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Nuno R. O. Bastos, Rui A. C. Ferreira and Delfim F. M. Torres
THE FRACTIONAL DIFFERENCE
CALCULUS OF VARIATIONS
Nuno R. O. Bastos1, Rui A. C. Ferreira2, Delfim F. M. Torres3
1Department of Mathematics
Polytechnic Institute of Viseu
3504-510 Viseu, Portugal
e-mail: [email protected]
2Faculty of Engineering and Natural SciencesLusophone University of Humanities and Technologies
1749-024 Lisbon, Portugal
e-mail: [email protected]
3Department of Mathematics
University of Aveiro
3810-193 Aveiro, Portugal
e-mail: [email protected]
Abstract. We introduce a discrete-time fractional calculus of variations. First order fractional
necessary optimality conditions of Euler-Lagrange type for the time scale hZ, h > 0, are es-tablished. Examples illustrating the use of the new condition are given. They show that the
solutions to the considered fractional problems: (i) converge to the classical discrete-time solu-
tions when the fractional order of the discrete-derivatives tend to integer values, (ii) converge to
the fractional continuous-time solutions when h tends to zero.
2010 Mathematics Subject Classification: 26A33, 39A12, 49K05.
Keywords: fractional difference calculus, fractional summation by parts, calculus of variations,
Euler-Lagrange equations, time scale hZ.
1 INTRODUCTION
The Fractional Calculus is currently an important research field in several different areas:
physics (including classical and quantum mechanics as well as thermodynamics), chemistry,
biology, economics, and control theory [13, 15, 17]. It has origin more than 300 years ago when
LHopital asked Leibniz what should be the meaning of a derivative of non-integer order. After
that episode several more famous mathematicians contributed to the development of Fractional
Calculus: Abel, Fourier, Liouville, Riemann, Riesz, just to mention a few names.
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The Fractional Difference Calculus of Variations
In [12] Miller and Ross define a fractional sum of order > 0 via the solution of a lineardifference equation. Namely, they present it as (see Section 2 for the notations used here)
f(t) =1
()
ts=a
(t (s))(1)f(s). (1)
This was done in analogy with the RiemannLiouville fractional integral of order > 0,
aDx f(x) =
1
()
xa
(x s)1f(s)ds,
which can be obtained via the solution of a linear differential equation [12, 13]. Some basic
properties of the sum in (1) were obtained in [12]. More recently, F. Atici and P. Eloe [4, 5]
defined the fractional difference of order > 0, i.e., f(t) = ((1)f(t)), and developedsome of its properties that allow to obtain solutions of certain fractional difference equations.
Fractional differential calculus has been widely developed in the past few decades due mainlyto its demonstrated applications in various fields of science and engineering. The study of frac-
tional problems of the Calculus of Variations and respective Euler-Lagrange equations is a fairly
recent issue see [1, 2, 7, 9, 14] and references therein and include only the continuous case. It
is well known that discrete analogues of differential equations can be very useful in applications
[10, 11]. Therefore, we consider pertinent to start a fractional discrete-time theory of the calculus
of variations.
Our objective is two-fold. On one hand we proceed to develop the theory of fractional dif-
ference calculus, namely, we introduce the concept of left and right fractional sum/difference
(cf. Definition 2.1). On the other hand, we believe that the present work will potentiate research
not only in the fractional calculus of variations but also in solving fractional difference equa-tions, specifically, fractional equations in which left and right fractional differences appear. We
formulate our main result in the time-scale hZ, h > 0.Because the theory of fractional difference calculus is in its infancy [4, 5, 12], the paper is
self contained. We begin, in Section 2, to give the definitions and results needed throughout. In
Section 3 we present the new results of the paper. Finally, in Section 4 we show some examples.
2 PRELIMINARIES
We begin by introducing some notation used throughout. The notation is borrowed from the
calculus on time scales [6]. Let a, b Z
with a < b. We putT
= [a, b] Z
,T
= [a, b 1] Z
and T2
= [a, b 2] Z. Denote by F the set of all real valued functions defined on T. Also,we will frequently write (t) = t + 1, (t) = t 1 and f(t) = f((t)). The usual conventionsc1
t=c f(t) = 0, c T, and1
i=0 f(i) = 1 remain valid here.As usual, the forward difference is defined by f(t) = f(t) f(t). If we have a func-
tion f of two variables, f(t, s), its partial (difference) derivatives are denoted by t and s,respectively. For arbitrary x, y R define (when it makes sense)
x(y) =(x + 1)
(x + 1 y),
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Nuno R. O. Bastos, Rui A. C. Ferreira and Delfim F. M. Torres
where is the gamma function. The following property of the gamma function,
(x + 1) = x(x),
will be frequently used.
It was mentioned in Section 1 that equality (1) was introduced in [12] as the fractional sum of
order > 0. In fact one finds the definition of left and right fractional sum (Definition 2.1) whenproving the fractional formula of summation by parts (Lemma 3.1), which is a crucial result in
order to fulfill our goal (see proof of the Euler-Lagrange equation (10) given by Theorem 3.4).
Definition 2.1. Letf F. The left fractional sum and the right fractional sum of order > 0are defined, respectively, as
at (f)(t) =
1
()
ts=a
(t (s))(1)f(s), (2)
and
tb (f)(t) =
1
()
bs=t+
(s (t))(1)f(s). (3)
Remark 2.1. The above sums (2) and (3) are defined for t = a + mod (1) and t = a mod (1), respectively, while f(t) is defined for t = a mod (1) (see [12]). Throughout we will
write (2) and (3), respectively, in the following way:
at f(t) =
1
()
ts=a
(t + (s))(1)f(s), t T,
tb f(t) =
1
()
bs=t
(s + (t))(1)f(s), t T.
Remark 2.2. The left fractional sum defined in (2) coincides with the fractional sum defined in
[12]. The analogy of (2) and (3) with the RiemannLiouville left and right fractional integralsof order > 0 is clear:
aDx f(x) =
1
()
xa
(x s)1f(s)ds,
xDb f(x) =
1
()
bx
(s x)1f(s)ds.
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The Fractional Difference Calculus of Variations
It was proved in [12] that lim0 at f(t) = f(t). We do the same for the right fractional
sum using a different method. Let > 0 be arbitrary. Then,
tb f(t) =
1
()
bs=t
(s + (t))(1)f(s)
= f(t) +1
()
bs=(t)
(s + (t))(1)f(s)
= f(t) +b
s=(t)
(s + t)
()(s t + 1)f(s)
= f(t) +b
s=(t)
st1i=0 (+ i)(s t + 1)
f(s).
Therefore, lim0 tb f(t) = f(t). It is now natural to define
a0tf(t) = t
0bf(t) = f(t),
which we do here, and to write
at f(t) = f(t) +
(+ 1)
t1s=a
(t + (s))(1)f(s), t T, 0, (4)
tb f(t) = f(t) +
(+ 1)
bs=(t)
(s + (t))(1)f(s), t T, 0.
The next theorem was proved in [5].
Theorem 2.2. Letf F and > 0. Then, the equality
at f(t) = (a
t f(t))
(t + a)(1)
()f(a), t T,
holds.
Remark 2.3. It is easy to include the case = 0 in Theorem 2.2. Indeed, in view of previousdefinitions, we get
at f(t) = (a
t f(t))
(+ 1)(t + a)(1)f(a), t T, (5)
for all 0.
We now present the counterpart of Theorem 2.2 for the right fractional sum:
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Theorem 2.3. Letf F and 0. Then, the equality
t
(b)f(t) =
(+ 1) (b + (t))
(1)
f(b) + (t
b f(t)), t T
, (6)
holds.
The proof of Theorem 2.3 is very similar to the one of Theorem 2.2.
Definition 2.4. Let 0 < 1 and set = 1 . Then, the left fractional difference and theright fractional difference of order of a function f F are defined, respectively, by
at f(t) = (a
t f(t)), t T
,
and
tb f(t) = (t
b f(t))), t T
.
3 MAIN RESULTS
Our aim is to introduce the discrete-time fractional problem of the calculus of variations and
to prove corresponding necessary optimality conditions. For that we need a fractional version of
the summation by parts formula.
3.1 Fractional summation by parts
Lemma 3.1 (Fractional summation by parts). Letf andg be real valued functions defined on TkandT, respectively. Fix 0 < 1 and put = 1 . Then,
b1t=a
f(t)at g(t) = f(b 1)g(b) f(a)g(a) +
b2t=a
t(b)f(t)g
(t)
+
( + 1)g(a)
b1
t=a
(t + a)(1)f(t) b1
t=(a)
(t + (a))(1)f(t)
. (7)
Proof. From (5) we can write
b1t=a
f(t)at g(t) =
b1t=a
f(t)(at g(t))
=b1t=a
f(t)
a
t g(t) +
( + 1)(t + a)(1)g(a)
=b1t=a
f(t)at g(t) +
b1t=a
( + 1)(t + a)(1)f(t)g(a). (8)
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Using the relation (4) we get
b1t=a
f(t)at g(t)
=b1t=a
f(t)
g(t) +
( + 1)
t1s=a
(t + (s))(1)g(s)
=b1t=a
f(t)g(t) +
( + 1)
b1t=a
f(t)t1s=a
(t + (s))(1)g(s)
=b1
t=af(t)g(t) +
( + 1)
b2
t=ag(t)
b1
s=(t)(s + (t))(1)f(s)
= f(b 1)[g(b) g(b 1)] +b2t=a
g(t)t(b)f(t),
where the third equality follows from the fact that if and are two functions defined on T
and is a function defined on T T, then the equality
b1t=a
(t)t1s=a
(t, s)(s) =b2t=a
(t)b1
s=(t)
(s, t)(s)
holds. We proceed to develop the right hand side of the equality
b1t=a
f(t)at g(t) = f(b 1)[g(b) g(b 1)] +
b2t=a
g(t)t(b)f(t)
as follows:
f(b 1)[g(b) g(b 1)] +b2t=a
g(t)t(b)f(t)
= f(b 1)[g(b) g(b 1)] +
g(t)t
(b)f(t)t=b1t=a
b2t=a g
(t)(t
(b)f(t))
= f(b 1)g(b) f(a)g(a)
( + 1)g(a)
b1s=(a)
(s + (a))(1)f(s)
+b2t=a
t
(b)f(t)
g(t) ,
where the first equality follows from the usual summation by parts formula. Putting this into (8),
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we get:
b1t=a
f(t)at g(t) = f(b 1)g(b) f(a)g(a) +
b2t=a
t
(b)f(t)
g(t)
+g(a)
( + 1)
b1t=a
(t + a)(1)
()f(t)
g(a)
( + 1)
b1s=(a)
(s + (a))(1)f(s).
The theorem is proved.
Remark 3.1. When = 1 andf andg are defined on {a, a + 1, . . . , b}, then we obtain from ourformula (7) the usual integration by parts formula in difference calculus:
b1t=a
f(t)g(t) = f(b 1)g(b) f(a)g(a) b2t=a
f(t)g(t)
= f(t)g(t)|ba b1t=a
f(t)g(t) .
3.2 Necessary optimality condition
We begin to fix two arbitrary real numbers and such that , (0, 1]. Further, we put = 1 and = 1 .
Let a function L(t,u,v,w) : TRRR R be given. We assume that the second-orderpartial derivatives Luu, Luv, Luw, Lvw , Lvv , and Lww exist and are continuous.
Consider the functional L : F R defined by
L(y()) =b1t=a
L(t, y(t), at y(t), t
b y(t)) (9)
and the problem, that we denote by (P1), of minimizing (9) subject to the boundary conditionsy(a) = A and y(b) = B (A, B R). Our aim is to derive necessary conditions of first andsecond order for problem (P1).
Definition 3.2. Forf F we define the norm
f = maxtT
|f(t)| + maxtT
|at f(t)| + max
tT|t
b f(t)|.
A function y F with y(a) = A and y(b) = B is called a local minimizer for problem (P1)provided there exists > 0 such thatL(y) L(y) for all y F with y(a) = A and y(b) = Bandy y < .
Definition 3.3. A function F is called an admissible variation for problem (P1) provided = 0 and(a) = (b) = 0.
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The next theorem presents a first order necessary condition for problem (P1).
Theorem 3.4 (The fractional discrete-time EulerLagrange equation). If y F is a local mini-
mizer for problem (P1), then
Lu[y](t) + t(b)Lv[y](t) + a
t Lw[y](t) = 0 (10)
holds for all t T2
, where the operator[] is defined by
[y](s) = (s, y(s), as y(s), s
b y(s)).
Proof. Suppose that y() is a local minimizer of L(). Let () be an arbitrary fixed admissible
variation and define the function :
() ,
()
R by
() = L(y() + ()).
This function has a minimum at = 0, so we must have (0) = 0, i.e.,
b1t=a
Lu[y](t)
(t) + Lv[y](t)at (t) + Lw[y](t)t
b (t)
= 0,
which we may write, equivalently, as
Lu[y](t)(t)|t=(b) +
b2t=a
Lu[y](t)(t)
+
b1t=a
Lv[y](t)at (t) +
b1t=a
Lw[y](t)tb (t) = 0. (11)
Using Lemma 3.1, and the fact that (a) = (b) = 0, we get for the third term in (11) that
b1t=a
Lv[y](t)at (t) =
b2t=a
t
(b)Lv[y](t)
(t). (12)
Using (6) we can write
b1
t=a
Lw[y](t)tb (t)
= b1t=a
Lw[y](t)(tb (t))
= b1t=a
Lw[y](t)
t
(b)(t)
(+ 1)(b + (t))(1)(b)
=
b1t=a
Lw[y](t)t(b)(t)
(b)
(+ 1)
b1t=a
(b + (t))(1)Lw[y](t)
.
(13)
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It follows that
b1t=a
Lw[y](t)t
(b)(t)
=b1t=a
Lw[y](t)
(t) +
(+ 1)
b1s=(t)
(s + (t))(1)(s)
=b1t=a
Lw[y](t)(t) +
(+ 1)
b2t=a
Lw[y](t)b1
s=(t)
(s + (t))(1)(s)
=b1
t=aLw[y](t)(t) +
(+ 1)
b1
t=a(t)
t1
s=a(t + (s))(1)Lw[y](s)
=b1t=a
(t)at Lw[y](t).
(14)
We apply again the usual summation by parts formula, this time to (14), to obtain:
b1t=a
(t)at Lw[y](t)
=b2t=a
(t)at Lw[y](t) + ((b) ((b)))a
t Lw[y](t)|t=(b)
=
(t)at Lw[y](t)
t=b1
t=a
b2t=a
(t)(at Lw[y](t))
+ (b)at Lw[y](t)|t=(b) (b 1)a
t Lw[y](t)|t=(b)
= (b)at Lw[y](t)|t=(b) (a)a
t Lw[y](t)|t=a
b2t=a
(t)at Lw[y](t).
(15)
Since (a) = (b) = 0 it follows, from (14) and (15), that
b1
t=a Lw[y](t)t(b)(t) =
b2
t=a (t)a
t Lw[y](t)
and, after inserting in (13), that
b1t=a
Lw[y](t)tb (t) =
b2t=a
(t)at Lw[y](t). (16)
By (12) and (16) we may write (11) as
b2t=a
Lu[y](t) + t
(b)Lv[y](t) + a
t Lw[y](t)
(t) = 0.
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Since the values of(t) are arbitrary for t T2
, the EulerLagrange equation (10) holds along
y.
Remark 3.2. If the initial condition y(a) = A is not present (i.e., y(a) is free), we can usestandard techniques to show that the following supplementary condition must be fulfilled:
Lv(a) +
( + 1)
b1t=a
(t + a)(1)Lv[y](t)
b1
t=(a)
(t + (a))(1)Lv[y](t)
+ Lw(a) = 0. (17)
Similarly, ify(b) = B is not present (i.e., y(b) is free), the equality
Lu((b)) + Lv((b)) Lw((b))
+
(+ 1)
b1t=a
(b + (t))(1)Lw[y](t)
b2t=a
((b) + (t))(1)Lw[y](t)
= 0 (18)
holds. We just note that the first term in (18) arises from the first term on the left hand side of
(11). Equalities (17) and (18) are the fractional discrete-time natural boundary conditions.
3.3 Generalization
Theorem 3.4 can be generalized from the time scale Z to hZ, h > 0. The proof is tech-nical, and we present the result here without proof. Illustrative examples of the application of
Theorem 3.6 are given in Section 4.
We begin with some standard notation of the calculus of variations on time scales [ 8]. Let
hZ = {hk : h > 0, k Z} and a, b hZ with a < b. The previous considered notation, validfor h = 1, is now generalized for t hZ by denoting (t) = t + h, (t) = t h, and (t) = h.We put T = [a, b] hZ, T = [a, (b)] hZ and T
2
= [a, 2(b)] hZ.
The forward difference is defined by
f(t) =f(t) f(t)
(t).
The delta h-integral or h-sum off is
ba
f(t)t =
b
h1
k= ah
f(kh)h .
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If we have a function f of two variables, f(t, s), its partial (difference) derivatives are denotedby t,h and s,h, respectively. For arbitrary x, y R define (when it makes sense)
x(y) = hy(xh + 1)
(xh
+ 1 y),
where is the gamma function.Often, the left fractional delta integration of order > 0 is denoted as a
t f(t) and the
right fractional delta integration of order > 0 by tb f(t). Here, like Ross et. al. in [16], we
omit the subscript t on the operator and we will write ah f(t) and h
b f(t).
Definition 3.5. Letf F. The left fractional h-sum is defined as
ah f(t) = h
f(t) +
(+ 1) t
a
(t + h (s))(1)f(s)s, t T, 0,
while the right fractional h-sum of order 0 is given by
hb f(t) = h
f(t) +
(+ 1)
(b)(t)
(s + h (t))(1)f(s)s, t T .
As before, we begin to fix two arbitrary real numbers and such that , (0, 1], andwe put := 1 and := 1 . Given a function L(t,u,v,w) : T R R R R weconsider the problem
L(y()) = b
a
L(t, y(t), ahy(t), h
b y(t))t min
y(a) = A , y(b) = B ,
(Ph)
where A, B R are given.
Theorem 3.6 (The h-fractional EulerLagrange equation for problem (Ph)). If y F is a localminimizer for problem (Ph), then the following equality must be satisfied:
Lu[y](t) + h(b)Lv[y](t) + a
hLw[y](t) = 0, t T
2 , (19)
where the operator[] is defined by
[y](s) = (s, y(s), ahy(s), h
b y(s)) .
Remark 3.3. The Euler-Lagrange equation (19) coincides with (10) in the particular case h = 1.If the initial condition y(a) = A is not present (y(a) is free), one can prove that the followingsupplementary condition must be fulfilled:
hLv(a) +
(+ 1)
ba
(t + h a)(1)Lv [y](t)t
b(a)
(t + h (a))(1)Lv[y](t)t
+ Lw(a) = 0. (20)
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Similarly, ify(b) = B is not present (y(b) is free), the following equality
hLu((b)) + h
Lv((b)) h
Lw((b))
+
(+ 1)
ba
(b + h (t))(1)Lw[y](t)t
(b)a
((b) + h (t))(1)Lw[y](t)t
= 0, (21)
holds. The natural boundary conditions (20) and (21) reduce to (17) and (18) when h = 1.
4 EXAMPLES
In this section we present two illustrative examples. The results were obtained using the open
source Computer Algebra System Maxima (cf. http://maxima.sourceforge.net).
All computations were done running Maxima on an Intel CoreTM2 Duo, CPU of 2.27GHz
with 3Gb of RAM.
Example 4.1. Let us consider the following problem:
J(y) =
10
1
2(0
hy(t))
2 y(t)
t min , y(0) = 0 , y(1) = 0 . (22)
We begin by considering problem (22) with = 1 and different values of h. Our numericalresults show that when h tends to zero the extremal of the problem tends to the extremal of thecorresponding continuous classical problem of the calculus of variations. More precisely, when
h 0 problem (22) tends to the fractional continuous problem [3, Example 2] with solutiongiven by
y(t) =1
2t(1 t)
when = 1. This is illustrated in Figure 1. The computation times ranged from 0.02 seconds forh = 0.5 to 0.44 seconds forh = 0.0625.
Consider now problem (22) with h = 0.05 and different values of . Our numerical resultsshow that when tends to one our extremal tends to the classical (integer order) discrete-time
case. This is illustrated in Figure 2. The computation times ranged from 2.5 minutes forh = 0.7to 6.5 minutes forh = 0.99.
Example 4.2. Let us consider the following problem:
J(y) =
10
1
2(0
hy(t))
2 t min , y(0) = 0 , y(1) = 1 . (23)
We consider problem (23) with = 0.75 and different values of h. Our numerical resultsshow that when h tends to zero our extremal tends to the fractional continuous extremal. Indeed,
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Nuno R. O. Bastos, Rui A. C. Ferreira and Delfim F. M. Torres
0
0.05
0.10
0.15
0 1
+
+
+
++
+
+
+
+*
*
*
*
*
**
* * **
*
*
*
*
*
*
y(t)
t
Figure 1: Extremal y(t) for problem of Example 4.1 with = 1 and different hs (: h = 0.50; :
h = 0.25; +: h = 0.125; : h = 0.0625).
0
0.05
0.10
0.15
0.20
0.25
0.30
0.35
0 1
++
++
++
+ ++ + + + + + +
++
++
++*
*
**
**
** *
* * * * **
**
**
**
y(t)
t
Figure 2: Extremal y(t) for problem of Example 4.1 with h = 0.05 and differents (: = 0.70; :
= 0.75; +: = 0.95; : = 0.99).
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The Fractional Difference Calculus of Variations
when h 0 problem (23) tends to the fractional continuous problem of the calculus of variations[1, Example 1], with solution given by
y(x) = 2
x
0
dt
[(1 t)(x t)]0.25 . (24)
This is illustrated in Figure 3. The computation times ranged from 10.46 seconds forh = 0.5 to25 minutes forh = 1/30.
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
1.0
0 1
+
+
+
+
+
+
+
+
+
*
*
*
*
*
*
*
*
*
*
*
*
**
*
*
*
y(t)
t
Figure 3: Extremal y(t) for problem of Example 4.2 with = 0.75 and differenths (: h = 0.50; +:h = 0.125; : h = 0.0625; : h = 1/30). The solid line represent (24).
ACKNOWLEDGEMENTS
This work is part of the first authors PhD project which is carried out at the University of
Aveiro under the Doctoral Programme Mathematics and Applications of Universities of Aveiro
and Minho. The second author was supported by The Portuguese Foundation for Science and
Technology (FCT) through the PhD fellowship SFRH/BD/39816/2007; the third author was sup-ported by FCT through the R&D unit Centre for Research on Optimization and Control (CEOC),
cofinanced by FEDER/POCI 2010.
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