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HAL Id: jpa-00247047

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Submitted on 1 Jan 1995

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Study of the Response to Pulses and Possible Prediction of Catastrophes

Muktish Acharyya, Bikas Chakrabarti

To cite this version:

Muktish Acharyya, Bikas Chakrabarti. Study of the Response to Pulses and Possible Prediction of Catastrophes. Journal de Physique I, EDP Sciences, 1995, 5 (2), pp.153-158. �10.1051/jp1:1995119�.

�jpa-00247047�

(2)

Classification

Physics Abstracts 91.30 -41.70

Short Communication

Study of the Response to Puises and Possible Prediction of Catastrophes

Muktisll

Acharyya(*)

and Bikas K.

Chakrabarti(**)

Salla Institute of Nuclear Physics,

1/AF,

Bidhannagar, Calcutta-700064, India

(Received

19 November 1994, revised 6 December 1994, accepted 14 December

1994)

Abstract. We show in a numerical study of the Burridge-Knopoff spring-block model of

earthquake, that if one applies very weak puises

(fixed

amount of

momentum)

to any particular

block at regular intervals and studies the response on the same block

(the

stress developed on

it), then accurate predictions of the timings of the imminent earthquakes are possible. This is

shown by studying the

(local)

puise susceptibility xp, which grows exponentially with the inverse of the time interval from the next

(global)

earthquake and saturates to a

(nonuniversal)

value

dependent on the model parameters

(fixed

for any particular serres of

earthquakes).

Considerable progress bas

recently

been made in the statistical

study

of trie

(fracture,

break- down or

earthquake) strength

or

magnitude

distribution of disordered solids

(porous media,

random composites

etc.),

of

granular packings,

or of trie

dynamical

mortels of

earthquake,

etc.

iii.

Several

simple

mortels

(at

a semi-microscopic

level)

bave been introduced for mechan- ical [2] and electrical [3] failure of such

randomly

disordered

media,

modelled

by randomly

disordered lattices with individual bonds

breaking irreversibly.

These theoretical results about the fracture or breakdown

strength

distribution etc. have also been checked in several exper- iments [4]. Failure processes

playmg

intrinsic roles in many systems of industrial importance and in many natural

catastrophic (disaster) phenomena,

the above mentioned statistical stud-

ies

establishing

the nature of

(non-self averaging) fracture-strength distribution,

its

(critical) fluctuations,

consequent power laws for trie average

strength

of such solids, etc.

iii,

are of extreme

importance. Although

a

significant

amount of literature has been

developed

for these studies of failure

strength distribution,

not much studies have been made

regarding

the

dynam-

ics of

microscopic

failures. Since the

microscopic

failures are irreversible and therefore

require

intermediate redistributions of the forces

(potentials),

the

equations

for the

dynamics

of failure

are

intrinsically

nonlinear and

dissipative.

The formulation and studies of such

equations

are

necessary for the search of any precursor effect of trie macroscopic failure

(if

trie macroscopic iailure is at most a critical and not a

fully

chactic

phenomenon).

In some recent

experiments

[5]

(*) E-mail: [email protected].

(**) E-mail: [email protected].

© Les Editions de Physique 1995

(3)

154 JOURNAL DE PHYSIQUE I N°2

on the

dynamics

of the cracks in thin

glass plates,

with thermal stresses, the

dynamics

seems

to under go a sequence of

(numerous

but

reproducible

instabilities

(not

sensitive to every de- tait of the fluctuations in initial

conditions).

The

dynamics

of fracture is thus observed to be

mostly

critical, on the verge of chaos

(depending

on the

velocity

of the crack

tip),

but not

quite chaotic [6]. Similar is the case for the

dynamical (Burridge-Knopoff

I?i

type)

mortels of

earthquake

[8], where also one gets the

Guttenberg-Richter

type power law for the

magnitude (strength)

variation of the

density

of

quakes (failure

distribution

being critical).

There has been indications

recently

[9] that some linear

properties je-g-,

the ratio of shear modulus and bulk

modulus)

show abnormal

(but universal) properties

near the breakdown

(macroscopic failure)

point of disordered solids. The detailed

study

of such

(linear)

response

(before breakdown)

would thus

provide prior

indication of the

catastrophe. However,

such

indications are found to be very selective and it bas not been

possible

to

study

in cases of important

catastrophic

failures like trie

earthquake

etc. The

study

of trie response of such

dynan1icaI

systems to short-duration

pulses

indicates that another kind of linear response,

namely

the

pulse-susceptibility [10],

has indeed universal behaviour near the fail,Jre

point.

It locates very

accurately

the

magnetic

transition

point

[10], and the

self-organized

critical

point~ il Ii

in various models [12]. We present here the results of our numerical

study

of

pulse

response in the uniform

Burridge-Knopoff

model

(Carlson-Langer

[8]

), indicating

the

possibility

of accurate

prediction

of

"earthquakes"

in the model.

It was seen

[loi,

both in a Monte Carlo

study

and in the numerical solutions of the mean field equation of motion of an

Ising

magnet, that if one

applies

an externat

magnetic

field

pulse

of

height hp

and width ôt on such a system m

equilibrium,

and if the response

magnetization pulse

is characterized

by

its

height

mp and

(half)

width At

(> ôt),

then both the

pulse susceptibility

xp =

mp/hp

and the width ratio

Rp

=

At/ôt incorporates (senses)

the

equilibrium (critical)

fluctuations of the

unperturbed

system. Both xp and

Rp

have

sharp divergence (peak)

at the order-disorder transition

point

of the

unperturbed (hp

=

0)

system. The

precision

in the location of the transition point can be made accurate with somewhat

langer pulse amplitude hp

and

extremely

small width ôt

(it

may be noted that the

pulse susceptibility

xp reduces to

the

ordinary susceptibility

as

hp

- o and ôt -

cc). Similary,

we found [12] in a computer simulation

study

that a

pulsed

addition of

"particles"

at a central site for a short time ôt in the BTW mortel

Ill],

after its avalanche

dynamics

has

stopped,

causes a successive series of local avalanches

persisting

for a response time At

(after

which the

dynanlics

stops

again).

The width ratio

Rp

=

At/ôt

was found to

diverge

with a power law as the average

"slope"

approaches

its

self-organized

critical value. In

fact,

one can

predict

quite

accurately

this critical.

value of the

slope by determming

the

extrapolated

average

slope

value where the inverse width ratio vanishes

(with

some

appropriate

power it

gives

linear

fit)

[12]. These successes of such

dynamic (pulse response)

measurements to locate the

(self-organized)

critical

points prompted

us to

investigate

similar response behaviour in the

earthquake

mortels [7, 8].

We have studied the

stick-slip

mortel of

earthquake

I?i. In this

mortel,

a linear array of N blocks, each

coupled

to its nearest

neighbours by

elastic

springs

and each connected to a

rigid

support

(at

the

top) by

elastic

springs,

is put on a

uniformly

moving

rough platform.

The equations of motion

(after

linear scale

transformation)

for any of the

blocks,

in the uniform

spring

constant

Burndge-Knopoff

mortel

(Carlson-Langer [8]),

can be written as:

d~Uj /dT~

= l~

(Uj+1 2Uj

+

Uj-i Uj #[20u

+

20(dUj /dT)], (1)

where, Uj

denotes the

displacement

of the

j-th

block from its

equilibrium position,

l~ is the ratio of the

spring

constants, a is a constant

(linear

transformation

factor),

and u is the uniform

pulling velocity

of the

rough (frictional) platform.

The nonlinear friction force is

given by

the

function

#(y)

=

sign(y) /(1

+

(y().

(4)

43 (Q)

io

3

0

o ioo00 20000 30000 40000 50000 60000 70000 60000 ?0000 >00000

o

~ (b)

4

z

g ~

~

-2

-4

-6

-o

o 10000 20000 30000 40000 so000 60000 70000 00000 yoo00 >ooooo

o.42

o4 (C)

om

o.30

1 ~

'~ '

~u .

~ l

i t

~' °'~ .j

Î ~ ÎÎr

h.

Î Î.

'~ ~, «.

.

~-

~

" *4~ °

o ioo00 20000 30000 40000 so000 G0000 >0000 H0000 90000 io0000

à

Fig. 1.

(a)

The time variation of the total elastic energy ET of the entire system.

(b)

shows the time variation of the elastic stress

(force)

/hUk developed on the block on which puise has been applied

(k

= 50

here).

(c) Time variation of inverse of the logarithm of the puise susceptibility (Xp). The linearly extrapolated saturation (+w 0.25) point

(time)

ofthis quantity gives the possible location

(time)

of the

imminent earthquake (compare with the major energy release points in

la)).

(5)

156 JOURNAL DE PHYSIQUE I N°2

In such

dynamical models,

the elastic stresses

(energy) developed

compete with the

(velocity dependent)

frictional force as

long

as the blocks stick to the

moving platform.

As it

fails,

there

occurs local failures

(shppage

for a finite number of

blocks)

or

global

failures

(simultaneus

slippage

of almost all the

blocks).

Initially the

(elastic)

energy mcreases and then

suddenly

falls

(causing

an avalanche or

quake) releasing

the excess elastic energy. As the released energy

is often more than the

"excess",

the system

again

becomes "sub-critical". The energy starts

0.38

0.35

1 0.34

'~

d

_~° 0.32

~W

0~3 4

, ,,

o,za # ,

~

, ,

,,

,

°"~~

-~L,~ -' Î-~-

~

Àooo0 42000 44000 w6000 wsooo soooo s2000 s4000

45

40

33

30

y~

25

20

io

~

40000 42000 44000 4600n 46000 50000 52000 54000

Îô

Fig. 2. A close view of the puise susceptibility variation near some major events or earthquakes

(enlarged

from a portion of Fig. 1). The time variation of the total elastic energy is also compared.

(6)

to build up

again

and after some time it

falls;

and the process continues. The strain energy released in any such failure is identified as the

magnitude (strength)

of the

earthquake

in this mortel system. We have solved the above set of

equations using

fourth-order

Runge-Kutta

method

taking

100 blocks

(N

=

100).

We have checked the distributions etc. of

earthquakes (the Guttenberge-Richter law)

for the mortel and

reproduced

the previous results [8] for various initial randomness of the block velocities and positions. We then

apply

very weak

pulses

to an

arbitrarily

chosen

(central; k-th)

block

(giving

fixed

arbitrary

ôÙk '~ 0.01for a duration ôt

+w

0.01;

k = 50

here)

at a

regular

time interval of T

= 1000 We then calculate

again

the total elastic energy

ET(" (£j l~(Uj+j 2Uj

+

Uj-j)~

+

U))/2)

at each time step and

plot

them

against

time

(Fig. la).

In all the

figures

we show the

typical

results for N

=

100,

l~ = 10, a

=

2.5,

u

= 0.01,

although

the

general

features we discuss are observed for any combinations of these parameter values. We also show in

Figure

1, the time variation of the elastic stress

AUk

(" l~(Uk+1

2Uk +

Uk-i) Uk) developed

on the k-th block, on which the

pulses

are

being applied (Fig. lb).

We also show there

lin Fig. lc),

the time variation of the

pulse

susceptibility

Xp, defined as xp =

AUjf /Uf

with

AUjf denoting

the maximum of AUk within the

pulse period

and

Uf

=

f/~ ôÙkdt.

We find xp +w

exp[A(t~~ /(t~~ t)]

for t < t~~, where

A(t~~

is a constant and t~~ denote the onset time of the n-th

earthquake

or

catastrophe.

It

may be noted

(from Figs.

lc and

2)

that

log(xp)~~ finally

saturates to a value around 0.25 before the

earthquakes.

Indeed the linear

extrapolation (with time)

to this saturation value of

(log xp)~~ gives quite

accurate prior indication about the location

(time)

of the imminent

earthquake (compare

with the

large

elastic energy releases for the entire system, shown in

s

+

«

4 -~

~

fi

_j_

x 3 , +

ce o

~ 4

-1'

2

+ +

4 +

4 ~~

0

-2 -1 s -1 -o,s 0 O,s 1,s

Loq [El

Fig. 3. Earthquake energy distribution, givmg the variation of the number N

(El

of quakes releasing

elastic energy E:

(Q)

For unperturbed system.

(+)

For the

same system perturbed with the application

of puises.

(7)

158 JOURNAL DE PHYSIQUE I N°2

Figs.

l and

2).

This is

quite

similar to the observation of Sahimi and Arbabi [9]

regarding

the convergence of the elastic constant ratio to a universal value before fracture.

However,

the saturation value

(for (log xp)~~)

in this case is found to be nonuniversal and

depends

on the parameters of the

dynamics

(1, a and u; the saturation value decreases as u

increases). Still,

the saturation value

being

fixed for a

particular

series of

earthquakes,

the above

procedure

for the

prediction

of the

earthquake

should be useful. In

Figure

3, we

just

show the distribution

NIE)

of

earthquakes releasing

energy E. The distribution indeed follows the

Guttenberg-Richter

type power law

decay (N(E)

+~

E~P, fl

+~ 2.0 1?i

),

both in the

unperturbed

system

(without puise)

and the system

perturbed by

weak

pulses (on

the k-th

block)

at

regular

intervals. It may be noted

however, although

the nature of the distribution remains

unchanged,

because of the sensitivity of the initial

conditions,

the exact

magnitude

and the

timings

of the

quakes

are

somewhat different in the two cases.

In summary, we find that

by applying

very weak

(mechanical) pulses

on any

particular block,

and

by studying

the local response

(studying

the

pulse susceptibility

Xp at the sanie

block),

one

can locate very

accurately

almost all

(more

than 75 per

cent)

of the

major (global) earthquakes (for

the entire

system)

in the

Burndge-Knopoff

type model.

Acknowledgments

We are

extremely

thankful to D. Stauffer for a careful

reading

of the manuscript and for critical remarks.

References

[ii

See e-g-, K. K. Bardhan, B. K. Chakrabarti and A. Hansen Eds., Nonlinearity and Breakdown in Soft Condensed Matter, Lecture notes m Physics, Vol. 437

(Springer-Verlag, 1994).

[2] Ray P. and Chakrabarti B. K., J. Phys. C18

(1985)

L185;

Chakrabarti B-K-, Chowdhury D. and Stauffer D., Z. Phys. B 62

(1986)

343;

Sahimi M. and Goddard J. D., Phys. Reu. B 33 (1986) 7848;

Sahimi M. and Arbabi S., Phys. Reu. B 47

(1993)

713.

[3] de Arcangelis L., Redner S. and Herrman H. J., J. Phys. France Lett. 46

(1985)

L585;

Duxbery P. M., Beale P. D. and Leath P. L., Phys. Reu. Lent. 57

(1986)

1052;

Duxbery P. M., Leath P. L, and Beale P. D., Phys. Reu. B 36

(1987)

367;

Beale P. D. and Srolovitz J. D., Phys. Reu. B 37

(1988)

5500;

Duxbery P. M, and Leath P. L., Phys. Reu. Lent. 72

(1994)

2805.

[4] Benguigm L., Ron P. and Bergman D. J., J. Phys. France 48

(1987)

1547;

Seiradzki K. and Li R., Phys. Reu. Lent. 56

(1986)

2509;

Benguigui L., Phys. Reu. B 38

(1988)

7211;

Li R. and Seiradzki K., Phys. Reu. Lent. 68

(1992)

1168.

[Si Yuse A. and Sano M., Nature

(London)

362

(1993)

329.

[6] Marder M., Phys. Reu. E 49

(1994)

R51;

Bradley R. M, and Wu K., J. Phys. A 26

(1993)

327; Phys. Reu. E 50

(1994)

R631;

Langer J. S., Phys. Reu. Lent. 70

(1993)

3592.

[7] Burridge R. and KnopooE L., Bull. Seismol. Soc. Am. 57

(1967)

341.

[8] Carlson J. M, and Langer J. S., Phys. Reu. Lent. 62

(1989)

2632; Phys. Reu. A 40

(1989)

6470;

de Sousa Viera M., Vasconcelos G. L, and Nagel S. R., Phys. Reu. E 47

(1993)

2221.

[9] Sahimi M, and Arbabi S., Phys. Reu. Lent. 68

(1992)

608.

[loi

Acharyya M. and Chakrabarti B. K., Ind. J. Phys. 69A

(1995)

(in press).

[iii

Bak P., Tang C, and Wiesenfeld K., Phys. Reu. Lent. 60 (1985) 2347.

[12] Acharyya M. and Chakrabarti B. K.

(1994) (To

be

published).

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