中文

Generalized macroscopic Schrodinger equation in scale relativity

广义相对论与量子宇宙学 2007-05-23 v1

摘要

The scale transformation laws produce, on the motion equations of gravitating bodies and under some peculiar assumptions, effects which are anologous to those of a "macroscopic quantum mechanics". When we consider time and space scales such that the description of the trajectories of these bodies (planetesimals in the case of planetary system formation, interstellar gas and dust in the case of star formation, etc...) is in the shape of non-differentiable curves, we obtain fractal curves of fractal dimension 2. Continuity and non-differentiability yield a fractal space and a symmetry breaking of the differential time element which gives a doubling of the velocity fields. The application of a geodesics principle leads to motion equations of Schrodinger-type. When we add an outside gravitational field, we obtain a Schrodinger-Poisson system. We give here the derivation of the Schrodinger equation for chaotic systems, i.e., with time scales much longer than their Lyapounov chaos-time.

关键词

引用

@article{arxiv.gr-qc/0505012,
  title  = {Generalized macroscopic Schrodinger equation in scale relativity},
  author = {Marie-Noelle Celerier and Laurent Nottale},
  journal= {arXiv preprint arXiv:gr-qc/0505012},
  year   = {2007}
}

备注

4 pages, oral communication in the framework of the 4eme Semaine de l'Astrophysique Francaise, Paris, 2004