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We combine the Macroscopic Fluctuation Theory and the Inverse Scattering Method to determine the full long-time statistics of the energy density averaged over a given spatial interval, in a freely expanding Kipnis-Marchioro-Presutti (KMP) lattice gas on the line, following the release at of a finite amount of energy at the origin. In particular, we show that, as time goes to infinity at fixed , the large deviation function of approaches a universal, -independent form when expressed in terms of the energy content of the interval . A key part of the solution is the determination of the most likely configuration of the energy density at time , conditional on .

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