q-SIMPSON’S RULES OF QUANTUM CALCULUS

ALNASR M.H.1*
1Department of Mathematics and physics, Qatar University, P.O. Box: 2713, Doha, Qatar.
* Corresponding Author : modialnasr@qu.edu.qa

Received : 16-08-2012     Accepted : 15-09-2012     Published : 01-11-2012
Volume : 2     Issue : 1       Pages : 11 - 16
Bioinfo Comput Math 2.1 (2012):11-16

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Abstract

This paper is devoted to the derivation of q-Simpson’s rules for numerical integration. Instead of the classical Newton divided differences used to establish the classical Simpson’s method, we apply the Jackson q-differences in our new approach. A rigorous error analysis is given without assuming differentiability conditions on the integrands. Illustrative examples with comparison with classical results are also demonstrated.

Keywords

q-calculus, q-integration, Simpson’s rule, q-Simpson’s rule, q-Taylor series.

Introduction

The q-calculus, or quantum calculus, cf. e.g. [9,13,20] has received more attenstion in the last two decades, especially, analogues of classical results, its application in physics as well as approximation theory, cf. e.g. [10,21,22] . So, it is a desirable task to derive q-analogues of classical results in a self dependent manner, within the frame of q-calculus. This paper aims to develop a new method for computing integrals numerically. This technique is q-analogues of the well known Simpson’s rule. In this setting q-type Taylor theroems are employed. The q-Taylor series has been introduced first by Jackson [17] as the following



where q is a positive number with 0<q<1, Dq is the q-difference operator defined by Jackson [18] and the q-shifted factorial is defined by



Rigorous definitions are given below. Al-Salam and Verma [3] , introduced another q-Taylor series



Since can be expressed in terms of , then both series can be considred as interpolation ones. However, neither papers contain any proofs of these expansions. Both series are derived formally by assuming the expandability of the functions and then computing the corresponding coefficients. Annaby and Mansour have given analytic proofs of both expansions [4] .
In this paper we will use the q-type Taylor theroems to derive a q-analog of Simpson’s rule to compute integrals numerically, cf. [4,7-8] . Therefore we will use finite q-Taylor polynomials with q -integral remainders. Since we have two of such polynomials we will derive two different rules. Each rule is a family of uncountable rules since Composite rules are also given. In the next section we will define the necessary notations and state the important results for our investigations. Section 3 contains the main results of this paper. We derive two q-type Simpson’s rules to compute integrals numerically. Rigorous error estimates are proved without assuming any differentiability conditions on the integrands. This is another advantage of using q-differences. The last section is fully devoted to numerical examples with comparisons.

q-Notations and Results

This section involves notations and results that will be needed in the sequel. By a q-geometric set , it is meant that for all . Intervals containing zero are example of q-geometric sets.
The q-difference operator [17] , is defined by the following.

Definition 2.1: Let be a function defined on a q-geometric set A. The q-difference operator is defined for to be



Since , then always exists for and it is called the q-derevative of f at x. The q-derevative at zero is defined to be



provided that the limit exists without depending on x. The q-derivative at zero is defined in many literature to be the if it exists [11,13] .

Definition 2.2: A function f defined on a q-geometric set is said to be q-regular at zero if for every .
In some occasions q-regularity at zero plays the role of continuity in the classical sense. Notice that continuity at zero implies q-regularity at zero, but the converse is not necessarily true. For example, cf. [1] , the function



Is q-regular at zero for any rational q, but it is not continuous at zero. The relationship between the classical derivative and the q -derivative can be explained as follows. If A contains a neighborhood of a point x, x≠0 and f is differentiable at x then . Also if and exists, then also . Moreover if exists, then f is q-regular at zero. Nevertheless, (2.3) indicates that the existence of does not imply continuity at zero. The q-integration on intervals of the form [x,1] x>0 had been introduced by Jackson and Hahn [5] .

Definition 2.3: The q-integration over using the division points

is defined by



Definition 2.4: The q-integration over , x>0 using the division points



is defined by the formula



Jackson in [16] introduced an integral denoted by .

Definition 2.5: The q-integration for on a q-geometric set A to be,



where



provided that the series at the right-hand side of (2.7) converges at x=a and b. Although one can prove some algebraic properties of q-integration in a straight forward manner, some properties do not hold. For instance the inquality



is not always true. Obviously such an inquality would play an important role in deriving error estimates of numerical methods if it exists. To see this, define the function to be



Clearly g is q-integrable [0,1] and



Direct calculations yield



Consequently,



However, inequality (2.8) holds when the forms have
The q-shifted factorial for is defined by



The limit, , exists since . It will be denoted by . The q-Gamma function [11,19] is defined by



where we take the principal branches for and . One can easily deduce



For our purpose we consider functions defined on . Let be the polynomial



Let f be defined on and , such that the q-derivative of f up to order n exist at zero and is q-integrable on . Then for a fixed we have the following two q-Taylor formulas





see [4,8] for proofs and references. In [14,15] Ismail and Stanton derived with analytic proofs q-type Taylor series for entire functions of q-exponential growth, [26] . Ismail and Stanton’s results stand for the Askey-Wilson difference operator.
Lo’pez, et al. [23] using [24] established sufficient conditions for the convergence of Ismail and Stanton’s q-Taylor series, but not necessarily to the original function. In [4] , analytic proofs of for Jackson and Al-Salam-Verma q-Taylor series are given using q-Cauchy integral formulas, see e.g. [2,8] .

q- Simpson’s Rules

In the following we are considering the interval . The classical Simpson’s rule states that for , the class of functions which are continously differentiable up to order four, we have



where and lies in (a,b). Based on this, the composite Simpson’s rule is derived when splitting the interval [a,b] into n even number of subintervals with equal lengths via an equidistant partition



Then, the composite Simpson's rule is given by



where for with [5,7,12] . In the following we will derive q-Simpson’s rules which depend on the q-differences instead of the clasical ones. With the same numbers of nodes, the new techique gives better results. The proposed rules are families of rules with the same stepsize. The present work, which is the first in this direction, as far as we know, indicates that the new technique enriches numerical integration techniques. Moreover in the new setting, no differentiability conditions are imposed on the function, which may badly behave. In what follows we consider functions defined on [0,b] and we will derived two q-Simpson’s rules to compute integrals on [a,b] 0q-mean value theorem, taken from [25] . It will be needed in establishing error estimates. It states that if f(x) and g(x) continous on [0,b] then there exists such that



Now start with deriving a backward q-Simpson’s rule. Letting n=3 in (2.13) and simplifying we obtain



Theorem 3.1: Let be such that exists. Then



where



and



Moreover, if f is continuous; is bounded on [0,b] and q→1, then the error has the estimate



where

Proof: By integrating (3.4), we have



Computing and simplifying the first integral of the previous equation directly leads to the q-Simpson’s rule



Now we estimate the error. Since q→1, we can apply the q-mean value theorem stated above, and consequently



for some . From the definition of q-integral and direct calculations we obtain



Combining (3.11), (3.12) and (3.7) yields,



where q is closer to one such that a≤qb We call the previous rule backward because it is derived in terms of f(b), f(qb) and f(q2b). It should be noted that the condition q→1 is not very much restrictive because h is supposed to be small to guarantee that . Therefore



The composite rule directly follows when we have the partition (3.2) to be.

Corollary 3.2: Let be such that exists. Then



where



and



Moreover, if f is continuous; is bounded on [0,b] and q→1, then the error has the estimate



where on

Next we derive a forward rule in terms of , and . Therefore q should be chosen closer to one again to make sure that Indeed

as .

Let n=3 in (2.14). Then



Theorem 3.3: Let be such . Then



where



and



Moreover, if f is continuous; is bounded on [0,b] as q→1 then the error has the estimate



where on [0,b] From (3.18), we have



Simple manipulations imply q-Simpson’s rule



We estimate the error as in the previous theorem. Suppose that q→1 and use the mean value theorem of [25] then there exists such that



From the definition of q-integrals we obtain



Substitution from (3.26) and (3.25) in (3.21) yields,



As indicated before the condition q→1 is not restrictive here too. Also the composite rule for the forward rule with respect to the partition (3.2) will be the following.

Corollary 3.4: Let be such that exists. Then



where ,



and



Moreover, if f is continuous; is bounded on [0,b] and q→1 then the error has the estimate



where

Numerical Results

In this section we present the results for some numerical experiments. We apply these methods to two numerical examples. In each case, the approximate solution and the maximum absolute error between the exact solution and the approximate solution were given. The results are presented in [Table-1] and [Table-2] numerical methods tested are as follows.

The numerical methods tested are as follows.
Simp R = Simpson’s rule (3.3)
CBQ SimpR = Composite backward q-Simpson’s rule (3.15)
CFQ SimpR = Composite forward q-Simpson’s rule (3.29)
For our computations we have adopted a Mathematica module.

Example 1: Consider the following integral



Example 2: Consider the following integral.

Conclusions

We implement our numerical methods, as described above, to two examples. The methods give comparable results with those obtained by simpson’s rule. In the second example the composite Simpson’s rule and CFQSimp rule are inappropriate when integrating a function on an interval that contains both regions with large functional variation and regions with small functional variation. But CBQSimp rule was employed successfully for solving such type of integral. The difficulty in this method, which needs future investigations, is that we need to estimate the value of for each n.

Acknowledgements

I would like to thank Professor M.H.Annaby for helpful discussions. This work is supported by Qatar National Research Fund under the grant number NPRP08-056-1-014.

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