<?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">JCPT</journal-id><journal-title-group><journal-title>Journal of Crystallization Process and Technology</journal-title></journal-title-group><issn pub-type="epub">2161-7678</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jcpt.2014.43019</article-id><article-id pub-id-type="publisher-id">JCPT-47789</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>CHEMISTRY &amp; MATERIALS SCIENCE</subject></subj-group></article-categories><title-group><article-title>Theoretical Model of Diffraction Line Profiles as Combinations of Gaussian and Cauchy Distributions</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Girija</surname><given-names>Bhushan Mitra</given-names></name><xref ref-type="aff" rid="aff1"><sub>1</sub></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff1"><label>1</label><addr-line>Indian Association for the Cultivation of Science, Jadavpur, Kolkata, India</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>gbmitra@gmail.com</email></corresp></author-notes><pub-date pub-type="epub"><day>23</day><month>06</month><year>2014</year></pub-date><volume>04</volume><issue>03</issue><fpage>145</fpage><lpage>155</lpage><history><date date-type="received"><day>6</day>	<month>May</month>	<year>2014</year></date><date date-type="rev-recd"><day>29</day>	<month>May</month>	<year>2014</year>	</date><date date-type="accepted"><day>17</day>	<month>June</month>	<year>2014</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>
	Previously
we derived equations determining line broadening in ax-ray diffraction profile
due to stacking faults. Here, we will consider line broadening due to particle
size and strain which are the other factors affecting line broadening in a
diffraction profile. When line broadening in a diffraction profile is due to
particle size and strain, the theoretical model of the sample under study is
either a Gaussian or a Cauchy function or a combination of these functions,
e.g. Voigt and Pseudovoigt functions.
Although the overall nature of these functions can be determined by Mitra’s &lt;i&gt;R&lt;/i&gt;(x) test and the Pearson and Hartley &lt;i&gt;x&lt;/i&gt; test, details of a predicted model will be lacking. Development of a
mathematical model to predict various parameters before embarking upon the
actual experiment would enable correction of significant sources of error prior
to calculations. Therefore, in this study, predictors of integral width, Fourier
Transform, Second and Fourth Moment and Fourth Cumulant of samples represented
by Gauss, Cauchy, Voigt and Pseudovoigt functions have been worked out. An
additional parameter, the coefficient of excess, which is the ratio of the
Fourth Moment to three times the square of the Second Moment, has been
proposed. For a Gaussian profile the coefficient of excess is one, whereas for
Cauchy distributions, it is a function of the lattice variable. This parameter
can also be used for determining the type of distribution present in aggregates
of distorted crystallites. Programs used to define the crystal structure of
materials need to take this parameter into consideration.
</p></abstract><kwd-group><kwd>Line Broadening</kwd><kwd> Diffraction Profile</kwd><kwd> Theoretical Model</kwd><kwd> Gaussian Function</kwd><kwd> Cauchy Function</kwd><kwd> Voigt Function</kwd><kwd> Pseudovoigt Function</kwd><kwd> Fourier Transform</kwd><kwd> Second Moment</kwd><kwd> Fourth Moment</kwd><kwd> Fourth  Cumulant</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Diffraction line profiles due to polycrystalline materials have long been recognized to be caused by physical parameters like sizes of and defects in constituent powder particles. For this purpose, parameters like full width at half maximum (FWHM) intensity, integral width of line profile, Fourier transforms of intensity profile etc. have been utilized. Additionally, the moments [<xref ref-type="bibr" rid="scirp.47789-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.47789-ref2">2</xref>] and cumulants [<xref ref-type="bibr" rid="scirp.47789-ref3">3</xref>] of the line profile have also been used. These methods include recording of the line profile and correcting them for various sources of errors prior to calculations. Therefore, it may be beneficial to develop a reasonable mathematical model for the sample, the profile and the process. Such models are also required for structure refining methods as in Reitveld refinement.</p><p>The author previously showed that line broadening in a diffraction intensity profile of powdered crystalline materials due to stacking fault can be characterized in terms of the Zeroth, the First, the Second, the Third, and the Fourth Moment and the Fourth Cumulant [<xref ref-type="bibr" rid="scirp.47789-ref4">4</xref>] . In the present article, the scope of the characterization has been expanded to include line broadening due to particle size and strain as well. An example of a model that includes these factors may be found using Cauchy and Gauss functions. When the size effect is more predominant, the function is found to be more Cauchy-like and when the effect of strain is predominant, the Gauss model preponderates. So, the ideal model would be a suitable combination of both.</p><p>The author has in the past described a method of differentiating between Cauchy and Gauss distributions in diffraction line profiles [<xref ref-type="bibr" rid="scirp.47789-ref5">5</xref>] . These distributions are now standard and are used by investigators all over the world to identify the characteristics of crystalline materials. The two distributions are given as follows:</p><p>1) Gauss distribution:</p><disp-formula id="scirp.47789-formula3541"><label>(1)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\7bc3f158-627b-4a10-9516-4edd12b8976f.png"/></disp-formula><p>2) Cauchy distribution:</p><disp-formula id="scirp.47789-formula3542"><label>(2)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\e81c5c1e-c834-4216-a84b-990949f882af.png"/></disp-formula><p>where f(x) is the distribution for the variable x. The author also showed that the cumulative distribution</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\a0dc9b78-e550-4ff7-b4e0-c4d03eb2590c.png" xlink:type="simple"/></inline-formula>for these two distributions was provided in the past [<xref ref-type="bibr" rid="scirp.47789-ref5">5</xref>] as follows:</p><p>For Gauss distribution:</p><disp-formula id="scirp.47789-formula3543"><label>(3)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\a3070071-54ee-46ff-a536-de3bce3642d8.png"/></disp-formula><p>For Cauchy distribution:</p><disp-formula id="scirp.47789-formula3544"><label>(4)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\36dd9daa-cbd7-4c3a-a468-4251c9e652f3.png"/></disp-formula><p>Therefore, comparison of a graph of</p><disp-formula id="scirp.47789-formula3545"><label>vs x</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\738fcc1a-646f-48e5-a690-dbfe670491b4.png"/></disp-formula><p>with the calculated values of</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\dec28119-bf44-4893-9681-836d2b67702f.png" xlink:type="simple"/></inline-formula>and<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\55db98aa-bdcc-4314-9856-29c209e1a5f9.png" xlink:type="simple"/></inline-formula>,</p><p>would determine the nature of the distribution, i.e., whether it is of a Cauchy or Gauss type. Using these criteria, a plot of</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\fb6f8cc1-89c3-45cb-8565-ae745402e357.png" xlink:type="simple"/></inline-formula>vs <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\9f45c0f5-1da8-45ac-8eab-72144a88b174.png" xlink:type="simple"/></inline-formula></p><p>for a sample of Kaolinite, to test the formula</p><disp-formula id="scirp.47789-formula3546"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\f22d82e6-5428-4b56-a098-04362e1ff5b3.png"/></disp-formula><p>yielded the value of μ, the physical parameter describing the diffraction pattern, and revealed that the distribution in this case was of a Cauchy type [<xref ref-type="bibr" rid="scirp.47789-ref6">6</xref>] . On the other hand, if the material had a Gauss distribution, a plot of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\be6e36c2-8cf8-4b03-bdee-b67e62c64364.png" xlink:type="simple"/></inline-formula> vs <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\b09927f3-96d2-41ff-8bac-ddcda0e44d0b.png" xlink:type="simple"/></inline-formula> would yield the value of μ. Hence the R(x) test can be used to distinguish between crystallites that are purely Gauss vs purely Cauchy.</p></sec><sec id="s2"><title>2. Distributions for Convolution(s) of Gauss and Cauchy Functions</title><p>In actual practice, the distribution may be neither pure Gaussian nor pure Cauchy—but a combination of both. Several options are possible—1) a sum of partly Gaussian or partly Cauchy, 2) the convolution of partly Gaussian or partly Cauchy functions, 3) or even the same proportion of Gauss and Cauchy functions. These combinations may be purely additive or purely convolutional. The convolution may be of purely Gaussian and purely Cauchy (Voigt profile) [<xref ref-type="bibr" rid="scirp.47789-ref7">7</xref>] or partly Gaussian and partly Cauchy distributions (Pseudovoigt profiles) [<xref ref-type="bibr" rid="scirp.47789-ref8">8</xref>] . Therefore, the goal of the present effort was to identify criteria to distinguish between these various combinations. Since the convolutional combinations are likely to be the most abundant, here we shall concentrate on these criteria.</p><sec id="s2_1"><title>2.1. Voigt Functions</title><p>Convolution of two functions is by definition the inverse Fourier Transform of the product of the Fourier Transforms of the two functions i.e.</p><disp-formula id="scirp.47789-formula3547"><label>(5)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\cd7391d6-765c-4e90-9a98-954150861255.png"/></disp-formula><p>where F<sub>g</sub> is of the Fourier Transform of the function g and F<sub>c</sub> is the Fourier Transform of the function c (F<sup>−1</sup> is the inverse Fourier Transform of the product).</p><p>The Fourier Transform of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\e2e2d7a0-d8fc-4755-b4e1-d60ef517e4e8.png" xlink:type="simple"/></inline-formula> is <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\c2748e0a-00cc-4d6e-a54e-d4031ead851d.png" xlink:type="simple"/></inline-formula> and Fourier Transform of<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\d49420c7-e71a-4ffa-8ffc-93be3ea846f6.png" xlink:type="simple"/></inline-formula>, so the product of the Fourier Transform of the function <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\3be9884d-9f8f-4003-af2d-547a1dd77551.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\8ebd8994-477a-4ffa-aee1-d4c12a8acd44.png" xlink:type="simple"/></inline-formula> is</p><disp-formula id="scirp.47789-formula3548"><label>(6)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\1690c45b-0cf7-40b0-be18-14aa371b12f4.png"/></disp-formula><p>Since Fourier Transform carries a function in x space into t space while inverse Fourier Transform takes it back into x space,</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\e36d9bee-fc65-4e23-a305-d2a8376566d0.png" xlink:type="simple"/></inline-formula>, using <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\a74a26c1-b270-4ca3-b64f-23b711a2e1fc.png" xlink:type="simple"/></inline-formula></p><p>Thus for convolutions representing the Voigt function:</p><disp-formula id="scirp.47789-formula3549"><label>(7)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\44344f4f-7013-4ce1-a541-5de1503376b1.png"/></disp-formula></sec><sec id="s2_2"><title>2.2. Pseudovoigt Functions</title><p>Pseudovoigt functions may be additive like η Cauchy + (1 − η) Gauss or of convolution type like</p><disp-formula id="scirp.47789-formula3550"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\b3821a3d-1704-4d92-b225-d7c56fa9aed5.png"/></disp-formula><p>where η is called the mixing fraction, and can be used to denote the proportion of intensity of the Cauchy type.</p></sec></sec><sec id="s3"><title>3. Fourier Transform of Integral Width Explaining Why Particle Size and Strain Affect Diffraction Line Profile</title><sec id="s3_1"><title>3.1. Integral Width to Express Intensity Distribution in a Diffraction Profile</title><p>Although peak position, peak height, half intensity width etc. have been used to describe an intensity distribution in a diffraction profile, the first satisfactory parameter has been the integral width <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\51ce1600-af65-4279-99ca-8c161a3d9121.png" xlink:type="simple"/></inline-formula> where I(θ) is the intensity diffracted in the direction θ. For Voigt function the integral width will be</p><disp-formula id="scirp.47789-formula3551"><label>(7a)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\24f713d6-5ebb-494d-974b-db575f4e2645.png"/></disp-formula><p>and for the Pseudovoigt function of the additive type, this can be described in terms of</p><disp-formula id="scirp.47789-formula3552"><label>(7b)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\b721e584-f501-4585-a801-5dbc41b5ffd6.png"/></disp-formula><p>Whereas for the Pseudovoigt function of the convolution type,</p><disp-formula id="scirp.47789-formula3553"><label>(7c)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\f0883e2f-ad00-406e-905f-b47a8678e6bd.png"/></disp-formula><p>Langford introduced the Voigt function through the integral width [<xref ref-type="bibr" rid="scirp.47789-ref7">7</xref>] . Instead of considering the convolution of the Gauss and Cauchy functions he used the convolution of the expressions of integral width as functions of Gauss and Cauchy types—</p><disp-formula id="scirp.47789-formula3554"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\49b2584e-1616-46e0-9307-02fd33dd15bf.png"/></disp-formula><p>Fourier Transform of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\e12ae814-8cce-49d2-8d78-e911ec193537.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\38c5f622-3fcd-472c-b45c-da8cf26d8f6b.png" xlink:type="simple"/></inline-formula> are given by</p><disp-formula id="scirp.47789-formula3555"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\5fc22e41-437c-431a-9e21-629b4a364b2d.png"/></disp-formula><disp-formula id="scirp.47789-formula3556"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\5fc22e41-437c-431a-9e21-629b4a364b2d.png"/></disp-formula><disp-formula id="scirp.47789-formula3557"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\5fc22e41-437c-431a-9e21-629b4a364b2d.png"/></disp-formula><p>Thus</p><disp-formula id="scirp.47789-formula3558"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\28d99b6b-b0dc-4348-8705-3564698175ac.png"/></disp-formula><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\b9545394-1117-4053-8964-cb46d7cb8d0c.png" xlink:type="simple"/></inline-formula>is a complex error function defined by <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\e5d61883-35d3-41a3-a523-865a3f56b602.png" xlink:type="simple"/></inline-formula></p><p>then <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\a64f9b14-c85d-42e4-87b8-1f71c24c5a23.png" xlink:type="simple"/></inline-formula></p><p>Integral width <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\952329ac-aeb7-41bb-9590-645f985f47b2.png" xlink:type="simple"/></inline-formula></p><p>Ida [<xref ref-type="bibr" rid="scirp.47789-ref9">9</xref>] expressed the convolution in the form</p><disp-formula id="scirp.47789-formula3559"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\c24422d5-c515-4bfd-ac55-43858ee55c35.png"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\c051271a-7953-44ab-b221-d6043a5a61cf.png" xlink:type="simple"/></inline-formula> is a scaled complex error function called the Faddeva Function.</p></sec><sec id="s3_2"><title>3.2. Fourier Transform of Diffraction Profile Based on Integral Width</title><p>As mentioned in Section 2 above, Fourier Transform of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\8b175cdc-7e12-4361-809b-bd7272b35f51.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\722e6d1e-7fc2-4d5e-b976-b88497365afd.png" xlink:type="simple"/></inline-formula> are <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\b04388f4-3142-4d41-89d8-0f0268e370f4.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\7b7b1d0c-9ae3-46f0-a4fe-a865c1884299.png" xlink:type="simple"/></inline-formula> respectively.</p><p>For Voigt function the Fourier Transform is<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\fb2cc5c8-3cfb-4945-bd7e-9d00c3c2183b.png" xlink:type="simple"/></inline-formula>.</p><p>While the Fourier Transform for Pseudovoigt function of additive type is</p><disp-formula id="scirp.47789-formula3560"><label>(7d)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\72f000c8-e500-43dd-bd41-473dd1c94724.png"/></disp-formula></sec><sec id="s3_3"><title>3.3. Moments of Diffraction Profiles Broadened by Particle Size and Strain</title><p>Intensity of X-ray diffracted in the direction<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\da62910d-f301-4e9d-a440-db01a766c32d.png" xlink:type="simple"/></inline-formula>, where θ is the angle of scattering and λ is the wave length of the radiation scattered, is given by</p><disp-formula id="scirp.47789-formula3561"><label>(8)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\4f2ad785-c077-4f80-8b7b-e4ba1b95b507.png"/></disp-formula><p>where τ is the limit where A(t) vanishes. By inverse Fourier Transform</p><disp-formula id="scirp.47789-formula3562"><label>(9)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\8433d705-5085-447d-b00c-83913adf799e.png"/></disp-formula><p>And so, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\a6d7ff50-73ca-4f47-95c5-b95cfd412225.png" xlink:type="simple"/></inline-formula>, and</p><disp-formula id="scirp.47789-formula3563"><label>(10)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\f2f82fb0-1f7b-46fe-b526-c890dc3894f8.png"/></disp-formula><p>By differentiating Equation (8) with respect to t over and over again and then assuming t = 0, we obtain the values of<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\e8604b95-d90e-4563-b336-a986a5eea901.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\e8784a71-bf8d-4129-b571-305e292dd7c3.png" xlink:type="simple"/></inline-formula>etc.</p><p>Wilson has shown that [<xref ref-type="bibr" rid="scirp.47789-ref1">1</xref>] , the variance or the Second Moment of the diffraction profile can be given by</p><disp-formula id="scirp.47789-formula3564"><label>(11)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\7c49945b-f245-4288-ba7d-8ba777bb46df.png"/></disp-formula><p>where σ<sub>1</sub> and σ<sub>2</sub> are limits of the integral (8) instead of 0 to τ where A(t) vanishes. Very often σ<sub>1</sub> = σ<sub>2</sub>.</p><p>The author [<xref ref-type="bibr" rid="scirp.47789-ref2">2</xref>] previously showed that the Fourth Moment of the intensity expression is given by</p><disp-formula id="scirp.47789-formula3565"><label>(12)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\cca3d6f1-3aed-4e75-925d-6f9b0b852715.png"/></disp-formula><p>In Equations (11) and (12), there are other terms involving <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\6a981ab3-e9bc-422f-bcf5-f1ace2d1a385.png" xlink:type="simple"/></inline-formula> in Equation (11) and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\0a9e8be5-e0d9-4866-8a7a-324b0224440e.png" xlink:type="simple"/></inline-formula> in Equ-</p><p>ation (12). But these terms are negligible compared to the remaining terms. The size of the particle comprising the powder is given by the 0<sup>th</sup> Moment of I(s) i.e.</p><disp-formula id="scirp.47789-formula3566"><label>(13)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\a2066fa5-5051-4291-9168-4a9e72be1f4f.png"/></disp-formula><p>The Second and the Fourth Moment of the line profile yield the shape of the particles comprising the powdered sample. Of course, they and other moments yield information regarding crystal deformations due to strain, stacking faults, nature and the extent of dislocations etc. In Equations (11)-(13) we have used equations for particle size only, disregarding other factors like strain, dislocation density etc.</p><p>The author previously also showed that for a powder particle of size <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\edb5ad9c-9ea8-41cf-acf3-daa26ceb975d.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\03a213c8-d9af-468c-a308-7d77d3155c1f.png" xlink:type="simple"/></inline-formula> with interfacial angles α, β and γ and Lattice constants a, b, c, the volume common to the crystal and its ghost removed by t in the hkl direction, is given by [<xref ref-type="bibr" rid="scirp.47789-ref6">6</xref>]</p><disp-formula id="scirp.47789-formula3567"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\77c38ee2-101c-4ce0-8af8-f37bcd543eb5.png"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\59b9e11e-4aff-49a5-ba6c-5d7e17a9599a.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\a84e70ef-d627-4036-a661-a6b6d09ef15d.png" xlink:type="simple"/></inline-formula>, d is the interplanar spacing in the direction of diffraction and</p><disp-formula id="scirp.47789-formula3568"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\c162e477-14d3-4d98-a443-cfc5559d8cfa.png"/></disp-formula><p>where α, β and γ are angles between the axes</p><p>Thus <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\a1ec43eb-9a6b-4372-a7e8-28a5b2dd4927.png" xlink:type="simple"/></inline-formula></p><p>Therefore,</p><disp-formula id="scirp.47789-formula3569"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\b3d2bd98-9d17-44ff-9066-5500aec9ba8e.png"/></disp-formula><disp-formula id="scirp.47789-formula3570"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\b3d2bd98-9d17-44ff-9066-5500aec9ba8e.png"/></disp-formula><disp-formula id="scirp.47789-formula3571"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\b3d2bd98-9d17-44ff-9066-5500aec9ba8e.png"/></disp-formula><disp-formula id="scirp.47789-formula3572"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\b3d2bd98-9d17-44ff-9066-5500aec9ba8e.png"/></disp-formula><p>Hence</p><disp-formula id="scirp.47789-formula3573"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\6d00bc83-ecdf-45ad-93b7-ee1dc15b7345.png"/></disp-formula><disp-formula id="scirp.47789-formula3574"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\6d00bc83-ecdf-45ad-93b7-ee1dc15b7345.png"/></disp-formula><disp-formula id="scirp.47789-formula3575"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\6d00bc83-ecdf-45ad-93b7-ee1dc15b7345.png"/></disp-formula><p>For h00, 0k0 and 00l reflection, only one dimension of the particle will be obtained, with hk0, 0kl and h0l reflections only two dimensions will be obtained. For a cylindrical crystal, the above equations will be modified in terms of equations derived by Langford and Lou&#235;r [<xref ref-type="bibr" rid="scirp.47789-ref10">10</xref>] .</p></sec></sec><sec id="s4"><title>4. Moments of Different Distributions</title><sec id="s4_1"><title>4.1. The Gaussian Profile</title><p>It is known from Equation 509 [<xref ref-type="bibr" rid="scirp.47789-ref11">11</xref>] that</p><disp-formula id="scirp.47789-formula3576"><label>(14)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\950dda68-3220-43a9-9579-77d7a9d52464.png"/></disp-formula><p>Putting n = 1 and a = 1/2, we have the expression for the Second Moment of a Gaussian function,</p><disp-formula id="scirp.47789-formula3577"><label>(15)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\f93ee37d-bb6d-4392-88e7-7e5d283a62b9.png"/></disp-formula><p>And putting n = 2 and a = 1/2, we have the expression for the Fourth Moment of a Gaussian function</p><disp-formula id="scirp.47789-formula3578"><label>(16)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\b73d6aae-abdd-4a2e-a962-5779a3eab7f2.png"/></disp-formula><p>Equations (15) and (16) represent the Second and the Fourth Moment of a Gaussian profile. Cernansky has derived the equations [<xref ref-type="bibr" rid="scirp.47789-ref3">3</xref>]</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\9ff795a1-aff6-49bc-9430-eee62a410918.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\975798d4-0380-4ef2-8332-beaec0447c29.png" xlink:type="simple"/></inline-formula> (16a)</p><p>and</p><disp-formula id="scirp.47789-formula3579"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\f3609515-0c6f-4793-8b20-ed6c9a73d8f3.png"/></disp-formula></sec><sec id="s4_2"><title>4.2. The Cauchy Profile</title><p>For a Cauchy profile<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\e8e28cea-20c9-4150-8678-cf44ca146802.png" xlink:type="simple"/></inline-formula>, the Second Moment, using Equation 67 [<xref ref-type="bibr" rid="scirp.47789-ref11">11</xref>] , is</p><disp-formula id="scirp.47789-formula3580"><label>(17)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\82a128c6-6959-42f6-9637-3842113aab60.png"/></disp-formula><p>and the Fourth Moment, from Equation 2.147.3 [<xref ref-type="bibr" rid="scirp.47789-ref10">10</xref>] , is</p><disp-formula id="scirp.47789-formula3581"><label>(18)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\868437be-37a3-4f39-88a7-0e42c5537413.png"/></disp-formula></sec><sec id="s4_3"><title>4.3. The Voigt Profile</title><p>The Second Moment of the Voigt profile is given by</p><disp-formula id="scirp.47789-formula3582"><label>(19)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\cb113bf1-f68a-4102-a16d-6c8ca7b298bd.png"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\9a3118e0-5fbc-4961-a0b1-8f84fc59d4a8.png" xlink:type="simple"/></inline-formula> from Equation (7a)</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\aba0234f-e222-471d-9e67-4b9dd5dc5902.png" xlink:type="simple"/></inline-formula>from Equation 811 [<xref ref-type="bibr" rid="scirp.47789-ref11">11</xref>]</p><disp-formula id="scirp.47789-formula3583"><label>.</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\bc77041a-2009-4457-a535-7c925300c6e4.png"/></disp-formula><p>For large positive value of x</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\9b62b3ae-b73e-46b1-95b9-d9c03eae680a.png" xlink:type="simple"/></inline-formula>from Equation 812 [<xref ref-type="bibr" rid="scirp.47789-ref11">11</xref>] .</p><p>Similarly the Fourth Moment of the Voigt profile is given by</p><disp-formula id="scirp.47789-formula3584"><label>(20)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\88f86e3b-b4cb-4098-911d-a9667b47742e.png"/></disp-formula></sec><sec id="s4_4"><title>4.4. The Pseudovoigt Profile</title><p>For the Pseudovoigt profile of the convolution type the Second and Fourth Moment will be given by Equations</p><p>(19) and (20) multiplied by <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\abb24fc5-7e22-4890-a1d6-aaca2c2025d7.png" xlink:type="simple"/></inline-formula> and for Pseudovoigt profiles of additive type</p><p>1) Second Moment</p><disp-formula id="scirp.47789-formula3585"><label>(21)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\c6b6ec9b-0b30-4573-90b5-c2620c292d8d.png"/></disp-formula><p>2) Fourth Moment</p><disp-formula id="scirp.47789-formula3586"><label>(22)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\57adfe93-68c0-419a-9403-21c53a19dfe5.png"/></disp-formula></sec></sec><sec id="s5"><title>5. The Fourth Cumulant for the Different Distributions</title><p>Since the Second Moment and Second Cumulant are equal and we have already studied the Second Moment, we shall be examining only the Fourth Cumulant. All cumulants along with the Fourth Cumulant have the additive property namely</p><disp-formula id="scirp.47789-formula3587"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\37374081-4b81-439d-be79-c512a79ec8bd.png"/></disp-formula><p>x<sub>1</sub>, x<sub>2</sub>, x<sub>3</sub> being specific properties like size, strain, stacking fault, probability etc. The Fourth Cumulant C<sub>4</sub> is given by</p><disp-formula id="scirp.47789-formula3588"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\2d677a81-c1a7-4d78-9dd7-b2b8b67af875.png"/></disp-formula><p>where μ<sub>4</sub> and μ<sub>2</sub> are the Fourth and Second Moment respectively which have been described in this paper. The Fourth Cumulant is given as shown below.</p><sec id="s5_1"><title>5.1. For Gaussian Distribution</title><p>Fourth Cumulant <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\6c2c993e-244e-487b-a871-e794c0a7e347.png" xlink:type="simple"/></inline-formula></p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\b6065074-1888-49ae-ba94-ff5df82c837b.png" xlink:type="simple"/></inline-formula>by Equation (16)</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\9b3dcfa9-5498-4f12-ab86-2a5323609000.png" xlink:type="simple"/></inline-formula>by Equation (15)</p><disp-formula id="scirp.47789-formula3589"><label>(23)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\ff18d8e2-a106-4c4e-b4be-91bc92767712.png"/></disp-formula><p>according to Cernansky <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\e1c8522f-086e-46d3-b735-4f33b933c74d.png" xlink:type="simple"/></inline-formula> [<xref ref-type="bibr" rid="scirp.47789-ref3">3</xref>] . Indeed, Equations (22) and (23) indicate that it is a very small quantity.</p></sec><sec id="s5_2"><title>5.2. For Cauchy Distribution</title><p>By Equation (18) <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\3c087b90-587c-4318-9aa9-1322d271f755.png" xlink:type="simple"/></inline-formula></p><p>By Equation (17) <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\f8cce54a-8ca9-472a-8d2e-8005f5de4aca.png" xlink:type="simple"/></inline-formula></p><p>Thus</p><disp-formula id="scirp.47789-formula3590"><label>(24)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\bb394cd3-bf82-4b14-8b91-ae2c35acc6cd.png"/></disp-formula></sec><sec id="s5_3"><title>5.3. For Voigt Distribution</title><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\518477b9-6972-481c-ab21-5fba49f0735a.png" xlink:type="simple"/></inline-formula>from Equations (19) and (20).</p></sec><sec id="s5_4"><title>5.4. For Pseudovoigt Distributions</title><p>The Fourth Cumulant can be found similarly from Equations (21) and (22). Now, to distinguish between Voigt and Pseudovoigt functions, an additional parameter, the coefficient of excess, is introduced here. It is the ratio of the Fourth Moment and three times the square of the Second Moment [<xref ref-type="bibr" rid="scirp.47789-ref12">12</xref>] . According to Cernansky for a Gaussian system the ratio is 1 [<xref ref-type="bibr" rid="scirp.47789-ref3">3</xref>] . The above calculations show that for the Cauchy system, the ratio is</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\ade41a40-4ec4-4aee-b69b-95aecb4fa70f.png" xlink:type="simple"/></inline-formula>from Equations (18) and (17) respectively.</p><p>Hence this study proposes that Equations (19) and (21) may be used for identifying Voigt and Pseudovoigt distributions, respectively.</p></sec><sec id="s5_5"><title>5.5. The χ Test</title><p>Pearson and Hartley [<xref ref-type="bibr" rid="scirp.47789-ref13">13</xref>] have described the χ test for determining the nature of the lineprofile. Here  <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\667506bb-f477-458d-b7eb-93ad461d4b62.png" xlink:type="simple"/></inline-formula> for Gaussian function and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\eafd5cc7-39f7-4d2c-9f87-f2038f76544f.png" xlink:type="simple"/></inline-formula> for Cauchy distribution.</p><p>For Voigt and Pseudovoigt distribution Equations (20) and (19), (22) and (21) should be used.</p></sec></sec><sec id="s6"><title>6. Parameters from Either a Single or a Few Lines</title><sec id="s6_1"><title>6.1. The Method of Line Breadth</title><p>That more than one parameter can be studied from one line in a Debye Scherrer pattern was noticed by Williamson &amp; Hall who assumed that particle size and strain broadenings had Cauchy like distribution [<xref ref-type="bibr" rid="scirp.47789-ref14">14</xref>] . This means that the observed breadth of a line β is the sum of breadths due to particle size and strain i.e.</p><disp-formula id="scirp.47789-formula3591"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\0eb86043-4819-44ef-b1bc-a9b739cb817c.png"/></disp-formula><p>or</p><disp-formula id="scirp.47789-formula3592"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\f050e63c-ffb9-465e-a2ea-0831e088bd39.png"/></disp-formula><p>where t is the apparent particle size and e is apparent strain, θ is the angle of scattering and λ is the wave length scattered.</p><p>Thus</p><disp-formula id="scirp.47789-formula3593"><label>(25)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\cfb734a1-665a-4418-874c-62040126fd80.png"/></disp-formula><p>Plotting <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\0a98ad2a-3021-491e-a178-a5cd131febc2.png" xlink:type="simple"/></inline-formula> vs<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\c4baa7e5-d4c5-4f83-bdb9-f3815d21fe93.png" xlink:type="simple"/></inline-formula>, one can obtain the particle size t from the intercept one from the slope of the</p><p>curve. Equation (25) is the well-known Williamson-Hall relation much used by many investigators [<xref ref-type="bibr" rid="scirp.47789-ref14">14</xref>] . Particle size and strain also can be determined by the famous Warren-Averbach method [<xref ref-type="bibr" rid="scirp.47789-ref15">15</xref>] .</p></sec><sec id="s6_2"><title>6.2. The Method of Line Profile</title><p>Warren and Averbach showed that the Fourier Transform of a line profile yield significant information regarding particle size, particle strain, probability of faulting and many other crystal defects [<xref ref-type="bibr" rid="scirp.47789-ref15">15</xref>] . They also showed that an intensity profile can be expressed as a Fourier series</p><disp-formula id="scirp.47789-formula3594"><label>(26)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\92da5077-bc8c-44ab-9d33-84ecdb09c089.png"/></disp-formula><p>where v(t) is the Fourier Transform of the particle size, (st) stands for strain. For determining particle size and strain only, Warren and Averbach has developed a simple method [<xref ref-type="bibr" rid="scirp.47789-ref15">15</xref>] . Convert hkl reflection into h<sub>1</sub>k<sub>1</sub>l<sub>1</sub>, 2h<sub>1</sub>2k<sub>1</sub>2l<sub>1</sub> etc. reflections by suitably changing axes as far as possible. Then let them be considered as 00l, 002l, 003l etc. by necessarily changing axes. Then write</p><disp-formula id="scirp.47789-formula3595"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\fc97d616-8588-4019-a61d-8470c6f90b33.png"/></disp-formula><p>Now</p><disp-formula id="scirp.47789-formula3596"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\685de294-f184-4274-8dda-d782fe1ce956.png"/></disp-formula><p>For small value of l and n, the logarithm of the measured Fourier coefficient is given by</p><disp-formula id="scirp.47789-formula3597"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\b5e6f7c1-b916-4679-ac3d-1484d5e51448.png"/></disp-formula><p>By plotting l<sub>n</sub>A<sub>(n)</sub> against l<sup>2</sup> we obtain at l = 0, the value of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\cefc6554-621d-43ad-a7d2-5c8104383941.png" xlink:type="simple"/></inline-formula> and from the slope,<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\cc6f29a5-b8b8-4734-88d6-e232419e6892.png" xlink:type="simple"/></inline-formula>. The distance l = na<sub>3</sub> is the undistorted distance a<sub>3</sub>Z<sub>n</sub>.</p><p>In general, Equation (26) can be written in a summation form</p><disp-formula id="scirp.47789-formula3598"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\61a71ee4-2fc4-47e9-a6f4-4e33aa24c5a1.png"/></disp-formula><p>where<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\39e96e51-33b3-4d0a-b269-0f98fc8a12cd.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\a33f6c22-7c87-4a05-9529-1df9e48fd5a0.png" xlink:type="simple"/></inline-formula>is the coefficient for particle size broadening, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\762764c3-ab50-4db0-a6e8-c5a1340c9eb6.png" xlink:type="simple"/></inline-formula>for strain. Warren and Warekois [<xref ref-type="bibr" rid="scirp.47789-ref16">16</xref>] showed that this causes a shift in peak position in 70.50 α brass and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\9fd71c0d-3e12-4394-8266-acc88e6bcfb1.png" xlink:type="simple"/></inline-formula> radiation.</p><disp-formula id="scirp.47789-formula3599"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\6db39b3a-2fd0-4ed0-a802-c9a3ddd78335.png"/></disp-formula><p>where p is the stalking fault probability. Also</p><disp-formula id="scirp.47789-formula3600"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\9794f93f-c5bf-42f8-8ac3-77b40f302d02.png"/></disp-formula><p>And</p><disp-formula id="scirp.47789-formula3601"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\bdeab1d2-de66-4979-9fdc-044cfac6c3b8.png"/></disp-formula><p>where γ is the twin fault probability, and a is the lattice constant.</p></sec></sec><sec id="s7"><title>7. Conclusion</title><p>The application of the above formulae depends on the recognition of the proper mathematical model. To achieve this, the best way is the <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\786f94cf-76c3-4812-a24d-618030bb2a56.png" xlink:type="simple"/></inline-formula> test devised by Mitra [<xref ref-type="bibr" rid="scirp.47789-ref5">5</xref>] to distinguish between Gauss and Cauchy profiles (described in [<xref ref-type="bibr" rid="scirp.47789-ref13">13</xref>] ). Plot of intensity vs the angle of curve will yield considerable information. For each peak—non- overlapped by neighboring peaks, the corresponding intensity vs angle of scattering curve should be examined to determine if it belongs to Gaussian, Cauchy, Voigt and Pseudovoigt type and if so, the mixing parameter can</p><p>be obtained by comparing with<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\c017a238-9532-45dc-9692-f0145ac94b9f.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\c9c8d13a-cb2f-44ea-8b40-585b9222a35b.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\b176c5db-7d03-42db-953c-9647ac4846ab.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\0c55b220-ffae-44df-a0a9-6639462a26ad.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\67afdb98-440b-4333-a145-00ae63adcbd0.png" xlink:type="simple"/></inline-formula>and</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\a15f8bd7-4700-4010-9a5a-3b1887c73bae.png" xlink:type="simple"/></inline-formula>respectively. There is a likelihood of confusion between Gaussian, Voigt and Pseudo-</p><p>voigt of convolution type. This can probably be resolved by examining additional peaks. Similarly, determining particle sizes by trying the relevant formulae may be helpful. The advantage of this procedure is that overlapping of lines will not interfere with the determination of the parameters. It is important to note that the Fourth Cumulant is an important parameter—since it is the only parameter which can decompose the observed line profile into profiles for different reasons of line shape. By a reverse analysis of the shape of the diffraction profile, it should be possible to identify the nature of the line profile—Gauss, Cauchy, Voigt, Pseudovoigt and hence, of the mixing parameter. From these—it should be possible to determine the parameters of line broadening. It is expected to be a good test for pattern decomposition. In this connection, another test—the χ test due to Pearson and</p><p>Hartley may be mentioned [<xref ref-type="bibr" rid="scirp.47789-ref13">13</xref>] .<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\3-1010119x\91f3025f-505d-400f-bb6c-b319cc6bcc27.png" xlink:type="simple"/></inline-formula>, and this can be calculated for the Gauss, Cauchy, Voigt and Pseudo-</p><p>voigt functions using Formulae (15), (17) and (18). Pearson and Hartley have given numerical values to identify Pearson type IV and Pearson type VII curves as well [<xref ref-type="bibr" rid="scirp.47789-ref13">13</xref>] .</p></sec><sec id="s8"><title>Acknowledgements</title><p>Sincere and heartfelt thanks are due to Dr. Paramita M Ghosh of the University of California at Davis, California, USA for encouragement and helping in many ways and to Mr. Bishwajit Halder for secretarial help. 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