CHAPTER IV
1. F = 0 for y > 0.
2. Use the relation
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3. Integrate uxx by parts twice (special precautions necessary in the case where p < 5/2).
4. Integrate J0' by parts.
1. p/24
2. 0.
3. 0.
4. p/8 if the region of integration is restricted by the condition z > 0; otherwise 0.
5. 1/50 400.
6. p[2 - (3/2)log 3].
7. Introduce polar co-ordinates and integrate first with respect to j and q: p[2 + (3/2)log 3].
8. ![]()
9. Subdivide the interval of integration into the segments
![]()
and find the limits of the integrals along each segment.
1. Apply the substitution ![]()
2. Introduce polar co-ordinates: ![]()
3. Substitute ![]()
7. Introduce new rectangular co-ordinates (x', h',
z ') such that
Then
(Exercise 9) and
![]()
throughout the sphere
. Hence, if we perform the integrations
with respect to h' and z',
![]()
Answer: ![]()
8. Substitute
and integrate with
respect to -h'.
1. Apply Guldin's role, using the fact that the centre of an ellipse is also its centre of mass: 2p²ab.
2. mabh²/2
3. Substitute x = ax,, y = bh, z = cz:
![]()
4. (a) Compare
corresponding elements of area.
![]()
![]()
5.
where 2a is
the major axis.
6. Volume = ½pcp², surface area = p(a + b)p, where a, b, c are the sides of the triangle and p is the perpendicular from C to AB.
7. From the differential equation, satisfied by the tube-surface u = u(x, y), we have
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If we introduce as parameters the length of arc a on L and the distance t along the normal to L, then (cf. Volume I and Volume 2 )
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where k denotes the curvature of L.
8. Integrate first with respect to x and y: (a) 16r³/9; (b) 8r².
9. ![]()
10. Introduce polar co-ordinates-: p²/2.
1. On the axis of the cone, two-thirds of the way from the vertex to the centre of the base.
2. x = 2x0/3, y = z = 0
3. Cf. tube surface Exercise 1
4. ![]()
5. For example,
, which is
positive.
6. Substitute x= ax , y = bh, z = cz; use the expressions for the moments of inertia given in the text and the properties of symmetry of the ellipsoid:
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7. The distance of the point (x, y, z) from the plane ux + vy + wz = -1 is given by
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The moment of inertia of the ellipsoid with respect to this plane is therefore given by
![]()
where A, B, C denote the moments of inertia with respect to the co-ordinate planes and V is the volume of the ellipsoid, i.e.,
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We must now find the envelope of the planes for which this expression is equal to h. The envelope is given by the equations
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where l denotes a common multiplier, which from the expression for the moment of inertia and the equation of the plane is found to be V. By squaring the three equations we obtain the equation of the envelope, namely,
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9. ![]()
10. (1/3, 0, 0).
11. ![]()
13.
14. Integrate first with respect to x and y:
![]()
where the upper or lower sign is to be taken according to whether the origin is inside the body or not.
1. S consists of unit circles orthogonal to C and with their centres on C.
1. Substitute 
2. By A4.3.2
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taken throughout the interior of the (n - l)-dimensional unit sphere in the x2, ··· , xn-space.. Introducing polar co-ordinates, we obtain

where S(r) denotes the sphere of radius r and Centre O in x2, ··· , xn-space. As the integrand depends on r only,
![]()
Setting
we have
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1. Set
then In(a)=
-I"n-1(a), where
dashes denote differentiation with respect to a.
Alternatively, integrate by parts,![]()
2. Substitute x = ax + by, h = gx + dy, where a, b, g, d are chosen so that
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Then (ad - bg)² = ac - b² and the integral is transformed into
![]()
3. Make the same substitution as in 2. and evaluate the resulting integrals, (a) using the result of 1. (b) introducing polar co-ordinates.

4. (a) Forming K'(a), where the
dash denotes differentiation with respect to a, and integrating
by parts twice (taking
as one factor), we have K'(a) = -K(a)/2a
+ K(a)/4a², i.e.,
![]()
where C is given by

(b) Integrate the formula
with
respect to t from a to b.
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(c) Substituting x = l/t in the expression for I' (a), prove that I' = -2I, i.e.,
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![]()
(d) Substitute the integral expression for J0 and change the order of integration. Use the formula
cf.. the expression
for ![]()
p/2 when a > b, arsin a/b when a < b.
6. There exists an e > 0 such that there is every for A an A' > A such that
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1. Substitute ![]()
3. Integrate first with respect to y and x:
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4. ![]()
5. Show that
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then let n ® ¥ and apply Wallis's formula
CHAPTER V
1. ![]()
2. Let
and u1
and v1 be defined by
![]()
Then, u1 and v1 are twice continuously differentiable (and so also at the origin), and (u1)y = (v1)x . Then
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1. (a) Example 3.
(c) Let B be an arbitrary region and v
an arbitrary function vanishing on the boundary of R.
Then, by Green's first formula,

Now,
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and
![]()
Hence,

where
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Applying Gauss' theorem to the vector (U1v, U2v, U3v), we obtain
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Thus, we have for an arbitrary v vanishing on the boundary of R
![]()
and hence by Lemma I

(d) Use Exercise 6

where j(x) = (a x)(b x)(c x).
1.
![]()
where the volume integral is to be extended throughout the upper half of the ellipsoid. (The base of this half of the ellipsoid contributes nothing to the surface integral
![]()
2. Since H is a homogeneous function of the fourth degree, we have

1. The two equations u = fx,
v = fy can be solved for x
and y, since
Let x =s(u,
v), y = t(u,
v); since
uy=vx,
we have xv=yu ,
sv=tu, whence there
exists a function g such that x = gu(u,
v), y = gv(u,
v).
2.
![]()
2. If (x ,h) and (x, y) are rectangular co-ordinates in P and P, respectively, then the motion of the point M(x, y) can be described by the equations
![]()
(i.e., by a rotation and translation). Then,
![]()
(a) If A = np ¹ 0, we have S(M)
= np[(x - x0)²
+ (y - y0)²] + S(C),
where C is the point x=x0= -B/2np, y=y0= -C/2np, whence A, B,
C, D have the values in 1.
(b1) If A =
np = 0, but B²
+ C² > 0, then
![]()
where
and D is the line Bx
+ Cy + D = 0.
(b2) If A =
B = C = 0, we have S(M)
= D = const.
3. .For the motion of the plane P rigidly attached to the connecting-rod AB, we have
Hence D passes through A and, by symmetry, D is perpendicular to AB at A, whence
4. For the motion of the plane P rigidly
attached to the chord AB we have n = 1, S(A)
= S(B) = S = area of G. The point C of Steiner's theorem
is therefore equidistant from A and B and
whence
S(A) - S(M) = area of G - area of ![]()
5. If l is the length of G, Frenet's formulae yield

6. Let n' == (a, b, g), x = (x, y, z). If we substitute in Gauss' formula
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a = 1, b = c = 0, and a = 0, b = -z, c = y, we get
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7. Take orthogonal co-ordinates (x, y, z) such that x = 0 is the free horizontal surface of the fluid and Oz points downwards. The pressure on ds is nzds, wherez is the depth of ds. By repeated applications of Gauss' formula in three dimensions, with obvious choices of the functions a, b, c, we find for the components of the resultant of the fluid pressure
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We find for the components of the resultant moment with respect to the origin O, by Gauss' formula,

Now we note that the components of the force f are 0,0, -V and the components of its moment with respect to O , are Vy0, Vx0, 0.
8. We readily obtain from the parametric equations
![]()
of the ellipsoid the formulae
![]()
where
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10. The integral represents the flat solid angle which the plane z = 0 subtends at the point M = (0, 0, 1). For a direct analytical proof, use plane polar co-ordinates.
12. Verify the identity
![]()
for all points (x, y, z) different from (a,
b, c). We conclude from Gauss' formula in three
dimensions
(i) that W = 0, if S
is a closed surface such that A = (a, b, c)
is outside the volume bounded by S; (
ii) that if A is within S, the
value of the integral is independent of the shape of S. Taking for S a
sphere with centre A, we easily see that W = 4p.
13. The integral
![]()
is independent of S and depends only on its boundary G, because the identity given in the answer to 12. implies that
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3. ![]()
![]()
and the variables are separated.
4. ![]()
5. 
6. Introduce l/y as new unknown function; the equation then becomes homogeneous:

1. Use induction. Suppose that there holds a
linear relation
. Divide by
and differentiate (nk+1)
times, if Pk(x) is of degree nk.
The degree of the coefficients of the other
is
unchanged, so that they remain different from zero.
2. Multiply both sides of the equation by (1 - n)y -n.

3. If we set y = y1 +
u-1, the equation reduces to the linear
equation

4. By equating the right-hand sides of (a) and (b), we obtain the common integral y = x².
5. 
In order to draw the graphs of the corresponding family of curves, first plot the two branches of the curve
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which divides the plane into two regions where y' < 0 and one region where y' > 0. The two infinite branches of this curve are asymptotic to the two parabolas y = ± x². Show that all the integral curves are asymptotic to these parabolas by proving the two relations

where o(1) denotes a function which tends to zero.
6. Set
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Then
![]()
so that

Similarly,
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Hence,
![]()
and similarly, by subtraction,
![]()
7. Cf. the relation
![]()
in the proof of 6.
Particular solutions of the special equation are
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8. The common solution ex of (a) and (b) is obtained by eliminating y" from the two equations
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. 6.4
1. It follows from the fundamental theorem of algebra it follows that f(z) may be written as
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where the mn are positive integers such that
![]()
Now,
![]()
On differentiating this relation (mn - 1) times and setting l = an in the result, we get by. Leibnitz's rule

So we have n particular solutions

which are linearly independent, by 1. of Exercises 6.3.
2. 
3. On substituting in the differential equation, we get
![]()
an identity if a0b0 = 1, a0b1 + a1b0 = 0, ··· , from the expansion.The second case reduces to the first if we substitute y' for y.
4. 
5. ![]()
6. y = ex(x²/2 + 3x/2 + 7/4) + c1e3x + c2e2x.
1. (a) Use the fact that the curvilinear integral
![]()
is independent of the path. Integrating between (0, 0) and (x, y) along the broken line (0, 0) ··· (x, 0) ··· (x, y), we get
![]()
(b) By inspection, we find the general integral
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2. Here dy/dx is a function of y/x alone.
3. x² y 2xy² 2cy 2 = 0 (integrating factor m = 1/y²)
4. The equation is linear in x and its general integral is (xy² +1)² = cy. The identity
![]()
displays an integrating factor of the equation.
5. ![]()
(c) The differential equation of this family of confocal conics is found to
be
![]()
which is unaltered if y' is replaced by -l/y';
the family of ellipses (-b²<c<¥ ) is orthogonal to the family
of hyperbolas (-a²<c<-b²).
(d) y = log |tan(x/2)| + c and
the vertical lines x = kp
(k an integer).
(e) The family of curves (tractrix)
![]()
and the same family reflected in the x-axis.
6. (a) The family of parabolas y =
cx².
(b) The family of hyperbolas xy = c.
7. (a) y= x³, (b) y= -x + x log(-x) (0 > x > -¥ ).
8. ![]()
9. ![]()
Note that this gives for c = 0 the parabola y = x² - a²/4. What is the geometrical meaning of this result?
10. 
which is a family of cycloids and can be expressed in the
parametric form x = c + a(j - sin j),
y = a(l - cos j).
Singular solution y = 2a.

11.
and the differential equation is ![]()
By the general method this is easily reduced to
![]()
The various cases, all of importance in the differential
geometry of surfaces (Eisenhart, Differential Geometry,
pp. 270-4 (Princeton Press)), are as follows:

12. Eliminate b from the equations obtained by differentiating the equation of the circle twice and three times:
![]()
13. ![]()
14.
If we substitute the power series for cos
xt in the expression for Jo(x)
in Exercise 4
and interchange summation and integration (why is this
permissible?), we get
![]()
the value of
![]()
as it is found by setting t = sin t and referring to Volume I, 4.4.4. The power series for y(x) and Jo(x) are
1. Poisson's formula gives a potential function u(r, q) inside the unit circle, with boundary values f(q). Now u( 1/r, q) is also a potential function with the same boundary values, and it is bounded in the region outside the unit circle; thus the expression
![]()
is a solution of the problem.
2. The potential is

Since on the ellipsoid
![]()
the potential is
![]()
the confocal ellipsoids
![]()
are equipotential surfaces. The lines of force are the orthogonal trajectories and hence (Exercises 6.5, 5c) are the confocal hyperbolas given by the same equation when 0 £ a £ 1 and the ratio of x to y is constant.
3. Let S be a sphere of radius r and centre (x, y, z), lying inside S. Since D(1/r ) = 0 and Du = 0 in the region bounded by S and S, by Green's theorem ,
![]()
where in the first integral n is the outward normal to S and in the second the outward normal to S. Now, we have on the sphere S
![]()
hence
![]()
since u is a harmonic function; in addition,
![]()
and, as r ® 0, this espression obviously tends to u(x, y, z), because it is the mean value of u on S.
1. (a) u= f(x) + g(y)
(f and g are arbitrary functions).
(b) u == f(x, y) + g(x,
z) + h(y, z) (f, g,
h are arbitrary functions).
(c) The most general solution is obtained from a
particular solution by adding the general solution of the
homogeneous equation uxy = 0.
![]()
2. Apply the linear transformation

3. ![]()
4.

by differentiating the first equation and comparing it with the second one, we have
![]()
or
![]()
For t
Moreover, for t ³ r,
![]()
i.e.,
. As always a + at ³ 0 and hence g(a + at)
= - c, it it follows that

if both x and t are not negative.
5. If
then
![]()
in addition,
![]()
Hence,

where J0 is the the Bessel function
6. (a) The differential equation yields
![]()
As the left hand side does not depend on y, nor the right hand side on x, both sides are equal to a constant (which has to be positive or zero), say c², i.e.,
![]()
Hence,
![]()
is a solution, where c and b are arbitrary
and c² £ 1.
(b) u = f(x)+ g(y)
yields
so that

(where a and b are constants).
If u = f(x)/g(y), then

so that in this case

where a, b, c are arbitrary constants.
7. A one-parameter family is obtained from the two-parameter family of solutions z = u(x, y, a, b) by making a and 6 depend in some way on a parameter t:

The envelope of this one-parameter family is obtained by finding t from the equation
![]()
and substituting this expression for t in z = u(x, y, f(t), g(t)). The result is again a solution of F(x; y, z, zx, zy) = 0, as

and z = u(x, y, a, b) satisfies the equation F(x; y, z, zx, zy) = 0.
8.

Chapter VII

1.
![]()
2. Circle with centre on x-axis.


only depends on the end-points of the curve y = y(x)).
7.

8. Consider F(x, y) for
fixed x as a function of y; let this function of y
have a minimum for y =
. Then, F(x,
y) ³ F(x,
)
for a certain neighbourhood of
and F(x,
) = 0.
will depend on the parameter x. i.e.,
= (x).
Then, for any neighbouring y, we have

where
(x) satisfies the equation Fy(x,
(x))
= 0.
9. 
If y = 1/f(r), then T is given by
![]()
Euler's equation for the variable j yields

along a ray. Now, let the polar co-ordinates be chosen in such
a way that the plane j = 0
passes through the initial point and the end-point; since j = 0 at both these points, we have
for some intermediate point, by the
mean value theorem, i.e., C =
0; but then
for the whole ray, i.e. j = 0. Hence the whole ray must lie
in the plane j = 0.
The law of conservation of energy gives
hence ds/dt = const = C = ini
tial velocity.
Then Hamilton's principle asserts the stationary character of

a stationary character of Hamilton's integral implies that the length of the path is stationary.
1. From the differential equations for geodesics, we find that for a cylinder, i.e., if G does not depend on z, dz/dt = const; hence the geodesics on a cylinder make a constant angle with the xy-plane.

from this equation and
we have

(b) For any continuous, admissible j, we have

the equality sign holding for j = u.
1. For x ³ 0,
2. Use the principle of comparison.
3. By Volune I, Exercise 1.3, 3b, the coefficient of zn in the expansion of cos² z + sin² z for n > 0 is

4. The series converges if, and only if, |z| < 1. In fact, if |z| = 0 < 1, then

and we may compare it with the geometric series. If |z| > 1, then zv/(1 - zv) tends to -1 as n increases, whereas in a convergent series the terms must tend to 0. If |z| = 1, either there are terms in the series which are not defined, or at least its terms are not bounded, since zv may approach 1 as closely as we please.
Let f(z) = u + iv, g(z) = u' + iv', fg = p + iq, where p = uu' - vv', q = uv' + vu'. Assume that u, v and also u', v' satisfy the Cauchy-Riemann equations and prove that the same is true of p, q.
1. The functions (a), (b), (c) are continuous everywhere; (d) is discontinuous at z = 0.
2. None.
3.

Now, for
, the difference between the numerator and the
denominator is
![]()
so that the numerator is larger than the denominator for |z|
> 1 and smaller for |z| < 1. If » \
< 1. If
the converse is true.

6. First transform by setting z = az + b into the unit circle; then apply the transformation

7. The equation of a circle or straight line in the z-plane has the form
![]()
where a and g are real; if we substitute here the expression for z, we get an equation of the same.form for z.
For a fixed point z = z, we hare the quadratic equation
![]()
which, in general, has two different solutions. A circle through the fixed points is, as we have just shown, transformed into a circle and must again pass through the fixed points; the family of orthogonal circles transforms into itself, because circles become circles and the transformation is conformal.
2. The series is absolutely convergent.
By the Cauchy-Riemann equations, the partial derivatives vx and vy are given; a function v with these derivatives does exist, since the condition of integrability uxx + uyy = 0 is satisfied; v is uniquely determined, apart from an additive constant c, and is given by the curvilinear integral

It also follows from the Cauchy-Riemann equations that v is a potential function.
1. lt is easily seen that

is an analytic function of z. By differentiating under the integral sign and using Leibnitz's rule, we find that h(m)(z) is

Only the terms with m - n £
n differ from zero, as otherwise
vanishes. On the other hand, a term with m
- n < n vanishes
for z = 0; if (m
< n, there are no other terms, so that h(m)(0) = 0. If
m ³ 0, there
remains only the term with m-n = n so that

2.

where C is the circle of radius r about the origin.
3.
is equal to the sum of the residue of f'/f
in the interior of C, Now, if f has a zero
of order n at z = z0,

so the residue of
at z = z0 is 2pin.
4. (a) The number of roots of the equation P(z) + qQ(z) = 0, by 3,, is

The denominator differs from zero for every q for which 0 £
q £ 1at any point of
C; the entire integral is therefore a continuous function of q. As its value is always an
integer, it is constant, and hence the same for q = 0 and q
= 1.
(b) If |a| < r4 -
1/r, then r > 1; so the equation z5
+ 1 = 0 has five roots inside the circle |z| = r;
if we set P(z) = z5 + 1,
Q(z)=az, we have on the circle z|
= r
![]()
5. Cf. proof of 3.
The left-hand side of the formula is the sum of the residues
of the function zk/f(z)
and is therefore equal to
taken around a circle
enclosing all the roots an.
But this integral tends to zero as the radius of the circle tends
to infinity (the centre remaining fixed).