Fields of singular probabilities are inherent to quantum mechanics, but what method determines the statistics of curve segments like random geodesics bounded by definite black hole singularities, horizons or observers? Have Feynman path integrals been of use there, and if so, how?(adsbygoogle = window.adsbygoogle || []).push({});

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# Probability of (geodesic) curvature configurations (in 4-D spacetime)

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