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Astron. Astrophys. 327, 867-889 (1997) 1. IntroductionThe theory of scale relativity (Nottale 1993a) is founded on the
realization that the whole of present physics relies on the implicit
assumption of differentiability of the space-time continuum. Giving up
the a priori hypothesis of the differentiability of coordinates has
important physical consequences: one can indeed demonstrate
(Nottale 1993a,
1994a,
1995a) that a continuous but nondifferentiable
space-time is necessarily fractal. Here the word fractal
(Mandelbrot 1975,
1983) is taken in a general meaning, as defining a
set, object or space that shows structures at all scales. More
precisely, one can demonstrate that a continuous but nondifferentiable
function is explicitly resolution-dependent, and that its length
It is important to be by now more specific about the precise meaning of the withdrawal of the axiom of differentiability. That does not mean that we a priori assume that the coordinates are not differentiable with certainty, but instead that we consider a generalized framework including all continuous functions, those which are differentiable and those which are not. Thus this framework includes the usual differentiable functions, but as very particular and rare cases. It is an extension of the usual framework, so that the new theory is expected, not to contradict, but instead to generalize the standard theory, since standard differentiable physics will be automatically included in it as a special case. An historical example of such an extension is the passage to curved spacetimes in general relativity, which amounts to giving up the previous implicit assumption of flatness of Euclidean geometry, and which anyway includes flat spacetimes in its description. Since a nondifferentiable, fractal space-time is explicitly resolution-dependent, the same is a priori true of all physical quantities that one can define in its framework. (Once again, this means that we shall formally introduce such a scale-dependence as a generalization, but that the new description will also include the usual scale-independence as a special case, in a way similar to the relations between statics and kinematics: statics is a special, degenerate case of the laws of motion). We thus need to complete the standard laws of physics (which are essentially laws of motion and displacement in classical physics) by laws of scale, intended to describe the new resolution dependence. We have suggested (Nottale 1989, 1992, 1993a) that the principle of relativity of Galileo and Einstein, that is known since Descartes and Huygens to be a constructive principle for motion laws, can be extended to constrain also these new scale laws. Namely, we generalize Einstein's (1916) formulation of the principle of relativity, by requiring that the laws of nature be valid in any reference system, whatever its state. Up to now, this principle has been applied to changes of state of the coordinate system that concerned the origin, the axes orientation, and the motion (measured in terms of velocity, acceleration, ...) . In scale relativity, the space-time resolutions are not only a characteristic of the measurement apparatus, but acquire a universal status. They are considered as essential variables, inherent to the physical description. We define them as characterizing the "state of scale" of the reference system, in the same way as the velocity characterizes its state of motion. The principle of scale relativity consists of applying the principle of relativity to such a scale-state. Then we set a principle of scale-covariance, requiring that the equations of physics keep their simplest form under resolution transformations (dilations and contractions). The domains of application of this theory are typically the
asymptotic domains of physics, small length-scales and small
time-scales Initially, the theory of scale relativity was mainly an attempt at refounding quantum mechanics on first principles (Nottale 1993a). We have demonstrated that the main axioms of quantum mechanics can be recovered as consequences of the principle of scale relativity, and that the behavior of the quantum world can be understood as the various manifestations of the non-differentiability and fractality of space-time at small scales (Nottale 1993a, 1994a, b, 1995c, 1996a). Moreover, the theory allows one to generalize standard quantum mechanics. Indeed, we have shown that the usual laws of scale (power law, self-similar, constant fractal dimension) have the status of "Galilean" scale laws, while a full implementation of the principle of scale relativity suggests that they could be medium scale approximations of more general laws which take a Lorentzian form (Nottale 1992, 1993a). In such a "special scale relativity" theory, the Planck length- and time-scale becomes a minimal, impassable scale, invariant under dilations and contractions, which replaces the zero point (since owning all its physical properties) and plays for scales the same role as played by the velocity of light for motion (see Appendix B). In this new framework, several still unsolved problems of fundamental physics find simple and natural solutions: new light is brought on the nature of the Grand Unification scale, on the origin of the electron scale and of the electroweak scale, on the scale-hierarchy problem, and on the values of coupling constants (Nottale 1993a, 1994a, 1996a); moreover, our scale-relativistic interpretation of gauge invariance allowed us to give new insights on the nature of the electric charge, then to predict new mass-charge relations for elementary particles (Nottale 1994a, b, 1996a). The same approach has been applied to the cosmological domain,
leading to similar conclusions. Namely, new special scale-relativistic
dilation laws can be constructed, in terms of which there exists a
maximal length-scale of resolution, impassable and invariant under
dilations. Such a scale can be identified with the scale
In the present series of papers, we shall not consider the
consequences of this new interpretation of the cosmological constant,
which mainly apply to the domain of very large scales
( We are mainly concerned here with the physical description of
systems when they are considered on very large time-scales. As we
shall see, this question is directly related to the problem of chaos.
It is indeed now widely known that most classical equations describing
the evolution of natural systems, when integrated on sufficiently
large times, have solutions that show a chaotic behavior. The
consequence of strong chaos is that, at time-scales very large
compared with the "chaos time", But we shall suggest in the present paper an even more profound
connection between chaos and scale relativity. After all, chaos has
been discovered (Poincaré 1892) as a general, empirical
property of the solutions of most classical equations of physics and
chemistry, when applied to natural systems in all their complexity.
But this does not mean that we really understand its origin. On the
contrary, it is rather paradoxical that deterministic equations, built
in the framework of a causal way of thinking (one gives oneself
initial conditions in position and velocity, then the evolution of the
system is predicted in a totally deterministic way), finally lead to a
complete loss of predictability of individual trajectories. Our first
proposal (Nottale 1993a,
b) has therefore been (following the above
reasoning) to jump to a non-deterministic description, that would act
as a large-time scale approximation. We suggest in the present
paper to reverse the argument, and to take into account the particular
chaos that takes its origin in the underlying, non-differentiable and
fractal character of space-time, since, as we shall see, it is
expected to become manifest not only at small scales but also at very
large length-scales and time-scales. The advantages of this
viewpoint reversal are important: In the present paper, we shall first be more specific about our motivations for constructing such a new theory (Sect. 2), then we shall describe our general method (Sect. 3), and apply it to the fundamental equations used in several domains of fundamental physics having astrophysical implications (Sect. 4). Additional informations, in particular about the general framework of which the present developments are a subset, are given in Appendices A and B. Paper II will be specially devoted to the application of our theory to gravitational structures, and Paper III to a first comparison of our theoretical predictions with observational data. ![]() ![]() ![]() ![]() © European Southern Observatory (ESO) 1997 Online publication: April 6, 1998 ![]() |