A modern student usually meets elliptic curves in a very polished form: Then one defines a group law by drawing lines, introduces divisors, Abel maps, Jacobians, period lattices, and so on. This is beautiful, but historically it is backwards.
The older story began with much more concrete questions: How long is an arc of an ellipse? Can one compute integrals such as Can such integrals be added, transformed, tabulated, and inverted? Can one build a new trigonometry out of them?
The answer, discovered gradually by Euler, Fagnano, Legendre, Abel, Jacobi, and others, was yes. But the route was computational. It began with integrals, not abstract curves.
The purpose of this article is to reconstruct that route. We will start with the circle, because the circle is the prototype. Then we will move to the lemniscate and elliptic integrals. Then we will see why addition formulae appear. Then we will see how Abel generalized the whole story to higher-degree algebraic integrals. Only near the end will we mention the modern language, and even then only as a summary of what the old computations were already saying.
The circle: sine as an inverse integral
Let us begin with the unit circle On the upper semicircle,
the length element is
Equivalently,
Now compute with
Then
Therefore
we get
Thus the arc length from
to
is
But on the unit circle, arc length equals angle. Thus if then
This is an important shift in viewpoint. Instead of thinking of sine first as a triangle ratio, we may think of sine as the inverse of the integral
In this view, trigonometry is the theory of the inverse function of a particular algebraic integral. This is the template for everything that follows.
Addition for Circle
Now suppose
Then Also
We know In terms of
and
, this becomes
So the identity
can be written as an integral identity:
This is the first model of an addition theorem. It says that the sum of two integrals of the same kind can be replaced by one integral of the same kind, with a new algebraic upper limit.
That is exactly the sort of thing eighteenth- and nineteenth-century mathematicians searched for. They wanted to know: If we replace by a more complicated square root, do addition formulae still exist?
Ellitptic Functions
For the ellipse , write
and
. Then
and
, so the arc-length element is
. If
and
, this becomes
. Now factor out
: Hence the arc length from
to
is
This integral is called an elliptic integral of the second kind :
Now put to get
This is already an integral involving the square root of a quartic expression, because it equals
This is the important structural point. The ellipse has led us to integrals of the form
The polynomial under the square root is which has degree four. This is why elliptic integrals are naturally attached to cubic and quartic polynomials.
The integral of the first kind is
Using the same substitution , it becomes
This one is not exactly the arc length of the ellipse. The arc length gives , the second kind. But the first kind appears just as naturally once one studies the whole family of algebraic integrals built from the same square root.
Legendre’s achievement was to organize this entire world. Before him, many integrals appeared in different disguises: arc lengths of ellipses, pendulum motion, attraction problems, transformations of radicals, and integrals involving square roots of cubic or quartic polynomials. Legendre showed that a vast collection of such expressions could be reduced to a small number of standard forms. His three basic types were the first kind,
the second kind,
and the third kind,
These are called incomplete elliptic integrals because the upper limit is variable. If
, one gets the complete elliptic integrals
Legendre’s work was not just naming these integrals. It was a program of reduction. Given an integral of the rough form where
is cubic or quartic and
is rational, one tries to transform the roots of
into a standard arrangement, usually leading to a radical like
Then one decomposes the rational part into pieces corresponding to
,
,
, plus elementary terms. In this sense Legendre did for elliptic integrals something like what earlier algebraists had done for rational functions: he made a normal form theory. Abel and Jacobi later changed the emphasis. Instead of only reducing and tabulating the integrals, they inverted them. That is, from
they studied
, or
, as a function of
. This inversion is what produced elliptic functions.
.
The lemniscate integral
The simplest non-circular example is the lemniscate integral
This should be compared directly with the circular integral , whose inverse is
. By analogy, we define the inverse of the lemniscate integral by
, called the lemniscatic sine. This means that
. If we write
, then the defining relation gives
, and hence, by inverting the derivative,
. Therefore
This is the exact analogue of the ordinary sine calculation. If , then
, so
. Thus ordinary sine is governed by
, while the lemniscatic sine is governed by
. The change from
to
is small in notation but enormous in consequence: it is the first step from trigonometric functions to elliptic functions.
Now define the lemniscatic cosine by . Then the previous equation becomes
, or equivalently
This is not the circular identity , but it plays the same role. It says that the moving point
lies on the algebraic curve
. Differentiating
gives
. Since
, this becomes
, and canceling gives
. Thus the pair
satisfies the differential system
Compare this with ordinary trigonometry: and
. The first derivative relation is formally the same; the second has become nonlinear. That nonlinearity is the analytic signature that we have left the circular world and entered the elliptic one.
The lemniscate addition formula
Now comes the real test: does this new sine have an addition formula? For ordinary trigonometry, the inverse of satisfies
For the lemniscatic sine, write
Then and
. The addition formula is
The numerator looks exactly like the sine addition formula; the denominator
is the new elliptic correction. It is the new feature obtained after replacing the circular equation
by the quartic equation
.
To verify the formula, define We want to prove that
. First check the initial value. When
, we have
and
, so
Thus
has the correct starting value:
.
Now differentiate with respect to
, keeping
fixed. We use
Let
Then
, and
We need Substituting
gives an expression in
. Then using only
one simplifies it to
Thus satisfies the same differential equation as
, namely
, and it also has the same value at
. Therefore
So the lemniscatic addition law is
In integral form, the same statement says the following. Let
then
Algebraic Curve
The differential equation can be rewritten by setting
. Then
So the inverse lemniscate function naturally moves on the algebraic curve
Indeed, if and
, then the point
satisfies
. The integral being inverted is
which, on the curve
, is simply
Thus is the special parameter measured by the differential
. It is not ordinary Euclidean arc length along the curve
. Rather, it is the parameter for which motion along the curve satisfies
This is exactly analogous to the circle. On the unit circle, if
and
, then
and
. In that special case,
is also the ordinary angle and arc length. But that coincidence is special to the unit circle.
Thus is the parameter measured by the differential
. It is the analogue of angle, not because it is literally Euclidean angle or ordinary arc length, but because it is the coordinate in which addition becomes simple. For the unit circle this
is both the angle and the arc length. But that is a special accident of the circle. In the lemniscatic case,
is not ordinary length along the curve
; it is the algebraic angle obtained by integrating
.
Now the addition formula has a precise meaning. If then adding the hidden parameters gives the new point
The formula
is the rule for recovering the visible
-coordinate of
from the visible coordinates of
and
. So the addition is not happening directly in the coordinate
; it is happening in the hidden angle coordinate
, and the displayed formula translates that simple addition back into algebraic coordinates.
Thus the integral is not merely a way of measuring something. It is the coordinate in which the elliptic addition law becomes ordinary addition. This is why
deserves to be called a generalized angle.
Cubics and the line construction
The quartic model is good for integrals. But the group law is more visibly geometric in the cubic model
Take a line Its intersections with
are obtained by substituting into the cubic:
Equivalently, define This is a cubic equation in
, so it has three roots
The corresponding points are
The central analytic fact is that, as the line moves,
Let us prove this, because it is the computational heart of the subject.
Here is the computation. Since , differentiating with respect to the moving line parameters
gives
But
Therefore and hence
Summing over gives
Now so
For any cubic with roots , the identities
hold. They are just the Lagrange interpolation identities saying that a polynomial of degree at most one has no
term when expanded in the basis
. Hence both sums vanish, and we obtain
Integrating this infinitesimal identity gives Thus, if three points
are collinear on a cubic, their elliptic parameters add to zero. This is the analytic content behind the chord law. Modernly one writes
but historically the key fact was the integral identity: a line relation among points produces a linear relation among the integrals
.
Why this is really addition?
The word addition can feel mysterious here. Why should points on a curve be addable? The answer is that the point is merely the visible representative of a hidden parameter. For the circle, the hidden parameter is the angle . A point is
The group law is
For an elliptic curve, the hidden parameter is The group law is designed so that
The line construction is not arbitrary. It is the algebraic machine that computes addition of these hidden parameters without explicitly calculating the integrals. This is the central idea.
Periods
The integral does not behave like an ordinary single-valued function once complex paths are allowed. Different paths can give values differing by constants called periods.
For the circle, one loop gives the period For elliptic functions, there are two independent periods.
For the lemniscate, define Then, along the real direction, the inverse function passes through
as
moves through
So
is a real period.
But the same integral also has a vertical symmetry. If , then
Thus
So there is also an imaginary period, essentially
Thus the inverse function repeats in two directions. This is the analytic origin of double periodicity of the ellitpic function like ..
Higher Degree Curves
Now consider a general algebraic integral
For of degree
or
, one integral is enough. There is essentially one basic integral,
and one point of the curve carries one hidden parameter. This is why elliptic addition is a law on single points.This is the elliptic case.
But if has degree
or
, something new happens.Let
with
or
. One hidden parameter is no longer enough. The natural integral are the integral of the Abelian differentials:
So the basic Abelian quantities (“hidden angles”) are not one number but two: .
This already tells us that a single point cannot be the whole story. A single point gives two numbers
and
, but the correct inversion problem asks for two points
satisfying
Thus in genus two the basic object is not one point but a pair of points. This is the first major break from ordinary elliptic curves.
For a general degree or
ciurve, one needs three points and three integrals:
In general, for
with
one needs
integrals
The number is the genus. It measures how many independent Abelian integrals are needed, and therefore how many points must usually be used in the inversion problem.
Let us see how the addition works concretely in genus two.
Let . with
a polynomial of degree six. This is a genus two curve. Before trying to add arbitrary pairs of points, let us first do the simplest geometric experiment: cut the curve by a line
Substituting this into
gives
Equivalently,
Since has degree six, the line meets the curve in six points, say
Similar computation as above gives
This shows that the hidden angles satisfy
This is the genus two analogue of the elliptic fact that three collinear points on a cubic have elliptic parameters summing to zero. But now, because the curve has genus two, there are two integral coordinates, and
, and because a line meets the degree-six curve in six points, the relation involves six points. This already gives a kind of addition relation. Group the six points into three pairs: Then the two integral relations say that the Abelian coordinates of these three pairs add to a fixed constant.
Thus a line gives a special three-pair relation. This is already the right genus two pattern: the objects being added are not single points, but pairs of points. However, a line does not give the most general addition of two arbitrary pairs. If we start with two arbitrary pairs a line is too small a family to pass through all four prescribed points. So for the general pair-addition law one uses a larger auxiliary curve, for example
This cubic graph has four coefficients, so it can be chosen to pass through
. Substituting into
gives
This is again a degree-six equation. Four intersections are the prescribed points, and two new intersections remain which give the pair satisfying the addition law
So to add arbitrary pairs, one uses a higher auxiliary curve chosen to contain the desired known points and lets the remaining intersections produce the sum.
Singularities
The degree of is not enough. What matters is whether the roots of
are distinct. For a smooth curve
with
or
, one normally gets
independent integrals:
So degree or
gives one integral; degree
or
gives two; degree
or
gives three, and so on. But if two roots collide, the integral becomes simpler. Let
, then writing
gives
, and the basic differential becomes
. Near
, if
, this behaves like
, whose integral is
. Thus when two roots collide, one Abelian direction degenerates into a logarithmic direction: a genus two integral may partly collapse to an elliptic integral plus a logarithm, a genus three integral may collapse toward genus two plus logarithmic pieces, and so on.
In the simplest case , one gets
, so
. Thus distinct roots give genuinely elliptic or Abelian integrals, while repeated roots make part of the theory degenerate into logarithms, exponentials, hyperbolic functions, or rational functions.
Modern Language
Modern language packages the old calculation by saying that a function on a curve has a divisor: its zeros counted positively and its poles counted negatively. Thus, if a line meets a cubic elliptic curve at
, then as a function on the curve it vanishes at those three points and has a triple pole at the point at infinity
. So one writes
. In older language, this simply says: the algebraic function
has zeros at
and its compensating pole at infinity.
Abel’s theorem says that such a zero-pole relation forces the corresponding Abelian integral sum to vanish, up to periods. In genus one, with , the divisor relation above gives
. Since
, we get
. This is exactly the analytic content behind the geometric statement that three collinear points on a cubic add to zero. A modern reader says “the divisor of a function is zero in the Jacobian”; the older computational statement is “the zeros and poles of an algebraic function give an identity among Abelian integrals.
The reason divisors are tied to integrals can be seen from the logarithm of a function. Let be an algebraic function on the curve, and suppose
has a zero of order
at a point
. Choose a local coordinate
near
, with
. Then locally
, where
, so
. When one goes once around
,
changes by
, and therefore
changes by
. At a pole of order
, the same calculation gives a jump of
. Thus the jumps of
remember exactly the divisor of
: zeros contribute positively, poles negatively. Now multiply by an Abelian differential
, such as
, and integrate
around a cut-up version of the curve. Across a cut ending at
, the two values of
differ by
, so that cut contributes
. Summing over all zeros and poles gives
which is precisely the Abel sum of the divisor . Since
is a globally defined function, these logarithmic jumps must balance, except for possible period contributions coming from loops on the curve. Hence
This is the analytic bridge: zeros and poles give a divisor, the logarithm detects that divisor by its jumps, and integrating those jumps against gives the corresponding Abelian integral relation.
Abel’s theorem tells us what happens to sums of Abelian integrals when the points satisfy an algebraic relation. Jacobi inversion asks the opposite question: if the integral sums are given, can we recover the points? In genus one this means: given , recover the point
. Writing the coordinates of
as functions of
gives elliptic functions. This is exactly the same pattern as ordinary trigonometry: given
, recover
.
In genus two the inversion problem already becomes genuinely different. Given two numbers , one must recover two points
from
The solutions then become functions of the two variables
; these are Abelian functions. In genus
, the same pattern uses
points and
integrals. Modern language says that the variables
live on the Jacobian, modulo periods. But historically the question was more concrete: can we invert these multi-integral systems and express the algebraic coordinates of the points as functions of the new generalized angle variables?
Conclusion
The historical progression can be summarized in one line: trigonometry begins with the circle, elliptic functions begin with elliptic integrals, and Abelian functions begin when several such integrals must be inverted at once. For the circle, the integral is inverted by
. For elliptic integrals, one meets radicals such as
, and the inverse functions become elliptic functions. Their addition formulae generalize the ordinary sine and cosine addition formulae. The deeper reason is that algebraic relations among points on a curve force linear relations among the corresponding integrals.
Abel’s great step was to see that this is not limited to elliptic integrals. For higher-degree equations , one needs several integrals, such as
, and several moving points. Thus higher genus means several generalized angle variables. Jacobi inversion then asks how to recover the points from those variables. Modern language says that these variables live on a Jacobian, and that divisors package the zero-pole relations of algebraic functions. But historically the essential phenomenon was simpler and more concrete:
This is the heart of Abel’s theorem. The algebraic curve is not decoration; it is the machine that organizes the upper limits of integration and makes addition formulae possible. Ordinary trigonometric functions are the natural trigonometry of the circle. Elliptic functions are the natural trigonometry of cubic and quartic curves. Abelian functions are the natural trigonometry of higher-genus curves.