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Submitted on 1 Jan 1985

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Jumping particle model. A study of the phase space of a non-linear dynamical system below its transition to

chaos

Pi. Pierański, Z. Kowalik, M. Franaszek

To cite this version:

Pi. Pierański, Z. Kowalik, M. Franaszek. Jumping particle model. A study of the phase space of a non- linear dynamical system below its transition to chaos. Journal de Physique, 1985, 46 (5), pp.681-686.

�10.1051/jphys:01985004605068100�. �jpa-00210008�

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Jumping particle model. A study of the phase space of a non-linear

dynamical system below its transition to chaos (+)

Pi. Piera0144ski (*), Z. Kowalik and M. Franaszek

Institute of Molecular Physics, Smoluchowskiego 17, 60-179 Poznan, Poland (Reçu le 16 mai 1983, révisé le 28 novembre 1984, accepti le 3 janvier 1985)

Résumé.

2014

On observe directement les cascades de bifurcations d’un système dynamique

non

linéaire. Les résultats

expérimentaux sont comparés

aux

prédictions de l’application de Zaslavskij-Rachko. On montre la coexistence d’un certain nombre de modes individuels.

Abstract.

2014

Bifurcation cascades in

a

non-linear dynamical system are directly observed. Experimental results are compared with predictions of the Zaslavskij-Rachko mapping. Experimental evidence for coexistence of

a

number of individual modes is provided.

Classification Physics Abstracts

03.20

1. Introduction.

Period doubling [1] and intermittency [2] are the two

basic phenomena which, as predicted theoretically,

were found to bridge chaos and order in a number of

experimental systems [3] which display a transition

from periodic to chaotic behaviour (1).

It is the aim of the present paper to describe an expe- rimental study of the phase space of a non-linear dyna-

mical system, whose simplicity enables one to interpret

in plain terms all phenomena which appear in the sys-

tem before it enters the region of chaos.

2. ExperimentaL

The experimental model we designed, described in detail previously [5], can be seen as a practical realiza-

tion of a modification of the Fermi-Ulam thought experiment [4]. The model (see Fig. 1) consists of a

(+) Work carried out under Project MR-I.9.

(*) Present address : Universite Paris-Sud, Laboratoire de Physique des Solides, Batiment 510, 91405 Orsay, France.

(1) It seems worth reminding, however, that real physical systems may reach the chaotic regime in ways which are different from the two above-mentioned scenarios. For

instance, recent systematic studies of the Rayleigh-Benard instability performed by M. Dubois, P. Berg6 and V. Cro- quette [10] with the

use

of

an

ingenious technique (which

enables one to observe directly the Poincare section of the

phase space of the system) show that the hydrodynamical system may reach its chaotic regime via

a

biperiodic oscilla-

tion.

steel sphere jumping perpendicularly on a slightly

concave, horizontal surface of a lens made to vibrate

harmonically by a loudspeaker to the membrane of which the lens is fixed. The loudspeaker is supplied

with a sine-shaped signal from an audio generator at a frequency v - 101 : 102 Hz.

Complex AC signals from the microphone, which

«listens to the vibrating surface-steel sphere colli-

sion sounds, are shaped into identical pulses which

modulate the electron beam intensity (Z-coordinate

of the beam). Thus, each collision is marked on the

oscilloscope screen by a brighter spot. The recording system is provided by a saw-tooth generator synchro-

nized by the main audio generator. The piece-wise

linear signal from the saw-tooth generator controls the Y-coordinate of the oscilloscope beam; thus (at an appropriate choice of the synchronization phase) the

Y-coordinate follows the actual phase 9=0 [mod 2 n]

(where, 0 = 2 nvt, t being the real time) of the surface velocity function - A sin 0. As a result, the Y-coor-

dinate of the bright spot which marks the Oi collision

moment is proportional to 0-i. Obviously, when the

collision sequence is periodic (and commensurate with the surface vibration frequency) one observes on

the oscilloscope screen a standing set of points the

number and distribution of which represents comple- tely the sequence.

To record behaviour of a jumping mode versus the

vibration amplitude A, the X-coordinate of the beam is controlled by an AC/DC converter supplying a DC voltage proportional to A. Thus, using a slow sweep

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01985004605068100

(3)

682

Fig. 1.

-

Experimental set-up. Description in text.

of the amplitude one is able to study the history of

a jumping mode versus A. Photographs presented in figures 2 and 3 were obtained using this technique.

The intensity of the oscilloscope .image and para- meters of the photographic exposure were chosen such that a clear recording of the collision sequence was

obtained only when the sequence was periodic; any chaotic sequence of collisions produced an image too dispersed to be recorded by the photographic film.

3. Results.

It has been found that in the experimental conditions

we created the sphere can easily be put into a number of jumping modes, whose evolution versus A is recorded

in figure 2.

The simplest mode M(’) recorded in figure 2a con-

sists of a sequence of equidistant (in time) jumps

between consecutive maxima of the surface displace-

ment function, i.e. its period T is equal to that of the surface vibration. Consecutive collision moments

Oi are located at a phase 6 of the surface vibration such that the amount of momentum gained by the particle during the collisions compensates its losses due to

dissipation (inelastic collisions, viscous friction during

the particle’s flight, etc...).

Elementary analysis shows [5], that the M(l) mode

can be excited and sustained but at 9’ e (7c/2,7r).

Consequently the M(l) mode is described by relation :

e(l){A) denotes the shift of the collision phase from

% = n, where it would be located in absence of any

dissipation. Obviously, there exists a minimum value

A 0 (’) of the surface vibration amplitude A below which

the M(l) mode cannot be sustained. When A -+ AÓ1) (from above) then e(1 )(A)

-+

n/2, i.e. the collision

phase shifts to the point of maximum surface velocity.

Below the point the M(l) mode must decay.

As seen in figure 2a, the M(1) mode is bounded also from above. Beyond A

=

A11) the mode becomes unstable giving way to its modulated version M(1,2) in which a jump shorter than T is followed by a longer jump. The periodicy in 2 T is preserved. The M(1,2)

mode is described by :

_ - _ ,,, .

where 01, ljJ2 > 0.

The splitting ql

i

+ ljJ 2 increases with A and at Ai 1) the

M (1, 2) mode becomes unstable, bifurcating into the

second order modulation mode M(1,2,2) the periodicity

of which is preserved in 4 T. The story repeats itself

once more, but the third period doubling occurring

at an Aá1) results in a mode which proves to be on the verge of destruction by noise. The fourth bifurcation has never been observed; instead the system enters the region of chaos.

A simple reasoning convinces one that the equi-

distant jumps of the particle may take place not only

between consecutive, but also between every second,

every third etc. periods of the surface vibration.

Figures 2b and 2c provide evidence for these kinds of

equidistant jumping modes. A strong enough perturba-

tion (e. g. a knock at the loudspeaker membrane) may

drive the particle trajectory from the attractor of the

(4)

Fig. 2.

-

Bifurcation diagrams of the basic jumping modes : M(1), M(2), M(3); a, b,

c -

experimental recordings; a’, b’, c’

-

theoretical plots calculated for k

=

0.86. Arrows in the experimental recordings indicate positions of the bifurcation points

as

predicted by numerical calculations.

M(1) mode into basins of its 2 T or 3 T versions : M(2) or M(3). Due to the doubled (or triple) momentum

with which the particle arrives, in these modes, at

the vibrating surface dissipation losses are propor-

tionally higher and, consequently, the collision phase

must be shifted to phases of higher surface velocity, i.e.

closer to 9

=

n12. Figures 2b and 2c indicate clearly

that this is the case.

Energetic collisions which take place in the high velocity modes perturb considerably the sine-shaped

motion of the collision surface (generally, the level

of noise increases) which destroys some of the more

subtle versions of the modes. Thus, as seen in figure 2b

second bifurcation vanishes from the diagram of the M(2) mode, while in the case of the M(3) mode (Fig. 2c)

even the first bifurcation is hardly visible.

Let us point out that diagrams of the M(2 ) and M(3)

modes are very difficult to record in a single sweep,

- Fig. 3.

-

M(1,3) modulation mode;

a - an

overall view.

Experimental recording obtained for decreasing A ; b, c, b’,

c’

-

experimental and theoretical plots of the M(1,3) mode

under decreasing and increasing vibration amplitude. Direc-

tions of the A sweep

are

indicated by arrows in the b’ and c’

plots. Theoretical curves have been calculated for k

=

0.86.

(5)

684

since one can never start the sweep from the AÓ1)

threshold, where the modes decay, but the starting

value of A must be located in a safe distance from it.

Thus, diagrams presented in figures 2b and 2c have

their initial parts cut off. The diagram of the M(1)

mode presented in figure 2a has been recorded for

decreasing A. This is possible, since sometimes the particle enters the M(1) solution spontaneously.

Equidistant jumping modes M(1), M(2), M(3) and

their period doubled versions were not the only modes

we observed. Figure 3 presents evidence for a diffe- rent solution. Namely, before the M(1) mode becomes unstable (giving way to its period doubled version

M(1,2») another possibility appears. The particle does

not take this route spontaneously but a patient persua- sion (knocking at the loudspeaker membrane) forces

it to do so. As shown in the figure the new mode denot- ed by M(1,3) can be seen as a period-three modulation

of the basic M(1) mode. Moments of consecutive colli- sions in this mode are given by

where

As seen in figure 3c, the new mode follows its own

period doubling route, from which we observe only

the first step i.e. the M(1,2,3) mode. The Mini,3,-..) mode is obviously metastable and, as soon as its period doubling route ends, the particle comes back to the

main M(l) mode, which in the meantime has bifurcat- ed on its own. Figure 3 explains clearly why we do not

observe the particle to enter the M(1,3) solution spon-

taneously. As seen in the figure, branches of the mode appear in a jump-like manner and an energetic fluctua-

tion is needed to cross the gap. (The M(2,3) mode has

been also observed.)

4. Theoretical.

As shown before [5], the jumping particle model may be approximated well by a dissipative (i.e. area- contracting) version of the standard mapping :

which originating from the old Fermi-Ulam accelera- tion problem [4] has been modified in a number of ways [6] to cope with a whole variety of different pro- blems in non-linear dynamics. In its dissipative version

the mapping is often referred to as the Zaslavskij-

Rachko mapping [7].

Elementary algebra provides expressions for the

A(’)(k) and A(’)(k) thresholds which limit (from below

and from above) all equidistant jumping modes M(a) :

where a denotes the number of consecutive surface vibration periods over which the particle jumps in the M(a) mode. Figure 4 presents a plot of the r(1)

=

;.B1)/

A(’) ratio, which can be conveniently used to determine

the value of the dissipation parameter k. As indicated in the figure, F (1)

=

4.06 (found from data recorded in Fig. 2a) leads to k

=

0.86.

The simplicity of equation (4) enables one to simulate numerically any jumping mode and its evolution ver- sus A. Consequently, the bifurcation diagram of any M(a) mode can be easily obtained. Figures 2a’, b’, c’

present such diagrams calculated for k

=

0.86. The

same value of k has been also used in calculating plots presented in figure 3.

As seen in the figures, good qualitative agreement has been obtained in all cases. Two significant discre- pancies seem worth pointing out :

1) The difference in splitting of the upper and lower branches of the M(1,2,2) mode is much less distinct in the experimental diagram than in its theoretical counterpart, where it is striking.

2) The two lower branches of the M(1,3) mode

apparently cross each other in the experimental record- ing, while no such effect is seen in the theoretical plot.

It seems that the discrepancies may stem from an

essential simplification which one makes describing

the experimental model by mapping (4). Namely, in

the experiment the collision surface truly vibrates while

equations of mapping (4) describe a thought experi-

ment in which the collision surface provides momen-

tum to the particle without changing its own position.

Whether this is the proper explanation we do not know

at present, but numerical calculations we are perform- ing should answer the question soon.

Fig. 4. - r(1)(k) and b(l)(k) plots calculated numerically

from equation (5). Arrows indicate the experimental value

of r (1) and resulting value of k.

(6)

Feigenbaum 6 (1) = (A(l) - À.B1»)/(À.1) - A(’)). As shown in figure 4,

the ratio depends strongly on k and for k = 0.86

(determined from the r(1)(k) dependence) 6(,’) 7.15.

Arrows in figure 2a indicate the values of A at which the second and third bifurcations should take place (position A(1) of the first bifurcation has been used to fix the scale of the theoretical drawings). As seen, the agreement is not bad.

The value of k we determined in the present study

differs considerably from that determined previously (k

=

0.2 [5]). The difference is, however, well justified

since the experimental system has been redesigned so

as to reduce dissipation : we applied a bigger loud- speaker (diameter of the membrane 0

=

25 cm, pre-

viously 4>

=

10 cm) and a smaller steel sphere (dia-

meter Q

=

3 mm, previously J

=

4 mm).

Results of the experimental study of the M(1,3)

mode we report in the present paper are in agreement with what we intuitively predicted previously [5].

Namely, as A increases in the k

=

1 area-preserving mapping, the (7r, z) centre of its lJi+ 1 (lJ) map gives

birth to consecutive modulations of the main jumping

mode (represented by the centre). The period L of the newly born modulations is given by :

L

=

2 n/arccos (1

-

A/2) (7) thus, as £ increases, L shortens (e.g. for

=

1, 2, 3, 4,

L

=

5, 4, 3, 2 respectively). As the (n, n) centre gives

birth to a new modulation mode; those born pre-

viously (seen in the map as eliptic orbits surrounding

the (n, n) centre) move away from it. The fate of a

modulation mode depends on whether it is commensu- rate or not. Those of a low order commensurability

soon fix their phase turning into belts of smaller islands which represent secondary modulations imposed on

the primary one. For instance, the L

=

6 mode born

at A

=

1.5 turns into a well visible belt of six islands located on the periphery of the main island (see Fig. 1 b in [5]).

When the dissipation is switched on (k 1), the mapping (4) becomes area-contracting and the (J i + 1 «(J i) map loses its periodicity. Elliptic orbits turn

into spirals converging onto centres of islands point

attractors with their basins are formed. Not all com- mensurate modulations survive the process. Every- thing depends on their order, distance from the (n, n) centre, dimensions of their own island and, of course, the level of dissipation. For k

=

0.86 which we manag-

figure [5],

not been observed; apparently, at this level of dissi-

pation the mode has been destroyed.

In general, effects of the dissipation on the landscape

of the k

=

1, ()i+ 1 «()¡) maps are far from trivial and

require careful analysis.

5. Conclusions.

It seems that the o la bille cahotante » (2) model we

have presented is one of the simplest physical objects

in which the period doubling cascade can be demons-

trated [8]. Due to the audio frequency range in which the bifurcating jumping modes are located, consecu-

tive bifurcations can actually be heard. This is of educa- tional value, since a few of the first period doubling

threshold can be determined without any sophisticated equipment enabling one to calculate both the dissipa-

tion factor k and the first convergence ratio 6"), though due to effects of noise (induced in the system by

the jumping itself) accuracy with which the latter value is determined is not high. The model, in general,

is not well suited for quantitative studies of the univer- sal aspects of the period doubling behaviour. In parti- cular, there is no chance of reaching such stages of the bifurcation cascade at which the convergence ratio would come close to its universal limit 61D

=

4.67.

The coincidence of the experimental value of 61

1

we

determined previously [5] with the universal limit b 1 °

must be seen as an effect of high dissipation. On the

other hand, the effects of noise are interesting on their

own [9], since no doubt they are present in any natural mechanical system which displays the period doubling

transition to a chaotic behaviour.

Acknowledgments.

We are indebted to Prof. J. Malecki for many stimulat-

ing discussions. A generous grant of computer time from the Institute of Nuclear Physics and Technology, AGH, Krakow, is gratefully acknowledged. In parti- cular, we thank Prof K. Przewlocki for his support.

One of us (P. P.) would like to thank his brother Pawel and other workers from Laboratoire de Phy- sique des Solides, Orsay, and Service de Physique du

Solide et de Resonance Magn6tique, Gif-sur-Yvette, for their -tiorts in keeping our scientific contacts alive.

(2) We

are

grateful to P. Berge for this apt term.

(7)

686

References

[1] FEIGENBAUM, M., J. Stat. Phys. 19 (1978) 25.

[2] MANNEVILLE, P., POMEAU, Y., Phys. Lett. 75A (1979) 1.

[3] See references [3] to [6] in [5].

[4] See e.g. : ZASLAVSKIJ, G. M., Statistical Irreversibility

in Nonlinear systems (in Russian), Nauka, Mos-

cow (1970).

[5] PIERA0144SKI, P., J. Physique 44 (1983) 573.

[6] LICHTENBERG, A. J., LIEBERMAN, M. A., Physica 10 (1980) 291.

[7] ZASLAVSKIJ, G. M., RACHKO, K. R., JETF 76 (1979)

2052.

[8] CROQUETTE, V., Pour la Science, December (1982).

[9] CRUTCHFIELD, J. P., FARMER, J. D., HUBERMAN, B. A., Phys. Rep. 92 (1982) 46.

[10] DUBOIS, M., BERGÉ, P., CROQUETTE, V., J. Physique

Lett. 43 (1982) L-295.

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