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Chaos in Fractional Standard
Map and Fractional Dissipative
Standard Map
Mark Edelman
Stern College for Women at Yeshiva University,
Courant Institute of Mathematical Sciences at NYU
Dresden, Germany, 2011
Outline
• Motivation
• Fractional Maps.
• Fractional attractors.
• Summary.
Chaos in Fractional Standard
Map and Fractional Dissipative
Standard Map
books published in 2010-2011:
Physics:
1. V. E. Tarasov Dynamics: Application of Fractional Calculus to Dynamics of
Particles, Fields and Media. (Springer) 2011.;
2. V. E. Tarasov, Theoretical Physics Models with Integro-Differentiation of
Fractional Order. (IKI, RCD) 2011 (in Russian)
3. R. Herrmann, Fractional Calculus: An Introduction for Physicists. (World Scientific)
2011;
Modeling and Control:
4. R. Caponetto, G. Dongola, and L. Fortuna, Fractional Order Systems: Modeling
and Control Applications. (World Scientific ) 2010;
5. I. Petras, Fractional-Order Nonlinear Systems. (Springer) 2011.
Viscoelasticity:
6. F. MainardiG. M. , Fractional Calculus and Waves in Linear Viscoelasticity: An
Introduction to Mathematical Models. (Imperial College Press) 2010;
Systems with Long-Rang Interaction:
7. A. C. J. Luo and V. Afraimovich (Eds.), Long-range Interaction, Stochasticity and
Fractional Dynamics. (Springer) 2010;
8. Zaslavsky, Hamiltonian Chaos and Fractional Dynamics. (Oxford University
Press) 2005.
Motivation
• Recognition of the importance of non-linearity in fractional dynamics: references 1, 5 ,and 7 above;
A. Wineman (2007 and 2009) in viscoelasticity, V. Gafiychuk et al. (2008, 2008, 2009, 2010) in reaction - diffusion systems;
and in systems (biological) with memory that can be described by the Volterraintegral equations of the second kind : F. Hoppensteadt, A nonlinear renewal equation with periodic and chaotic solutions. SIAM-AMS Proc., 10 1976.
• Important role of maps in regular dynamics (easy for theoretical analysis and computer simulations).
• New types of attractors and stability discovered as a result of initial
investigation of fractional maps:
1. V.E. Tarasov, G.M. Zaslavsky, Fractional equations of kicked systems and
discrete maps. J. Phys. A 41 2008,
2. M. Edelman, V. E. Tarasov, Fractional standard map. Phys. Let. A 374 2009;
3. V. E. Tarasov, M. Edelman, Fractional dissipative standard map. Chaos 20
2010.
4 M. Edelman, Fractional Standard Map: Riemann-Liouville vs. Caputo. Com.
Nonlin. Sci. Num. Sim., 16 2011.
Motivation
Fractional Attractor
What are the conditions for the existence of different types of
fractional attractors and cascade of bifurcation type
trajectories in particular?
Problem we are trying to address
Fractional Standard Map
)2 (mod
)2 (mod sin
11
1
nnn
nnn
PXX
XKPP
0 where
0)(sin0
ε
nT
txKx
n
Standard Map (SM) also known
as “Chirikov standard map”
Fractional Riemann-Liouville Standard Map.
.)1()( where
),2 (mod )1(1
sin
0
1
11
1
sss
n
i
in
nnn
mmmV
inVPΓ(α)
X
XKPP
Derived from Derived from
.0where
0)(sin0
0
ε
nT
txKxD
n
t
)21( ,)(
)(
)2(
1
0 12
2
0
t
tt
dx
dt
dxD
Fractional Standard MapsFractional Riemann-Liouville
Standard Map
).()( where
),2 (mod )1(1
sin
1
0
0
1
11
1
tXDntPP
inVPΓ(α)
X
XKPP
nn
n
i
in
nnn
Derived from Derived from
0)sin(0
0
n
t nT
txKxD
Fractional Caputo
Standard Map
With the initial conditions
.0 requires and giveswhich
,0)0)(( and )0)((
010
2
01
1
0
Xp P
xDpxD tt
torusaon considered becan , and both, where
,sin11
sinsin11
0
1
01
1
0
2
1
PX
)(X)i(nVΓ(α)
P XX
X)(X)i(nV)Γ(α
KPP
i
n
i
αnn
ni
n
i
αnn
0)sin(0
0
n
t
C nT
txKxD
With the initial conditions
;)0( ,)0)(()0)(()0( 00
11
0 xxpxDxDp tt
C
and momentum P defined as .xP
(Tarasov, Nov.2009)
Fractional Dissipatice Standard
Map (Fractional Zaslavsky Map)
),2 (mod P
sin
1nn1
1
XX
XKPeP
n
nnn
From the equation
1 ,21 where,)sin()()(0
00 α-βαR,qntxtxDqtxDn
tt
The dissipative standard map
can be derived in the form
0
)sin(n
ntXXqX
. ,
1)/q,-( where
qΓεμeK
e
q
q
Two forms of the fractional dissipative standard map where derived in Tarasov &
Edelman, Chaos, Jun. 2010. Here we consider one of them derived from the equation
in the form
function. Gamma incomplete theis and
,)1(,1(),1(),( where
),2 (mod 11
sin
)1(1
0
11
1
Γ(a,b)
baabeabaW
) (q,k-n-WP)Γ(α
μ X
XKPeP
ba
α
n
k
αkn
nnn
Fractional Attractors for K>Kc (example K=4.5)
)sin(2
)(
)(2 ),sin(
)(2
11
111
ll
l
clll
xK
p
VKxV
Kx
)sin(2
)(
)( ,
)()sin(
22
22
ll
l
c
l
l
xK
p
VK
KVx
ncomputatiodirect and
)1( ,)1(
n) large(for sassumption From
. , 11
l
n
nl
n
n
nnnn
ppxx
ppxx
ncomputatiodirect and
1
])1(1[2
n) large(for sassumption From
. ,
1
11
-α
l
n
n
n
ln
nnnn
Anp)(-p
xx
ppxx
CBTT
Evolution of the cascade of
bifurcation type trajectories
with the change in α.
Weak Chaos in CBTT
Cascade of bifurcation type trajectory for α=1.1, K=3.5.
Separation of two trajectories with initial separation Δp=10-6.
FDSM: x0=0, p0=0.7
α=1.2;
K=10 on the right,
K=9.1 on the left
Fractional Attractors (FDSM)
Structure of the chaotic attractor for K =12.93 and different values of α
Fractional Chaotic Attractors (FDSM)
(Γ=5, Ω=0).
105 iterations on each trajectory.
Summary
• The FDSs in general, are more stable than corresponding
systems of higher integer order without memory. They demonstrate
asymptotically attracting fixed and periodic points (sinks),
attracting trajectories, strange attractors, cascade of bifurcation
type trajectories.
• Fractional attractors are different from the regular attractors in
the following: a) they exist in the asymptotic sense; b) the
attracting trajectories may intersect and the strange attractors may
overlap; c) there can be more than one way to approach the same
attractor; d) existence of the cascade of bifurcation type attractors
is a general property of the FDSs.
• In order to find CBTTs in the physical systems or models described
by FDEs it is important to investigate areas of parameters where in
the corresponding integer systems a transition from regular motion
to chaos through the period-doubling bifurcations occurs.
α=1.9 in all cases
a) and d): K=3;
b) K=2; c) K=0.6 .
a), b), and d): n=200;
c): n=500;
N=105 in all cases.
Fractional Attractors (FSMRL phase space, K<Kc)
Fixed Points and
Attracting Slow
Diverging Trajectories
(ASDT)
b) FSMRL; K=2, α=1.4; p0=0.3 - fast; p0=5.3
ASCT; 50000 iterations;
c) FSMRL; K=2, α=1.4; p0=0.3;
d) FSMRL; K=2, α=1.4; p0=5.3 (ASCT);
e) FSMC; K=2, α=1.4; p0=0.3;
f) FSMC; K=3, α=1.9; p0=1.6+0.002i, 0≤i<50
Fractional Attractors (convergence, K<Kc)
FSMRL
Trajectories from the basin of attraction converge
to the stable fixed point fast:
xn~n-1-α , pn~n-α ;
from outside of the basin, slow (attracting slow
converging trajectories - ASCT):
xn~n-α , pn~n-α+1.
FSMC
All trajectories converge at the same slow rate:
xn~n-α+1 , pn~n-α+1.
Attracting Slow Diverging Trajectories (ASDT)
Numerical evaluation of ASDTs
(Fig. a) reveals that pn=Cn2-α .
Then it is possible to deduce
analytically that in ASDTs with
xlim=0 for α≥1.8
Fractional Attractors (FSMRL, K<Kc)
.)1(
)()2(2
,1
)(2
1
2
0
K
nMx
nMpp
n
n
α=1.9 in all cases.
a) FSMRL; K=3, p0=1.6+0.002i,
0≤i<50; SM (α=2) has only one central
island;
b) FSMC; K=3, α=1.9, p0=1.7+0.002i,
0≤i<50;
c) FSMRL; K=2, p0=4+0.08i,
0≤i<125; SM has T=4 islands;
d) FSMC; K=2, p0=-3.14+0.0314i,
0≤i<200;
e) FSMRL; K=0.6, p0=2+0.04i,
0≤i<50; SM has T=2 and T=3 islands;
f) FSMC; K=0.6, p0=-3.14+0.0314i,
0≤i<200;
Fractional Attractors(K<Kc)
FSMRL
Fractional Attractors for K>Kc (K=4.5 attractors)
FSMC
a) xn+1=-xn
pn+1=-pn;
b) two sets
xn+1=xn-π
pn+1=-pn;
c,d,e)a single
trajectory
with po=0.3;
f) FSMRL:
7 disjoint
chaotic
attractors;
FSMC: two
overlaping
attractors
a) α=1.8; b) α=1.71; c,d) α=1.65
e) α=1.45; f) α=1.02
On the left: FSMRL
• K=4.5; α=1.65
• K=3.5; α=1.1
On the right: Caputo
with the same
parameters as in the
case a).
Fractional Attractors
Attracting Cascade of
Bifurcations Type
Trajectories (CBTT)
FSMC p0=2, K=4, α=1.5 FSMC p0=5, K=5.2, α=1.5
Fractional Attractors
Cascade of Bifurcations
Type Trajectories (CBTT)
Vs. Inverse CBTT.
Fractional AttractorsFSM with Caputo derivative.
Fractional Chaotic Attractor: case K=3.5, α=1.1
iterations 500 200,n0
,200/2 ,0 00
npx
iterations 20000 5,n0
,5/2 ,0 00
npx
iterations 50000
,20 ,0 00 px
Fractional chaotic attractors are similar to the chaotic attractors of the dissipative
systems but they depend on the initial conditions. Different attractors may overlap.
Phase Space (K>2π)Riemann-Liouville Fractional Standard Map (FSMRL).
a) K=6.908745; α=1.999 b) K=6.908745; α=1.9