On the transition from the classical to the quantum regime in fractal space–time theory
L. Nottale
Chaos, Solitons & Fractals, 2005, vol. 25, issue 4, 797-803
Abstract:
In the scale-relativity theory, space–time is described as a nondifferentiable continuum and the trajectories as its geodesics. In such a space–time, the coordinates are defined as the sum of a ‘classical part’ that remains differentiable, and a fluctuating, ‘fractal part’, that is divergent and nondifferentiable. The nondifferentiable geometry has three minimal consequences, namely infinite number, fractality and irreversibility of geodesics. These three effects are accounted for by the introduction of three new terms in the total derivative acting on the ‘classical part’ of the coordinates. When it is written using this total derivative, Newton’s equation is integrated in terms of a Schrödinger equation. Such an equation is therefore both classical and quantum. In the present paper, we use this property to analyze the specific roles played by each of the individual contributions, in order to shed some light on the complicated transition from the classical to the quantum regime.
Date: 2005
References: View complete reference list from CitEc
Citations: View citations in EconPapers (4)
Downloads: (external link)
http://www.sciencedirect.com/science/article/pii/S0960077904007763
Full text for ScienceDirect subscribers only
Related works:
This item may be available elsewhere in EconPapers: Search for items with the same title.
Export reference: BibTeX
RIS (EndNote, ProCite, RefMan)
HTML/Text
Persistent link: https://EconPapers.repec.org/RePEc:eee:chsofr:v:25:y:2005:i:4:p:797-803
DOI: 10.1016/j.chaos.2004.11.071
Access Statistics for this article
Chaos, Solitons & Fractals is currently edited by Stefano Boccaletti and Stelios Bekiros
More articles in Chaos, Solitons & Fractals from Elsevier
Bibliographic data for series maintained by Thayer, Thomas R. ().