We show that it is possible to go beyond the simple kinematical aspects of the analog models of gravity. We exhibit the form of the Lagrangian that describes the dynamics of a self-interacting field φ as an interaction between φ and its associated effective metric ĝμν. In other words the non-linear equation of motion of the field may be interpreted as the gravitational influence on φ by its own effective metric which, in our scheme becomes an active partner of the dynamics of φ.
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Novello et al. (2011) studied this question.
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