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Elliptic function
Elliptic function
from Wikipedia

In the mathematical field of complex analysis, elliptic functions are special kinds of meromorphic functions, that satisfy two periodicity conditions. They are named elliptic functions because they come from elliptic integrals. Those integrals are in turn named elliptic because they first were encountered for the calculation of the arc length of an ellipse.

Important elliptic functions are Jacobi elliptic functions and the Weierstrass -function.

Further development of this theory led to hyperelliptic functions and modular forms.

Definition

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A meromorphic function is called an elliptic function, if there are two -linear independent complex numbers such that

and .

So elliptic functions have two periods and are therefore doubly periodic functions.

Period lattice and fundamental domain

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The fundamental domain of an elliptic function as the unit cell of its period lattice.
Parallelogram where opposite sides are identified

If is an elliptic function with periods it also holds that

for every linear combination with .

The abelian group

is called the period lattice.

The parallelogram generated by and

is a fundamental domain of acting on .

Geometrically the complex plane is tiled with parallelograms. Everything that happens in one fundamental domain repeats in all the others. For that reason we can view elliptic function as functions with the quotient group as their domain. This quotient group, called an elliptic curve, can be visualised as a parallelogram where opposite sides are identified, which topologically is a torus.[1]

Liouville's theorems

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The following three theorems are known as Liouville's theorems (1847).

1st theorem

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A holomorphic elliptic function is constant.[2]

This is the original form of Liouville's theorem and can be derived from it.[3] A holomorphic elliptic function is bounded since it takes on all of its values on the fundamental domain which is compact. So it is constant by Liouville's theorem.

2nd theorem

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Every elliptic function has finitely many poles in and the sum of its residues is zero.[4]

This theorem implies that there is no elliptic function not equal to zero with exactly one pole of order one or exactly one zero of order one in the fundamental domain.

3rd theorem

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A non-constant elliptic function takes on every value the same number of times in counted with multiplicity.[5]

Weierstrass ℘-function

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One of the most important elliptic functions is the Weierstrass -function. For a given period lattice it is defined by

It is constructed in such a way that it has a pole of order two at every lattice point. The term is there to make the series convergent.

is an even elliptic function; that is, .[6]

Its derivative

is an odd function, i.e. [6]

One of the main results of the theory of elliptic functions is the following: Every elliptic function with respect to a given period lattice can be expressed as a rational function in terms of and .[7]

The -function satisfies the differential equation

where and are constants that depend on . More precisely, and , where and are so called Eisenstein series.[8]

In algebraic language, the field of elliptic functions is isomorphic to the field

,

where the isomorphism maps to and to .

Relation to elliptic integrals

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The relation to elliptic integrals has mainly a historical background. Elliptic integrals had been studied by Legendre, whose work was taken on by Niels Henrik Abel and Carl Gustav Jacobi.

Abel discovered elliptic functions by taking the inverse function of the elliptic integral function

with .[9]

Additionally he defined the functions[10]

and

.

After continuation to the complex plane they turned out to be doubly periodic and are known as Abel elliptic functions.

Jacobi elliptic functions are similarly obtained as inverse functions of elliptic integrals.

Jacobi considered the integral function

and inverted it: . stands for sinus amplitudinis and is the name of the new function.[11] He then introduced the functions cosinus amplitudinis and delta amplitudinis, which are defined as follows:

.

Only by taking this step, Jacobi could prove his general transformation formula of elliptic integrals in 1827.[12]

History

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Shortly after the development of infinitesimal calculus the theory of elliptic functions was started by the Italian mathematician Giulio di Fagnano and the Swiss mathematician Leonhard Euler. When they tried to calculate the arc length of a lemniscate they encountered problems involving integrals that contained the square root of polynomials of degree 3 and 4.[13] It was clear that those so called elliptic integrals could not be solved using elementary functions. Fagnano observed an algebraic relation between elliptic integrals, what he published in 1750.[13] Euler immediately generalized Fagnano's results and posed his algebraic addition theorem for elliptic integrals.[13]

Except for a comment by Landen[14] his ideas were not pursued until 1786, when Legendre published his paper Mémoires sur les intégrations par arcs d’ellipse.[15] Legendre subsequently studied elliptic integrals and called them elliptic functions. Legendre introduced a three-fold classification – three kinds – which was a crucial simplification of the rather complicated theory at that time. Other important works of Legendre are: Mémoire sur les transcendantes elliptiques (1792),[16] Exercices de calcul intégral (1811–1817),[17] Traité des fonctions elliptiques (1825–1832).[18] Legendre's work was mostly left untouched by mathematicians until 1826.

Subsequently, Niels Henrik Abel and Carl Gustav Jacobi resumed the investigations and quickly discovered new results. At first they inverted the elliptic integral function. Following a suggestion of Jacobi in 1829 these inverse functions are now called elliptic functions. One of Jacobi's most important works is Fundamenta nova theoriae functionum ellipticarum which was published 1829.[19] The addition theorem Euler found was posed and proved in its general form by Abel in 1829. In those days the theory of elliptic functions and the theory of doubly periodic functions were considered to be different theories. They were brought together by Briot and Bouquet in 1856.[20] Gauss discovered many of the properties of elliptic functions 30 years earlier but never published anything on the subject.[21]

See also

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References

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Literature

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Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
In , elliptic functions are meromorphic functions on the that exhibit double periodicity with respect to a lattice Λ=Zω1+Zω2\Lambda = \mathbb{Z} \omega_1 + \mathbb{Z} \omega_2, where ω1\omega_1 and ω2\omega_2 are linearly independent over the reals and (ω1/ω2)>0\Im(\omega_1 / \omega_2) > 0. These functions are non-constant only if they possess poles within each fundamental defined by the lattice, and by a variant of , any entire elliptic function must be constant. The residues of an elliptic function sum to zero over a fundamental domain, and the total multiplicity of its poles equals that of its zeros in a fundamental domain, and is equal to the order of the function (at least 2 for non-constant elliptic functions). The theory of elliptic functions originated from efforts to invert elliptic integrals, which arose in the 17th and 18th centuries through studies of arc lengths on ellipses and lemniscates by mathematicians such as , , Giulio Carlo Fagnano, and Leonhard Euler. classified elliptic integrals into three types in 1792, but the breakthrough came in 1827 when demonstrated the double periodicity of their inverses, independently followed by in 1829, who introduced the elliptic functions sn(u)\operatorname{sn}(u), cn(u)\operatorname{cn}(u), and dn(u)\operatorname{dn}(u). later formalized the theory in the mid-19th century with his \wp-function, defined as (z)=1z2+λΛ{0}(1(zλ)21λ2)\wp(z) = \frac{1}{z^2} + \sum_{\lambda \in \Lambda \setminus \{0\}} \left( \frac{1}{(z - \lambda)^2} - \frac{1}{\lambda^2} \right), which satisfies the differential equation (z)2=4(z)3g2(z)g3\wp'(z)^2 = 4\wp(z)^3 - g_2 \wp(z) - g_3, where g2g_2 and g3g_3 are invariants depending on the lattice. Elliptic functions find extensive applications across mathematics and related fields, including the rectification of curves like the via Fagnano's doubling formula and the computation of periods using Jacobi functions, where the period T=4K/ωT = 4K / \omega involves the complete KK. In , they describe phenomena such as Poncelet's porism for polygons inscribed in conics and the surface area of ellipsoids through integrals of the second kind. More abstractly, elliptic functions underpin the theory of s, which are crucial in for results like the Mordell-Weil theorem and in for protocols such as elliptic curve Diffie-Hellman.

Basic Concepts

Definition

In complex analysis, an elliptic function is defined as a meromorphic function f:CCf: \mathbb{C} \to \mathbb{C} that is doubly periodic with respect to two linearly independent complex periods ω1\omega_1 and ω2\omega_2, satisfying f(z+ω1)=f(z)f(z + \omega_1) = f(z) and f(z+ω2)=f(z)f(z + \omega_2) = f(z) for all zCz \in \mathbb{C}. This means the function repeats its values over translations by ω1\omega_1 and ω2\omega_2, which generate a discrete lattice in the known as the period lattice. The meromorphic nature implies that ff is holomorphic except at isolated poles, with only finitely many poles in any fundamental domain of the lattice. Double periodicity distinguishes elliptic functions from singly periodic meromorphic functions, such as the exp(z)\exp(z), which possesses only one fundamental period (up to multiples) and repeats along a single direction in the . In contrast, the two independent periods of an elliptic function create a two-dimensional repetition pattern, tiling the plane with identical copies of the function's behavior within each lattice cell. Prototype examples of elliptic functions include the Weierstrass \wp-function, which has a single double pole per period parallelogram, and the Jacobi sine function sn(z)\operatorname{sn}(z), which exhibits two simple poles in the same domain. These functions embody the essential features of the class without relying on explicit constructions here. Understanding elliptic functions presupposes familiarity with key concepts from , including meromorphic functions, residues at poles, and the notion of periodicity in the .

Period Lattice and Fundamental Domain

The period lattice Λ\Lambda associated with an elliptic function is the discrete additive of the C\mathbb{C} generated by two linearly independent complex numbers ω1\omega_1 and ω2\omega_2, explicitly given by Λ={mω1+nω2m,nZ}\Lambda = \{ m \omega_1 + n \omega_2 \mid m, n \in \mathbb{Z} \}, where the ω2/ω1\omega_2 / \omega_1 is not real to ensure the generators are linearly independent over the reals. This lattice forms a two-dimensional grid in C\mathbb{C}, serving as the set of all periods of the function, and any elliptic function f(z)f(z) satisfies f(z+λ)=f(z)f(z + \lambda) = f(z) for all λΛ\lambda \in \Lambda. The fundamental spanned by ω1\omega_1 and ω2\omega_2 is the set {sω1+tω20s,t1}\{ s \omega_1 + t \omega_2 \mid 0 \leq s, t \leq 1 \}, which tiles the plane under translations by lattice points and captures the basic repeating unit of the function's periodicity. The fundamental domain for the lattice Λ\Lambda is a subset DCD \subset \mathbb{C} such that the quotient map CC/Λ\mathbb{C} \to \mathbb{C}/\Lambda induces a bijection from DD to the quotient space, with a standard choice being the open parallelogram {sω1+tω20<s,t<1}\{ s \omega_1 + t \omega_2 \mid 0 < s, t < 1 \} augmented by appropriate boundary points to account for identifications. In this quotient C/Λ\mathbb{C}/\Lambda, points differing by elements of Λ\Lambda are identified, resulting in a compact Riemann surface topologically equivalent to a torus, where opposite boundaries of the parallelogram are glued together: the side from 00 to ω1\omega_1 is identified with the side from ω2\omega_2 to ω1+ω2\omega_1 + \omega_2 via translation by ω2\omega_2, and similarly for the other pair of sides. This toroidal structure ensures that elliptic functions, being meromorphic on C\mathbb{C}, descend to well-defined meromorphic functions on the torus with controlled poles and zeros. To classify lattices up to similarity (homothety by nonzero complex scalars), the modular parameter τ=ω2/ω1\tau = \omega_2 / \omega_1 is introduced, which lies in the upper half-plane H={τC(τ)>0}\mathbb{H} = \{ \tau \in \mathbb{C} \mid \Im(\tau) > 0 \}. Two lattices Λ\Lambda and Λ\Lambda' are similar if and only if their corresponding τ\tau and τ\tau' are related by an element of the SL2(Z)\mathrm{SL}_2(\mathbb{Z}), acting via fractional linear transformations τ(aτ+b)/(cτ+d)\tau \mapsto (a\tau + b)/(c\tau + d) for a,b,c,dZa, b, c, d \in \mathbb{Z} with adbc=1ad - bc = 1; this parameterization reduces the study of elliptic functions to those associated with τH\tau \in \mathbb{H}. Elliptic functions repeat their values across the lattice translations, visualizing the periodicity as a tiling of the by fundamental parallelograms, where the function's behavior on one such domain determines it everywhere, akin to wrapping the plane onto a surface. This geometric repetition underscores the double-periodic nature, with the lattice points acting as sites of potential singularities in specific elliptic functions.

Liouville's Theorems

First Theorem

Liouville's first theorem asserts that every holomorphic elliptic function is constant. This result forms the foundation for understanding the structure of elliptic functions, emphasizing that non-constant examples must necessarily have poles. The proof proceeds by leveraging the double periodicity inherent to elliptic functions. Consider a holomorphic elliptic function f(z)f(z), which is entire and satisfies f(z+ω1)=f(z+ω2)=f(z)f(z + \omega_1) = f(z + \omega_2) = f(z) for fundamental periods ω1,ω2\omega_1, \omega_2. The values of ff are fully determined by its restriction to the fundamental formed by the period lattice, a compact set. Since ff is continuous on this compact domain, it attains a , hence is bounded there. By periodicity, ff is then bounded on the entire C\mathbb{C}. As a bounded , ff must be constant by the standard Liouville's theorem in . This theorem implies that no non-constant elliptic functions exist without poles, underscoring the essential role of singularities in generating the rich behavior of these functions. It was originally established by in his 1847 memoir on the of doubly periodic functions.

Second Theorem

Liouville's second theorem asserts that any elliptic function, being meromorphic and doubly periodic with respect to a lattice Λ\Lambda, has only finitely many poles in a fundamental domain, such as the fundamental Ω\Omega spanned by the basis periods ω1\omega_1 and ω2\omega_2, and that the sum of the residues at these poles vanishes. The finiteness of poles follows from the isolated of poles in meromorphic functions and the of the quotient C/Λ\mathbb{C}/\Lambda, which is topologically a ; thus, the preimage of any discrete set under the projection intersects Ω\Omega in finitely many points. Equivalently, supposing infinitely many poles in Ω\Omega would, by periodicity, generate infinitely many poles accumulating everywhere in C\mathbb{C}, implying an at infinity on the extended and contradicting the global meromorphicity of the function. To establish the vanishing sum of residues, consider the contour integral of the elliptic function ff over the boundary Ω\partial \Omega of the fundamental parallelogram, oriented positively. By the residue theorem, Ωf(z)dz=2πikRes(f,ak),\oint_{\partial \Omega} f(z) \, dz = 2\pi i \sum_{k} \operatorname{Res}(f, a_k), where the sum is over all poles aka_k inside Ω\Omega. However, the double periodicity f(z+ω1)=f(z)f(z + \omega_1) = f(z) and f(z+ω2)=f(z)f(z + \omega_2) = f(z) implies that the integrals along opposite sides of Ω\partial \Omega cancel pairwise, yielding Ωf(z)dz=0\oint_{\partial \Omega} f(z) \, dz = 0. Therefore, kRes(f,ak)=0\sum_{k} \operatorname{Res}(f, a_k) = 0. This theorem underscores the controlled analytic behavior of elliptic functions over the lattice, ensuring that their meromorphic extensions remain well-defined and that pole data alone suffices to determine the function up to a constant multiple, thereby enabling systematic construction and analysis in the theory.

Third Theorem

Liouville's third theorem asserts that a non-constant elliptic function ff attains every complex value aCa \in \mathbb{C} exactly the same number of times in any fundamental of its period lattice, counting multiplicities; this number equals the order of ff, which is the number of its poles (also counting multiplicities) in the parallelogram. This uniform distribution of values underscores the balanced structure inherent to doubly periodic meromorphic functions on the . The proof relies on the argument principle applied to the function g(z)=f(z)ag(z) = f(z) - a. Since gg is also elliptic with the same period lattice as ff, it shares the same poles as ff, each with identical orders, and thus has the same fixed number mm of poles in the fundamental Ω\Omega. Consider the contour over the boundary Ω\partial \Omega of Ω\Omega: 12πiΩf(z)f(z)adz=NP,\frac{1}{2\pi i} \oint_{\partial \Omega} \frac{f'(z)}{f(z) - a} \, dz = N - P, where NN is the number of zeros of g(z)g(z) (i.e., solutions to f(z)=af(z) = a) in Ω\Omega, counting multiplicity, and P=mP = m is the number of poles. Due to the periodicity of ff, the contributions from opposite sides of the parallelogram cancel pairwise, rendering the entire integral zero. Therefore, NP=0N - P = 0, so N=mN = m for every aa, independent of the specific value. This theorem implies a uniform coverage of the complex plane by the image of the fundamental domain under ff, ensuring that no value is omitted or overrepresented relative to others. It forms a cornerstone for deriving addition theorems and other identities in elliptic function theory, as the consistent multiplicity facilitates algebraic manipulations and connections to elliptic integrals.

Classical Elliptic Functions

Weierstrass ℘-Function

The Weierstrass ℘-function, denoted ℘(z | Λ) or simply ℘(z) for a given period lattice Λ in the , is defined by the convergent series (z)=1z2+ωΛ{0}(1(zω)21ω2).℘(z) = \frac{1}{z^2} + \sum_{\omega \in \Lambda \setminus \{0\}} \left( \frac{1}{(z - \omega)^2} - \frac{1}{\omega^2} \right). This series converges absolutely and uniformly on compact subsets of ℂ excluding the points of Λ, making ℘(z) a on ℂ. As an elliptic function with respect to Λ, ℘(z) is doubly periodic, satisfying ℘(z + ω) = ℘(z) for all ω ∈ Λ, where the fundamental periods are typically taken as ω₁ and ω₂ generating Λ. It is an even function, ℘(-z) = ℘(z), and possesses double poles at each lattice point z ≡ 0 mod Λ, with residue zero and principal part 1/z². These pole and periodicity properties follow from Liouville's theorems on elliptic functions, ensuring ℘(z) has exactly two poles (counting multiplicity) per fundamental . The derivative ℘'(z) satisfies the nonlinear [(z)]2=4(z)3g2(z)g3,[℘'(z)]^2 = 4℘(z)^3 - g_2 ℘(z) - g_3, where the invariants g₂ and g₃ are absolute constants depending only on the lattice Λ, defined by the absolutely g2=60ωΛ{0}1ω4,g3=140ωΛ{0}1ω6.g_2 = 60 \sum_{\omega \in \Lambda \setminus \{0\}} \frac{1}{\omega^4}, \quad g_3 = 140 \sum_{\omega \in \Lambda \setminus \{0\}} \frac{1}{\omega^6}. These invariants characterize the isomorphism class of the elliptic curve associated with Λ via the Weierstrass form y² = 4x³ - g₂x - g₃. The right-hand side of the differential equation factors as 4(℘(z) - e₁)(℘(z) - e₂)(℘(z) - e₃), where e₁, e₂, e₃ are the distinct roots of the cubic 4x³ - g₂x - g₃ = 0, satisfying e₁ + e₂ + e₃ = 0 and ordered such that e₁ > e₂ > e₃ when g₂ > 0 and g₃ real. These roots correspond to the values of ℘ at the half-periods: e₁ = ℘(ω₁/2), e₂ = ℘(ω₃/2), e₃ = ℘(ω₂/2), where the half-periods are ω₁/2, ω₂/2, ω₃/2 with ω₃ = ω₁ + ω₂, and ℘'(ωⱼ/2) = 0 for j = 1,2,3. The Δ = g₂³ - 27g₃² = 16(e₁ - e₂)²(e₂ - e₃)²(e₃ - e₁)² > 0 ensures the roots are real and distinct for non-degenerate lattices. The ℘-function can also be expressed in terms of Jacobi theta functions, providing an alternative representation via infinite products or quotients involving the nome q = exp(πi τ) with τ = ω₃/ω₁.

Jacobi Elliptic Functions

The Jacobi elliptic functions provide an alternative parameterization of elliptic functions, particularly suited for applications involving elliptic integrals and rectangular period lattices, in contrast to the Weierstrass ℘-function's use of general lattices. These functions, introduced by in the , are defined in terms of the inverse of the incomplete elliptic integral of the first kind and are widely used in physics and engineering for solving nonlinear differential equations, such as those describing motion or electrical circuits. The primary Jacobi elliptic function is the sine amplitude sn(u,k)\operatorname{sn}(u,k), defined as the inverse of the F(ϕ,k)=0ϕdθ1k2sin2θF(\phi,k) = \int_0^\phi \frac{d\theta}{\sqrt{1 - k^2 \sin^2 \theta}}
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