Abstract
Employing Poincaré degrees of freedomM jk=(¯K,¯J) andP k=(E,¯p) transforming linearly (but inhomogeneously) under the action of the Poincaré group we define a number of quantities which we later identify with physical observables. The identifications are consistent with the nonrelativistic limit and with other requirements following from the Poincaré covariance. Next, we treat a free relativistic particle as composed of two interacting parts. Relativistic quantum commutation relations for their Poincaré algebras and a kind of (inverse) relativistic correspondence principle are used to generate (quasi-) classical equations of their relative motion. A simple example based on these ideas is explicitly solved.
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I am indebted to Prof. B. Laurent, Dr. S. Flodmark, and Prof. I. Fischer-Hjalmars for pointing this out to me.
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Bette, A. Relativistic interactions without fields or potentials. Int J Theor Phys 19, 877–888 (1980). https://doi.org/10.1007/BF00671479
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DOI: https://doi.org/10.1007/BF00671479