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arXiv · 1802.01959

Collective classical motion on hyperbolic spacetimes of any dimensions

Ion I. Cotaescu
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Abstract

The geodesics equations on de Sitter and anti-de Sitter spacetimes of any dimensions, are the starting point for deriving the general form of the Boltzmann equation in terms of conserved quantities. The simple equation for the non-equilibrium Marle and Anderson-Witting models are derived and the distributions of the Boltzmann-Marle model on these manifolds are written down first in terms of conserved quantities and then as functions of canonical variables.

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Ion I. Cotaescu. 2018-02-06. Collective classical motion on hyperbolic spacetimes of any dimensions. https://doi.org/10.1142/s0217732319501657

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