<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">AM</journal-id><journal-title-group><journal-title>Applied Mathematics</journal-title></journal-title-group><issn pub-type="epub">2152-7385</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/am.2013.42043</article-id><article-id pub-id-type="publisher-id">AM-28188</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  What Is the Difference between Gamma and Gaussian Distributions?
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>iao-Li</surname><given-names>Hu</given-names></name><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><author-notes><corresp id="cor1">* E-mail:<email>xiaoli.hu@newcsatle.edu.au, xlhu@amss.ac.cn</email>;<email>School of Electrical Engineering and Computer Science, University of Newcastle, Newcastle, Australia</email>;</corresp></author-notes><pub-date pub-type="epub"><day>22</day><month>02</month><year>2013</year></pub-date><volume>04</volume><issue>02</issue><fpage>285</fpage><lpage>289</lpage><history><date date-type="received"><day>November</day>	<month>19,</month>	<year>2012</year></date><date date-type="rev-recd"><day>December</day>	<month>25,</month>	<year>2012</year>	</date><date date-type="accepted"><day>January</day>	<month>3,</month>	<year>2013</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
   An inequality describing the difference between Gamma and Gaussian distributions is derived. The asymptotic bound is much better than by existing uniform bound from Berry-Esseen inequality. 
 
</p></abstract><kwd-group><kwd>Gamma Distribution; Gaussian Distribution; Berry-Esseen Inequality; Characteristic Function</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><sec id="s1_1"><title>1.1. Problem</title><p>We first introduce some notations. Denote Gamma distribution function as</p><disp-formula id="scirp.28188-formula83960"><label>(1)</label><graphic position="anchor" xlink:href="3-7401259\0a554dfb-2183-4b81-aca4-cfb69195723c.jpg"  xlink:type="simple"/></disp-formula><p>for <img src="3-7401259\6a49609d-19cf-44ff-80fe-6f1b24c9ea54.jpg" /> and<img src="3-7401259\1b43304e-962e-4cc8-8983-3419e28dabb2.jpg" />, where <img src="3-7401259\f8eddcc2-e6ca-4890-a6a9-b1746d2269c0.jpg" /> is the Gamma function, i.e.,</p><p><img src="3-7401259\b8181c97-8d4a-461b-8598-cc3d8a23756f.jpg" /></p><p>Assume <img src="3-7401259\5af62325-c2c8-4cf1-b8db-7f6d60b39051.jpg" /> for<img src="3-7401259\2f06a242-695b-481b-9f3f-f1e3c0acd120.jpg" />. The density of chisquare distributed random variable <img src="3-7401259\7d7ebe56-c1ea-4f29-b763-5a78039e8b33.jpg" /> with <img src="3-7401259\87fb9302-6267-4412-97db-94bbecda911b.jpg" /> degrees of freedom is</p><p><img src="3-7401259\b7a78b36-44ac-41aa-a449-e040cd66f327.jpg" /></p><p>It is well-known that the random variable <img src="3-7401259\94621695-d2e8-4385-8975-68330b411350.jpg" /> can be interpreted by <img src="3-7401259\8419b2fd-d722-4b38-a07f-d4f277c724fb.jpg" /> with <img src="3-7401259\764d1e9c-9aed-4348-a24d-36d137a11672.jpg" /> independent and identically distributed (i.i.d.) random variables <img src="3-7401259\1990af94-2f25-409d-a9d2-8e5e1f041e9b.jpg" /> <img src="3-7401259\aa887a87-957f-484d-ab3e-a8f368b6c183.jpg" /> where <img src="3-7401259\75d37aa5-838e-4fd5-93da-6eeb67b7557d.jpg" /> denotes the standard Gaussian distribution. The mean and variance of <img src="3-7401259\e7141b5a-4bb5-4d1f-834d-a4f2935bcf3d.jpg" /> is respectively</p><p><img src="3-7401259\eb75b7e7-1a2f-4f20-b2a5-3f35c57da5e3.jpg" /></p><p>Then, by simple change of variable we find</p><disp-formula id="scirp.28188-formula83961"><label>(2)</label><graphic position="anchor" xlink:href="3-7401259\fecb9bef-7648-44dc-864a-4ca2b509ea6e.jpg"  xlink:type="simple"/></disp-formula><p>On the other side, by the Berry-Esseen inequality to</p><p><img src="3-7401259\f2d8efda-a918-4edb-ae66-3ae0776faeb9.jpg" />, it is easy to find a bound</p><p><img src="3-7401259\88fe1976-9103-49c8-9b75-b4e64981d5b9.jpg" />such that</p><disp-formula id="scirp.28188-formula83962"><label>(3)</label><graphic position="anchor" xlink:href="3-7401259\58094679-9216-412a-bf07-6f0ecef346e7.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="3-7401259\46779a99-38c6-45cb-bda3-5dcdded68c84.jpg" /> is the standard Gaussian distribution function, i.e.,</p><disp-formula id="scirp.28188-formula83963"><label>(4)</label><graphic position="anchor" xlink:href="3-7401259\8e918a4f-cf01-431d-a4d7-02f7a2ad9746.jpg"  xlink:type="simple"/></disp-formula><p>Then, by Equations (2) and (3) it follows</p><disp-formula id="scirp.28188-formula83964"><label>(5)</label><graphic position="anchor" xlink:href="3-7401259\fb155ba7-a596-4bd4-8d8b-9071ae94d65d.jpg"  xlink:type="simple"/></disp-formula><p>which describes the distance between Gamma and Gaussian distributions. The purpose of this paper is to derive asymptotic sharper bound <img src="3-7401259\28ed98d7-8c7b-48ba-9744-7de534c94e7a.jpg" /> in Equation (5), which much improves the constant <img src="3-7401259\800367bb-8904-4894-9867-30f7e85690ec.jpg" /> by directly using Berry-Esseen inequality. The main framework of analysis is based on Gil-Pelaez formula (essentially equivalent to Levy inversion formula), which represents distribution function of a random variable by its characteristic function.</p><p>The main result of this paper is as following.</p><p>Theorem 1.1 A relation of the Gamma distribution (1) and Gaussian distribution (4) is given by</p><disp-formula id="scirp.28188-formula83965"><label>(6)</label><graphic position="anchor" xlink:href="3-7401259\db6ccb3c-07e9-4d23-a6aa-d6f08744c5fe.jpg"  xlink:type="simple"/></disp-formula><p>where</p><p><img src="3-7401259\77f7fa12-b54c-41db-b185-0322e4b7bc06.jpg" /></p><p><img src="3-7401259\49f48db1-c80e-4d45-8c76-dff3293f65f8.jpg" /></p><p>with <img src="3-7401259\cc7c156b-46c8-4d62-8889-455a78d7fc52.jpg" /> and <img src="3-7401259\d9de58ee-f685-4166-8776-dfb10ae6e8d9.jpg" /> for any<img src="3-7401259\ec60f751-7bea-4b57-a778-05e002d6feac.jpg" />.</p><p>Clearly, <img src="3-7401259\502999fe-579f-4fe6-963f-6fc1fdebdeac.jpg" />as<img src="3-7401259\83508f11-c6f1-4a08-a5c3-cd5776d3bbc2.jpg" />. Thus, the asymptotical bound is</p><p><img src="3-7401259\25484925-36b2-4d92-9148-628d4b163242.jpg" /></p><p>as<img src="3-7401259\a2e0732e-6dde-4f0a-b9d6-24eb7172c715.jpg" />. To check the tightness of the limit value of<img src="3-7401259\8cecb9b2-25ff-4c92-88e5-33392751043b.jpg" />, we plot in <xref ref-type="fig" rid="fig1">Figure 1</xref> the multiplication</p><p><img src="3-7401259\356f1b35-8ddd-4982-a3f1-8d3f63854dd3.jpg" /></p><p>for<img src="3-7401259\af7bf775-263d-44a3-bfc5-770fa9b38191.jpg" />, where the straight line is the limit value<img src="3-7401259\d231e81b-710e-42a1-8969-c5b3864ec72c.jpg" />. From this experiment it seems that <img src="3-7401259\e9e4b28a-d88b-4ff5-aa70-472437ec1cda.jpg" /></p><p>is the best constant. The tendency of the theoretical formula <img src="3-7401259\2aa9f71e-35c7-41f6-92d4-93ae54738868.jpg" /> is plotted for <img src="3-7401259\23823368-cafb-4cbb-930e-14efdf40abea.jpg" /> in <xref ref-type="fig" rid="fig2">Figure 2</xref>, which also shows the tendency to the limit value</p><p><img src="3-7401259\71326757-f811-41e2-9a3e-ae965c5a8a8d.jpg" />. The slow trend is due to that some upper bounds formulated over interval <img src="3-7401259\e32861d7-3c8f-4672-b402-741b2c7ac7a9.jpg" /> have been weakly estimated, e.g., the third and fourth terms of<img src="3-7401259\8ef3c1e4-0e92-49c3-9c8c-2fae5bb137bd.jpg" />.</p></sec><sec id="s1_2"><title>1.2. Comparison to the Bound Derived by Berry-Esseen Inequality</title><p>Let <img src="3-7401259\5cd8fc13-4797-477b-8e68-2518a16dd777.jpg" /> be a sequence of independent identically distributed random variables with EX<sub>1</sub> = 0 <img src="3-7401259\c25adb2d-ce4b-4076-867a-b7bba732da8d.jpg" /></p><p>and finite third absolute moment<img src="3-7401259\a3a209a2-d127-4a7d-a283-9c7c811799e0.jpg" />. Denote</p><p><img src="3-7401259\bf33ef34-1f19-40ef-b5fc-7bde3da7d091.jpg" /></p><p>By classic Berry-Esseen inequality, there exists a finite positive number <img src="3-7401259\27da194f-0ceb-4327-be87-7b7565304506.jpg" /> such that</p><disp-formula id="scirp.28188-formula83966"><label>(7)</label><graphic position="anchor" xlink:href="3-7401259\a7472a78-25b3-4cfc-afc6-8309816c6b03.jpg"  xlink:type="simple"/></disp-formula><p>The best upper bound <img src="3-7401259\26e0a89f-4e53-44c1-8fbc-90b7f10b035b.jpg" /> is found in [<xref ref-type="bibr" rid="scirp.28188-ref1">1</xref>] in 2009. The bound is improved in [<xref ref-type="bibr" rid="scirp.28188-ref2">2</xref>] at some angle in a slight different form as</p><disp-formula id="scirp.28188-formula83967"><label>(8)</label><graphic position="anchor" xlink:href="3-7401259\1362d333-5f24-444d-a77e-825a22dafd26.jpg"  xlink:type="simple"/></disp-formula><p>with</p><p><img src="3-7401259\6d346f0f-82a1-428e-a22d-2987f3d8c9dd.jpg" /></p><p>The inequality (8) will be sharper than Equation (7) for<img src="3-7401259\c081748d-44c4-4302-a02c-4d6c14f8fdd6.jpg" />.</p><p>Now let us derive the constant <img src="3-7401259\de0ab3cd-db42-42f1-8f6e-29ae8cb05b27.jpg" /> in (5) by applying Berry-Esseen inequality to<img src="3-7401259\1fe91e87-b692-4aca-80fa-77adac97f00e.jpg" />. It is difficult to calculate the exact value of third absolute moment of the random variable<img src="3-7401259\5ffb1699-06dd-452d-acfe-c0f168ced845.jpg" />. Thus, it is approximated as</p><p><img src="3-7401259\821e4f8b-d398-4176-9730-10121ebdb144.jpg" /></p><p>by using Matlab to integrate over interval <img src="3-7401259\925ce197-168e-451e-9d3d-3819137eadbe.jpg" /> divided equivalently 100,000 subinterval for its half value.</p><p>By Equation (7) with <img src="3-7401259\b0a4b703-45fb-47ff-a24b-7e2a2c5103e7.jpg" /> we have</p><p><img src="3-7401259\2bb5691c-4f40-4f47-9882-304658a1dca8.jpg" /></p><p>and by Equation (8) we have</p><p><img src="3-7401259\2890e4e7-b576-45bb-bb25-0273e4874d35.jpg" /></p><p>Hence, the best constant <img src="3-7401259\8e0d055a-cec6-4ad4-9438-b6ffbe51855c.jpg" /> in Equation (5) by applying Berry-Esseen inequality is<img src="3-7401259\e2929994-efa2-4c4d-8618-624a46775df6.jpg" />. Obviously, the limit bound</p><p><img src="3-7401259\420896bd-e105-45a5-88b6-b9cc5e63e465.jpg" /></p><p>found in this paper for chi-square distribution is much better.</p><p>The technical reason is that the Berry-Esseen inequality deals with general i.i.d. random sequences without exact information of the distribution.</p></sec></sec><sec id="s2"><title>2. Proof of Main Result</title><p>Before to prove the main result, we first list a few lemmas and introduce some facts of characteristic function theory.</p><sec id="s2_1"><title>2.1. Some Lemmas</title><p>Lemma 2.1 For a complex number <img src="3-7401259\314682c9-6a81-4a87-9115-71d734b9f8d1.jpg" /> satisfying<img src="3-7401259\2ea88d08-553a-4484-b510-1f46b506b1f9.jpg" />, <img src="3-7401259\d2f4814e-04ca-454e-8889-515923fd242e.jpg" /></p><p>Proof First show that</p><p><img src="3-7401259\8f4d904d-9a49-41bf-bce1-bff7f5b6eae1.jpg" /></p><p>By Taylor’s expansion and noting<img src="3-7401259\247a6ef2-a2b8-4e4d-aa21-e71127990dae.jpg" />, we have</p><p><img src="3-7401259\41172861-000a-461f-a35e-bd38f4aec010.jpg" /></p><p>Together with</p><p><img src="3-7401259\8c199492-7c35-4fa6-b6c8-3798957f0868.jpg" /></p><p>the assertion follows.</p><p>Lemma 2.2 For a real number <img src="3-7401259\754a1fb2-c4d1-4132-8bc0-3b4b162df52a.jpg" /> satisfying<img src="3-7401259\d3837096-29dd-40ec-bb1f-eaff20716ff7.jpg" />,</p><p><img src="3-7401259\e5329700-e7aa-4650-af4f-29a5797f7702.jpg" /></p><p>where <img src="3-7401259\11f8b0c3-acaa-4541-b4e1-3f666f4cd167.jpg" /> is the imaginary unit and</p><p><img src="3-7401259\9085747b-2103-4b54-a4c5-0bca8934d404.jpg" /></p><p>Clearly,</p><p><img src="3-7401259\65c263df-12f8-4bad-beb5-c66ab473aa63.jpg" /></p><p>Proof. By Taylor expansion for complex function, for <img src="3-7401259\9716a4d9-f483-4842-8eae-8150d49ce584.jpg" /> we have</p><p><img src="3-7401259\c42fe502-52ce-4f8c-a9eb-e912a09b480e.jpg" /></p><p>where <img src="3-7401259\8833faeb-78e3-40f2-87f7-a1e20587de10.jpg" /> is shown above. By further noting the two alternating real series above, it follows the upper bound.</p><p>We cite below a well-known inequality [<xref ref-type="bibr" rid="scirp.28188-ref3">3</xref>] as a lemma.</p><p>Lemma 2.3 The tail probability of the standard normal distribution satisfies</p><p><img src="3-7401259\500962db-3634-4d41-a9ee-3651351997b6.jpg" /></p><p>for<img src="3-7401259\509be7f8-dd98-4889-abfd-56ec70c62ae5.jpg" />.</p></sec><sec id="s2_2"><title>2.2. Characteristic Function</title><p>Let us recall, see e.g., [<xref ref-type="bibr" rid="scirp.28188-ref4">4</xref>], the definition and some basic facts of characteristic function (CF), which provides another way to describe the distribution function of a random variable. The characteristic function of a random variable <img src="3-7401259\5d0bbb2c-13bc-48f2-8995-fe1a5268039f.jpg" /> is defined by</p><p><img src="3-7401259\cf621cb4-433d-4993-b874-9d2a3de9ba7a.jpg" /></p><p>where <img src="3-7401259\43be2466-dad5-42f3-a5be-7d9b38a0cdfb.jpg" /> is the imaginary unit, and <img src="3-7401259\714d9fe5-f90e-4092-8010-a97172ca60ad.jpg" /> is the argument of the function. Clearly, the CF for random variable <img src="3-7401259\4aa2380d-3fa7-4da0-888b-e54f7b985584.jpg" /> with real numbers <img src="3-7401259\b9808944-d41b-4eee-98c1-917484310000.jpg" /> and <img src="3-7401259\4f520a76-17e8-47e1-b7ba-e286c75a65ca.jpg" /> is</p><p><img src="3-7401259\ec6bf695-98f9-4f43-8359-70974778ec53.jpg" /></p><p>Another basic quality is</p><p><img src="3-7401259\2d40b3ed-caa3-4940-b7ed-c786d087cd27.jpg" /></p><p>for <img src="3-7401259\ed19111a-f802-43e8-94cd-00582d821769.jpg" /> with <img src="3-7401259\0d3aad25-aed5-4717-85d4-b8e5c23b7fd9.jpg" /> and <img src="3-7401259\b21c556a-7b08-401f-bd79-17f063cbc146.jpg" /> independent to each other.</p><p>It is well-known that the CF of standard Gaussian <img src="3-7401259\63ae748e-3c58-4785-8909-4d1c8831ae5d.jpg" /> is</p><disp-formula id="scirp.28188-formula83968"><label>(9)</label><graphic position="anchor" xlink:href="3-7401259\73a2ef6d-7421-4f77-814d-fc4494fc3b58.jpg"  xlink:type="simple"/></disp-formula><p>and the CF of chi-square distributed variable <img src="3-7401259\c868ebe4-f9e9-41e5-a883-26fa4212d6c1.jpg" /> is</p><p><img src="3-7401259\b50fba78-cefd-4a6b-9a17-b9dc233ab174.jpg" /></p><p>Thus, the CF for <img src="3-7401259\9bba598c-9b0c-45af-8f24-79c8a20a9e13.jpg" /> is</p><disp-formula id="scirp.28188-formula83969"><label>(10)</label><graphic position="anchor" xlink:href="3-7401259\f17a0686-f7a9-4c92-b37c-b357b9cbdce7.jpg"  xlink:type="simple"/></disp-formula><p>The CF is actually an inverse Fourier transformation of density function. Therefore, distribution function can be expressed by CF directly, e.g., Levy inversion formula. We use another slightly simpler formula. For a univariate random variable<img src="3-7401259\2a753e6f-c0ae-4eca-ac4a-47b26b0b7dd9.jpg" />, if <img src="3-7401259\b33b26c4-dcb9-45d6-972c-b4894e3e7e4f.jpg" /> is a continuity point of its distribution<img src="3-7401259\b84cf595-cecf-4ee6-8a58-58527d2a6dd4.jpg" />, then</p><disp-formula id="scirp.28188-formula83970"><label>(11)</label><graphic position="anchor" xlink:href="3-7401259\d2a6e7b8-b051-4fb7-85b2-9904cd4df1c4.jpg"  xlink:type="simple"/></disp-formula><p>which is called Gil-Pelaez formula, see, e.g., page 168 of [<xref ref-type="bibr" rid="scirp.28188-ref4">4</xref>].</p></sec><sec id="s2_3"><title>2.3. Proof of Main Result</title><p>We are now in a position to prove the main result.</p><p>Proof of Theorem 1.1 First analyze CF of <img src="3-7401259\927f4f60-83ae-4861-bed3-743ddc1ccad2.jpg" /> given by Equation (10). Denote<img src="3-7401259\0814afcb-0973-413f-97dc-738281bd1a53.jpg" />. For<img src="3-7401259\bd232443-aba1-4a21-a6c8-50bf67caec5c.jpg" />, i.e., <img src="3-7401259\86828f8e-78e3-4ae8-a3db-a94de4487a0f.jpg" />, by Lemma 2.2,</p><disp-formula id="scirp.28188-formula83971"><label>(12)</label><graphic position="anchor" xlink:href="3-7401259\0e3c5a3e-fe43-48d3-bbe5-ef087073a058.jpg"  xlink:type="simple"/></disp-formula><p>where</p><p><img src="3-7401259\03e81df1-a4d8-418b-afcc-b50486a8f183.jpg" /></p><p>Clearly,</p><p><img src="3-7401259\218cfeb4-3311-4b11-b36d-6ed70053ea01.jpg" /></p><p>To make sure <img src="3-7401259\cb64bb75-27c2-4aba-895b-3e902e2fd630.jpg" /> for some<img src="3-7401259\c7b318f3-b063-488c-bf6a-bccf2537886b.jpg" />denote<img src="3-7401259\a97da777-c267-4001-84fc-a827d7927dc2.jpg" />. Then, it is easy to see that</p><disp-formula id="scirp.28188-formula83972"><label>(13)</label><graphic position="anchor" xlink:href="3-7401259\e86fe467-343a-4e62-8266-a16dd13ce636.jpg"  xlink:type="simple"/></disp-formula><p>for<img src="3-7401259\e3bfe658-6981-445d-941e-b904ae3b8550.jpg" />. Hence, by Equations (12) and (13) and Lemma 2.1,</p><disp-formula id="scirp.28188-formula83973"><label>(14)</label><graphic position="anchor" xlink:href="3-7401259\4702eb0e-ae70-418b-9b59-2c27a9dbf3e0.jpg"  xlink:type="simple"/></disp-formula><p>for<img src="3-7401259\9a8eb7a7-3cfe-44dd-b8b1-48a22ef0fb61.jpg" />.</p><p>Now let us consider the difference between <img src="3-7401259\1d52ac37-2627-4d46-a606-4a14dc34791a.jpg" /> and<img src="3-7401259\57f64afd-28ef-40fe-aaee-c2d3ca20c8e5.jpg" />, i.e., the CF (9) of Gaussian distribution, over the interval<img src="3-7401259\d5ee7608-58f7-44dd-9840-0c8662661b3a.jpg" />. By Equation (14)</p><p><img src="3-7401259\4fc22c47-cf19-4f99-b98f-db8030b6bbb3.jpg" /></p><p>Note that</p><p><img src="3-7401259\0af7f2f3-860d-41ba-a328-c8beac2d22f8.jpg" /></p><p>it follows</p><disp-formula id="scirp.28188-formula83974"><label>(15)</label><graphic position="anchor" xlink:href="3-7401259\c2aca897-80d3-4373-84a5-56de43e5f785.jpg"  xlink:type="simple"/></disp-formula><p>Similarly,</p><disp-formula id="scirp.28188-formula83975"><label>(16)</label><graphic position="anchor" xlink:href="3-7401259\6d1a2e14-5988-4588-81c4-e521ff53d630.jpg"  xlink:type="simple"/></disp-formula><p>Below let us analyze the residual integrals over the interval<img src="3-7401259\5f19fbe2-6bfd-4ce7-ab82-709be8fccfe0.jpg" />. By Lemma 2.3,</p><disp-formula id="scirp.28188-formula83976"><label>(17)</label><graphic position="anchor" xlink:href="3-7401259\8109b657-7a34-4762-83a7-5e77e9307918.jpg"  xlink:type="simple"/></disp-formula><p>Similarly,</p><disp-formula id="scirp.28188-formula83977"><label>(18)</label><graphic position="anchor" xlink:href="3-7401259\84218f94-1c0c-4da5-a4f2-6cafd3be2399.jpg"  xlink:type="simple"/></disp-formula><p>It is somewhat difficult to analyze the residual integral over <img src="3-7401259\a3f177a1-aab1-41ad-968e-9ec76df21250.jpg" /> for<img src="3-7401259\2896e962-40fa-4ae4-bb5d-cf0f345564ef.jpg" />. We divide it into two subintervals as following:</p><p><img src="3-7401259\d3b4be44-2996-4e56-89ef-eccc2cdc0763.jpg" /></p><p>where<img src="3-7401259\fdaa5a23-e870-4fb4-8aa4-230a85e2dda9.jpg" />.</p><p>Observe that <img src="3-7401259\c7beaa63-2e48-400c-bd35-a40f16043110.jpg" /> decreases on interval <img src="3-7401259\91eb4eda-1cf6-4c3f-818d-0d848e7df912.jpg" /> and <img src="3-7401259\12407c0f-d76e-4582-b6ed-40ced743546e.jpg" /> for<img src="3-7401259\82093d98-417a-4e89-a2ad-d4f84f2af1c7.jpg" />, we have</p><p><img src="3-7401259\2209240f-70d6-4281-be79-d3382a3a7cfd.jpg" /></p><p>where</p><p><img src="3-7401259\dd6894a5-ec3e-486a-b1b8-b64a4a05278a.jpg" /></p><p>The fact <img src="3-7401259\cdf4a935-7d85-474c-92cd-e7612a08f4df.jpg" /> is used in above formula. Thus,</p><disp-formula id="scirp.28188-formula83978"><label>(19)</label><graphic position="anchor" xlink:href="3-7401259\a3f7724a-a991-4ad9-a790-6facadef53af.jpg"  xlink:type="simple"/></disp-formula><p>For the other interval<img src="3-7401259\61ecadf9-fe98-4b98-ac7a-d73008346f96.jpg" />, we proceed as</p><disp-formula id="scirp.28188-formula83979"><label>(20)</label><graphic position="anchor" xlink:href="3-7401259\0f18092c-5547-4294-8f04-7b502171dcd0.jpg"  xlink:type="simple"/></disp-formula><p>By Equations (19) and (20)</p><disp-formula id="scirp.28188-formula83980"><label>(21)</label><graphic position="anchor" xlink:href="3-7401259\a9d03469-ce05-4b9f-a4ae-3d4d11436e8d.jpg"  xlink:type="simple"/></disp-formula><p>Similarly,</p><disp-formula id="scirp.28188-formula83981"><label>(22)</label><graphic position="anchor" xlink:href="3-7401259\cd5ebfdc-4746-4056-aeb3-9483899f9419.jpg"  xlink:type="simple"/></disp-formula><p>By Equation (15), Equation (17), Equation (21) and Equation (16), Equation (18), Equation (22)</p><p><img src="3-7401259\5211c61e-e02b-4364-9545-b30426bf02b0.jpg" /></p><p>where</p><p><img src="3-7401259\b9ba0a83-84be-4c7d-8e0e-73be66430ceb.jpg" /></p><p>In view of Formula (11) , the formula to be proved follows directly.</p></sec></sec><sec id="s3"><title>REFERENCES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.28188-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">I. S. Tyurin, “On the Accuracy of the Gaussian Approximation,” Doklady Mathematics, Vol. 80, No. 3, 2009, pp. 840-843. doi:10.1134/S1064562409060155</mixed-citation></ref><ref id="scirp.28188-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">V. Koroleva and I. Shevtsova, “An Improvement of the Berry-Essen in Equality with Application to Possion and Mixed Poison Random Sums,” Scandinavian Actuarial Journal, Vol. 2012, No. 2, 2012, pp. 81-105.  
doi:10.1080/03461238.2010.485370</mixed-citation></ref><ref id="scirp.28188-ref3"><label>3</label><mixed-citation publication-type="other" xlink:type="simple">R. D. Gordon, “Values of Mills’ Ratio of Area to Bounding Ordinate and of the Normal Probability Integral for Large Values of the Argument,” The Annals of Mathematical Statistics, Vol. 12, No. 3, 1941, pp. 364-366.  
doi:10.1214/aoms/1177731721</mixed-citation></ref><ref id="scirp.28188-ref4"><label>4</label><mixed-citation publication-type="other" xlink:type="simple">K. L. Chung, “A Course in Probability Theory,” 3rd Edition, Probability and Mathematical Statistics, Academic, New York, 2001.</mixed-citation></ref></ref-list></back></article>