P-stability, Trigonometric-fitting and the numerical solution of the radial Schrödinger equation

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Abstract

In this paper we will study the importance of the properties of P-stability and Trigonometric-fitting for the numerical integration of the one-dimensional Schrödinger equation. This will be done via the error analysis and the application of the studied methods to the numerical solution of the radial Schrödinger equation.

Introduction

The one-dimensional Schrödinger equation can be written as:y(x)=[l(l+1)/x2+V(x)k2]y(x). The boundary conditions are:y(0)=0 and a second boundary condition, for large values of x, determined by physical considerations.

The above boundary value problem occurs frequently in theoretical physics and chemistry, material sciences, quantum mechanics and quantum chemistry, electronics, etc. (see for example [1], [2], [3], [4]).

We can define now some terms in (1):

  • The function W(x)=l(l+1)/x2+V(x) is called the effective potential. This satisfies W(x)0 as x.

  • The quantity E=k2 is a real number denoting the energy.

  • The quantity l is a given integer representing the angular momentum.

  • V is a given function which denotes the potential.

The last years a detailed investigation has been taken place on the development of numerical methods for the solution of the Schrödinger equation. The aim of this research is the development of fast and reliable methods for the solution of the Schrödinger equation and related problems (see for example [5], [6], [7], [8], [9], [10], [11], [12], [13], [14], [15], [16], [17], [18], [22], [23], [24], [25], [26], [27], [28], [29], [30], [31], [32], [33], [34], [35], [36], [37], [38], [39], [40], [41], [42], [43], [44], [45], [46], [47], [48], [49], [50], [51], [52], [53], [54], [55], [56], [57], [58], [59], [60], [61], [62], [63], [64], [65], [66]).

The methods for the numerical solution of the Schrödinger equation can be divided into two main categories:

  • (1)

    Methods with constant coefficients.

  • (2)

    Methods with coefficients depending on the frequency of the problem.3

The purpose of this paper is to study the importance of the properties of P-stability and Trigonometric-Fitting for the numerical integration of the one-dimensional Schrödinger equation. This will be done via the study of the error analysis and the application of the investigated methods to the numerical solution of the radial Schrödinger equation. We will investigate both categories of methods, i.e.:
  • The category of trigonometrically-fitted linear multistep methods and

  • The category of P-stable linear multistep methods.

More specifically, we will develop a family of methods of sixth algebraic order for the numerical solution of the radial Schrödinger equation. We will investigate the stability of the two categories of methods. We will study the error of the both categories of methods. Finally, we will apply both categories of methods the new obtained method to the resonance problem. This is one of the most difficult problems arising from the radial Schrödinger equation. The paper is organized as follows. In Section 2 we present the development of the new family of methods. The error analysis is presented in Section 3. In Section 4, we will investigate the stability properties of the new developed methods. In Section 5 the numerical results are presented. Finally, in Section 6 remarks and conclusions are discussed.

Section snippets

First method of the family

We introduce the following family of methods to integrate y=f(x,y):yn+22c1yn+1+2ayn2c1yn1+yn2=h2[b0(yn+2+yn2)+b1(yn+1+yn1)+b2yn]. In order the above method (3) to be exact for any linear combination of the functions{1,x,x2,x3,x4,x5,exp(±Ivx)}, where I=1, the following system of equations must hold:4cos(vh)24c1cos(vh)+2a2=(310cos(vh)2+2b1cos(vh)+b2320)h2v2,24c1+2a=0,84c1=310+4b1+2b2,324c1=365+24b1. Solving the system of Eqs. (5), (6), (7), (8) and demanding that b0=340, we

Error analysis

We will study the following methods:

Classical method4LTECL=19h86048yn(8). The P-stable trigonometrically-fitted method produced by Wang [67]LTEWANG=2h8945(yn(8)v8yn). First trigonometrically-fitted method produced in this paperLTENEW-I=19h86048(yn(8)+v2yn(6)). Second trigonometrically-fitted method produced in this paperLTENEW-II=19h86048(yn(8)+2v2yn(6)+v4yn(4)). The P-stable method produced in this paper.

The same with (36).

The error analysis is

Stability analysis

Theorem 2

(See [20].) A symmetric Four-Step Method with the characteristic equation given by (24) is said to have a nonzero interval of periodicity (0,H02) if, for all H(0,H02) the following relations are holdP1(H,w)0,P2(H,w)0,P3(H,w)0,P2(H,w)24P1(H,w)P3(H,w)0, where H=qh, w=vh and:P1(H,w)=2A(H,w)2B(H,w)+C(H,w)0,P2(H,w)=12A(H,w)2C(H,w)0,P3(H,w)=2A(H,w)+2B(H,w)+C(H,w)0,N(H,w)=P2(H,w)24P1(H,w)P3(H,w)0.

Definition 3

A method is called singularly almost P-stable if its interval of periodicity is equal to (0,)

Numerical results – conclusion

In order to illustrate the efficiency of the new obtained method given by coefficients (9), (10) we apply it to the radial time independent Schrödinger equation.

In order to apply the new method to the radial Schrödinger equation the value of parameter v is needed. For every problem of the one-dimensional Schrödinger equation given by (1) the parameter v is given byv=|q(x)|=|V(x)E|, where V(x) is the potential and E is the energy.

Conclusions

In the present paper we have developed a family of methods of sixth algebraic order for the numerical solution of the radial Schrödinger equation.

More specifically we have developed:

  • (1)

    A four-step sixth algebraic order exponentially-fitted method which integrated any linear combination of the functions:{1,x,x2,x3,x4,x5,exp(±Ivx)}.

  • (2)

    A four-step sixth algebraic order exponentially-fitted method which integrated any linear combination of the functions:{1,x,x2,x3,exp(±Ivx),xexp(±Ivx)}.

  • (3)

    A P-stable

Acknowledgements

The author wishes to thank the anonymous referee for his/her careful reading of the manuscript and his/her fruitful comments and suggestions.

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    Active Member of the European Academy of Sciences and Arts. Corresponding Member of the European Academy of Sciences. Corresponding Member of European Academy of Arts, Sciences and Humanities.

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    Current address: 10 Konitsis Street, Amfithea – Paleon Faliron, GR-175 64 Athens, Greece.

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