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Covariant Newtonian limit of Lorentz space-times

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Abstract

The formulation of this limit given by Dautcourt [1] is slightly improved using the notions of Galilei manifold and Newtonian connection. It is then shown under what conditions the conservation equations ▽μ μα = 0 for an arbitrary relativistic continuum have the correct (also covariantly formulated) Newtonian limit. For electromagnetism one obtains a curved space generalization of the electric or magnetic Galileian theory of LeBellac and Lévy-Leblond [4] depending on whether the contravariant or the covariant Maxwell tensor is required to have a regular Galileian limit.

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References

  1. Dautcourt, G. (1964).Acta Phys. Polon.,65, 637.

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  3. Künzle, H. P. (1972).Ann. Inst. Henri Poincaré 17A, 337.

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  4. LeBellac, M., and Lévy-Leblond, J.-M. (1973).Nuov. Cimento,14B, 217.

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  5. Souriau, J.-M. (1974).Ann. Inst. Henri Poincaré,20AB.

  6. Toupin, R. A. (1958).Arch. Rat. Mech. Anal.,1, 181.

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Supported in part by the National Research Council.

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Künzle, H.P. Covariant Newtonian limit of Lorentz space-times. Gen Relat Gravit 7, 445–457 (1976). https://doi.org/10.1007/BF00766139

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