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Quantum–classical transition in scale relativity

Marie-Noëlle Célérier et al 2004 J. Phys. A: Math. Gen. 37 931-955   doi: 10.1088/0305-4470/37/3/026  Help

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Marie-Noëlle Célérier and Laurent Nottale
LUTH, CNRS, Observatoire de Paris-Meudon, 5 place Jules Janssen, 92195 Meudon Cedex, France
E-mail: marie-noelle.celerier@obspm.fr and laurent.nottale@obspm.fr

Abstract. The theory of scale relativity provides a new insight into the origin of fundamental laws in physics. Its application to microphysics allows us to recover quantum mechanics as mechanics on a non-differentiable (fractal) spacetime. The Schrödinger and Klein–Gordon equations are demonstrated as geodesic equations in this framework. A development of the intrinsic properties of this theory, using the mathematical tool of Hamilton's bi-quaternions, leads us to a derivation of the Dirac equation within the scale-relativity paradigm. The complex form of the wavefunction in the Schrödinger and Klein–Gordon equations follows from the non-differentiability of the geometry, since it involves a breaking of the invariance under the reflection symmetry on the (proper) time differential element (ds ↔ −ds). This mechanism is generalized for obtaining the bi-quaternionic nature of the Dirac spinor by adding a further symmetry breaking due to non-differentiability, namely the differential coordinate reflection symmetry (dxμ ↔ −dxμ) and by requiring invariance under the parity and time inversion. The Pauli equation is recovered as a non-motion-relativistic approximation of the Dirac equation.

PACS number: 03.65.Pm

Print publication: Issue 3 (23 January 2004)
Received 3 June 2003
Published 7 January 2004

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