falls within any given limits of energy ( and ) is represented by
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If we expand
and
in ascending powers of
, without going beyond the squares, the probability that the energy falls within the given limits takes the form of the 'law of errors'—
|
(353)
|
This gives
|
(354)
|
and
|
(355)
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We shall have a close approximation in general when the quantities equated in (355) are very small,
i. e., when
|
(356)
|
is very great. Now when
is very great,
is of the same order of magnitude, and the condition that (356) shall be very great does not restrict very much the nature of the function
.
We may obtain other properties pertaining to average values in a canonical ensemble by the method used for the average of . Let be any function of the energy, either alone or with and the external coördinates. The average value of in the ensemble is determined by the equation
|
(357)
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