SUPPORT THE WORK

GetWiki

Legendre polynomials#Applications of Legendre polynomials in physics

ARTICLE SUBJECTS
aesthetics  →
being  →
complexity  →
database  →
enterprise  →
ethics  →
fiction  →
history  →
internet  →
knowledge  →
language  →
licensing  →
linux  →
logic  →
method  →
news  →
perception  →
philosophy  →
policy  →
purpose  →
religion  →
science  →
sociology  →
software  →
truth  →
unix  →
wiki  →
ARTICLE TYPES
essay  →
feed  →
help  →
system  →
wiki  →
ARTICLE ORIGINS
critical  →
discussion  →
forked  →
imported  →
original  →
Legendre polynomials#Applications of Legendre polynomials in physics
[ temporary import ]
please note:
- the content below is remote from Wikipedia
- it has been imported raw for GetWiki
{{Short description|System of complete and orthogonal polynomials}}{{for|Legendre's Homogeneous equation|Legendre's equation}}{{distinguish|text = Lagrange polynomial (the interpolating polynomial)}}(File:Legendrepolynomials6.svg|360px|thumb|The first six Legendre polynomials)In mathematics, Legendre polynomials, named after Adrien-Marie Legendre (1782), are a system of complete and orthogonal polynomials with a vast number of mathematical properties and numerous applications. They can be defined in many ways, and the various definitions highlight different aspects as well as suggest generalizations and connections to different mathematical structures and physical and numerical applications.Closely related to the Legendre polynomials are associated Legendre polynomials, Legendre functions, Legendre functions of the second kind, big q-Legendre polynomials, and associated Legendre functions.

Definition by construction as an orthogonal system

In this approach, the polynomials are defined as an orthogonal system with respect to the weight function w(x) = 1 over the interval [-1,1]. That is, P_n(x) is a polynomial of degree n, such thatint_{-1}^1 P_m(x) P_n(x) ,dx = 0 quad text{if } n ne m.With the additional standardization condition P_n(1) = 1, all the polynomials can be uniquely determined. We then start the construction process: P_0(x) = 1 is the only correctly standardized polynomial of degree 0. P_1(x) must be orthogonal to P_0, leading to P_1(x) = x, and P_2(x) is determined by demanding orthogonality to P_0 and P_1, and so on. P_n is fixed by demanding orthogonality to all P_m with m < n . This gives n conditions, which, along with the standardization P_n(1) = 1 fixes all n+1 coefficients in P_n(x). With work, all the coefficients of every polynomial can be systematically determined, leading to the explicit representation in powers of x given below.This definition of the P_n's is the simplest one. It does not appeal to the theory of differential equations. Second, the completeness of the polynomials follows immediately from the completeness of the powers 1, x, x^2, x^3, ldots. Finally, by defining them via orthogonality with respect to the most obvious weight function on a finite interval, it sets up the Legendre polynomials as one of the three classical orthogonal polynomial systems. The other two are the Laguerre polynomials, which are orthogonal over the half line [0,infty), and the Hermite polynomials, orthogonal over the full line (-infty,infty), with weight functions that are the most natural analytic functions that ensure convergence of all integrals.

Definition via generating function

The Legendre polynomials can also be defined as the coefficients in a formal expansion in powers of t of the generating function{{harvnb|Arfken|Weber|2005|loc=p.743}}{{NumBlk||frac{1}{sqrt{1-2xt+t^2}} = sum_{n=0}^infty P_n(x) t^n ,.|{{EquationRef|2}}}}The coefficient of t^n is a polynomial in x of degree n with |x| leq 1. Expanding up to t^1 givesP_0(x) = 1 ,,quad P_1(x) = x.Expansion to higher orders gets increasingly cumbersome, but is possible to do systematically, and again leads to one of the explicit forms given below.It is possible to obtain the higher P_n's without resorting to direct expansion of the Taylor series, however. Equation {{EquationNote|2}} is differentiated with respect to {{mvar|t}} on both sides and rearranged to obtainfrac{x-t}{sqrt{1-2xt+t^2}} = left(1-2xt+t^2right) sum_{n=1}^infty n P_n(x) t^{n-1} ,.Replacing the quotient of the square root with its definition in Eq. {{EquationNote|2}}, and equating the coefficients of powers of {{math|t}} in the resulting expansion gives Bonnet’s recursion formula
(n+1) P_{n+1}(x) = (2n+1) x P_n(x) - n P_{n-1}(x),.
This relation, along with the first two polynomials {{math|P0}} and {{math|P1}}, allows all the rest to be generated recursively.The generating function approach is directly connected to the multipole expansion in electrostatics, as explained below, and is how the polynomials were first defined by Legendre in 1782.

Definition via differential equation

A third definition is in terms of solutions to Legendre's differential equation:{{NumBlk||(1 - x^2) P_n''(x) - 2 x P_n'(x) + n (n + 1) P_n(x) = 0.|{{EquationRef|1}}}}This differential equation has regular singular points at {{math|1=x = ±1}} so if a solution is sought using the standard Frobenius or power series method, a series about the origin will only converge for {{math|{{abs|x}} < 1}} in general. When {{math|n}} is an integer, the solution {{math|Pn(x)}} that is regular at {{math|1=x = 1}} is also regular at {{math|1=x = −1}}, and the series for this solution terminates (i.e. it is a polynomial). The orthogonality and completeness of these solutions is best seen from the viewpoint of Sturm–Liouville theory. We rewrite the differential equation as an eigenvalue problem,frac{d}{dx} left( left(1-x^2right) frac{d}{dx} right) P(x) = -lambda P(x) ,,with the eigenvalue lambda in lieu of n(n+1). If we demand that the solution be regular atx = pm 1, the differential operator on the left is Hermitian. The eigenvalues are found to be of the form{{math|n(n + 1)}}, with n = 0, 1, 2, ldots and the eigenfunctions are the P_n(x). The orthogonality and completeness of this set of solutions follows at once from the larger framework of Sturm–Liouville theory.The differential equation admits another, non-polynomial solution, the Legendre functions of the second kind Q_n.A two-parameter generalization of (Eq. {{EquationNote|1}}) is called Legendre's general differential equation, solved by the Associated Legendre polynomials. Legendre functions are solutions of Legendre's differential equation (generalized or not) with non-integer parameters.In physical settings, Legendre's differential equation arises naturally whenever one solves Laplace's equation (and related partial differential equations) by separation of variables in spherical coordinates. From this standpoint, the eigenfunctions of the angular part of the Laplacian operator are the spherical harmonics, of which the Legendre polynomials are (up to a multiplicative constant) the subset that is left invariant by rotations about the polar axis. The polynomials appear as P_n(costheta) where theta is the polar angle. This approach to the Legendre polynomials provides a deep connection to rotational symmetry. Many of their properties which are found laboriously through the methods of analysis — for example the addition theorem — are more easily found using the methods of symmetry and group theory, and acquire profound physical and geometrical meaning.

Orthogonality and completeness

The standardization P_n(1) = 1 fixes the normalization of the Legendre polynomials (with respect to the {{math|L2}} norm on the interval {{math|−1 ≤ x ≤ 1}}). Since they are also orthogonal with respect to the same norm, the two statements{{clarify|reason=unclear what two statements are being referred to|date=April 2022}} can be combined into the single equation,int_{-1}^1 P_m(x) P_n(x),dx = frac{2}{2n + 1} delta_{mn},(where {{math|δmn}} denotes the Kronecker delta, equal to 1 if {{math|1=m = n}} and to 0 otherwise).This normalization is most readily found by employing Rodrigues' formula, given below.That the polynomials are complete means the following. Given any piecewise continuous function f(x) with finitely many discontinuities in the interval {{closed-closed|−1, 1}}, the sequence of sums
f_n(x) = sum_{ell=0}^n a_ell P_ell(x)
converges in the mean to f(x) as n to infty , provided we take
a_ell = frac{2ell + 1}{2} int_{-1}^1 f(x) P_ell(x),dx.
This completeness property underlies all the expansions discussed in this article, and is often stated in the formsum_{ell=0}^infty frac{2ell + 1}{2} P_ell(x)P_ell(y) = delta(x-y), with {{math|−1 ≤ x ≤ 1}} and {{math|−1 ≤ y ≤ 1}}.

Rodrigues' formula and other explicit formulas

An especially compact expression for the Legendre polynomials is given by Rodrigues' formula:P_n(x) = frac{1}{2^n n!} frac{d^n}{dx^n} (x^2 -1)^n ,.This formula enables derivation of a large number of properties of the P_n's. Among these are explicit representations such asbegin{align}P_n(x) & = [t^n] frac{left((t+x)^2 - 1right)^n}{2^n} = [t^n] frac{left(t+x+1right)^n left(t+x-1right)^n}{2^n}, [1ex]P_n(x)&= frac{1}{2^n} sum_{k=0}^n binom{n}{k}^{!2} (x-1)^{n-k}(x+1)^k, [1ex]P_n(x)&= sum_{k=0}^n binom{n}{k} binom{n+k}{k} left( frac{x-1}{2} right)^{!k}, [1ex]P_n(x)&= frac{1}{2^n}sum_{k=0}^{leftlfloor n/2 rightrfloor} left(-1right)^k binom{n}{k}binom{2n-2k}n x^{n-2k},[1ex]P_n(x)&= 2^n sum_{k=0}^n x^k binom{n}{k} binom{frac{n+k-1}{2}}{n}.end{align}Expressing the polynomial as a power series, P_n(x) = sum a_k x^k , the coefficients of powers of x can also be calculated using a general formula:a_{k+2} = - frac{(l-k)(l+k+1)}{(k+2)(k+1)}a_k. The Legendre polynomial is determined by the values used for the two constants a_0 and a_1 , where a_0=0 if n is odd and a_1=0 if n is even.BOOK, Boas, Mary L., Mathematical methods in the physical sciences, 2006, Wiley, 978-0-471-19826-0, 3rd, Hoboken, NJ, In the fourth representation, lfloor n/2 rfloor stands for the largest integer less than or equal to n/2. The last representation, which is also immediate from the recursion formula, expresses the Legendre polynomials by simple monomials and involves the generalized form of the binomial coefficient.The first few Legendre polynomials are:{| class="wikitable" style="text-align: right;"! n !! P_n(x)
| 1
| x
| tfrac12 left(3x^2-1right)
| tfrac12 left(5x^3-3xright)
| tfrac18 left(35x^4-30x^2+3right)
| tfrac18 left(63x^5-70x^3+15xright)
| tfrac1{16} left(231x^6-315x^4+105x^2-5right)
| tfrac1{16} left(429x^7-693x^5+315x^3-35xright)
| tfrac1{128} left(6435x^8-12012x^6+6930x^4-1260x^2+35right)
| tfrac1{128} left(12155x^9-25740x^7+18018x^5-4620x^3+315xright)
| tfrac1{256} left(46189x^{10}-109395x^8+90090x^6-30030x^4+3465x^2-63right)
The graphs of these polynomials (up to {{math|1=n = 5}}) are shown below:(File:Legendrepolynomials6.svg|640px|none|Plot of the six first Legendre polynomials.)

Applications of Legendre polynomials

Expanding a 1/r potential

The Legendre polynomials were first introduced in 1782 by Adrien-Marie LegendreBOOK, A.-M., Legendre, Recherches sur l'attraction des sphéroïdes homogènes, Mémoires de Mathématiques et de Physique, présentés à l'Académie Royale des Sciences, par divers savans, et lus dans ses Assemblées, X, 411–435, Paris, 1785, 1782, fr,weblink dead,weblink" title="web.archive.org/web/20090920070434weblink">weblink 2009-09-20, as the coefficients in the expansion of the Newtonian potentialfrac{1}{left| mathbf{x}-mathbf{x}' right|} = frac{1}{sqrt{r^2+{r'}^2-2r{r'}cosgamma}} = sum_{ell=0}^infty frac{{r'}^ell}{r^{ell+1}} P_ell(cos gamma),where {{math|r}} and {{math|r′}} are the lengths of the vectors {{math|x}} and {{math|x′}} respectively and {{math|γ}} is the angle between those two vectors. The series converges when {{math|r > r′}}. The expression gives the gravitational potential associated to a point mass or the Coulomb potential associated to a point charge. The expansion using Legendre polynomials might be useful, for instance, when integrating this expression over a continuous mass or charge distribution.Legendre polynomials occur in the solution of Laplace's equation of the static potential, {{math|1=∇2 Φ(x) = 0}}, in a charge-free region of space, using the method of separation of variables, where the boundary conditions have axial symmetry (no dependence on an azimuthal angle). Where {{math|ẑ}} is the axis of symmetry and {{math|θ}} is the angle between the position of the observer and the {{math|ẑ}} axis (the zenith angle), the solution for the potential will bePhi(r,theta) = sum_{ell=0}^infty left( A_ell r^ell + B_ell r^{-(ell+1)} right) P_ell(costheta) ,.{{math|Al}} and {{math|Bl}} are to be determined according to the boundary condition of each problem.BOOK, Jackson, J. D., Classical Electrodynamics,weblink limited, 3rd, Wiley & Sons, 1999, 103, 978-0-471-30932-1, They also appear when solving the Schrödinger equation in three dimensions for a central force.

Legendre polynomials in multipole expansions

(File:Point axial multipole.svg|right|Diagram for the multipole expansion of electric potential.)Legendre polynomials are also useful in expanding functions of the form (this is the same as before, written a little differently):frac{1}{sqrt{1 + eta^2 - 2eta x}} = sum_{k=0}^infty eta^k P_k(x),which arise naturally in multipole expansions. The left-hand side of the equation is the generating function for the Legendre polynomials.As an example, the electric potential {{math|Φ(r,θ)}} (in spherical coordinates) due to a point charge located on the {{math|z}}-axis at {{math|1=z = a}} (see diagram right) varies asPhi (r, theta ) propto frac{1}{R} = frac{1}{sqrt{r^2 + a^2 - 2ar costheta}}.If the radius {{math|r}} of the observation point {{math|P}} is greater than {{math|a}}, the potential may be expanded in the Legendre polynomialsPhi(r, theta) propto frac{1}{r} sum_{k=0}^infty left( frac{a}{r} right)^k P_k(cos theta),where we have defined {{math|1=η = {{sfrac|a|r}} < 1}} and {{math|1=x = cos θ}}. This expansion is used to develop the normal multipole expansion.Conversely, if the radius {{math|r}} of the observation point {{math|P}} is smaller than {{math|a}}, the potential may still be expanded in the Legendre polynomials as above, but with {{math|a}} and {{math|r}} exchanged. This expansion is the basis of interior multipole expansion.

Legendre polynomials in trigonometry

The trigonometric functions {{math|cos nθ}}, also denoted as the Chebyshev polynomials {{math|Tn(cos θ) ≡ cos nθ}}, can also be multipole expanded by the Legendre polynomials {{math|Pn(cos θ)}}. The first several orders are as follows:begin{alignat}{2}T_0(costheta)&=1 &&=P_0(costheta),[4pt]T_1(costheta)&=cos theta&&=P_1(costheta),[4pt]T_2(costheta)&=cos 2theta&&=tfrac{1}{3}bigl(4P_2(costheta)-P_0(costheta)bigr),[4pt]T_3(costheta)&=cos 3theta&&=tfrac{1}{5}bigl(8P_3(costheta)-3P_1(costheta)bigr),[4pt]T_4(costheta)&=cos 4theta&&=tfrac{1}{105}bigl(192P_4(costheta)-80P_2(costheta)-7P_0(costheta)bigr),[4pt]T_5(costheta)&=cos 5theta&&=tfrac{1}{63}bigl(128P_5(costheta)-56P_3(costheta)-9P_1(costheta)bigr),[4pt]T_6(costheta)&=cos 6theta&&=tfrac{1}{1155}bigl(2560P_6(costheta)-1152P_4(costheta)-220P_2(costheta)-33P_0(costheta)bigr).end{alignat}Another property is the expression for {{math|sin (n + 1)θ}}, which isfrac{sin (n+1)theta}{sintheta}=sum_{ell=0}^n P_ell(costheta) P_{n-ell}(costheta).

Legendre polynomials in recurrent neural networks

A recurrent neural network that contains a {{math|d}}-dimensional memory vector, mathbf{m} in R^d, can be optimized such that its neural activities obey the linear time-invariant system given by the following state-space representation:theta dot{mathbf{m}}(t) = Amathbf{m}(t) + Bu(t),begin{align}A &= left[ a right]_{ij} in R^{d times d} text{,} quad&& a_{ij} = left(2i + 1right)begin{cases}
-1 & i < j
(-1)^{i-j+1} & i ge j
end{cases},B &= left[ b right]_i in R^{d times 1} text{,} quad&& b_i = (2i + 1) (-1)^i .end{align}In this case, the sliding window of u across the past theta units of time is best approximated by a linear combination of the first d shifted Legendre polynomials, weighted together by the elements of mathbf{m} at time t:u(t - theta') approx sum_{ell=0}^{d-1} widetilde{P}_ell left(frac{theta'}{theta} right) , m_{ell}(t) , quad 0 le theta' le theta .When combined with deep learning methods, these networks can be trained to outperform long short-term memory units and related architectures, while using fewer computational resources.CONFERENCE, Voelker, Aaron R., Kajić, Ivana, Eliasmith, Chris, Legendre Memory Units: Continuous-Time Representation in Recurrent Neural Networks,weblink Advances in Neural Information Processing Systems,weblink 2019,

Additional properties of Legendre polynomials

Legendre polynomials have definite parity. That is, they are even or odd,{{harvnb|Arfken|Weber|2005|loc=p.753}} according toP_n(-x) = (-1)^n P_n(x) ,.Another useful property isint_{-1}^1 P_n(x),dx = 0 text{ for } nge1,which follows from considering the orthogonality relation with P_0(x) = 1. It is convenient when a Legendre series sum_i a_i P_i is used to approximate a function or experimental data: the average of the series over the interval {{closed-closed|−1, 1}} is simply given by the leading expansion coefficient a_0.Since the differential equation and the orthogonality property are independent of scaling, the Legendre polynomials' definitions are "standardized" (sometimes called "normalization", but the actual norm is not 1) by being scaled so thatP_n(1) = 1 ,.The derivative at the end point is given byP_n'(1) = frac{n(n+1)}{2} ,. The Askey–Gasper inequality for Legendre polynomials readssum_{j=0}^n P_j(x) ge 0 quad text{for }quad xge -1 ,.The Legendre polynomials of a scalar product of unit vectors can be expanded with spherical harmonics usingP_ell left(r cdot r'right) = frac{4pi}{2ell + 1} sum_{m=-ell}^ell Y_{ell m}(theta,varphi) Y_{ell m}^*(theta',varphi'),,where the unit vectors {{math|r}} and {{math|r′}} have spherical coordinates {{math|(θ, φ)}} and {{math|(θ′, φ′)}}, respectively.The product of two Legendre polynomials Leonard C. Maximonweblink
sum_{p=0}^infty t^{p}P_p(costheta_1)P_p(costheta_2)=frac2pifrac{mathbf Kleft( 2sqrt{frac{tsintheta_1sintheta_2}{t^2-2tcosleft( theta_1+theta_2 right)+1}} right)}{sqrt{t^2-2tcosleft( theta_1+theta_2 right)+1}},,
where K(cdot) is the complete elliptic integral of the first kind.

Recurrence relations

As discussed above, the Legendre polynomials obey the three-term recurrence relation known as Bonnet's recursion formula given by
(n+1) P_{n+1}(x) = (2n+1) x P_n(x) - n P_{n-1}(x)
and
frac{x^2-1}{n} frac{d}{dx} P_n(x) = xP_n(x) - P_{n-1}(x)
or, with the alternative expression, which also holds at the endpoints
frac{d}{dx} P_{n+1}(x) = (n+1)P_n(x) + x frac{d}{dx}P_{n}(x) ,.
Useful for the integration of Legendre polynomials is(2n+1) P_n(x) = frac{d}{dx} bigl( P_{n+1}(x) - P_{n-1}(x) bigr) ,.From the above one can see also thatfrac{d}{dx} P_{n+1}(x) = (2n+1) P_n(x) + bigl(2(n-2)+1bigr) P_{n-2}(x) + bigl(2(n-4)+1bigr) P_{n-4}(x) + cdotsor equivalentlyfrac{d}{dx} P_{n+1}(x) = frac{2 P_n(x)}{left| P_n right|^2} + frac{2 P_{n-2}(x)}{left| P_{n-2} right|^2} + cdotswhere {{math|{{norm|Pn}}}} is the norm over the interval {{math|−1 ≤ x ≤ 1}} = sqrt{int_{-1}^1 bigl(P_n(x)bigr)^2 ,dx} = sqrt{frac{2}{2 n + 1}} ,.

Asymptotics

Asymptotically, for ell to infty, the Legendre polynomials can be written as BOOK, Orthogonal polynomials, Szegő, Gábor, 1975, American Mathematical Society, 0821810235, 4th, Providence, 194 (Theorem 8.21.2), 1683237, begin{align}P_ell (cos theta) &= sqrt{frac{theta}{sinleft(thetaright)}} , J_0{left(left(ell+tfrac{1}{2}right)thetaright)} + mathcal{O}left(ell^{-1}right) [1ex]&= sqrt{frac{2}{pi ellsinleft(thetaright)}}cosleft(left(ell + tfrac{1}{2} right)theta - tfrac{pi}{4}right) + mathcal{O}left(ell^{-3/2}right), quad theta in (0,pi),end{align}and for arguments of magnitude greater than 1WEB,weblink DLMF: 14.15 Uniform Asymptotic Approximations, begin{align}P_ell left(coshxiright) &= sqrt{frac{xi}{sinhxi}} I_0left(left(ell+frac{1}{2}right)xiright)left(1+mathcal{O}left(ell^{-1}right)right),,P_ell left(frac{1}{sqrt{1-e^2}}right) &= frac{1}{sqrt{2piell e}} frac{(1+e)^frac{ell+1}{2}}{(1-e)^frac{ell}{2}} + mathcal{O}left(ell^{-1}right)end{align}where {{math|J0}} and {{math|I0}} are Bessel functions.

Zeros

All n zeros of P_n(x) are real, distinct from each other, and lie in the interval (-1,1). Furthermore, if we regard them as dividing the interval [-1,1] into n+1 subintervals, each subinterval will contain exactly one zero of P_{n+1}. This is known as the interlacing property. Because of the parity property it is evident that if x_k is a zero of P_n(x), so is -x_k. These zeros play an important role in numerical integration based on Gaussian quadrature. The specific quadrature based on the P_n's is known as Gauss-Legendre quadrature.From this property and the facts that P_n(pm 1) ne 0 , it follows that P_n(x) has n-1 local minima and maxima in (-1,1) . Equivalently, dP_n(x)/dx has n -1 zeros in (-1,1) .

Pointwise evaluations

The parity and normalization implicate the values at the boundaries x=pm 1 to be
P_n(1) = 1
,, quad
P_n(-1) = (-1)^n
At the origin x=0 one can show that the values are given by
P_{2n}(0) = frac{(-1)^{n}}{4^n} binom{2n}{n} = frac{(-1)^{n}}{2^{2n}} frac{(2n)!}{left(n!right)^2}

(-1)^nfrac{(2n-1)!!}{(2n)!!}

P_{2n+1}(0) = 0

Legendre polynomials with transformed argument

Shifted Legendre polynomials

The shifted Legendre polynomials are defined aswidetilde{P}_n(x) = P_n(2x-1) ,.Here the "shifting" function {{math|x ↦ 2x − 1}} is an affine transformation that bijectively maps the interval {{closed-closed|0, 1}} to the interval {{closed-closed|−1, 1}}, implying that the polynomials {{math|P̃n(x)}} are orthogonal on {{closed-closed|0, 1}}:int_0^1 widetilde{P}_m(x) widetilde{P}_n(x),dx = frac{1}{2n + 1} delta_{mn} ,.An explicit expression for the shifted Legendre polynomials is given bywidetilde{P}_n(x) = (-1)^n sum_{k=0}^n binom{n}{k} binom{n+k}{k} (-x)^k ,.The analogue of Rodrigues' formula for the shifted Legendre polynomials iswidetilde{P}_n(x) = frac{1}{n!} frac{d^n}{dx^n} left(x^2 -x right)^n ,.The first few shifted Legendre polynomials are:{| class="wikitable" style="text-align: right;"! n !! widetilde{P}_n(x)
| 1
| 2x-1
| 6x^2-6x+1
| 20x^3-30x^2+12x-1
| 70x^4-140x^3+90x^2-20x+1
| 252x^5 -630x^4 +560x^3 - 210 x^2 + 30 x - 1

Legendre rational functions

The Legendre rational functions are a sequence of orthogonal functions on [0, ∞). They are obtained by composing the Cayley transform with Legendre polynomials.A rational Legendre function of degree n is defined as:R_n(x) = frac{sqrt{2}}{x+1},P_nleft(frac{x-1}{x+1}right),.They are eigenfunctions of the singular Sturm–Liouville problem:left(x+1right) frac{d}{dx} left(x frac{d}{dx} left[left(x+1right) v(x)right]right) + lambda v(x) = 0with eigenvalues lambda_n=n(n+1),.

See also

{{div col|colwidth=20em}} {{div col end}}

Notes

{{reflist|30em}}

References

  • {{Abramowitz_Stegun_ref2|8|332|22|773}}
  • BOOK, George B., Arfken, George B. Arfken, Hans J., Weber, 2005, Mathematical Methods for Physicists, Elsevier Academic Press, 0-12-059876-0,
  • BOOK, Bayin, S. S., 2006, Mathematical Methods in Science and Engineering, Wiley, 978-0-470-04142-0, ch. 2,
  • BOOK, Belousov, S. L., 1962, Tables of Normalized Associated Legendre Polynomials, Mathematical Tables, 18, Pergamon Press, 978-0-08-009723-7,
  • BOOK, Richard, Courant, Richard Courant, David, Hilbert, David Hilbert, 1953, Methods of Mathematical Physics, 1, Interscience, New York, NY, 978-0-471-50447-4,
  • {{dlmf|first=T. M. |last=Dunster|id=14|title=Legendre and Related Functions}}
  • BOOK, Refaat, El Attar, Legendre Polynomials and Functions, CreateSpace, 2009, 978-1-4414-9012-4,
  • {{dlmf|id=18|title=Orthogonal Polynomials|first=Tom H. |last=Koornwinder|authorlink=Tom H. Koornwinder|first2=Roderick S. C.|last2= Wong|first3=Roelof |last3=Koekoek|first4=René F. |last4=Swarttouw}}

External links

{{Commons category|Legendre polynomials}} {{Authority control}}

- content above as imported from Wikipedia
- "Legendre polynomials#Applications of Legendre polynomials in physics" does not exist on GetWiki (yet)
- time: 2:37pm EDT - Wed, May 15 2024
[ this remote article is provided by Wikipedia ]
LATEST EDITS [ see all ]
GETWIKI 23 MAY 2022
GETWIKI 09 JUL 2019
Eastern Philosophy
History of Philosophy
GETWIKI 09 MAY 2016
GETWIKI 18 OCT 2015
M.R.M. Parrott
Biographies
GETWIKI 20 AUG 2014
CONNECT