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dition from which to calculate the arbitrary constants we have introduced. This condition, after reduction and arrangement, is as follows:

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to

Substituting in this the series which H, represents, and equating the coefficient of the general term (1— μ2)"μ" zero, and reducing, we arrive at the formula

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By making s successively equal 1, 2, 3 ... we have 4,4,... in terms of A. Let these be substituted, and we have the coefficient of cos n (w — w' =

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call this Af(μ). The coefficient A is a function of μ', but is independent of μ: and because P is the same function of μ' that it is of μ, it follows that A=anf(u), where a, is a numerical quantity: and the coefficient of

an

cos n (w-w') = anf(u') ƒ (μ).

To find a, we must compare the first term of the ascending expansion of anf (u')f(u) in powers of μ with the corresponding term in the coefficient of c' in the actual expansion of

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[1+c2−2c {μμ' +√1 − μ2 √1 − μ22 cos (w — w')}] ̄*.

This leads to the following result:

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(1 . 3 . 5 ... (2¿ — 1))2 ¿ (¿ — 1) ... (i − n + 1)
1.2.3...i i ) (i+2)
(i + 1) (i + 2) ... (i + n) '

n=

this applies when n = 1, 2, 3..., but evidently not when n=0: a, is found by equating coefficients to be

(1.2.3... (2-1))2

1.2.3...i

We have now the complete value of P, in a series; it is as follows:

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38. The following numerical examples are written down for convenience of reference :

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39. The following are some examples of expanding a function in a series of Laplace's Functions, by an application of the formula

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Ex. 1. Arrange a + bμ2 in terms of Laplace's Functions.

Here Fu', w') = a+bμ2. First put i=0, P=1;

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Again, put i=1, P, is found in the last Article.

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1

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4π -1

between the proper limits, w' = 0 and w' = 2π,

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between the limits μ': · 1 and μ' = 1, = 0.

P. A.

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Next, put = 2, and substitute for P, from the last Article.

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Hence the function a+bu2 stands as follows, when arranged in terms of Laplace's Functions,

(a + b) + b (μ3 — — ),

and consists of two Functions, of the order 0 and 2 respectively. The above is a long process to arrive at this result. It might have been so arranged at a glance. But the calculation has been given as an example of the use of the formula, which in most cases is the only means of obtaining the desired result.

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Ex. 2. Arrange 49+30μ+3μ3+ √1−μ3 (40+72μ) cos (w—a) +24 (1 − μ3) cos 2 (wa) in terms of Laplace's Functions.

2

The result is 50+ {30μ + 40 √√1 − μ2 cos (w — a)}

+ {3μ2 − 1 + 72μ √1 — μ3 cos (∞ − a) +24 (1 − μ2) cos 2 (w—a)},

consisting of three functions of the orders 0, 1, 2.

Ex. 3. Let the function be

1+√√2 − 2μ3 cos (w + a) + — (1 − μ2) cos 2 (w+a).

The first term is a Laplace's Function of the order 0, and the second and third terms taken together are one of the second order.

Ex. 4. Let 1-(1-μ) cos w be the function. The arrange

ment is

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