Abstract
The paper gives a wide range, uniform, local approximation of symmetric binomial distribution. The result clearly shows how one has to modify the classical de Moivre–Laplace normal approximation in order to give an estimate at the tail as well as to minimize the relative error.
MSC:
60E15; 60F05
The topic of this paper is a wide range, uniform, local approximation of symmetric binomial distribution, an extension of the classical de Moivre–Laplace theorem in the symmetric case [1] (Ch. VII) [2]. In other words, I would like to approximate individual binomial probabilities not only in a classical neighborhood of the center, but at the tail as well. The result clearly shows how one has to modify the normal approximation in order to give a wide range estimate to minimize the relative error. The method will be somewhat similar to the ones applied by [3,4,5] or in the proof of Tusnády’s lemma, see, e.g., [6]; however, my task is much simpler than those. This simplification makes the proof short, transparent and natural. Moreover, the result is non-asymptotic, that is, it gives explicit, nearly optimal, upper and lower bounds for the relative error with a finite n. Thus, I hope that it can be used in both applications and teaching.
Let be a sequence of independent, identically distributed random steps with and , , be the corresponding simple, symmetric random walk. Then
Here, we use the convention that the above binomial coefficient is zero whenever is not divisible by 2. Since for any j, it is enough to consider only the case whenever it is convenient.
First we consider the case when , even. Let us introduce the notation
Also, introduce the notation
when and , and
Theorem 1.
(a) For any and , we have
(b) For any and , , we have
(c) In accordance with the classical de Moivre–Laplace normal approximation, for and one has
Proof.
As usual, the first step is to estimate the central term
By Stirling’s formula, see, e.g., [1] (p. 54), we have:
Thus, after simplification we obtain
Second, also by the standard way, for ,
So it follows that
To approximate the sum here, let us introduce the integral
for , and its approximation by a trapezoidal sum
where . It is well-known that the error of the trapezoidal formula for a function is
Since , we obtain that
Let us combine Formulas (8)–(12):
thus
where and
Clearly, (14) is the same as (2). Thus, (13) proves (a) and (b) of the theorem.
Let us see now, using Taylor expansions, a series expansion of when . First, for ,
Second, also for ,
So by (14), for we have a convergent series for :
The main moral of Theorem 1 is that the exponent in the exponent of the normal approximation is only a first approximation of the series (15). In (c), the bound was chosen somewhat arbitrarily. It is clear from the series (15) that the bound should be . The above given bound was picked because it seemed to be satisfactory for usual applications with large deviation and gave a nice relative error bound .
It is not difficult to extend the previous results to the odd-valued case of the symmetric binomial probabilities
Define
for and , and
Theorem 2.
(a) For any and , we have
(b) For any and , , we have
(c) In accordance with the classical de Moivre–Laplace normal approximation, for and one has
Proof.
Funding
This research received no external funding.
Institutional Review Board Statement
Not applicable.
Data Availability Statement
No new data were created or analyzed in this study. Data sharing is not applicable to this article.
Conflicts of Interest
The author declares no conflicts of interest.
References
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