We computethe transmission properties of electromagnetic (EM), gravitational wave, and static gravitational perturbations through geometric throats in spherically symmetric spacetimes. On the ultrastatic Ellis-Bronnikov background, decomposition of the four-dimensional Maxwell equations into vector spherical harmonics yields an effective Schrödinger problem with centrifugal barrier $V_{\ell }^{(\mathrm{EM})}=\ell (\ell +1)/({\sigma }^2+r_0^2)$ peaked at the throat. For the lowest physical EM mode ($\ell =1$), frequencies below the barrier-top frequency ${\omega }_{\max }=\sqrt{2}/r_0$ are strongly suppressed by sub-barrier tunneling. Gravitational wave perturbations ($\ell \ge 2$) see a qualitatively similar barrier and are likewise strongly suppressed below their respective barrier-top frequencies. By contrast, the static gravitational monopole ($\ell =0$), governed by the linearized Einstein equations on the same background, satisfies the source-free conservation law $(a^2{\mathrm{\Phi }}^{\prime }{)}^{\prime }=0$ with no potential barrier, yielding the exact solution $\mathrm{\Phi }\propto \arctan (\sigma /r_0)$. We extend these results to a one-parameter family of throat geometries with varying profile shapes, and to a reflected-Schwarzschild (Damour-Solodukhin-type) wormhole, demonstrating that the qualitative asymmetry—strong sub-barrier suppression for all propagating radiation ($\ell \ge 1$) versus polynomial attenuation for the static monopole ($\ell =0$)—is universal for static, spherically symmetric throats. Numerov integration, WKB estimates, and exact analytical solutions are compared throughout. The results establish a structural constraint-wave asymmetry arising from the multipole decomposition of the field equations, independent of the matter content sourcing the geometry, on a fixed background.

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• General relativity