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In this paper we consider the conservation laws for classical particles in . At first we parameterize a geodesic line and construct conserved quantities with analog of five dimensional Minkowski space-time . Consequently we change space to AdS-Beltrami space-time and write conserved quantities in the Beltrami coordinates. Finally we take a limit for small velocity and we get the conserved quantities in Lorentz-Fock space-time. And finally we give out the energy of the nonrelativistic noncosmological particle under the cosmological limit.

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