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where k is a constant that determines the throat radius of the wormhole, and l is a radial coordinate. We analyze the stability of this wormhole by considering perturbations of the metric.

The Morris-Thorne metric is a solution to Einstein's general relativity that describes a traversable wormhole. This metric is given by: downloadhub interstellar

ds^2 = -dt^2 + dl^2 + (k^2 + l^2)(dθ^2 + sin^2θ dφ^2) where k is a constant that determines the