Scale relativity

Scale relativity

Scale relativity is a theory of physics initially developed by Laurent Nottale, working at the French observatory of Meudon, near Paris, which extends special and general relativity with a new formulation of scale invariance preserving a reference length, postulated to be the Planck length, which becomes invariant under zoom. This requires abandoning the hypothesis of differentiability for space-time, instead suggesting that space-time has a fractal structure. The quantum/classical transition is replaced with a fractal/non-fractal transition, specifically a divergence in the length of quantum paths at short scale.

Galilean Scale Relativity

Observation and Motivation

Two everyday observations are, that if we look at an object at a very small distance, say through a microscope, than even the slightest movement of this object will appear very fast; if on the other hand we look up to the sky and follow the movement of a jumbo-jet we sometimes wonder why it doesn't fall down, because from this distance it appears to be almost standing still.
Is this a pure subjective perception? The passengers in the jet will say that the clouds rushing by prove that the plane is moving fast, whereas the earth below is nearly standing still. And if the 'object' under the microscope were an ant that just woke up from coma, it would observe itself moving - "relatively" to the surface it is bounded to - with merely a few centimeters per minute.
This reminds of the situation, where one walks inside a train. Oneself observes walking rather slow, while an observer outside will add the velocity of the train to the walking speed, and say that the person inside the train is walking fast "relatively" to the ground. A similar observation led Galileo to formulate a relativity principle of motion. Likewise the former observations led Nottale to formulate scale relativity.

Mathematical formulation

While Galilean relativity of "motion" can be expressed by differences:

v = v_2 - v_1 = (v_2 - v_0)-(v_1 - v_0)

The relativity of "scales" can be expressed by ratios:

ho = frac{ x_2 }{ x_1 } = left( frac{x_2}{x_0} ight) diagup left( frac{x_1}{x_0} ight)

This can be derived by taking the Perspective (visual) in account, which is the phenomena that as objects become more distant, they appear smaller, because their angular diameter (visual angle) decreases. Then an observer on the ground sees v ' as the tangential velocity v (observed inside the plane) scaled down by the ratio of r'/r , that's between radius r (distance to the observed movement) and r ' (distance to the projective plane, e.g. 'the window').

v'(r,r ')= frac{r '}{r } v quad Leftrightarrow quad ho = frac{ r ' }{ r } = frac{ v ' }{ v } = left( frac{r ' heta}{t} ight) diagup left( frac{r heta}{t} ight)

The last term follows from (*)
Now the difference between a jet flying in a circle from its own perspecitve , i.e. a rotation that our intuition would favor as a "real" movement, and a perspectively projected rotation conceived by a far away observer, is that
* in the real case the angular velocity omega is constant, while the "tangential velocity" depends on the radius v ;(r)= omega r = frac{ heta}{t} ; r (*)
* in the projective case the tangential velocity v (the speed the passengers observe) is constant, while here the "angular velocity" (a.k.a angular frequency) depends reciprocal on radius romega(r)= frac{1 }{r} v

That is a jet flying through your garden (small r) will have a much higher angular velocity, than one that is 'hanging' in the sky. Now what if r goes to zero? Then the angular velocity would become infinite for "any" non-zero v > 0 (ultraviolet catastrophe). This is the analog to infinite speed in Galilean Relativity, when one rides on a train that is riding on a train, ... ad infinitum. This leads to (Lorentzian) scale relativity that is analogous to special relativity.

(Lorentzian) Scale Relativity principle

The scale relativity extends to scales the reasoning made by Einstein on speeds in special relativity: just like a constant speed c= frac {1} {sqrt{varepsilon_0mu_0 in Maxwell's equations, which does not appear to depend on the speed of the observer, suggests that the law of combination of speeds must preserve this invariant, similalry, the appearance of a constant length ell_P = sqrt { frac {hbar G} {c^3} } in Schrödinger's equation suggests that the law of combination of scales must preserve this invariant. In other words, just like c is a physical speed limit, ell_P is a physical length limit.

Predictions and retrodictions

Scale relativity made a number of true predictions, as well as a number of retrodictions, both in cosmology and at small scale, including:

* Prediction of the location of exoplanets [http://luth2.obspm.fr/~luthier/nottale/ukresult.htm]
* Explanation of some observed large-scale structures [http://luth2.obspm.fr/~luthier/nottale/DaRochaNottaleL.pdf]
* Relation between mass and charge of the electron [http://luth2.obspm.fr/~luthier/nottale/ukmachar.htm]

See also

* Causal dynamical triangulation
* Conformal group
* Doubly special relativity
* Fractal cosmology
* Fractals
* Olbers' paradox
* Perspective (graphical)
* Scale invariance
* Theory of incomplete measurements

Links

* [http://luth.obspm.fr/~luthier/nottale/ Laurent Nottale's site]
* [http://luth.obspm.fr/~luthier/nottale/arIJMP2.pdf The original 1992 scale relativity article]
* [http://luth.obspm.fr/~luthier/nottale/ukdownlo.htm List of Papers Downloadable from the site]
* [http://www.amazon.com/dp/9810208782 Fractal Space-Time and Microphysics] , a book explaining the theory
* [http://arxiv.org/abs/0711.2418 Derivation of the postulates of quantum mechanics from the first principles of scale relativity] last article


Wikimedia Foundation. 2010.

Игры ⚽ Нужно решить контрольную?

Look at other dictionaries:

  • Scale invariance — In physics and mathematics, scale invariance is a feature of objects or laws that do not change if length scales (or energy scales) are multiplied by a common factor. The technical term for this transformation is a dilatation (also known as… …   Wikipedia

  • relativity — /rel euh tiv i tee/, n. 1. the state or fact of being relative. 2. Physics. a theory, formulated essentially by Albert Einstein, that all motion must be defined relative to a frame of reference and that space and time are relative, rather than… …   Universalium

  • Scale factor (cosmology) — The scale factor or cosmic scale factor parameter of the Friedmann equations is a function of time which represents the relative expansion of the universe. It is sometimes called the Robertson Walker scale factor.[1] It is the (time dependent)… …   Wikipedia

  • Scale factor (Universe) — The scale factor, parameter of Friedmann Lemaître Robertson Walker model, is a function of time which represents the relative expansion of the universe. It relates physical coordinates (also called proper coordinates) to comoving coordinates.: L …   Wikipedia

  • Doubly special relativity — (DSR) also called deformed special relativity or, by some, extra special relativity is a modified theory of special relativity in which there is not only an observer independent maximum velocity (the speed of light), but an observer independent… …   Wikipedia

  • Doubly-special relativity — (DSR) also called deformed special relativity or, by some, extra special relativity is a modified theory of special relativity in which there is not only an observer independent maximum velocity (the speed of light), but an observer independent… …   Wikipedia

  • Planck scale — In particle physics and physical cosmology, the Planck scale is an energy scale around 1.22 × 1028 eV (which corresponds by the mass–energy equivalence to the Planck mass 2.17645 × 10−8 kg) at which quantum effects of gravity become strong. At… …   Wikipedia

  • General relativity — For a generally accessible and less technical introduction to the topic, see Introduction to general relativity. General relativity Introduction Mathematical formulation Resources …   Wikipedia

  • Alternatives to general relativity — are physical theories that attempt to describe the phenomena of gravitation in competition to Einstein s theory of general relativity.There have been many different attempts at constructing an ideal theory of gravity. These attempts can be split… …   Wikipedia

  • Mass in special relativity — incorporates the general understandings from the concept of mass energy equivalence. Added to this concept is an additional complication resulting from the fact that mass is defined in two different ways in special relativity: one way defines… …   Wikipedia

Share the article and excerpts

Direct link
Do a right-click on the link above
and select “Copy Link”