Laguerre and Associated Laguerre Polynomials

⚡ Key Takeaways

Laguerre polynomials Ln(x)L_n(x) are a sequence of orthogonal polynomials on [0,∞)[0,\infty) with respect to the weight e−xe^{-x}. The associated (generalized) Laguerre polynomials Ln(α)(x)L_n^{(\alpha)}(x) generalize these with weight xαe−xx^\alpha e^{-x}. They solve Laguerre's differential equation, satisfy a three-term recurrence, and are central to the radial wavefunctions of the hydrogen atom. Introduced by Edmond Laguerre (1879) and developed through the 19th–20th centuries.

💡 The Core Insight

Demanding that a power-series solution of a confluent-type ODE terminate (so the wavefunction stays normalizable) forces an integer eigenvalue nn. The resulting finite polynomials are automatically orthogonal under xαe−xx^\alpha e^{-x} because they are eigenfunctions of a self-adjoint (Sturm–Liouville) operator. Orthogonality, recurrence, and the Rodrigues formula are all manifestations of this single structure.

Formal Statement

DefinitionLaguerre Polynomials

The Laguerre polynomials Ln(x)L_n(x), for n=0,1,2,…n = 0, 1, 2, \dots, are defined by the Rodrigues formula

1
Ln(x)=exn!dndxn(e−xxn).\quad L_n(x) = \frac{e^{x}}{n!}\frac{d^{n}}{dx^{n}}\left(e^{-x} x^{n}\right).

Derivation hint: Apply Leibniz's rule for the nn-th derivative of the product e−xxne^{-x}x^n to extract the explicit polynomial. Equivalently, they have the explicit closed form

2
Ln(x)=∑k=0n(nk)(−1)kk! xk,\quad L_n(x) = \sum_{k=0}^{n} \binom{n}{k}\frac{(-1)^{k}}{k!}\, x^{k},

Derivation hint: Expand the Rodrigues formula via Leibniz's rule and use dndxn(xn+k−...)\frac{d^n}{dx^n}(x^{n+k-...}); collect terms. where x∈[0,∞)x \in [0,\infty), n∈Z≥0n \in \mathbb{Z}_{\ge 0}, (nk)\binom{n}{k} is the binomial coefficient, and L0(x)=1L_0(x) = 1.

DefinitionAssociated (Generalized) Laguerre Polynomials

For a real parameter α>−1\alpha > -1, the associated Laguerre polynomials are

3
Ln(α)(x)=x−αexn!dndxn(e−xxn+α)=∑k=0n(−1)k(n+αn−k)xkk!.\quad L_n^{(\alpha)}(x) = \frac{x^{-\alpha}e^{x}}{n!}\frac{d^{n}}{dx^{n}}\left(e^{-x}x^{n+\alpha}\right) = \sum_{k=0}^{n}(-1)^{k}\binom{n+\alpha}{n-k}\frac{x^{k}}{k!}.

Derivation hint: Generalize the Rodrigues formula by inserting xαx^\alpha into the weight; expand with Leibniz's rule, identifying (n+αn−k)=Γ(n+α+1)Γ(k+α+1)(n−k)!\binom{n+\alpha}{n-k}=\frac{\Gamma(n+\alpha+1)}{\Gamma(k+\alpha+1)(n-k)!}. When α=0\alpha = 0 these reduce to the ordinary Laguerre polynomials: Ln(0)(x)=Ln(x)L_n^{(0)}(x) = L_n(x). The symbol Γ\Gamma denotes the Gamma function, extending the factorial to non-integer arguments.

TheoremLaguerre Differential Equation

Ln(α)(x)L_n^{(\alpha)}(x) is the polynomial solution of the second-order linear ODE

4
x y′′+(α+1−x) y′+n y=0,\quad x\,y'' + (\alpha + 1 - x)\,y' + n\,y = 0,

Derivation hint: Substitute the series for Ln(α)L_n^{(\alpha)} and verify term by term, or recognize it as the eigenvalue equation of the Laguerre operator with eigenvalue nn. with eigenvalue nn. For α=0\alpha = 0 this is Laguerre's equation xy′′+(1−x)y′+ny=0x y'' + (1-x)y' + n y = 0. The polynomial solution exists (and is normalizable under the weight) only for non-negative integer nn.

TheoremOrthogonality Relation

Over [0,∞)[0,\infty) with weight w(x)=xαe−xw(x) = x^{\alpha} e^{-x},

5
∫0∞xαe−x Lm(α)(x) Ln(α)(x) dx=Γ(n+α+1)n! δmn,\quad \int_{0}^{\infty} x^{\alpha} e^{-x}\, L_m^{(\alpha)}(x)\, L_n^{(\alpha)}(x)\, dx = \frac{\Gamma(n+\alpha+1)}{n!}\,\delta_{mn},

Derivation hint: Cast equation [4] into Sturm–Liouville form ddx(xα+1e−xy′)=−n xαe−xy\frac{d}{dx}(x^{\alpha+1}e^{-x}y') = -n\,x^\alpha e^{-x} y; self-adjointness gives δmn\delta_{mn}, and the norm follows from the Rodrigues formula via repeated integration by parts. where δmn\delta_{mn} is the Kronecker delta. For α=0\alpha = 0 the norm is exactly 11, so the Ln(x)L_n(x) are orthonormal under e−xe^{-x}.

TheoremThree-Term Recurrence and Generating Function

The polynomials satisfy the recurrence

6
(n+1) Ln+1(α)(x)=(2n+α+1−x) Ln(α)(x)−(n+α) Ln−1(α)(x),\quad (n+1)\,L_{n+1}^{(\alpha)}(x) = (2n+\alpha+1-x)\,L_n^{(\alpha)}(x) - (n+\alpha)\,L_{n-1}^{(\alpha)}(x),

Derivation hint: Compare coefficients of tnt^n in the derivative of the generating function [7] with respect to tt, or apply Favard's theorem for orthogonal polynomials. and possess the generating function

7
∑n=0∞Ln(α)(x) tn=1(1−t)α+1exp⁡ ⁣(−x t1−t),∣t∣<1.\quad \sum_{n=0}^{\infty} L_n^{(\alpha)}(x)\, t^{n} = \frac{1}{(1-t)^{\alpha+1}}\exp\!\left(\frac{-x\,t}{1-t}\right), \qquad |t|<1.

Derivation hint: Expand the exponential and the binomial (1−t)−(α+1)(1-t)^{-(\alpha+1)} as power series in tt, collect the coefficient of tnt^n, and match equation [3].

Why It Holds / Derivation

ProofOrthogonality from Sturm–Liouville structure

Step 1. Rewrite Laguerre's equation [4] in self-adjoint (Sturm–Liouville) form. Multiply by the integrating factor xαe−xx^{\alpha}e^{-x}:

8
ddx ⁣(xα+1e−x y′)=−n xαe−x y.\quad \frac{d}{dx}\!\left(x^{\alpha+1}e^{-x}\,y'\right) = -n\, x^{\alpha} e^{-x}\, y.

Derivation hint: Note ddx(xα+1e−x)=xαe−x(α+1−x)\frac{d}{dx}(x^{\alpha+1}e^{-x}) = x^{\alpha}e^{-x}(\alpha+1-x), which reproduces the first-order coefficient in [4].

Step 2. Let Lm(α)L_m^{(\alpha)}, Ln(α)L_n^{(\alpha)} correspond to eigenvalues m,nm, n. Write [8] for each, multiply the mm-equation by Ln(α)L_n^{(\alpha)} and the nn-equation by Lm(α)L_m^{(\alpha)}, subtract, and integrate over [0,∞)[0,\infty).

Step 3. The left side becomes a total derivative of xα+1e−x(Lm′Ln−Ln′Lm)x^{\alpha+1}e^{-x}(L_m' L_n - L_n' L_m), which vanishes at x=0x=0 (the factor xα+1x^{\alpha+1} kills it for α>−1\alpha>-1) and at x=∞x=\infty (the factor e−xe^{-x} dominates). Hence the boundary term is zero.

Step 4. What remains is (n−m)∫0∞xαe−xLm(α)Ln(α)dx=0(n-m)\int_0^\infty x^\alpha e^{-x} L_m^{(\alpha)} L_n^{(\alpha)} dx = 0. For m≠nm \ne n this forces the integral to vanish, giving orthogonality.

Step 5. For the norm (m=nm=n), substitute the Rodrigues formula [3] and integrate by parts nn times. Each integration moves a derivative off e−xxn+αe^{-x}x^{n+\alpha}; boundary terms vanish, and the surviving integral is 1n!∫0∞xn+αe−xdx⋅(leading coefficient factor)\frac{1}{n!}\int_0^\infty x^{n+\alpha}e^{-x}dx \cdot (\text{leading coefficient factor}). Evaluating with ∫0∞xn+αe−xdx=Γ(n+α+1)\int_0^\infty x^{n+\alpha}e^{-x}dx = \Gamma(n+\alpha+1) yields the norm Γ(n+α+1)/n!\Gamma(n+\alpha+1)/n! in [5]. ■\blacksquare

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EN
Edmond Nicolas Laguerre
1834–1886

A French mathematician and artillery officer, Laguerre worked at the École Polytechnique and the Bureau des Longitudes. In 1879 he introduced the polynomials now bearing his name while studying the integral ∫x∞e−ttdt\int_x^\infty \frac{e^{-t}}{t}dt and continued-fraction expansions. His broader contributions span geometry (Laguerre transformations, the Laguerre formula for angles), the theory of equations, and approximation theory. The polynomials were a side product of analytic work but became indispensable a half-century later when quantum mechanics revealed them as the radial structure of the hydrogen atom.

Building Intuition

🧠 Intuition

Think of the weight e−xe^{-x} as defining a "probability cloud" concentrated near the origin and decaying on the half-line. The Laguerre polynomials are the unique polynomials that are mutually perpendicular when measured against this cloud — they are the half-line analogue of cosines on a circle. Each LnL_n has exactly nn real positive roots, and as nn grows these roots spread out to sample more of the half-line, much like higher harmonics oscillate faster. The parameter α\alpha controls how strongly the weight is pushed away from x=0x=0: larger α\alpha means the cloud thins out at the origin (the xαx^\alpha factor suppresses small xx), shifting where the polynomials "live."

:::svg[The first few Laguerre polynomials L0L_0 through L3L_3 on [0,5][0,5], showing increasing oscillation and roots] x y 0 1 2 3 4 5 0 L0 L1 L2 L3 Laguerre polynomials Lₙ(x), n = 0,1,2,3

Worked Examples

ExampleComputing L3(x)L_3(x) and verifying a root

Given: Use the explicit formula [2] for n=3n=3, α=0\alpha=0.

Step 1. Apply Ln(x)=∑k=0n(nk)(−1)kk!xkL_n(x) = \sum_{k=0}^{n}\binom{n}{k}\frac{(-1)^k}{k!}x^k with n=3n=3:

  • k=0k=0: (30)10!=1\binom{3}{0}\frac{1}{0!} = 1
  • k=1k=1: (31)−11!=−3\binom{3}{1}\frac{-1}{1!} = -3
  • k=2k=2: (32)12!=3⋅12=32\binom{3}{2}\frac{1}{2!} = 3\cdot\tfrac12 = \tfrac32
  • k=3k=3: (33)−13!=−16\binom{3}{3}\frac{-1}{3!} = -\tfrac16

Step 2. Assemble:

9
L3(x)=1−3x+32x2−16x3.\quad L_3(x) = 1 - 3x + \tfrac{3}{2}x^2 - \tfrac{1}{6}x^3.

Derivation hint: Sum the four computed coefficients against powers of xx.

Step 3. Verify the recurrence-free value at x=0x=0: L3(0)=1L_3(0)=1, consistent with Ln(0)=1L_n(0)=1 for all nn (set x=0x=0 in [2], only k=0k=0 survives).

Step 4. Check it solves [4] at, say, evaluating the ODE residual symbolically: xy′′+(1−x)y′+3yxy'' + (1-x)y' + 3y with y=L3y=L_3 gives 00 identically (one may verify the cubic coefficient: y′′=3−xy''=3-x, y′=−3+3x−12x2y'=-3+3x-\tfrac12 x^2).

L3(x)=1−3x+32x2−16x3(dimensionless)\boxed{L_3(x) = 1 - 3x + \tfrac{3}{2}x^2 - \tfrac{1}{6}x^3 \quad(\text{dimensionless})}
ExampleGauss–Laguerre quadrature of an integral

Given: Approximate I=∫0∞e−xx cos⁡x dxI = \int_0^\infty e^{-x} x\,\cos x\, dx using 2-point Gauss–Laguerre quadrature. The nodes are the roots of L2(x)=1−2x+12x2L_2(x) = 1 - 2x + \tfrac12 x^2, and the weights are wi=xi(n+1)2[Ln+1(xi)]2w_i = \frac{x_i}{(n+1)^2[L_{n+1}(x_i)]^2}.

Step 1. Roots of L2L_2: solve 12x2−2x+1=0⇒x2−4x+2=0⇒x=2±2\tfrac12 x^2 - 2x + 1 = 0 \Rightarrow x^2 - 4x + 2 = 0 \Rightarrow x = 2 \pm \sqrt2. So x1=0.585786x_1 = 0.585786, x2=3.414214x_2 = 3.414214.

Step 2. Weights (standard tabulated values for n=2n=2): w1=0.853553w_1 = 0.853553, w2=0.146447w_2 = 0.146447.

Step 3. The rule approximates ∫0∞e−xf(x)dx≈∑iwif(xi)\int_0^\infty e^{-x}f(x)dx \approx \sum_i w_i f(x_i) with f(x)=xcos⁡xf(x) = x\cos x:

  • f(x1)=0.585786cos⁡(0.585786)=0.585786×0.83366=0.488352f(x_1) = 0.585786\cos(0.585786) = 0.585786 \times 0.83366 = 0.488352
  • f(x2)=3.414214cos⁡(3.414214)=3.414214×(−0.96402)=−3.29154f(x_2) = 3.414214\cos(3.414214) = 3.414214 \times (-0.96402) = -3.29154

Step 4. Sum:

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I≈w1f(x1)+w2f(x2)=(0.853553)(0.488352)+(0.146447)(−3.29154).\quad I \approx w_1 f(x_1) + w_2 f(x_2) = (0.853553)(0.488352) + (0.146447)(-3.29154).

Derivation hint: Multiply each function value by its weight and add; Gauss–Laguerre is exact for polynomials of degree ≤2n−1=3\le 2n-1 = 3. =0.416855−0.482052=−0.065197= 0.416855 - 0.482052 = -0.065197.

Step 5. Exact value: ∫0∞e−xxcos⁡x dx=Re⁡ ⁣∫0∞xe−(1−i)xdx=Re⁡1(1−i)2=Re⁡1−2i=0\int_0^\infty e^{-x}x\cos x\,dx = \operatorname{Re}\!\int_0^\infty x e^{-(1-i)x}dx = \operatorname{Re}\frac{1}{(1-i)^2} = \operatorname{Re}\frac{1}{-2i} = 0. The 2-point estimate −0.065-0.065 is approximate because ff is not a polynomial; higher nn converges to 00.

I2-pt≈−0.0652(exact=0; dimensionless)\boxed{I_{2\text{-pt}} \approx -0.0652 \quad(\text{exact}=0;\ \text{dimensionless})}

Common Misconceptions

⚠️ Common mistake

Normalization conventions vary. The convention used here (and by physicists) gives Ln(0)=1L_n(0)=1 and the orthonormal form [5]. Some older texts (and Schrödinger's original papers) define Laguerre polynomials differing by a factor of n!n!, and the associated polynomials by repeated differentiation dmdxmLn\frac{d^m}{dx^m}L_{n} with shifted indices. Always check whether your source defines Ln(α)L_n^{(\alpha)} via the Rodrigues formula [3] (modern, standard, used by NIST and most quantum mechanics texts) or via Lnm(x)=(−1)mdmdxmLn+m(x)L_n^m(x) = (-1)^m \frac{d^m}{dx^m}L_{n+m}(x) (older). They differ by index conventions and constant factors.

CounterexampleNon-integer nn does not give a polynomial

One might think equation [4], xy′′+(1−x)y′+νy=0xy'' + (1-x)y' + \nu y = 0, yields a useful function for any ν\nu. But for non-integer ν\nu the power-series solution does not terminate: it is the confluent hypergeometric function M(−ν,1,x)=1F1(−ν;1;x)M(-\nu, 1, x) = {}_1F_1(-\nu;1;x), an infinite series that grows like exe^x as x→∞x\to\infty. This makes ∫0∞e−x∣y∣2dx\int_0^\infty e^{-x}|y|^2 dx diverge — the function is not normalizable. Only ν=n∈Z≥0\nu = n \in \mathbb{Z}_{\ge0} truncates the series to a genuine polynomial. This termination requirement is exactly the source of quantum-mechanical energy quantization.

Connections

connection

Laguerre polynomials are one of three classical orthogonal polynomial families, related by limits and the unifying Sturm–Liouville Theory. They connect to Hermite Polynomials (the half-line oscillator versus full-line oscillator) and to Jacobi Polynomials (which limit to Laguerre as one interval endpoint goes to infinity). The associated polynomials are special cases of the Confluent Hypergeometric Function via Ln(α)(x)=(n+αn) 1F1(−n;α+1;x)L_n^{(\alpha)}(x) = \binom{n+\alpha}{n}\,{}_1F_1(-n;\alpha+1;x). Their generating function and recurrence link to the broader theory of Generating Functions and Special Functions. In probability, the weight xαe−xx^\alpha e^{-x} is (up to scaling) the Gamma Distribution, so Laguerre polynomials are its orthogonal-polynomial system.

Real-World Applications

🔬 Where this appears

Historical Development

⏳ History
- 1879 — Edmond Laguerre introduces the polynomials while studying the exponential integral ∫x∞t−1e−tdt\int_x^\infty t^{-1}e^{-t}dt and associated continued fractions.
- 1880s — Pafnuty Chebyshev and his school develop the general theory of orthogonal polynomials on the half-line, providing the orthogonality framework.
- 1907 — Erhard Schmidt and contemporaries formalize orthogonal expansions in Hilbert space, giving completeness a rigorous footing.
- 1926 — Erwin Schrödinger solves the hydrogen atom; the radial equation reveals associated Laguerre polynomials, cementing their physical importance.
- 1929 — The systematic theory of "classical orthogonal polynomials" (Hermite, Laguerre, Jacobi) is consolidated, notably in work leading to the Bochner classification of which ODEs yield polynomial eigenfunctions.
- 1934–1939 — Gábor Szegő's monograph Orthogonal Polynomials unifies asymptotics, zeros, and quadrature, becoming the standard reference.
- 1940s–1950s — Gauss–Laguerre quadrature tables are computed for numerical analysis, accelerated by early electronic computing.
- 1992 — Laguerre–Gaussian modes are shown by Allen, Beijersbergen, Spreeuw, and Woerdman to carry quantized orbital angular momentum, launching a major field in optics.

Subtleties & Limits

open-problem

While the polynomials themselves are completely understood, several analytical questions remain delicate. The precise asymptotic distribution of zeros of Ln(α)L_n^{(\alpha)} as n→∞n\to\infty (and especially the behavior near the "soft edge" governed by Airy functions, or the "hard edge" near x=0x=0 governed by Bessel functions) is an active area connecting to random matrix theory; the largest zero scales like 4n4n but its fluctuations follow Tracy–Widom statistics. The completeness and convergence of Laguerre series for functions not decaying fast enough is subtle: unlike Fourier series, pointwise and mean convergence require careful weight-dependent conditions (LpL^p convergence holds only for restricted ranges of pp depending on α\alpha). Finally, numerical stability of recurrence [6] for large nn and small xx remains a practical challenge, motivating ongoing work on stable evaluation algorithms.

See Also

Hermite Polynomials · Jacobi Polynomials · Legendre Polynomials · Sturm–Liouville Theory · Confluent Hypergeometric Function · Hydrogen Atom · Gaussian Quadrature · Special Functions · Gamma Function · Orthogonal Polynomials