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Elliptic function
View on WikipediaIn 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
[edit]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
[edit]

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
[edit]The following three theorems are known as Liouville's theorems (1847).
1st theorem
[edit]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
[edit]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
[edit]A non-constant elliptic function takes on every value the same number of times in counted with multiplicity.[5]
Weierstrass ℘-function
[edit]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 .
-
Weierstrass -function with period lattice
-
Derivative of the -function
Relation to elliptic integrals
[edit]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
[edit]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
[edit]References
[edit]- ^ Rolf Busam (2006), Funktionentheorie 1 (in German) (4., korr. und erw. Aufl ed.), Berlin: Springer, p. 259, ISBN 978-3-540-32058-6
- ^ Rolf Busam (2006), Funktionentheorie 1 (in German) (4., korr. und erw. Aufl ed.), Berlin: Springer, p. 258, ISBN 978-3-540-32058-6
- ^ Jeremy Gray (2015), Real and the complex : a history of analysis in the 19th century (in German), Cham, pp. 118f, ISBN 978-3-319-23715-2
{{citation}}: CS1 maint: location missing publisher (link) - ^ Rolf Busam (2006), Funktionentheorie 1 (in German) (4., korr. und erw. Aufl ed.), Berlin: Springer, p. 260, ISBN 978-3-540-32058-6
- ^ Rolf Busam (2006), Funktionentheorie 1 (in German) (4., korr. und erw. Aufl ed.), Berlin: Springer, p. 262, ISBN 978-3-540-32058-6
- ^ a b K. Chandrasekharan (1985), Elliptic functions (in German), Berlin: Springer-Verlag, p. 28, ISBN 0-387-15295-4
- ^ Rolf Busam (2006), Funktionentheorie 1 (in German) (4., korr. und erw. Aufl ed.), Berlin: Springer, p. 275, ISBN 978-3-540-32058-6
- ^ Rolf Busam (2006), Funktionentheorie 1 (in German) (4., korr. und erw. Aufl ed.), Berlin: Springer, p. 276, ISBN 978-3-540-32058-6
- ^ Gray, Jeremy (14 October 2015), Real and the complex : a history of analysis in the 19th century (in German), Cham, p. 74, ISBN 978-3-319-23715-2
{{citation}}: CS1 maint: location missing publisher (link) - ^ Gray, Jeremy (14 October 2015), Real and the complex : a history of analysis in the 19th century (in German), Cham, p. 75, ISBN 978-3-319-23715-2
{{citation}}: CS1 maint: location missing publisher (link) - ^ Gray, Jeremy (14 October 2015), Real and the complex : a history of analysis in the 19th century (in German), Cham, p. 82, ISBN 978-3-319-23715-2
{{citation}}: CS1 maint: location missing publisher (link) - ^ Gray, Jeremy (14 October 2015), Real and the complex : a history of analysis in the 19th century (in German), Cham, p. 81, ISBN 978-3-319-23715-2
{{citation}}: CS1 maint: location missing publisher (link) - ^ a b c Gray, Jeremy (2015). Real and the complex : a history of analysis in the 19th century. Cham. pp. 23f. ISBN 978-3-319-23715-2. OCLC 932002663.
{{cite book}}: CS1 maint: location missing publisher (link) - ^ John Landen: An Investigation of a general Theorem for finding the Length of any Arc of any Conic Hyperbola, by Means of Two Elliptic Arcs, with some other new and useful Theorems deduced therefrom. In: The Philosophical Transactions of the Royal Society of London 65 (1775), Nr. XXVI, S. 283–289, JSTOR 106197.
- ^ Adrien-Marie Legendre: Mémoire sur les intégrations par arcs d’ellipse. In: Histoire de l’Académie royale des sciences Paris (1788), S. 616–643. – Ders.: Second mémoire sur les intégrations par arcs d’ellipse, et sur la comparaison de ces arcs. In: Histoire de l’Académie royale des sciences Paris (1788), S. 644–683.
- ^ Adrien-Marie Legendre: Mémoire sur les transcendantes elliptiques, où l’on donne des méthodes faciles pour comparer et évaluer ces trancendantes, qui comprennent les arcs d’ellipse, et qui se rencontrent frèquemment dans les applications du calcul intégral. Du Pont & Firmin-Didot, Paris 1792. Englische Übersetzung A Memoire on Elliptic Transcendentals. In: Thomas Leybourn: New Series of the Mathematical Repository. Band 2. Glendinning, London 1809, Teil 3, S. 1–34.
- ^ Adrien-Marie Legendre: Exercices de calcul integral sur divers ordres de transcendantes et sur les quadratures. 3 Bände. (Band 1, Band 2, Band 3). Paris 1811–1817.
- ^ Adrien-Marie Legendre: Traité des fonctions elliptiques et des intégrales eulériennes, avec des tables pour en faciliter le calcul numérique. 3 Bde. (Band 1, Band 2, Band 3/1, Band 3/2, Band 3/3). Huzard-Courcier, Paris 1825–1832.
- ^ Carl Gustav Jacob Jacobi: Fundamenta nova theoriae functionum ellipticarum. Königsberg 1829.
- ^ Gray, Jeremy (2015). Real and the complex : a history of analysis in the 19th century. Cham. p. 122. ISBN 978-3-319-23715-2. OCLC 932002663.
{{cite book}}: CS1 maint: location missing publisher (link) - ^ Gray, Jeremy (2015). Real and the complex : a history of analysis in the 19th century. Cham. p. 96. ISBN 978-3-319-23715-2. OCLC 932002663.
{{cite book}}: CS1 maint: location missing publisher (link)
Literature
[edit]- Abramowitz, Milton; Stegun, Irene Ann, eds. (1983) [June 1964]. "Chapter 16". Handbook of Mathematical Functions with Formulas, Graphs, and Mathematical Tables. Applied Mathematics Series. Vol. 55 (Ninth reprint with additional corrections of tenth original printing with corrections (December 1972); first ed.). Washington D.C.; New York: United States Department of Commerce, National Bureau of Standards; Dover Publications. pp. 567, 627. ISBN 978-0-486-61272-0. LCCN 64-60036. MR 0167642. LCCN 65-12253. See also chapter 18. (only considers the case of real invariants).
- N. I. Akhiezer, Elements of the Theory of Elliptic Functions, (1970) Moscow, translated into English as AMS Translations of Mathematical Monographs Volume 79 (1990) AMS, Rhode Island ISBN 0-8218-4532-2
- Tom M. Apostol, Modular Functions and Dirichlet Series in Number Theory, Springer-Verlag, New York, 1976. ISBN 0-387-97127-0 (See Chapter 1.)
- E. T. Whittaker and G. N. Watson. A course of modern analysis, Cambridge University Press, 1952
External links
[edit]- "Elliptic function", Encyclopedia of Mathematics, EMS Press, 2001 [1994]
- MAA, Translation of Abel's paper on elliptic functions.
- Elliptic Functions and Elliptic Integrals on YouTube, lecture by William A. Schwalm (4 hours)
- Johansson, Fredrik (2018). "Numerical Evaluation of Elliptic Functions, Elliptic Integrals and Modular Forms". arXiv:1806.06725 [cs.NA].
Elliptic function
View on GrokipediaBasic Concepts
Definition
In complex analysis, an elliptic function is defined as a meromorphic function that is doubly periodic with respect to two linearly independent complex periods and , satisfying and for all .[4] This means the function repeats its values over translations by and , which generate a discrete lattice in the complex plane known as the period lattice.[5] The meromorphic nature implies that is holomorphic except at isolated poles, with only finitely many poles in any fundamental domain of the lattice.[4] Double periodicity distinguishes elliptic functions from singly periodic meromorphic functions, such as the exponential function , which possesses only one fundamental period (up to multiples) and repeats along a single direction in the complex plane.[4] 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 -function, which has a single double pole per period parallelogram, and the Jacobi sine function , which exhibits two simple poles in the same domain.[4] These functions embody the essential features of the class without relying on explicit constructions here. Understanding elliptic functions presupposes familiarity with key concepts from complex analysis, including meromorphic functions, residues at poles, and the notion of periodicity in the complex plane.[4]Period Lattice and Fundamental Domain
The period lattice associated with an elliptic function is the discrete additive subgroup of the complex plane generated by two linearly independent complex numbers and , explicitly given by , where the ratio is not real to ensure the generators are linearly independent over the reals.[6][1] This lattice forms a two-dimensional grid in , serving as the set of all periods of the function, and any elliptic function satisfies for all .[7] The fundamental parallelogram spanned by and is the set , which tiles the plane under translations by lattice points and captures the basic repeating unit of the function's periodicity.[6] The fundamental domain for the lattice is a subset such that the quotient map induces a bijection from to the quotient space, with a standard choice being the open parallelogram augmented by appropriate boundary points to account for identifications.[1] In this quotient , points differing by elements of 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 to is identified with the side from to via translation by , and similarly for the other pair of sides.[6] This toroidal structure ensures that elliptic functions, being meromorphic on , descend to well-defined meromorphic functions on the torus with controlled poles and zeros.[1] To classify lattices up to similarity (homothety by nonzero complex scalars), the modular parameter is introduced, which lies in the upper half-plane .[6] Two lattices and are similar if and only if their corresponding and are related by an element of the modular group , acting via fractional linear transformations for with ; this parameterization reduces the study of elliptic functions to those associated with .[6][1] Elliptic functions repeat their values across the lattice translations, visualizing the periodicity as a tiling of the complex plane by fundamental parallelograms, where the function's behavior on one such domain determines it everywhere, akin to wrapping the plane onto a torus surface.[7] This geometric repetition underscores the double-periodic nature, with the lattice points acting as sites of potential singularities in specific elliptic functions.[6]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 , which is entire and satisfies for fundamental periods . The values of are fully determined by its restriction to the fundamental parallelogram formed by the period lattice, a compact set. Since is continuous on this compact domain, it attains a maximum and minimum, hence is bounded there. By periodicity, is then bounded on the entire complex plane . As a bounded entire function, must be constant by the standard Liouville's theorem in complex analysis.[8] 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 Joseph Liouville in his 1847 memoir on the classification of doubly periodic functions.[9]Second Theorem
Liouville's second theorem asserts that any elliptic function, being meromorphic and doubly periodic with respect to a lattice , has only finitely many poles in a fundamental domain, such as the fundamental parallelogram spanned by the basis periods and , and that the sum of the residues at these poles vanishes. The finiteness of poles follows from the isolated nature of poles in meromorphic functions and the compactness of the quotient space , which is topologically a torus; thus, the preimage of any discrete set under the projection map intersects in finitely many points. Equivalently, supposing infinitely many poles in would, by periodicity, generate infinitely many poles accumulating everywhere in , implying an essential singularity at infinity on the extended complex plane and contradicting the global meromorphicity of the function. To establish the vanishing sum of residues, consider the contour integral of the elliptic function over the boundary of the fundamental parallelogram, oriented positively. By the residue theorem, where the sum is over all poles inside . However, the double periodicity and implies that the integrals along opposite sides of cancel pairwise, yielding . Therefore, .[4] 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 attains every complex value exactly the same number of times in any fundamental parallelogram of its period lattice, counting multiplicities; this number equals the order of , which is the number of its poles (also counting multiplicities) in the parallelogram.[10][11] This uniform distribution of values underscores the balanced structure inherent to doubly periodic meromorphic functions on the complex plane. The proof relies on the argument principle applied to the function . Since is also elliptic with the same period lattice as , it shares the same poles as , each with identical orders, and thus has the same fixed number of poles in the fundamental parallelogram . Consider the contour integral over the boundary of : where is the number of zeros of (i.e., solutions to ) in , counting multiplicity, and is the number of poles. Due to the periodicity of , the contributions from opposite sides of the parallelogram cancel pairwise, rendering the entire integral zero. Therefore, , so for every , independent of the specific value.[10] This theorem implies a uniform coverage of the complex plane by the image of the fundamental domain under , 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.[11]Classical Elliptic Functions
Weierstrass ℘-Function
The Weierstrass ℘-function, denoted ℘(z | Λ) or simply ℘(z) for a given period lattice Λ in the complex plane, is defined by the convergent series This series converges absolutely and uniformly on compact subsets of ℂ excluding the points of Λ, making ℘(z) a meromorphic function 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 parallelogram. The derivative ℘'(z) satisfies the nonlinear differential equation where the invariants g₂ and g₃ are absolute constants depending only on the lattice Λ, defined by the absolutely convergent series 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 discriminant 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 Carl Gustav Jacob Jacobi in the 19th century, 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 pendulum motion or electrical circuits. The primary Jacobi elliptic function is the sine amplitude , defined as the inverse of the elliptic integral , where is the modulus parameter, such that implies . The complementary functions are then and . These definitions ensure that and , analogous to trigonometric identities.[12][13] The Jacobi elliptic functions are doubly periodic, with real period and imaginary period , where is the complete elliptic integral of the first kind and . They exhibit quasi-periodicity over half-periods; for instance, and , leading to multipliers like signs or ratios of other Jacobi functions under these shifts. A key property is the addition formula: which facilitates computations and derivations in applications. Similar formulas exist for and .[14][15] The Jacobi functions relate to the Weierstrass ℘-function through expressions that connect their respective lattices and moduli; specifically, , where , are the roots of the Weierstrass cubic , and . As the modulus , the functions degenerate to elementary trigonometric forms: , , and , recovering circular functions from the elliptic case.[16]Relations and Applications
Relation to Elliptic Integrals
Elliptic integrals arise in the evaluation of arc lengths and areas bounded by certain algebraic curves, such as ellipses and lemniscates, and are classified into three kinds based on Legendre's canonical forms. The incomplete elliptic integral of the first kind is defined as where is the amplitude and (with ) is the modulus. The incomplete elliptic integral of the second kind is and the incomplete elliptic integral of the third kind is with parameter . The corresponding complete elliptic integrals are obtained by setting : These integrals cannot be expressed in terms of elementary functions for general , motivating the development of their inverses as elliptic functions. The historical motivation for elliptic functions traces back to problems in rectifying curves like the lemniscate of Bernoulli, whose arc length integral is a special case of the elliptic integral of the first kind with . In 1718, Giulio Carlo Fagnano dei Toschi solved the problem of dividing the lemniscate into equal arcs using geometric methods that implicitly involved elliptic integrals, though without explicit integration. This work laid foundational insights into addition formulas for such integrals, later expanded by Leonhard Euler in the 1760s through series expansions and transformations. The full inversion of these integrals to obtain doubly periodic functions was achieved independently by Niels Henrik Abel in 1827 and Carl Gustav Jacob Jacobi in 1829, transforming the study from transcendental integrals to a theory of meromorphic functions with applications in analysis and geometry.[17] Jacobi's approach to inversion defines the elliptic functions directly as the inverse mappings of these integrals. Specifically, if , then the amplitude function is , and the Jacobi sine is . Similarly, and arise from the second kind, providing a parametric representation that generalizes trigonometric identities. This inversion bridges the non-elementary nature of the integrals to functions satisfying algebraic differential equations and possessing double periodicity. Addition theorems for elliptic functions, such as the formula for , derive from the composition of elliptic integrals. To sketch the derivation, consider and ; then where satisfies a relation obtained by substituting into the integral form and using tangent addition via the identity , adjusted for the elliptic modulus, yielding . This algebraic form emerges from the integral's homogeneity and the geometry of the parameter space. In degenerate cases, elliptic integrals and their inverses reduce to elementary forms. When , the modulus vanishes, and , , \Pi(\phi, n, 0) = \int_0^\phi \frac{\mathrm{d}\theta}{1 - n \sin^2 \theta), with the complete integrals ; correspondingly, , , and , recovering circular integrals and trigonometric functions. When , the integrals simplify to hyperbolic forms, such as , leading to . These limits highlight the elliptic functions as generalizations of trigonometric and hyperbolic functions.Geometric Interpretations and Applications
Elliptic functions admit a profound geometric interpretation as meromorphic functions on the complex torus, which is the quotient of the complex plane by a lattice with (the upper half-plane), forming a compact Riemann surface of genus 1. This torus serves as the natural domain for elliptic functions with periods 1 and , where the functions are holomorphic except at lattice points. Certain quotients of the torus, such as by the involution , are biholomorphic to the Riemann sphere via uniformizing maps.[18] The double poles of these functions, such as the Weierstrass -function, are located at the images of the lattice points on the torus, providing a visual embedding where the torus is often depicted as a surface in with periodic identifications, highlighting the doubly periodic nature and pole structure that distinguishes elliptic functions from simpler trigonometric ones.[19] The geometry of elliptic functions is further illuminated by the action of the modular group on the modulus via Möbius transformations with , which identifies tori up to isomorphism and parametrizes the moduli space of elliptic curves. This action classifies elliptic curves through the -invariant, a modular function of weight zero given by where and are the invariants of the Weierstrass -function associated to the lattice, providing a bijection from the quotient to that labels isomorphism classes of elliptic curves.[20][19] In applications, Jacobi elliptic functions describe the nonlinear dynamics of a simple pendulum, where the angular displacement for large amplitudes is expressed using the sine amplitude function , with the period determined by the complete elliptic integral involving the modulus related to the energy; specifically, the Jacobi function captures the periodic variation in angular velocity.[21] The Weierstrass -function appears in solutions to integrable systems, such as the sine-Gordon and Korteweg-de Vries equations, where it parametrizes soliton interactions and traveling wave profiles on the torus.[22] Elliptic curves, geometrically linked to these functions via their period lattices, underpin modern cryptography through protocols like Elliptic Curve Diffie-Hellman (ECDH), where two parties exchange points on the curve to compute a shared secret from private keys and in a cyclic subgroup of order , enabling secure key agreement over insecure channels with smaller key sizes than RSA.[23] These curves also connect to modular forms, as the -invariant serves as a hauptmodul generating the field of modular functions for .[20] Modern extensions generalize this geometry using theta functions, where the Riemann theta function of genus is defined as \theta(z; \Omega) = \sum_{m \in \mathbb{Z}^g} \exp\left( \pi i \, ^t m \cdot \Omega \cdot m + 2\pi i \, ^t m \cdot z \right) on (the Siegel upper half-space), providing coordinates for higher-genus Riemann surfaces and abelian varieties beyond the toroidal case.[24]Historical Development
Early History
The study of elliptic functions originated in the 17th and 18th centuries from problems in geometry and analysis, particularly the computation of arc lengths of certain curves, long before the development of complex analysis.[25] Early efforts focused on real integrals arising in these contexts, such as those for the ellipse—ironically giving rise to the term "elliptic" despite the integrals not being directly tied to elliptical shapes in the modern sense.[26] These integrals proved intractable in elementary terms, marking a shift toward more advanced analytical techniques.[25] Key precursors emerged from variational problems in mechanics, notably Jakob Bernoulli's work on the shape of an elastic rod under compression and the arc length of the lemniscate curve (a figure-eight shape), which led to integrals resembling those later classified as elliptic.[25] In 1694, Bernoulli investigated the arc length of the lemniscate curve through the integral form that would become central to elliptic integrals, conjecturing it could not be expressed using known functions.[26] This built on earlier explorations, such as his 1679 study of spiral arc lengths, highlighting the challenges of non-elementary integrals in curvilinear geometry.[25] In 1718, Giovanni Fagnano advanced the rectification of the lemniscate arc length using methods that effectively employed elliptic integrals, developing algebraic relations to compute portions of the curve.[27] His contributions, published in the Giornale de’ letterati d’Italia, connected geometric properties of the lemniscate to integral computations, influencing subsequent analysts without yet formulating periodic functions.[26] Leonhard Euler expanded on lemniscatic integrals in the 1760s, deriving general theorems for their summation and exploring connections to beta functions, which hinted at underlying periodic structures in the solutions.[26] Through works like those in the Novi Commentarii Academiae Scientiarum Imperialis Petropolitanae (1756 and 1766–1767), Euler systematized these integrals, laying groundwork for recognizing their repetitive nature, though still treating them as real-valued expressions rather than invertible functions.[25] By the early 1800s, Adrien-Marie Legendre had compiled extensive tables of elliptic integrals in his Exercices de calcul intégral (1811–1816), classifying them into three standard forms for practical evaluation without inverting them to yield explicit functions.[26] This tabulation emphasized computational aspects for applications in mechanics and astronomy, solidifying the integrals' importance while deferring the conceptual leap to periodic functions.[25] The inversion of these integrals—expressing the variable as a function of the integral—remained an undeveloped idea at this stage.[26]Key Contributions in the 19th Century
In 1827, Niels Henrik Abel published his seminal paper "Recherches sur les fonctions elliptiques," where he proved the addition theorem for elliptic integrals using elementary methods and demonstrated the inversion of these integrals to yield doubly periodic functions, marking a pivotal shift toward treating elliptic functions as independent entities rather than mere inverses of integrals.[28] This work, appearing in the Journal für die reine und angewandte Mathematik, established the double periodicity property, distinguishing elliptic functions from previously known transcendental functions and laying the groundwork for their complex-domain analysis.[29] Building on Abel's foundations, Carl Gustav Jacob Jacobi advanced the theory in the late 1820s and 1830s, introducing the elliptic functions sn(u), cn(u), and dn(u) as inverses of elliptic integrals with modulus k, characterized by their double periodicity and relations to Jacobi theta functions.[2] In his 1829 treatise Fundamenta Nova Theoriae Functionum Ellipticarum, Jacobi developed a comprehensive transformation theory, including addition formulas and landen's transformations, which standardized the algebraic manipulation of these functions and emphasized their periodic nature over rectangular lattices. This publication, issued by the Borntraeger brothers in Königsberg, synthesized earlier results and promoted elliptic functions as a unified framework for solving problems in analysis and geometry.[30] Joseph Liouville contributed to the classification of elliptic functions in 1847 through theorems delineating their pole and zero structures, proving that non-constant elliptic functions are meromorphic with an equal number of zeros and poles (counting multiplicities) in each fundamental parallelogram, and that the sum of residues at poles vanishes.[10] These results, published in his papers from the 1840s in the Journal de Mathématiques Pures et Appliquées (which he founded in 1836), provided essential tools for understanding the global behavior of elliptic functions over the complex plane and confirmed their impossibility of single periodicity without constancy. Karl Weierstrass further unified the theory in the 1850s and 1860s by introducing the ℘-function, defined via a uniform approach over arbitrary lattices generated by periods 2ω₁ and 2ω₂, expressed as a Weierstrass series to ensure convergence and double periodicity.[31] In his lectures from 1863 (published posthumously in 1895 as Vorlesungen über die Theorie der elliptischen Funktionen), Weierstrass reformulated elliptic integrals in the canonical form ∫ dt / √(4t³ - g₂ t - g₃), where g₂ and g₃ are lattice invariants, enabling a rigorous elliptic curve parametrization via (℘(u), ℘'(u)) and shifting the focus from real-variable specifics to complex analytic generality.[32] This lattice-based framework standardized the domain and facilitated expansions to higher genera. Later in the century, unification efforts included the 1859 textbook Théorie des fonctions elliptiques by Charles Briot and Jean-Claude Bouquet, which synthesized Jacobi and Weierstrass approaches into an accessible treatment emphasizing double-periodic properties and applications to differential equations.[33] Concurrently, Bernhard Riemann's 1857 memoir "Theorie der Abel'schen Functionen" introduced theta functions θ(z; Ω) as multivariable generalizations of elliptic functions, providing a holomorphic framework for abelian integrals and extending periodicity to higher-dimensional tori, thus bridging elliptic theory with algebraic geometry.[34] These 19th-century developments marked a transition from real elliptic integrals to complex doubly periodic functions, standardizing their theory through addition theorems, modular forms, and lattice invariants, which profoundly influenced subsequent mathematics.[2]References
- https://en.wikisource.org/wiki/A_History_of_Mathematics/Recent_Times/Theory_of_Functions
