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An exact Kerr-like rotating Morris--Thorne wormhole: throat, ergoregion and equatorial shadow slice
We construct an exact Kerr-like rotating extension of the zero-redshift Morris--Thorne wormhole in a Teo-type stationary, axisymmetric ansatz. The Einstein equations for an anisotropic source comoving with zero angular momentum observers fix $\mathcal{K}(r)=r^2+a^2$ and reduce frame dragging to a ra
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