We present a derivation of a definite integral discovered by Ramanujan
(1887–1920) in his 1915 paper "Some Definite Integrals," from formulas and ideas
already developed by Euler (1707–1783). Additionally, it is argued why Euler did
not discover Ramanujan's integral himself, although he had all tools required
for this task at his disposal.
In physics and astronomy, Euler's three-body problem is to solve for the motion
of a body that is acted upon by the gravitational field of two other bodies.
This problem is named after Leonhard Euler (1707-1783), who discussed it in
memoirs published in the 1760s. In these publications, Euler found that the
parameter that controls the relative distances among three collinear bodies is
given by a quintic equation. Later on, in 1772, Lagrange dealt with the same
problem, and demonstrated that for any three masses with circular orbits, there
are two special constant-pattern solutions, one where the three bodies remain
collinear, and the other where the bodies occupy the vertices of two equilateral
triangles. Because of their importance, these five points became known as
Lagrange points. The quintic equation found by Euler for the relative distances
among the collinear bodies was also found later by Lagrange, and because of
that, Euler has also been given credit for the discovery of the three collinear
Lagrange points. A practical application of the collinear points for satellite
location is also presented.
In this note, we offer a historical perspective on solutions of the Basel
problem. In particular, we have a closer look at some of the less famous results
by Euler E41 and provide a review of a selection of the assemblage of earlier
proofs. Moreover, we show how to generate further proofs using
Karhunen-Lo\`{e}ve expansions of stochastic processes.
The history of the elastica is examined through the works of various
contributors, including those of Jacob and Daniel Bernoulli, since its first
appearance in a 1690 contest on finding the profile of a hanging flexible cord.
Emphasis will be given to Leonhard Euler’s variational approach to the elastica,
laid out in his landmark 1744 book on variational techniques. Euler’s
variational approach based on the concept of differential value is highlighted,
including the derivation of the general equation for the elastica from the
differential value of the first kind, from which nine shapes adopted by a flexed
lamina under different end conditions are obtained. To show the potential of
Euler’s variational method, the development of the unequal curvature of elastic
bands based on the differential value of the second kind is also examined. We
also revisited some of Euler’s examples of application, including the derivation
of the Euler-Bernoulli equation for the bending of a beam from the Euler-Poisson
equation, the pillar critical load before buckling, and the vibration of elastic
laminas, including the derivation of the equations for the mode shapes and the
corresponding natural frequencies. Finally, the pervasiveness of Euler’s
elastica solution found in various studies over the years as given on recent
reviews by third parties is highlighted, which also includes its major role in
the development of the theory of elliptic functions.
Euler derived the differential equations of elastica by the variational method
in 1744, but his original derivation has never been properly interpreted or
explained in terms of modern mathematics. We elaborate Euler's original
derivation of elastica and show that Euler used Noether's theorem concerning the
translational symmetry of elastica, although Noether published her theorem in
1918. It is also shown that his equation is essentially the static modified KdV
equation which is obtained by the isometric and isoenergy conditions, known as
the Goldstein-Petrich scheme.
We show that an apparently overlooked result of Leonhard Euler (1707-1783) from
[E421] is essentially equivalent to the general multiplication for- mula for the
Γ-function that was proven by Carl Friedrich Gauss (1777-1855) in [Ga28].