravitational Raman Scattering: Scalar Wave Perturbations in Schwarzschild-Tangherlini Spacetime
Derives closed 5D partial-wave Raman scattering amplitude via NS functions and computes non-vanishing dynamical ℓ=0 and static ℓ=1 scalar tidal Love numbers with RG running up to O(G²) for STBH.