The Negative Neumann Eigenvalues of Second Order Differential Equation with Two Turning Points

Σχετικά έγγραφα
Example Sheet 3 Solutions

Section 8.3 Trigonometric Equations

2 Composition. Invertible Mappings

Homework 3 Solutions

Exercises 10. Find a fundamental matrix of the given system of equations. Also find the fundamental matrix Φ(t) satisfying Φ(0) = I. 1.

The k-α-exponential Function

Second Order Partial Differential Equations

3.4 SUM AND DIFFERENCE FORMULAS. NOTE: cos(α+β) cos α + cos β cos(α-β) cos α -cos β

Chapter 6: Systems of Linear Differential. be continuous functions on the interval

D Alembert s Solution to the Wave Equation

SCITECH Volume 13, Issue 2 RESEARCH ORGANISATION Published online: March 29, 2018

Phys460.nb Solution for the t-dependent Schrodinger s equation How did we find the solution? (not required)

CHAPTER 25 SOLVING EQUATIONS BY ITERATIVE METHODS

Matrices and Determinants

Partial Differential Equations in Biology The boundary element method. March 26, 2013

Statistical Inference I Locally most powerful tests

Section 7.6 Double and Half Angle Formulas

Απόκριση σε Μοναδιαία Ωστική Δύναμη (Unit Impulse) Απόκριση σε Δυνάμεις Αυθαίρετα Μεταβαλλόμενες με το Χρόνο. Απόστολος Σ.

Congruence Classes of Invertible Matrices of Order 3 over F 2

Lecture 26: Circular domains

Practice Exam 2. Conceptual Questions. 1. State a Basic identity and then verify it. (a) Identity: Solution: One identity is csc(θ) = 1

Fourier Series. MATH 211, Calculus II. J. Robert Buchanan. Spring Department of Mathematics

Chapter 6: Systems of Linear Differential. be continuous functions on the interval

Differential equations

PARTIAL NOTES for 6.1 Trigonometric Identities

Homework 8 Model Solution Section

Concrete Mathematics Exercises from 30 September 2016

4.6 Autoregressive Moving Average Model ARMA(1,1)

1 String with massive end-points

Solution Series 9. i=1 x i and i=1 x i.

Inverse trigonometric functions & General Solution of Trigonometric Equations

Solutions to Exercise Sheet 5

Coefficient Inequalities for a New Subclass of K-uniformly Convex Functions

ST5224: Advanced Statistical Theory II

Reminders: linear functions

Problem Set 9 Solutions. θ + 1. θ 2 + cotθ ( ) sinθ e iφ is an eigenfunction of the ˆ L 2 operator. / θ 2. φ 2. sin 2 θ φ 2. ( ) = e iφ. = e iφ cosθ.

Math221: HW# 1 solutions

CHAPTER 101 FOURIER SERIES FOR PERIODIC FUNCTIONS OF PERIOD

Exercises to Statistics of Material Fatigue No. 5

EE512: Error Control Coding

DiracDelta. Notations. Primary definition. Specific values. General characteristics. Traditional name. Traditional notation

( y) Partial Differential Equations

Other Test Constructions: Likelihood Ratio & Bayes Tests

Differentiation exercise show differential equation

w o = R 1 p. (1) R = p =. = 1

On Numerical Radius of Some Matrices

HOMEWORK 4 = G. In order to plot the stress versus the stretch we define a normalized stretch:

Eigenvalues and eigenfunctions of a non-local boundary value problem of Sturm Liouville differential equation

SCHOOL OF MATHEMATICAL SCIENCES G11LMA Linear Mathematics Examination Solutions

Finite Field Problems: Solutions

Problem Set 3: Solutions

Jesse Maassen and Mark Lundstrom Purdue University November 25, 2013

Areas and Lengths in Polar Coordinates

forms This gives Remark 1. How to remember the above formulas: Substituting these into the equation we obtain with

Second Order RLC Filters

9.09. # 1. Area inside the oval limaçon r = cos θ. To graph, start with θ = 0 so r = 6. Compute dr

Areas and Lengths in Polar Coordinates

6.3 Forecasting ARMA processes

A General Note on δ-quasi Monotone and Increasing Sequence

Homomorphism in Intuitionistic Fuzzy Automata

Forced Pendulum Numerical approach

The Simply Typed Lambda Calculus

Ordinal Arithmetic: Addition, Multiplication, Exponentiation and Limit

ES440/ES911: CFD. Chapter 5. Solution of Linear Equation Systems

Srednicki Chapter 55

On the k-bessel Functions

Appendix to On the stability of a compressible axisymmetric rotating flow in a pipe. By Z. Rusak & J. H. Lee

Spherical Coordinates

PROPERTIES OF CERTAIN INTEGRAL OPERATORS. a n z n (1.1)

derivation of the Laplacian from rectangular to spherical coordinates

ANSWERSHEET (TOPIC = DIFFERENTIAL CALCULUS) COLLECTION #2. h 0 h h 0 h h 0 ( ) g k = g 0 + g 1 + g g 2009 =?

C.S. 430 Assignment 6, Sample Solutions

Econ 2110: Fall 2008 Suggested Solutions to Problem Set 8 questions or comments to Dan Fetter 1

A summation formula ramified with hypergeometric function and involving recurrence relation

5. Choice under Uncertainty

Every set of first-order formulas is equivalent to an independent set

Mock Exam 7. 1 Hong Kong Educational Publishing Company. Section A 1. Reference: HKDSE Math M Q2 (a) (1 + kx) n 1M + 1A = (1) =

Parametrized Surfaces

CRASH COURSE IN PRECALCULUS

Section 7.7 Product-to-Sum and Sum-to-Product Formulas

26 28 Find an equation of the tangent line to the curve at the given point Discuss the curve under the guidelines of Section

MATH423 String Theory Solutions 4. = 0 τ = f(s). (1) dτ ds = dxµ dτ f (s) (2) dτ 2 [f (s)] 2 + dxµ. dτ f (s) (3)

Tutorial problem set 6,

Lecture 2: Dirac notation and a review of linear algebra Read Sakurai chapter 1, Baym chatper 3

On the Galois Group of Linear Difference-Differential Equations

A Note on Intuitionistic Fuzzy. Equivalence Relation

Notations. Primary definition. Specific values. General characteristics. Traditional name. Traditional notation. Mathematica StandardForm notation

ON NEGATIVE MOMENTS OF CERTAIN DISCRETE DISTRIBUTIONS

Geodesic Equations for the Wormhole Metric

b. Use the parametrization from (a) to compute the area of S a as S a ds. Be sure to substitute for ds!

Tridiagonal matrices. Gérard MEURANT. October, 2008

Integrals in cylindrical, spherical coordinates (Sect. 15.7)

SOME PROPERTIES OF FUZZY REAL NUMBERS

Section 8.2 Graphs of Polar Equations

ECE Spring Prof. David R. Jackson ECE Dept. Notes 2

Space-Time Symmetries

Trigonometry 1.TRIGONOMETRIC RATIOS

SPECIAL FUNCTIONS and POLYNOMIALS

Chapter 6 BLM Answers

Derivation of Optical-Bloch Equations

Transcript:

Applied Mathematical Sciences, Vol. 3, 009, no., 6-66 The Negative Neumann Eigenvalues of Second Order Differential Equation with Two Turning Points A. Neamaty and E. A. Sazgar Department of Mathematics, Faculty of Basic Sciences Mazandaran University, Babolsar, Iran neamaty@math.com Abstract In this work, we have studied the solution of the second order differential equation with two turning points case. It is well known that the solutions of the equation are obtained by the asymptotic solution. The aim of this article is to show the higher order distribution negative eigenvalues of Sturm-Liouville problem with Neumann boundary conditions in two turning points case. Mathematics Subject Classification: 3E05 Keywords: Turning point, Sturm-Liouville problem, Neumann conditions, Eigenvalue Introduction In the case of ordinary differential equations the book by Wasow [6] discusses several aspects with detail and rigour. One of the basic tools in the sturmliouville theory is the idea of asymptotic of solution, for example see []. The start of the systematic investigations of the asymptotic eigenvalues of sturm- Liouville problems has been made in Haupt [3] and Richardson[]. In [5] we obtained the positive asymptotic eigenvalues for sturm-liouville problems with boundary condition w (a) =w (b) = 0 with two turning points. The purpose of this paper is to derive asymptotic eigenvalue for differential equation d w dξ = {u ( ξ )+ϕ(ξ)}w () in which the independent variable ξ range over (a, b), and u is a large parameter and the ϕ(ξ) is continuous function on (a, b). We also saw the asymptotic eigenvalues for equation (), when the boundary conditions are w(a) = w(b) = 0

6 A. Neamaty and E. A. Sazgar with one turning point (see []). In this paper we study the negative asymptotic eigenvalues with Neumann boundary condition w (a) =w (b) = 0 with two turning points case. Relevant properties of parabolic functions In this paper we will consider the equation (). Any particular integral of the equation whereas the general solution of the corresponding homogeneous equation. This section we study the standard form of approximating differential equation d W dx =(l x )W () when l>0, the turning points are at x = ±l and for large positive l when l = μ and x = μy, by [] the solutions of () are in following form k ( μ )W ( μ,μy ) = π μ 6 ( η y ) Bi ( μ 3 η)( + O(u )) (3) k ( μ )W ( μ, μy ) = η π μ 6 ( y ) Ai ( μ 3 η)( + O(u )), () where η = 3 y (τ )dτ 3, k( μ = e πμ +O ( e πμ) and W ( μ,μy ), W ( μ, μy ) are two independent solutions of (). 3 Derivative of solutions For next section, in Neumann boundary condition, we need the derivative of solutions. For this purpose, let θ =( η ) ξ then dθ = dξ θ = (ξ ) η 5 (ξ ) 5 so the derivative of solutions (3) and () are in form of W( u, ξ u) ξ W( u, ξ u) ξ = k ( u)u π (θ B i + θb i ), (5) = k ( u)u π (θ A i + θa i). We consider differential equation (). By [] for ξ>0 have two solutions in following form w (u, ξ) =k u ( )W ( u, ξ u)+ɛ, w (u, ξ) =k u ( )W ( u, ξ u)+ɛ, (6)

Differential equation with two turning points 63 where ɛ and ɛ are error terms. So the derivative of this solution are w ξ = u π (θ B i + θb i)+ɛ, w ξ = u π (θ A i + θa i)+ɛ, (7) Lemma The asymptotic form of A i (u 3 η), A i(u 3 η), B i (u 3 η), B i(u 3 η) are given by (u,ξ >0),α= uη 3 3 b π A i ( u 3 ηb ) M cosα + M sinα, A i( u π u 3 ηb ) u b B i ( u 3 ηb ) M cosα M sinα, B i( u π u 3 ηb ) u b b π b π {M3 sinα M cosα}, (8) {M3 cosα + M sinα}. For ξ<0, a<, β = 3 uη 3 a π the Airy function are given by, A i ( u 3 η a ) M 5cosβ + M 6 sinβ, A i( u π u 3 η a ) u a B i ( u 3 η a ) M 6cosβ M 5 sinβ,b i( u π u 3 η a ) u a where the M i are given by aπ aπ (9) {M7 sinβ M 8 cosβ}, (0) {M7 cosβ + M 8 sinβ}, M = s=0 ( ) s u s ( 3, M = 3 uη b s=0 ( ) s u s+ ) s M 3 = s=0 ( ) s V s ( 3, M = 3 uη b s=0 ( ) s V s+ ) s ( 3, 3 uη b ) s+ M 5 = s=0 ( ) s u s ( 3, M 6 = 3 uη a s=0 ( ) s u s+ ) s ( 3, 3 uη a ) s+ M 7 = s=0 ( ) s V s ( 3, M 8 = 3 uη a s=0 ( ) s V s+ ) s ( 3. 3 uη a ) s+ We suppose ( 3 uη 3 b ) s+, () ψ = M sinα + M cosα, ψ = M 3 cosα + M sinα, ψ = α (b)( M cosα M sinα), ψ = α (b)( M 3 sinα+m cosα) ψ 3 = M 6 cosβ M 5 sinβ, ψ = M 5 cosβ + M 6 sinβ, ψ 3 = β (a)( M 5 cosβ M 6 sinβ), ψ = β (a)( M 5 sinβ+m 6 cosβ), θ =(b ), γ =(a ). For ξ< the solutions of equation () are in form of w (u, a) = π u (a ) η a π u a ( M 5 sin β + M 6 cos β),

6 A. Neamaty and E. A. Sazgar similarly w (u, a) = 3 u (a ) (M6 cos β M 5 sin β), () w (u, a) = 3 u (a ) (M5 cos β + M 6 sin β). (3) The derivative of w (u, a) and w (u, a) are in form of w (u, a) = 3 u (γ ψ 3 + γψ 3 ) w (u, a) = 3 u (γ ψ + γψ ), () where β = 3 u(a )η a = β u, γ =(a ), ψ 3 = β (a) ψ, ψ = β (a) ψ 3. (5) Asymptotic of the eigenvalues Now we will study distribution of eigenvalue of equation () with Neumann condition w (a) =w (b) = 0. The eigenvalue of equation () are the zero of Δ(u) = 0 where Δ(u) is defined as following form therefore we get Δ(u) = w (u, b) w (u, b) w (u, a) w (u, a) w (u, b)w (u, a) w (u, a)w (u, b) =0, (6) Δ(u) =[γ ψ 3 γβ (a)ψ ](θ ψ +θψ ) (γ ψ +γβ (a)ψ 3 )(θ ψ +θψ ) = 0 (7) Δ(u) = [γ (M 6 cosβ M 5 sinβ) γβ (M 5 cosβ + M 6 sinβ)] [ θ (M 3 cosα + M sinα)+θα (b) ( M 3sinα + M cosα) ] [γ (M 5 cosβ + M 6 sinβ)+γβ ( M 5 sinβ + M cosβ)] [θ ( M sinα + M cosα)+θα ( M cosα M sinα)] = 0. Here we have M = M 5 = u 0 + O(u ) and M 3 = u 0 + O(u ) M 6 cos β M 5 sin β = ( ) s u s+ cos β ( ) s u s sin β s=0 ( uη 3 3 a ) s+ s=0 ( uη 3 3 a ) s u u 3 =( +...) cos β (u uη 3 3 a ( uη 0 u +...) sin β = (u 3 3 a ) uη 0 +O(u )) sin β. 3 3 a (8)

Differential equation with two turning points 65 Similarly we will have M 5 cos β M 6 sin β = (u 0 + O(u )) cos β M cos α + M sin α = O(u ) M 3 sin α + M cos α = (v 0 + O(u )) sin α M 5 cos β + M 6 sin β =(u 0 + O(u )) cos β M 5 sin β + M 6 cos β = (u 0 + O(u )) sin β M sin α + M cos α = (u 0 + O(u )) sin α M cos α M sin α = (u 0 + O(u )) cos α. (9) Therefore by substituting (9) in Δ(u) then we will have Δ(u) = [ ( γ sin β γβ u cos β)(u 0 + O(u )) ][ O(u ) θα u(v 0 + O(u )) sin α ] [ (γ cos β γβ u sin β)(u 0 + O(u )) ][ ( θ sin α θα u cos α)(u 0 + O(u )) ] =0 (0) where β = β u and α = α u. By deviation (0) to u then [O(u ) γβ (u 0 + O(u )) cos β][o(u ) θα (v 0 + O(u )) sin α] [O(u ) γβ (u 0 + O(u )) sin β][o(u ) θα (u 0 + O(u )) cos α] = 0 () O(u )+γθβ α (u 0 + O(u ))(v 0 + O(u )) sin α cos β (O(u )+γθβ α (u 0 + O(u ))(u 0 + O(u )) sin β cos α) =0. () By deviation from α β γθ in () then we will have [O(u )+(u 0 +O(u ))(v 0 +O(u )) sin α cos β (u 0 +O(u ))(u 0 +O(u )) sin β cos α =0 For u we have since tan β = β + β3 + β5 3 5 tan α = M 5 M 3 tan α. cot β = u 0 + O(u ) v 0 + O(u ) = M 5 M 3, +... then we see that [ tan β = M ] 5 β + β3 M 3 3 + β5 5 +..., we suppose tan α = x and we get arctan of two side, therefore α = nπ + arctan x = nπ + π x + 3x +... x > 3 5x5

66 A. Neamaty and E. A. Sazgar Hence we get at last 3 uη 3 b π = nπ + 3π ( +O(x ) ), x u n = nπ + 3π η 3 3 b 3 η 3 b x ( +O(x ) ). Theorem Under the conditions of the given Neumann problem, the eigenvalues of Neumann at the origin are References u n = nπ + 3π η 3 3 b 3 η 3 b x ( +O(x ) ). [] Olver.F.W.J., Second-order linear differential equations with two turning points. Phil. Trans. R. Soc. Lon. A.78 37-7(975) [] Jodayree Akbarfam A., Higher-order asymptotice approximatios to the eigenvalues of the Sturm -liouville problems in one turning point case, Bulletin Iranian Math. society, vol. 3, No..(997)37-53. [3] O. Haupt, Uber eine Methode zum Beweise von oszillations theoreme, Mat. Ann., 76 (95) 67-0. [] R.G.D. Richardson, Contributions to the study of oscillation properties of the solutions of linear differential equations of the second order, Amer.J. Math., 0, (98) 83-36. [5] A. Neamaty and A. Sazgar, The Neumann conditions for Sturm-Liouville problems with turning points, Int. J. Contemp. Math. Sciences,(To appear). [6] W. Wosow, Asymptotic expansions for ordinary differential equations,interscience Publishers, New York (965). Received: September 6, 008