Derives a Boltzmann-like distribution over actions via maximum entropy subject to a mean-action constraint, producing a Markovian stochastic propagator that matches Brownian motion and remains covariant at relativistic speeds.
Then the normalization condition (D1) becomes c∆t N Z 1 −1 eα √ 1−u2 −1 du=1.(D2) Hence N=c∆t I(α)−2 ,I(α) = Z 1 −1 eα √ 1−u2 du.(D3)
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Stochastic dynamics from maximum entropy in action space
Derives a Boltzmann-like distribution over actions via maximum entropy subject to a mean-action constraint, producing a Markovian stochastic propagator that matches Brownian motion and remains covariant at relativistic speeds.