Putting x = 1/t, it becomes

d^2y/dt^2 + (2t^-1 - at^-2)dy/dt + bt^-4 y = 0,

which is not regular about t = 0 unless 2 - at^-1 and bt^-2, that is,

unless ax and bx^2 are finite at x =[oo]; which we thus assume; putting

y = t^r(1 + A1t + ... ), we find for the index equation at x =

[inifinity] the equation r(r - 1) + r(2 - ax)_0 + (bx^2)_0 = 0. If

there be finite singular points at [xi]1, ... [xi]m, where we assume

m>1, the cases m = 0, m = 1 being easily dealt with, and if [phi](x) =

(x - [xi]1) ... (x -[xi]m), we must have a.[phi](x) and b.[[phi](x)]^2

finite for all finite values of x, equal say to the respective

polynomials [psi](x) and [theta](x), of which by the conditions at x =

[oo] the highest respective orders possible are m - 1 and 2(m - 1).

The index equation at x = [xi]1 is r(r - 1) +

r[psi]([xi]1)/[phi]'([xi]1) + [theta]([xi])1/[[phi]'([xi]1)]^2 = 0, and

if [alpha]1, [beta]1 be its roots, we have [alpha]1 + [beta]1 = 1 -

[psi]([xi]1)/[phi]'([xi]1) and [alpha]1[beta]1 =

[theta]([xi])1/[[phi]'([xi]1)]^2. Thus by an elementary theorem of

algebra, the sum [Sigma](1 - [alpha]i - [beta]i)/(x - [xi]i), extended

to the m finite singular points, is equal to [psi](x)/[phi](x), and

the sum [Sigma](1 - [alpha]i - [beta]i) is equal to the ratio of the

coefficients of the highest powers of x in [psi](x) and [phi](x), and

therefore equal to 1 + [alpha] + [beta], where [alpha], [beta] are the

indices at x = [oo]. Further, if (x, 1)m-2 denote the integral part of

the quotient [theta](x)/[phi](x), we have

[Sigma][alpha]_i[beta]_i[phi]'([xi]_i)/(x - [xi]_i) equal to -(x,

1)_m-2 + [theta](x)/[phi](x), and the coefficient of x^m-2 in (x,

1)_m-2 is [alpha][beta]. Thus the differential equation has the form

y" + y'[Sigma](1 - [alpha]_i - [beta]_i)/(x - [xi]_i) + y[(x, 1)_m-2 +

[Sigma][alpha]_i[beta]_i[phi]'([xi]_i)/(x - [xi]_i)]/[phi](x) = 0.

If, however, we make a change in the dependent variable, putting y =

(x - [xi]1)^[alpha]1 ... (x - [xi]_m)^[alpha] m[eta], it is easy to

see that the equation changes into one having the same singular points

about each of which it is regular, and that the indices at x = [xi]_i

become 0 and [beta]_i - [alpha]_i, which we shall denote by [lambda]i,

for (x -[xi]_i)^[alpha]j can be developed in positive integral powers

of x -[xi]_i about x = [xi]_i; by this transformation the indices at x

= [oo] are changed to

[alpha] + [alpha]1 + ... + [alpha]m, [beta] + [beta]1 + ... + [beta]m

which we shall denote by [lambda], [mu]. If we suppose this change to

have been introduced, and still denote the independent variable by y,

the equation has the form

y" + y'[Sigma](1 - [lambda]_i)/(x - [xi]_i) + y(x, 1)_m-2/[phi](x) = 0,

while [lambda] + [mu] + [lambda]1 + ... + [lambda]_m = m - 1.

Conversely, it is easy to verify that if [lambda][mu] be the

coefficient of x^m-2 in (x, 1)_m-2, this equation has the specified

singular points and indices whatever be the other coefficients in (x,

1)_m-2.

Hypergeometric equation.

Thus we see that (beside the cases m = 0, m = 1) the "Fuchsian

equation" of the second order with _two_ finite singular points is

distinguished by the fact that it has a definite form when the

singular points and the indices are assigned. In that case, putting (x

- [xi]1)/(x - [xi]2) = t/(t - 1), the singular points are transformed

to 0, 1, [oo], and, as is clear, without change of indices. Still

denoting the independent variable by x, the equation then has the form

x(1 - x)y" + y'[1 - [lambda]1 - x(1 + [lambda] + [mu])] - [lambda][mu]y = 0,

which is the ordinary hypergeometric equation. Provided none of

[lambda]1, [lambda]2, [lambda] - [mu] be zero or integral about x = 0,

it has the solutions

F([lambda], [mu], 1 - [lambda]1, x), x^[lambda]1 F([lambda] + [lambda]1, [mu] + [lambda]1, 1 + [lambda]1, x);

about x = 1 it has the solutions

F([lambda], [mu], 1 - [lambda]2, 1 - x), (1 - x)^[lambda]1 F([lambda] + [lambda]2, [mu] + [lambda]2, 1 + [lambda]2, 1 - x),

where [lambda] + [mu] + [lambda]1 + [lambda]2 = 1; about x = [oo] it

has the solutions

x^-[lambda] F([lambda], [lambda] + [lambda]1, [lambda] - [mu] + 1, x^-1),

x^-[mu] F([mu], [mu] + [lambda]1, [mu] - [lambda] + 1, x^-1),

where F([alpha], [beta], [gamma], x) is the series

[alpha][beta]x [alpha]([alpha] + 1)[beta]([beta] + 1)x^2

1 + -------------- + ----------------------------------------- ...,

[gamma] 1.2.[gamma]([gamma] + 1)

which converges when |x| < 1, whatever [alpha], [beta], [gamma] may

be, converges for all values of x for which |x| = 1 provided the real

part of [gamma] - [alpha] - [beta] < 0 algebraically, and converges

for all these values except x = 1 provided the real part of [gamma] -

[alpha] -[beta] > -1 algebraically.

In accordance with our general theory, logarithms are to be expected

in the solution when one of [lambda]1, [lambda]2, [lambda] - [mu] is

zero or integral. Indeed when [lambda]1 is a negative integer, not

zero, the second solution about x = 0 would contain vanishing factors

in the denominators of its coefficients; in case [lambda] or [mu] be

one of the positive integers 1, 2, ... (-[lambda]1), vanishing factors

occur also in the numerators; and then, in fact, the second solution

about x = 0 becomes x^[lambda]1 times an integral polynomial of degree

(-[lambda]1) - [lambda] or of degree (-[lambda]1) - [mu]. But when

[lambda]1 is a negative integer including zero, and neither [lambda]

nor [mu] is one of the positive integers 1, 2 ... (-[lambda]1), the

second solution about x = 0 involves a term having the factor log x.

When [lambda]1 is a positive integer, not zero, the second solution

about x = 0 persists as a solution, in accordance with the order of

arrangement of the roots of the index equation in our theory; the

first solution is then replaced by an integral polynomial of degree

-[lambda] or -[mu]1, when [lambda] or [mu] is one of the negative

integers 0, -1, -2, ..., 1 - [lambda]1, but otherwise contains a

logarithm. Similarly for the solutions about x = 1 or x = [oo]; it

will be seen below how the results are deducible from those for x = 0.

March of the Integral.

Denote now the solutions about x = 0 by u1, u2; those about x = 1 by

v1, v2; and those about x = [oo] by w1, w2; in the region (S0S1)

common to the circles S0, S1 of radius 1 whose centres are the points

x = 0, x = 1, all the first four are valid, and there exist equations

u1 =Av1 + Bv2, u2 = Cv1 + Dv2 where A, B, C, D are constants; in the

region (S1S) lying inside the circle S1 and outside the circle S0,

those that are valid are v1, v2, w1, w2, and there exist equations v1

= Pw1 + Qw2, v2 = Rw1 + Tw2, where P, Q, R, T are constants; thus

considering any integral whose expression within the circle S0 is au1

+ bu2, where a, b are constants, the same integral will be represented

within the circle S1 by (aA + bC)v1 + (aB + bD)v2, and outside these

circles will be represented by

[(aA + bC)P + (aB + bD)R]w1 + [(aA + bC)Q + (aB + bD)T]w2.

A single-valued branch of such integral can be obtained by making a

barrier in the plane joining [oo] to 0 and 1 to [oo]; for instance, by

excluding the consideration of real negative values of x and of real

positive values greater than 1, and defining the phase of x and x - 1

for real values between 0 and 1 as respectively 0 and [pi].

Transformation of the equation into itself.

We can form the Fuchsian equation of the second order with three

arbitrary singular points [xi]1, [xi]2, [xi]3, and no singular point

at x = [oo], and with respective indices [alpha]1, [beta]1, [alpha]2,

[beta]2, [alpha]3, [beta]3 such that [alpha]1 + [beta]1 + [alpha]2 +

[beta]2 + [alpha]3 + [beta]3 = 1. This equation can then be

transformed into the hypergeometric equation in 24 ways; for out of

[xi]1, [xi]2, [xi]3 we can in six ways choose two, say [xi]1, [xi]2,

which are to be transformed respectively into 0 and 1, by (x -

[xi]1)/(x - [xi]2) = t(t - 1); and then there are four possible

transformations of the dependent variable which will reduce one of the

indices at t = 0 to zero and one of the indices at t = 1 also to zero,

namely, we may reduce either [alpha]1 or [beta]1 at t = 0, and

simultaneously either [alpha]2 or [beta]2 at t = 1. Thus the

hypergeometric equation itself can be transformed into itself in 24

ways, and from the expression F([lambda], [mu], 1 - [lambda]1, x)

which satisfies it follow 23 other forms of solution; they involve

four series in each of the arguments, x, x-1, 1/x, 1/(1-x), (x-1)/x,

x/(x-1). Five of the 23 solutions agree with the fundamental solutions

already described about x = 0, x = 1, x = [oo]; and from the

principles by which these were obtained it is immediately clear that

the 24 forms are, in value, equal in fours.

Inversion. Modular functions.

The quarter periods K, K' of Jacobi's theory of elliptic functions, of

which K = [int] [0 to [pi]/2] (1 - h sin^2[theta])^-1/2 d[theta], and K'

is the same function of 1-h, can easily be proved to be the solutions

of a hypergeometric equation of which h is the independent variable.

When K, K' are regarded as defined in terms of h by the differential

equation, the ratio K'/K is an infinitely many valued function of h.

But it is remarkable that Jacobi's own theory of theta functions leads

to an expression for h in terms of K'/K (see FUNCTION) in terms of

single-valued functions. We may then attempt to investigate, in

general, in what cases the independent variable x of a hypergeometric

equation is a single-valued function of the ratio s of two independent

integrals of the equation. The same inquiry is suggested by the

problem of ascertaining in what cases the hypergeometric series

F([alpha], [beta], [gamma], x) is the expansion of an algebraic

(irrational) function of x. In order to explain the meaning of the

question, suppose that the plane of x is divided along the real axis

from -[oo] to 0 and from 1 to +[oo], and, supposing logarithms not to

enter about x = 0, choose two quite definite integrals y1, y2 of the

equation, say

y1 = F([lambda], [mu], 1-[lambda]1, x),

y2 = x^[lambda]1 F([lambda] + [lambda]1, [mu] + [lambda]1, 1 + [lambda]1, x),

with the condition that the phase of x is zero when x is real and

between 0 and 1. Then the value of [sigma] = y2/y1 is definite for all

values of x in the divided plane, [sigma] being a single-valued

monogenic branch of an analytical function existing and without

singularities all over this region. If, now, the values of [sigma]

that so arise be plotted on to another plane, a value p + iq of

[sigma] being represented by a point (p, q) of this [stigma]-plane, and

the value of x from which it arose being mentally associated with this

point of the [sigma]-plane, these points will fill a connected region

therein, with a continuous boundary formed of four portions

corresponding to the two sides of the two barriers of the x-plane. The

question is then, firstly, whether the same value of s can arise for

two different values of x, that is, whether the same point (p, q) of

the [sigma]-plane can arise twice, or in other words, whether the

region of the [sigma]-plane overlaps itself or not. Supposing this is

not so, a second part of the question presents itself. If in the

x-plane the barrier joining -[oo] to 0 be momentarily removed, and x

describe a small circle with centre at x = 0 starting from a point x =

-h - ik, where h, k are small, real, and positive and coming back to

this point, the original value s at this point will be changed to a

value [sigma], which in the original case did not arise for this value

of x, and possibly not at all. If, now, after restoring the barrier

the values arising by continuation from [sigma] be similarly plotted

on the s-plane, we shall again obtain a region which, while not

overlapping itself, may quite possibly overlap the former region. In

that case two values of x would arise for the same value or values of

the quotient y2/y1, arising from two different branches of this

quotient. We shall understand then, by the condition that x is to be a

single-valued function of x, that the region in the [stimga]-plane

corresponding to any branch is not to overlap itself, and that no two

of the regions corresponding to the different branches are to overlap.

Now in describing the circle about x = 0 from x = -h - ik to -h + ik,

where h is small and k evanescent,

[stigma] = x^[lambda]1 F([lambda] + [lambda]1, [mu] + [lambda]1, 1 + [lambda]1, x)/F([lambda], [mu], 1 - [lambda]1, x)

is changed to [sigma] = [stigma]e^(2[pi]i[lambda])1. Thus the two

portions of boundary of the s-region corresponding to the two sides of

the barrier (-[oo], 0) meet (at [sigmaf] = 0 if the real part of

[lambda]1 be positive) at an angle 2[pi]L1, where L1 is the absolute

value of the real part of [lambda]1; the same is true for the

[sigma]-region representing the branch [sigma]. The condition that the

s-region shall not overlap itself requires, then, L1 = 1. But,

further, we may form an infinite number of branches [sigma] =

[stigma]e^(2[pi]i[lambda])1, [sigma]1 = e^(2[pi]i[lambda])1, ... in

the same way, and the corresponding regions in the plane upon which

y2/y1 is represented will have a common point and each have an angle

2[pi]L1; if neither overlaps the preceding, it will happen, if L1 is

not zero, that at length one is reached overlapping the first, unless

for some positive integer [alpha] we have 2[pi][alpha]L1 = 2[pi], in

other words L1 = 1/a. If this be so, the branch [sigma]_a-1 =

[stigma]e^(2[pi]ia[lambda])1 will be represented by a region having

the angle at the common point common with the region for the branch

[stigma]; but not altogether coinciding with this last region unless

[lambda]1 be real, and therefore = [+-]1/a; then there is only a finite

number, a, of branches obtainable in this way by crossing the barrier

(-[oo], 0). In precisely the same way, if we had begun by taking the

quotient

[stigma]' = (x - 1)^[lambda]2 F([lambda] + [lambda]2, [mu] + [lambda]2, 1 + [lambda]2, 1 - x)/F([lambda], [mu], 1 - [lambda]2, 1 - x)

of the two solutions about x = 1, we should have found that x is not a

single-valued function of [stigma]' unless [lambda]2 is the inverse of

an integer, or is zero; as [stigma]' is of the form (A[stigma] +

B)/(C[stigma] + D), A, B, C, D constants, the same is true in our

case; equally, by considering the integrals about x = [oo] we find, as

a third condition necessary in order that x may be a single-valued

function of [stigma], that [lambda] - [mu] must be the inverse of an

integer or be zero. These three differences of the indices, namely,

[lambda]1, [lambda]2, [lambda] - [mu], are the quantities which enter

in the differential equation satisfied by x as a function of [stigma],

which is easily found to be

x111 3^2x^211

- ---- + -------- = 1/2(h - h1 - h2)x^-1 (x - 1)^-1 + 1/2h1 x^-2 + 1/2h2(x - 1)^-2,

x1^3 2x1^4

where x1 = dx/d[stigma], &c.; and h1 = 1 - y1^2, h2 = 1 - [lambda]2^2,

h3 = 1 - ([lambda] - [mu])^2. Into the converse question whether the

three conditions are sufficient to ensure (1) that the [stigma] region

corresponding to any branch does not overlap itself, (2) that no two

such regions overlap, we have no space to enter. The second question

clearly requires the inquiry whether the group (that is, the monodromy

group) of the differential equation is properly discontinuous. (See

GROUPS, THEORY OF.)

The foregoing account will give an idea of the nature of the function

theories of differential equations; it appears essential not to exclude

some explanation of a theory intimately related both to such theories

and to transformation theories, which is a generalization of Galois's

theory of algebraic equations. We deal only with the application to

homogeneous linear differential equations.

Rationality group of a linear equation.

Irreducibility of a rational equation.

In general a function of variables x1, x2 ... is said to be rational

when it can be formed from them and the integers 1, 2, 3, ... by a

finite number of additions, subtractions, multiplications and

divisions. We generalize this definition. Assume that we have assigned

a fundamental series of quantities and functions of x, in which x

itself is included, such that all quantities formed by a finite number

of additions, subtractions, multiplications, divisions _and

differentiations in regard to x_, of the terms of this series, are

themselves members of this series. Then the quantities of this series,

and only these, are called _rational_. By a rational function of

quantities p, q, r, ... is meant a function formed from them and any

of the fundamental rational quantities by a finite number of the five

fundamental operations. Thus it is a function which would be called,

simply, rational if the fundamental series were widened by the

addition to it of the quantities p, q, r, ... and those derivable from

them by the five fundamental operations. A rational ordinary

differential equation, with x as independent and y as dependent

variable, is then one which equates to zero a rational function of y,

the order k of the differential equation being that of the highest

differential coefficient y^(k) which enters; only such equations are

here discussed. Such an equation P = 0 is called _irreducible_ when,

firstly, being arranged as an integral polynomial in y^(k), this

polynomial is not the product of other polynomials in y^(k) also of

rational form; and, secondly, the equation has no solution satisfying

also a rational equation of lower order. From this it follows that if

an irreducible equation P = 0 have one solution satisfying another

rational equation Q = 0 of the same or higher order, then all the

solutions of P = 0 also satisfy Q = 0. For from the equation P = 0 we

can by differentiation express y^(k+1), y^(k+2), ... in terms of x, y,

y^(1), ... , y^(k), and so put the function Q rationally in terms of

these quantities only. It is sufficient, then, to prove the result

when the equation Q = 0 is of the same order as P = 0. Let both the

equations be arranged as integral polynomials in y^(k); their

algebraic eliminant in regard to y^(k) must then vanish identically,

for they are known to have one common solution not satisfying an

equation of lower order; thus the equation P = 0 involves Q = 0 for

all solutions of P = 0.

The variant function for a linear equation.

Now let y^(n) = [alpha]1y^(n-1) + ... + [alpha]_n y be a given

rational homogeneous linear differential equation; let y1, ... yn be n

particular functions of x, unconnected by any equation with constant

coefficients of the form c1y1 + ... + cnyn = 0, all satisfying the

differential equation; let [eta]1, ... [eta]n be linear functions of

y1, ... yn, say [eta]i = A_i1 y1 + ... + A_in yn, where the constant

coefficients Aij have a non-vanishing determinant; write ([eta]) =

A(y), these being the equations of a general linear homogeneous group

whose transformations may be denoted by A, B, .... We desire to form a

rational function [phi]([eta]), or say [phi](A(y)), of [eta]1, ...

[eta], in which the [eta]^2 constants Aij shall all be essential, and

not reduce effectively to a fewer number, as they would, for instance,

if the y1, ... yn were connected by a linear equation with constant

coefficients. Such a function is in fact given, if the solutions y1,

... yn be developable in positive integral powers about x = a, by

[phi]([eta]) = [eta]1 + (x - a)^n[eta]2 + ... + (x - a)^(n-1)n[eta]n.

Such a function, V, we call a _variant_.

The resolvent eqution.

Then differentiating V in regard to x, and replacing [eta]i^(n) by

its value a1[eta]^(n-1) + ... + an[eta], we can arrange dV/dx, and

similarly each of d^2/dx^2 ... d^NV/dx^N, where N = n^2, as a linear

function of the N quantities [eta]1, ... [eta]n, ... [eta]1^(n-1), ...

[eta]n^(n-1), and thence by elimination obtain a linear differential

equation for V of order N with rational coefficients. This we denote

by F = 0. Further, each of [eta]1 ... [eta]n is expressible as a

linear function of V, dV/dx, ... d^(N-1)V/dx^(N-1), with rational

coefficients not involving any of the n^2 coefficients A_ij, since

otherwise V would satisfy a linear equation of order less than N,

which is impossible, as it involves (linearly) the n^2 arbitrary

coefficients Aij, which would not enter into the coefficients of the

supposed equation. In particular, y1 ,.. yn are expressible rationally

as linear functions of [omega], d[omega]/dx, ...

d^(N-1)[omega]/dx^(N-1), where [omega] is the particular function

[phi](y). Any solution W of the equation F = 0 is derivable from

functions [zeta]1, ... [zeta]n, which are linear functions of y1, ...

yn, just as V was derived from [eta]1, ... [eta]n; but it does not

follow that these functions [zeta]i, ... [zeta]n are obtained from y1,

... yn by a transformation of the linear group A, B, ... ; for it may

happen that the determinant d([zeta]1, ... [zeta]n)/(dy1, ... yn) is

zero. In that case [zeta]1, ... [zeta]n may be called a singular set,

and W a singular solution; it satisfies an equation of lower than the

N-th order. But every solution V, W, ordinary or singular, of the

equation F = 0, is expressible rationally in terms of [omega],

d[omega]/dx, ... d^(N-1)[omega]/dx^(N-1); we shall write, simply, V =

r([omega]). Consider now the rational irreducible equation of lowest

order, not necessarily a linear equation, which is satisfied by

[omega]; as y1, ... yn are particular functions, it may quite well be

of order less than N; we call it the _resolvent equation_, suppose it

of order p, and denote it by [gamma](v). Upon it the whole theory

turns. In the first place, as [gamma](v) = 0 is satisfied by the

solution [omega] of F = 0, all the solutions of [gamma](v) are

solutions F = 0, and are therefore rationally expressible by [omega];

any one may then be denoted by r([omega]). If this solution of F = 0

be not singular, it corresponds to a transformation A of the linear

group (A, B, ...), effected upon y1, ... yn. The coefficients Aij of

this transformation follow from the expressions before mentioned for

[eta]1 ... [eta]n in terms of V, dV/dx, d^2V/dx^2, ... by substituting V

= r([omega]); thus they depend on the p arbitrary parameters which

enter into the general expression for the integral of the equation

[gamma](v) = 0. Without going into further details, it is then clear

enough that the resolvent equation, being irreducible and such that

any solution is expressible rationally, with p parameters, in terms of

the solution [omega], enables us to define a linear homogeneous group

of transformations of y1 ... yn depending on p parameters; and every

operation of this (continuous) group corresponds to a rational

transformation of the solution of the resolvent equation. This is the

group called the _rationality group_, or the _group of

transformations_ of the original homogeneous linear differential

equation.

The group must not be confounded with a subgroup of itself, the

_monodromy group_ of the equation, often called simply the group of

the equation, which is a set of transformations, not depending on

arbitrary variable parameters, arising for one particular fundamental

set of solutions of the linear equation (see GROUPS, THEORY OF).

The fundamental theorem in regard to the rationality group.

The importance of the rationality group consists in three

propositions. (1) Any rational function of y1, ... yn which is

unaltered in value by the transformations of the group can be written

in rational form. (2) If any rational function be changed in form,

becoming a rational function of y1, ... yn, a transformation of the

group applied to its new form will leave its value unaltered. (3) Any

homogeneous linear transformation leaving unaltered the value of every

rational function of y1, ... yn which has a rational value, belongs to

the group. It follows from these that any group of linear homogeneous

transformations having the properties (1) (2) is identical with the

group in question. It is clear that with these properties the group

must be of the greatest importance in attempting to discover what

functions of x must be regarded as rational in order that the values

of y1 ... yn may be expressed. And this is the problem of solving the

equation from another point of view.

LITERATURE.--([alpha]) _Formal or Transformation Theories for

Equations of the First Order_:--E. Goursat, _Lecons sur l'integration

des equations aux derivees partielles du premier ordre_ (Paris, 1891);

E. v. Weber, _Vorlesungen uber das Pfaff'sche Problem und die Theorie

der partiellen Differentialgleichungen erster Ordnung_ (Leipzig,

1900); S. Lie und G. Scheffers, _Geometrie der

Beruhrungstransformationen_, Bd. i. (Leipzig, 1896); Forsyth, _Theory

of Differential Equations, Part i., Exact Equations and Pfaff's

Problem_ (Cambridge, 1890); S. Lie, "Allgemeine Untersuchungen uber

Differentialgleichungen, die eine continuirliche endliche Gruppe

gestatten" (Memoir), _Mathem. Annal._xxv. (1885), pp. 71-151; S. Lie

und G. Scheffers, _Vorlesungen uber Differentialgleichungen mit

bekannten infinitesimalen Transformationen_ (Leipzig, 1891). A very

full bibliography is given in the book of E. v. Weber referred to;

those here named are perhaps sufficiently representative of modern

works. Of classical works may be named: Jacobi, _Vorlesungen uber

Dynamik_ (von A. Clebsch, Berlin, 1866); _Werke, Supplementband_; G

Monge, _Application de l'analyse a la geometrie_ (par M. Liouville,

Paris, 1850); J. L. Lagrange, _Lecons sur le calcul des fonctions_

(Paris, 1806), and _Theorie des fonctions analytiques_ (Paris,

Prairial, an V); G. Boole, _A Treatise on Differential Equations_

(London, 1859); and _Supplementary Volume_ (London, 1865); Darboux,

_Lecons sur la theorie generale des surfaces_, tt. i.-iv. (Paris,

1887-1896); S. Lie, _Theorie der transformationsgruppen_ ii. (on

Contact Transformations) (Leipzig, 1890).

([beta]) _Quantitative or Function Theories for Linear Equations_:--C.

Jordan, _Cours d'analyse_, t. iii. (Paris, 1896); E. Picard, _Traite

d'analyse_, tt. ii. and iii. (Paris, 1893, 1896); Fuchs, _Various

Memoirs, beginning with that in Crelle's Journal_, Bd. lxvi. p. 121;

Riemann, _Werke_, 2^r Aufl. (1892); Schlesinger, _Handbuch der Theorie

der linearen Differentialgleichungen_, Bde. i.-ii. (Leipzig,

1895-1898); Heffter, _Einleitung in die Theorie der linearen

Differentialgleichungen mit einer unabhangigen Variablen_ (Leipzig,

1894); Klein, _Vorlesungen uber lineare Differentialgleichungen der

zweiten Ordnung_ (Autographed, Gottingen, 1894); and _Vorlesungen uber

die hypergeometrische Function_ (Autographed, Gottingen, 1894);

Forsyth, _Theory of Differential Equations, Linear Equations_.

([gamma]) _Rationality Group (of Linear Differential

Equations)_:--Picard, _Traite d'Analyse_, as above, t. iii.; Vessiot,

_Annales de l'Ecole Normale_, serie III. t. ix. p. 199 (Memoir); S.

Lie, _Transformationsgruppen_, as above, iii. A connected account is

given in Schlesinger, as above, Bd. ii., erstes Theil.

([delta]) _Function Theories of Non-Linear Ordinary

Equations_:--Painleve, _Lecons sur la theorie analytique des equations

differentielles_ (Paris, 1897, Autographed); Forsyth, _Theory of

Differential Equations, Part ii., Ordinary Equations not Linear_ (two

volumes, ii. and iii.) (Cambridge, 1900); Konigsberger, _Lehrbuch der

Theorie der Differentialgleichungen_ (Leipzig, 1889); Painleve,

_Lecons sur l'integration des equations differentielles de la

mecanique et applications_ (Paris, 1895).

([epsilon]) _Formal Theories of Partial Equations of the Second and

Higher Orders_:--E. Goursat, _Lecons sur l'integration des equations

aux derivees partielles du second ordre_, tt. i. and ii. (Paris, 1896,

1898); Forsyth, _Treatise on Differential Equations_ (London, 1889);

and _Phil. Trans. Roy. Soc._ (A.), vol. cxci. (1898), pp. 1-86.

([zeta]) See also the six extensive articles in the second volume of

the German _Encyclopaedia of Mathematics_. (H. F. BA.)

DIFFLUGIA (L. Leclerc), a genus of lobose Rhizopoda, characterized by a

shell formed of sand granules cemented together; these are swallowed by

the animal, and during the process of bud-fission they pass to the

surface of the daughter-bud and are cemented there. _Centropyxis_

(Steia) and _Lecqueureuxia_ (Schlumberg) differ only in minor points.

DIFFRACTION OF LIGHT.--1. When light proceeding from a small source

falls upon an opaque object, a shadow is cast upon a screen situated

behind the obstacle, and this shadow is found to be bordered by

alternations of brightness and darkness, known as "diffraction bands."

The phenomena thus presented were described by Grimaldi and by Newton.

Subsequently T. Young showed that in their formation interference plays

an important part, but the complete explanation was reserved for A. J.

Fresnel. Later investigations by Fraunhofer, Airy and others have

greatly widened the field, and under the head of "diffraction" are now

usually treated all the effects dependent upon the limitation of a beam

of light, as well as those which arise from irregularities of any kind

at surfaces through which it is transmitted, or at which it is

reflected.

2. _Shadows._--In the infancy of the undulatory theory the objection

most frequently urged against it was the difficulty of explaining the

very existence of shadows. Thanks to Fresnel and his followers, this

department of optics is now precisely the one in which the theory has

gained its greatest triumphs. The principle employed in these

investigations is due to C. Huygens, and may be thus formulated. If

round the origin of waves an ideal closed surface be drawn, the whole

action of the waves in the region beyond may be regarded as due to the

motion continually propagated across the various elements of this

surface. The wave motion due to any element of the surface is called a

_secondary_ wave, and in estimating the total effect regard must be paid

to the phases as well as the amplitudes of the components. It is usually

convenient to choose as the surface of resolution a _wave-front_, i.e. a

surface at which the primary vibrations are in one phase. Any obscurity

that may hang over Huygens's principle is due mainly to the

indefiniteness of thought and expression which we must be content to put

up with if we wish to avoid pledging ourselves as to the character of

the vibrations. In the application to sound, where we know what we are

dealing with, the matter is simple enough in principle, although

mathematical difficulties would often stand in the way of the

calculations we might wish to make. The ideal surface of resolution may

be there regarded as a flexible lamina; and we know that, if by forces

locally applied every element of the lamina be made to move normally to

itself exactly as the air at that place does, the external aerial motion

is fully determined. By the principle of superposition the whole effect

may be found by integration of the partial effects due to each element

of the surface, the other elements remaining at rest.

We will now consider in detail the important case in which uniform

plane waves are resolved at a surface coincident with a wave-front

(OQ). We imagine a wave-front divided into elementary rings or

zones--often named after Huygens, but better after Fresnel--by spheres

described round P (the point at which the aggregate effect is to be

estimated), the first sphere, touching the plane at O, with a radius

equal to PO, and the succeeding spheres with radii increasing at each

step by 1/2[lambda]. There are thus marked out a series of circles,

whose radii x are given by x^2 + r^2 = (r + 1/2n[lambda])^2, or x^2 =

n[lambda]r nearly; so that the rings are at first of nearly equal

area. Now the effect upon P of each element of the plane is

proportional to its area; but it depends also upon the distance from

P, and possibly upon the inclination of the secondary ray to the

direction of vibration and to the wave-front.

O x Q

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