Abstract
At first we derive a field equation by means of essentially geometry free demands, that is, by means of a Cauchy-problem, superposition principle, finite propagation speed and a conservation law. These requirements characterise a symmetric hyperbolic system of partial differential equations of first order.
In what follows, the field equation will define the geometry of space-time (in the same way as light rays and point particles define ‘their’ geometry, cf. Ehlers, Pirani and Schild (1972)). A general discussion of the derived field equation leads to a metrical structure of Finslerian type, to the propagation of helicity states, to a path structure and to the propagation of spin states. We thereby investigate the concept of a generalised Clifford-algebra.
Specialisation to two light cones, two helicity and spin states and the requirement that there is at least one time-like group velocity, then leads to the usual Dirac equation which defines as its geometry a Riemann-Cartan spacetime with axial torsion only and interaction with the Maxwell field.
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Lämmerzahl, C. (1990). The Geometry of Matter Fields. In: Audretsch, J., de Sabbata, V. (eds) Quantum Mechanics in Curved Space-Time. NATO ASI Series, vol 230. Springer, Boston, MA. https://doi.org/10.1007/978-1-4615-3814-1_2
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DOI: https://doi.org/10.1007/978-1-4615-3814-1_2
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