<?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.2013.44085</article-id><article-id pub-id-type="publisher-id">AM-30367</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>
 
 
  Some One Parameter Models for Continuous Random Variables Defined on the Interval [0, 1]
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>ohn</surname><given-names>J. Wiorkowski</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>The University of Texas at Dallas, Richardson, USA</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>wiorkow@utdallas.edu</email></corresp></author-notes><pub-date pub-type="epub"><day>16</day><month>04</month><year>2013</year></pub-date><volume>04</volume><issue>04</issue><fpage>604</fpage><lpage>613</lpage><history><date date-type="received"><day>January</day>	<month>9,</month>	<year>2013</year></date><date date-type="rev-recd"><day>February</day>	<month>14,</month>	<year>2013</year>	</date><date date-type="accepted"><day>February</day>	<month>21,</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>
 
 
   The Beta Distribution is almost exclusively used for situations, after range normalization, wherein a continuous random variable is defined on the closed range [0, 1]. Since the beta distribution is intrinsically a two parameter distribution, this creates problems in some applications where specification of more than one parameter is difficult. In this note, two new classes of single parameter continuous probability distributions on a closed interval are introduced. These distributions remove some of the theoretical and practical problems of using the Beta Distribution for applications. The Burr Type XI Distribution has desirable characteristics for many applications especially when there is ambiguity in the definition of the specified parameter. 
 
</p></abstract><kwd-group><kwd>Probability Distribution; Risk Assessment; Reliability Assessment; PERT CPM</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>The standard two parameter Beta Distribution is the most widely used distribution for situations wherein a continuous random variable is confined to a bounded interval<img src="4-7401339\0a7ed4e3-826c-4824-8a1e-725bffd35791.jpg" />. After appropriate normalization to the interval<img src="4-7401339\d42a215e-f95d-406f-8a1b-178670edc7a9.jpg" />, the Beta Distribution provides a flexible family of probability density functions capable of modeling a wide variety of natural phenomena. There are situations, however, where the Beta Distribution cannot model natural phenomena or its use is problematic. In their recent book, Kotz and van Dorp [<xref ref-type="bibr" rid="scirp.30367-ref1">1</xref>] introduce and discuss the properties of other continuous families of distributions with bounded support. This widely extends the types of natural phenomena which can be modeled. But even this wide array of probability distributions have problems when modeling a low risk event. Consider the problem of providing a distribution for the situation where a subject matter expert subjectively estimates that the probability of a risky event as 0.01. Since the Beta Distribution is a two parameter model, this single estimate is inadequate for determining an appropriate Beta Distribution model. Except for the Triangular Distribution, all the alternative models in Kotz and van Dorp [<xref ref-type="bibr" rid="scirp.30367-ref1">1</xref>] are also at least two parameter models and thus indeterminate based on a single estimate of the risk probability. A substantial literature exists to aid the statistician in eliciting further information from subject matter experts to remove this indeterminacy (see O’Hagan et al. [<xref ref-type="bibr" rid="scirp.30367-ref2">2</xref>] for a review of the area). These techniques involve specifying a numerical estimate for another characteristic of the distribution such as the mean or a percentile. Taking the initial estimate as the mode and the estimate of some other distribution characteristic, allows a two parameter model to be fit (See Donaldson [<xref ref-type="bibr" rid="scirp.30367-ref3">3</xref>], Johnson [<xref ref-type="bibr" rid="scirp.30367-ref4">4</xref>], Lau, A. et al. [<xref ref-type="bibr" rid="scirp.30367-ref5">5</xref>], Lau H. et al. [<xref ref-type="bibr" rid="scirp.30367-ref6">6</xref>], Mohan et al. [<xref ref-type="bibr" rid="scirp.30367-ref7">7</xref>] and Premachandra [<xref ref-type="bibr" rid="scirp.30367-ref8">8</xref>]. Another example involves the management of large scale complex projects. A common methodology used in this situation is called PERT-CPM (Program and Evaluation and Review Technique-Critical Path Method). This technique has been used for the development of the Polaris Missile System and also for planning and managing the hosting activities of the International Olympics. In this approach the large project is broken down into a myriad of component parallel or sequential activities, each of which are uncertain in duration. Experts are asked to provide estimates of durations of these components. But as stated by Fazar [<xref ref-type="bibr" rid="scirp.30367-ref9">9</xref>] “PERT quantifies knowledge about the uncertainties involved in developmental programs requiring effort at the edge of, or beyond, current knowledge of the subject—effort for which little or no previous experience exists”. In discussion with individuals involved in either of these two situations, I have found that although they are comfortable in providing a subjective “most likely” estimate of an event, most would have difficulty specifying any other characteristic of the distribution. Indeed many seem to hold that their subjective estimate is not only the most likely, (corresponding to the mode of the distribution) but simultaneously would be willing to give even odds that the actual probability is above or below their estimate (corresponding to the median). This ambiguity has also been reported by Trout [<xref ref-type="bibr" rid="scirp.30367-ref10">10</xref>]. Accordingly, there is a need for one parameter probability models to handle the real situation of having only one reliable estimate from a subject matter expert and for which the mode and median are very close. Of course it is possible to create probability distributions where the mode and median exactly coincide, however, there may be circumstances where other criteria may be paramount so that general methods for creating one parameter distributions may be of value.</p></sec><sec id="s2"><title>2. Tilted Distributions</title><p>Exponential tilting is a well known method (See Davison [<xref ref-type="bibr" rid="scirp.30367-ref11">11</xref>] Section 5.2 for example) which can be used to induce a one parameter family of distributions. Let <img src="4-7401339\3c6baf6b-8937-4987-b9d0-9aa27ac81246.jpg" /> denote a probability density function on the closed interval <img src="4-7401339\a642e26e-cf30-48cf-b01d-0c6c489093b1.jpg" /> with the property that <img src="4-7401339\d9981cb9-86dc-4ea1-b6d1-3f578d77dcac.jpg" /> and such that,</p><p><img src="4-7401339\32e1e2e6-d83d-4752-a3d6-36403327a0e8.jpg" /> (1).</p><p>Define the moment generation function of <img src="4-7401339\4545c839-ccf1-489a-8ddc-4affd5fe0755.jpg" /> as,</p><disp-formula id="scirp.30367-formula98843"><label>(2)</label><graphic position="anchor" xlink:href="4-7401339\2d4167f8-5fe2-47d1-b1cf-4465af25deb6.jpg"  xlink:type="simple"/></disp-formula><p>then</p><disp-formula id="scirp.30367-formula98844"><label>(3)</label><graphic position="anchor" xlink:href="4-7401339\a1f47e33-34cd-42e1-a8ad-31bd32e19ccc.jpg"  xlink:type="simple"/></disp-formula><p>is also a probability density function on the closed interval<img src="4-7401339\17124b14-8a3f-4811-8b26-bd2c692e1fbc.jpg" />. If <img src="4-7401339\58761291-c4f7-45f5-b877-f2ecf5d40eb4.jpg" /> has no parameters, then <img src="4-7401339\69437f26-cd7e-4414-94dc-8a414119e58e.jpg" /> defines a one parameter family on <img src="4-7401339\cb2549bd-46ae-42e3-b6b9-4dd277e1ca27.jpg" /> with parameter t, where t can range over the interval <img src="4-7401339\4ee27c76-cf96-4329-bc5d-4de16dc79a8f.jpg" /> to<img src="4-7401339\506bede2-961c-484f-ad5f-82be4de30080.jpg" />. The probability density function <img src="4-7401339\28cdaf73-5051-4c70-b4ec-9c663927ba85.jpg" /> has several desirable properties. First, the moment generating function of <img src="4-7401339\728ca506-d206-4a15-87f6-a612f2087fd3.jpg" /> is given by <img src="4-7401339\c3f3ad42-ca1f-4e93-82fa-848f02fb07e4.jpg" /> so that the mean and variance of the density function are given by the equations</p><disp-formula id="scirp.30367-formula98845"><label>(4)</label><graphic position="anchor" xlink:href="4-7401339\7a64b614-17f4-43c7-857f-4535a7d1cf9d.jpg"  xlink:type="simple"/></disp-formula><p>from which explicit formulae for the mean and variance can be obtained. The function <img src="4-7401339\27431bcd-150f-44b8-9ab2-3f6c1281b700.jpg" /> is the cumulant generating function of the density<img src="4-7401339\ed54d00b-b1aa-467c-925a-2cbb24af2ec5.jpg" />. Secondly, the form of (3) implies that <img src="4-7401339\9c4febd9-d27f-4dc9-a436-1df0332889ce.jpg" /> is in the exponential family of distributions. This family of distributions has been well studied and has several desirable properties. For example, in this case, if one has a random sample from<img src="4-7401339\d4872c50-d8f9-4dcc-9036-16e71d3ab938.jpg" />, then one can obtain the maximum likelihood estimate of t by simply setting the sample mean equal to <img src="4-7401339\4e2a8166-3793-461b-9ea1-fd8672bcd6b6.jpg" /> and solving for t. The asymptotic variance of this estimate if given by<img src="4-7401339\28896481-79b4-4529-b48e-07ce9b45fd70.jpg" />. Finally, if</p><p><img src="4-7401339\764c8b9b-a1b5-4148-bce3-c221fc3b1030.jpg" />is a concave function, then t can be uniquely related to the mode, <img src="4-7401339\5ef7a0f7-4606-4568-b797-bc3711dfbce5.jpg" />, through the relationship,</p><disp-formula id="scirp.30367-formula98846"><label>(5)</label><graphic position="anchor" xlink:href="4-7401339\16660da3-a347-4fb3-924d-b2e06e6ea3cc.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="4-7401339\102a275a-87a9-4b18-998e-958cb6722ca9.jpg" /> is the first derivative of <img src="4-7401339\2996b057-5cd5-4c7b-9253-74210dcc2852.jpg" /> with respect to x, evaluated at<img src="4-7401339\868489bb-78a2-4336-805b-38ac7f7d238b.jpg" />. This means that one can specify a distribution by specifying the mode<img src="4-7401339\9a229f78-913e-45cd-87ab-ca9c26c67d0e.jpg" />, use (5) to find t, and then use (4) to determine the basic statistical properties of the distribution.</p><p>The choice of <img src="4-7401339\52fe3088-fdaa-4409-a5b6-b4b247fff13c.jpg" /> is extremely broad, but as pointed out by one of the referees, it is best to start with <img src="4-7401339\fc94b0e7-47b6-4573-9080-3b6c1e1cd374.jpg" /> which is symmetric about the point <img src="4-7401339\4c55881a-e9f2-43e0-8da5-3b6564ab75de.jpg" /> to guarantee that any modal value between 0 and 1 can be modeled As examples of the above, consider three simple choices for <img src="4-7401339\67036287-330a-4af0-ac02-86688033919e.jpg" /> on the closed interval<img src="4-7401339\8454206e-fe9f-4ef6-b0fd-0a61db28cca7.jpg" />. The first is the Beta (2, 2) distribution with probability density function,</p><disp-formula id="scirp.30367-formula98847"><label>(6)</label><graphic position="anchor" xlink:href="4-7401339\2d71c0fd-37b2-4f07-a5d9-b066052f921e.jpg"  xlink:type="simple"/></disp-formula><p>The second is the Gilbert distribution (Edwards [<xref ref-type="bibr" rid="scirp.30367-ref12">12</xref>]) with probability density function,</p><disp-formula id="scirp.30367-formula98848"><label>(7)</label><graphic position="anchor" xlink:href="4-7401339\c7d4ea07-5bb7-4b83-9122-6379dc70c0b1.jpg"  xlink:type="simple"/></disp-formula><p>The third is a translated version of the Raised Cosine distribution (Proakis [<xref ref-type="bibr" rid="scirp.30367-ref13">13</xref>], p. 189), and is also a special case of the Burr Type XI distribution (Burr [<xref ref-type="bibr" rid="scirp.30367-ref14">14</xref>] and Kotz and Johnson [<xref ref-type="bibr" rid="scirp.30367-ref15">15</xref>], p. 335). It has probability density function,</p><disp-formula id="scirp.30367-formula98849"><label>(8)</label><graphic position="anchor" xlink:href="4-7401339\3353ef3b-f145-41af-a853-fbf919bb6f80.jpg"  xlink:type="simple"/></disp-formula><p>These probability density functions are shown in <xref ref-type="fig" rid="fig1">Figure 1</xref>. As can be seen, the Beta (2, 2) and Gilbert densities are quite close to one another. Further, the Burr density differs distinctly from the other two being much more concentrated around the value 0.5, and showing much greater tapering as x approaches 0 or 1. (As pointed out by the referee, in some applications one might prefer to start with symmetric beta distributions but the above three choices illustrate the distribution construction approach adequately.)</p><p><xref ref-type="fig" rid="fig2">Figure 2</xref> shows the three tilted distributions with a mode, <img src="4-7401339\f2918663-c76a-4c1e-9b04-5e7a02a176e7.jpg" />, of 0.01. The values of t corresponding to a mode of 0.01 are –98.9898 for the tilted beta, –99.9671 for the tilted Gilbert, and –199.9342 for the tilted Burr distribution.</p><p>As can seen, the tilted Beta and Gilbert densities are</p><p>almost indistinguishable and quite distinct from the tilted Burr density. This similarity between the tilted Gilbert and tilted Beta distributions seems to be typical for both low and high values of the mode<img src="4-7401339\f448205a-4e23-4dc3-b0e7-068244fd3022.jpg" />.</p><p>The skewness of the distributions might be viewed as a desirable characteristic if one believed that experts tend to underestimate the probability of rare events. (In a reliability situation with a mode say of 0.99, the tilted densities would be left skewed and model a situation wherein experts tend to overestimate the reliability.)</p><p><xref ref-type="fig" rid="fig3">Figure 3</xref> shows the relationship between <img src="4-7401339\a36e8116-83cb-400a-a0bb-5602be615cfb.jpg" /> and <img src="4-7401339\6f82e614-9995-4102-bb65-ebaefbc538c5.jpg" /> for the three tilted distributions. The closer <img src="4-7401339\8b424e3e-c51d-4210-a0f3-cf485031e50e.jpg" />is to 0.5, the closer the median and mode of the distributions are (Berny [<xref ref-type="bibr" rid="scirp.30367-ref16">16</xref>] uses one minus this probability as a parameter in his model).</p><p>Again, there is almost no difference between the tilted Beta and tilted Gilbert distributions over the whole range of the mode<img src="4-7401339\dc7f421f-3c08-4fd7-8836-a20765da5581.jpg" />. Further the probabilities of being less than the mode for the tilted Burr distribution are uniformly closer to 0.5 than the other two distributions. However, the deviation from 0.5 is large even for the tilted Burr distribution. Accordingly, if one agreed with Trout [<xref ref-type="bibr" rid="scirp.30367-ref10">10</xref>], none of these distributions would provide Adequate models for modeling expert assessment of</p><p>probabilities since the modes and medians do not seem close.</p></sec><sec id="s3"><title>3. MAX Distributions</title><p>Let <img src="4-7401339\a066891c-62ee-4124-aad2-e12c17268edb.jpg" /> be the cumulative probability distribution function corresponding to the probability density function <img src="4-7401339\79687b8e-8de2-4acb-b65b-3dca9973f877.jpg" /> on<img src="4-7401339\6068fc99-5b5d-4631-8000-f74efb11946a.jpg" />, i.e.</p><disp-formula id="scirp.30367-formula98850"><label>(9)</label><graphic position="anchor" xlink:href="4-7401339\1a4f4b82-c175-4d69-9367-8c1c7982fd3a.jpg"  xlink:type="simple"/></disp-formula><p>Then for<img src="4-7401339\a200d3ed-c4a0-4f86-8c56-0c728f22f1e0.jpg" />, <img src="4-7401339\e184eaca-c76f-4e7e-a135-8a1748d3ddf4.jpg" />is also a cumulative probability distribution function on the range<img src="4-7401339\eefb3a3c-5c3a-4b73-9773-295b175432bf.jpg" />. Indeed, if K is an integer, n, then <img src="4-7401339\eddc1e25-508c-4fb4-be27-bc398f8bfa7b.jpg" /> is the cumulative distribution function of the maximum value of X from a random sample of size n where X has probability density function<img src="4-7401339\a9556dd5-9899-411b-8f9b-a316e214efd7.jpg" />. Define,</p><disp-formula id="scirp.30367-formula98851"><label>(10)</label><graphic position="anchor" xlink:href="4-7401339\6d03d1fb-2d99-46ef-bcba-6e126402fe7c.jpg"  xlink:type="simple"/></disp-formula><p>then <img src="4-7401339\58bfd31b-da9d-4bbd-afb6-9a4ac6e3c339.jpg" /> is a probability density function on<img src="4-7401339\122a63b3-4762-4d63-9673-28b7bf503af4.jpg" />. Further, <img src="4-7401339\a27752d2-9cf5-40d0-93a7-dfd80136d76b.jpg" />is also a probability density function, the rotated image of <img src="4-7401339\9aae2153-1024-4719-a9c7-24cf3bb3747c.jpg" /> about the fixed point<img src="4-7401339\bce9cd8a-12f7-4a22-b98e-bdf5cf4e4608.jpg" />. If <img src="4-7401339\36e8adbc-0ca4-408c-85c4-d54e08268a94.jpg" /> and <img src="4-7401339\cd193097-fc46-455e-96cd-903df0c41c35.jpg" /> are both concave, then <img src="4-7401339\a917ad92-ce63-459e-9c9e-57486fa414dc.jpg" /> has a unique mode <img src="4-7401339\3886b771-07a6-4141-a12b-21064ac9634d.jpg" /> on<img src="4-7401339\354ae71a-f1b2-4353-9baf-a8debcff9159.jpg" />. Under these conditions, it is straightforward to show that the relationship between K and <img src="4-7401339\ec6fb6aa-8a75-47b7-97b7-2bffce0d2553.jpg" /> is given the by the equations,</p><disp-formula id="scirp.30367-formula98852"><label>(11)</label><graphic position="anchor" xlink:href="4-7401339\bcd607ec-b830-4ae7-bc62-6e3bfd27a4aa.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="4-7401339\2d54d515-9e60-4d9a-9958-78d0455f3a96.jpg" /> is the first derivative of <img src="4-7401339\7487395b-91f0-4108-8952-1c0946281b88.jpg" /> with respect to x. Accordingly, one can generate a probability distribution by specifying the mode<img src="4-7401339\d5720a2a-74fb-4534-819d-b9cdb201885a.jpg" />, use (11) to find K and if the mode is greater than 0.5 use (10) to find the density function. If the mode is less than 0.5, then one uses (10) with x replaced by<img src="4-7401339\87106a72-8129-4197-9d7d-ae0613661ae0.jpg" />. Percentiles x<sub>p</sub> for the density <img src="4-7401339\a5907f54-0293-4fcb-a6d8-8c7397a0fe7b.jpg" /> can easily be found by solving the equation</p><disp-formula id="scirp.30367-formula98853"><label>(12)</label><graphic position="anchor" xlink:href="4-7401339\166afd84-b6d4-45f2-998f-139430cffa5d.jpg"  xlink:type="simple"/></disp-formula><p>Unfortunately, the form of (10) does not lend itself to closed form solutions for moments.</p><p>If one has a random sample of size n from<img src="4-7401339\e65602eb-b973-4259-af54-8b4bd57f4112.jpg" />, then the maximum likelihood of K is,</p><disp-formula id="scirp.30367-formula98854"><label>(13)</label><graphic position="anchor" xlink:href="4-7401339\7f5a7048-6534-4a3f-8749-d2f512e3ae38.jpg"  xlink:type="simple"/></disp-formula><p>with asymptotic variance<img src="4-7401339\345ee09b-4612-41d7-a8d0-f770a2ec6796.jpg" />. A form of this distribution was discussed by Topp and Leone [<xref ref-type="bibr" rid="scirp.30367-ref17">17</xref>] and further discussed in Kotz and van Dorp [<xref ref-type="bibr" rid="scirp.30367-ref1">1</xref>].</p><p><xref ref-type="fig" rid="fig4">Figure 4</xref> shows the three MAX distributions for the case<img src="4-7401339\079c5d13-172f-4cd2-a63c-142481979f0d.jpg" />. The BetaMAX distribution would have K = 1667, the GilbertMAX distribution would have K = 2026.59, and the BurrMAX distribution would have K = 101321.5.</p><p>As can be seen, as in the case of the Tilted distributions, the BetaMAX and GilbertMAX densities are indistinguishable and quite distinct from the BurrMAX distribution. Both the BetaMAX and GilbertMAX distributions show right skew (they would be left skewed if<img src="4-7401339\def8daa2-abce-40fd-b7ed-e3fcfc8973c2.jpg" />) while the BurrMAX is almost symmetric. In contrast to the Tilted distributions shown in <xref ref-type="fig" rid="fig2">Figure 2</xref>, the Max distributions are much less variable with almost all the probability mass confined to the range 0 to 0.03. This is a much smaller range than the Tilted Beta and Tilted Gilbert which essentially go from 0 to 0.06. Accordingly, if one expected greater underestimation of probabilities by experts, the Tilted distributions would be preferred. However, as mentioned earlier, it may be the case that when asked to determine “most likely” values, experts are estimating the median rather than the mode.</p><p>Accordingly, in <xref ref-type="fig" rid="fig5">Figure 5</xref>, the probability of being less than the median is plotted as a function of the mode for the three Max densities discussed in this paper.</p><p><xref ref-type="fig" rid="fig5">Figure 5</xref> is plotted on the same scale as <xref ref-type="fig" rid="fig3">Figure 3</xref>. It is immediately clear, that all of the Max distributions have modes which are much closer to the median. The median and mode are remarkably close for the BurrMAX distribution, with <img src="4-7401339\0599ac04-9a5c-412d-bb1e-b10638782ff7.jpg" /> differing from 0.5 by a maximum value of 0.0281 at approximately λ = 0.28 and 0.72. Accordingly, the Max distributions seem better suited for handling the ambiguity of expert estimation of the “most likely value”. Specifically, the BurrMax distribution, for which the mode and median are extremely close over whole range of possible values, seems an useful one parameter distribution for applications wherein individuals are asked to provide “most likely values”.</p></sec><sec id="s4"><title>4. The BurrMAX or Burr Type XI Distribution</title><p>When <img src="4-7401339\db541e7a-6702-4402-a372-5e774a129111.jpg" /> is the Burr distribution, (11) can be written as</p><disp-formula id="scirp.30367-formula98855"><label>(14)</label><graphic position="anchor" xlink:href="4-7401339\859f8edf-7f95-4156-8f15-15c25371621c.jpg"  xlink:type="simple"/></disp-formula><p>With the appropriate value of K, the cumulative distribution function of the Burr Type XI distribution is given by</p><disp-formula id="scirp.30367-formula98856"><label>(15)</label><graphic position="anchor" xlink:href="4-7401339\301bfd78-c963-406d-bb89-9e941fed5317.jpg"  xlink:type="simple"/></disp-formula><p>The first equation in (15) was first given by Burr [<xref ref-type="bibr" rid="scirp.30367-ref14">14</xref>], and given the designation Type XI by Kotz and Johnson [<xref ref-type="bibr" rid="scirp.30367-ref15">15</xref>] Vol. 1, p. 335, in their discussion of the Burr Family of distributions. The probability density functions of the BurrMAX distributions are</p><disp-formula id="scirp.30367-formula98857"><label>(16)</label><graphic position="anchor" xlink:href="4-7401339\3e92578f-b3e6-49a4-9154-29c839bde3f2.jpg"  xlink:type="simple"/></disp-formula><p>Since (14) are mixed trigonometric equations, there is no closed form equation to find the mode, <img src="4-7401339\0024082f-0300-42b6-8f5c-dc6cb28799b4.jpg" />, given K .</p><p>The median, <img src="4-7401339\3cc0dd06-b5ed-4e84-85b6-1f81445ecaf0.jpg" />, or indeed any percentile x<sub>p</sub>, for<img src="4-7401339\ac6bc133-2c4f-4456-99d0-fa8940f3e654.jpg" />, can be obtained by solving the equation</p><disp-formula id="scirp.30367-formula98858"><label>(17)</label><graphic position="anchor" xlink:href="4-7401339\cbc696a0-c2db-4ce6-9116-5f9a6b1a3f3b.jpg"  xlink:type="simple"/></disp-formula><p>which, since it is a mixed trigonometric equation, has no closed form solution. Equation (17), however, can be solved using numerical procedures. If<img src="4-7401339\e090f7d2-ab06-4dab-803a-3ca887f15676.jpg" />, then to find x<sub>p</sub>, replace p with <img src="4-7401339\e1a9f32f-1d42-47dd-9e86-a1b6897669b7.jpg" /> in (54), solve, and subtract the solution from 1.</p><p>No closed form solution or general numerical solutions can be found for the mean and standard deviation of the Burr Type XI distribution. Accordingly, direct numerical integration of the integrals defining the first and second central moments was performed to obtain the resulting means and standard deviations as given in <xref ref-type="table" rid="table1">Table 1</xref>.</p></sec><sec id="s5"><title>5. Extreme Value Distribution Approximation</title><p>In risk situations where one estimates very small probabilities, or in a reliability context when one estimates probabilities very close to 1, use of a Max distribution becomes problematic as the values of K become very large. One can capitalize, however, on the fact that for K = n, an integer, all of the Max distributions can be thought of as representing the distributions of the maximum (if<img src="4-7401339\094aafa7-f400-4738-b6ad-098ac9b7a088.jpg" />) or the minimum (if<img src="4-7401339\b6d0834e-3c9a-4e00-b58f-1e301a594933.jpg" />) of n random samples taken from the appropriate distribution. Accordingly, one can use the theory of extreme values and extend the results from integer values, n, to a continuous value<img src="4-7401339\c69117e6-ed00-4003-8471-b787a6c00fbe.jpg" />.</p><p>Following the discussion in Johnson et al. [<xref ref-type="bibr" rid="scirp.30367-ref18">18</xref>] Chapter 22, the distribution of the maximum of a sample of size n, for large enough n, for the distributions discussed in this paper, converge in law to a Weibull distribution which for <img src="4-7401339\71680a01-6b25-4329-9cf3-442317ff4b97.jpg" /> has the cumulative distribution function is given by the equation</p><disp-formula id="scirp.30367-formula98859"><label>(18)</label><graphic position="anchor" xlink:href="4-7401339\1631e351-c930-4993-9ad0-b680529e750d.jpg"  xlink:type="simple"/></disp-formula><p>If the value of <img src="4-7401339\a9c072dc-aae7-4a2d-8da8-8035be0f906d.jpg" /> can be determined, then the above distribution becomes a function of <img src="4-7401339\1b8beb5e-9701-4103-80fb-f93bdc1ff0aa.jpg" /> alone and is a one parameter distribution. In Johnson et al. [<xref ref-type="bibr" rid="scirp.30367-ref18">18</xref>] Chapter 22, a method is given for finding <img src="4-7401339\4a255cee-4c96-4b04-9da7-575bf4f8746a.jpg" /> based on the cumulative distribution function <img src="4-7401339\a9e8ab05-7f2e-4cf5-aac0-0eeece19e0f9.jpg" /> of the initial generating distribution. The result is that</p><disp-formula id="scirp.30367-formula98860"><label>(19)</label><graphic position="anchor" xlink:href="4-7401339\09eb20f1-a804-44a3-a8de-93f599d635b6.jpg"  xlink:type="simple"/></disp-formula><p>For the Burr distribution, (19) yields the value <img src="4-7401339\78f33547-391b-45c8-b66b-8d0a906501ee.jpg" /> so that for <img src="4-7401339\90c0facd-9d43-44f4-9491-38b1ab412860.jpg" /> or <img src="4-7401339\5e0b1e66-0f75-41c6-ac11-8c17f5eb63d0.jpg" /> the theory of Extreme Value Distributions indicates that the Burr Type</p><p><xref ref-type="table" rid="table1">Table 1</xref>. Characteristics of the Burr Type XI Distribution.</p><p><img src="4-7401339\2cb8f2a1-a39e-4cda-8eb6-5331da508e41.jpg" /></p><p>XI distribution can be closely approximated to nine decimal places by a Weibull extreme value distribution on the range<img src="4-7401339\84018b76-5f78-4793-bb25-3b45236ec5dd.jpg" />. Specifically, the cumulative distribution function is given by</p><disp-formula id="scirp.30367-formula98861"><label>(20)</label><graphic position="anchor" xlink:href="4-7401339\d46bbee2-445b-4825-b78b-21e6527de8e5.jpg"  xlink:type="simple"/></disp-formula><p>with corresponding probability density functions,</p><disp-formula id="scirp.30367-formula98862"><label>(21)</label><graphic position="anchor" xlink:href="4-7401339\82cf113b-7a8c-4d46-8b1f-67b2349af579.jpg"  xlink:type="simple"/></disp-formula><p>If<img src="4-7401339\0d8b1e8d-f136-458c-85f8-720ed29734ed.jpg" />, we have from the properties of the Weibull distribution [Johnson et al. [<xref ref-type="bibr" rid="scirp.30367-ref19">19</xref>] Chapter 21], that</p><disp-formula id="scirp.30367-formula98863"><label>(22)</label><graphic position="anchor" xlink:href="4-7401339\a82874b8-1aac-4cd7-b852-3064f2628056.jpg"  xlink:type="simple"/></disp-formula><p>For<img src="4-7401339\fe2e88d0-22ec-4653-9924-c284d4430a70.jpg" />, the corresponding results are,</p><disp-formula id="scirp.30367-formula98864"><label>(23)</label><graphic position="anchor" xlink:href="4-7401339\54904c34-7ed9-4083-925f-864e01d1b7a6.jpg"  xlink:type="simple"/></disp-formula><p>For the BetaMAX and GilbetMAX distributions, (19) indicates that <img src="4-7401339\cbb8cbdc-dc8d-497a-8efe-d2dc1ea30c45.jpg" /> so that for λ ≤ 0.1473 or λ ≥ 0.8527 both distributions can be closely approximated to nine decimal places by a Weibull extreme value distribution on the range <img src="4-7401339\3f920ea9-8e3b-4dee-b297-e2881031ee6f.jpg" /> which coincides with a form of the Rayleigh distribution Johnson et al. (1995), Chapter 18, Section [<xref ref-type="bibr" rid="scirp.30367-ref10">10</xref>].</p><p><xref ref-type="fig" rid="fig6">Figure 6</xref> shows the Extreme value distributions for<img src="4-7401339\93f0bcd6-b089-4d2c-85e2-ec668372c6d6.jpg" />. As expected it’s appearance is similar to that of <xref ref-type="fig" rid="fig4">Figure 4</xref>. The distribution for <img src="4-7401339\f52dfbdb-80d5-4b9f-8bde-35733b234c95.jpg" /> (limiting value of the Burr Type XI distribution) has expected value of 0.0102, a median of 0.0101, and a standard deviation of 0.0037. When <img src="4-7401339\cd056391-2668-40ac-b97a-141c0ba4b274.jpg" /> (limiting form of the GilbertMax and BetaMax distributions) the corresponding values are 0.0125, 0.0118, and 0.0066.</p></sec><sec id="s6"><title>6. Applications</title><p>It is clear from the previous discussion that the Gilbert distribution and Beta (2, 2) distributions yield Tilted, MAX and Extreme Value distributions which are essentially numerically indistinguishable. Accordingly, I see no applications for any form of the Gilbert distribution. In risk or reliability studies, where <img src="4-7401339\19880ab1-c982-471e-bc0c-af1fc88bd639.jpg" /> would be expected to be close to 0 or close to 1 respectively, the Extreme value distributions would seem to be most useful. They have a relatively simple form and one can obtain good approximations to their moments using (20) and (21). Further one can obtain percentiles of the extreme value distributions using the formulas,</p><disp-formula id="scirp.30367-formula98865"><label>(24)</label><graphic position="anchor" xlink:href="4-7401339\dabb16df-fa92-40c2-9a59-49474b9a9be0.jpg"  xlink:type="simple"/></disp-formula><p>By replacing p or 1 − p in (24) with a uniformly distributed random variable U, one can easily simulate samples of any size from these distributions. The choice of whether to use <img src="4-7401339\b9c05346-580c-4764-a54e-32ac0d0f2183.jpg" /> hinges on whether one believes that experts are truly estimating the mode and not the median. If they are, then choosing <img src="4-7401339\2116ceb0-7a57-4b47-be35-65e2826a4c48.jpg" /> would seem to be preferred since it allows for expert under estimation of probabilities in the case of risk applications, or over estimation of probabilities in reliability applications. On the other hand, if there is ambiguity as to whether experts are estimating the mode or median when asked for the “most likely value”, then using the Extreme Value distribution with <img src="4-7401339\0d6b37d8-cbba-4e28-b67d-8688ca2626cc.jpg" /> would seem most appropriate since for this distribution the median and mode are almost identical.</p><p>In PERT or stochastic CPM applications where <img src="4-7401339\e9104130-4b01-410c-be2e-82c069aecea5.jpg" /> would not be expected to be either very small or very large, the Extreme Value distributions would not be appropriate. Typically either the Triangle distribution with mode <img src="4-7401339\d4bba711-0415-45b7-bfd4-60df3542f096.jpg" /> or the Beta distribution with mean <img src="4-7401339\3d67a202-a822-4660-8508-8f7a819fe532.jpg" /> and standard deviation of <img src="4-7401339\8928dc4c-7602-4287-8aa5-7eccbc7bcfdc.jpg" /> have been used in this situation. The standard deviations of these two distributions as well as the BetaMax and Burr Type XI distributions are shown in <xref ref-type="fig" rid="fig7">Figure 7</xref>. Unlike the usual Beta approximation or Triangular distribution cases, the two Max distributions show the variability declining as the mode approaches 0 or 1.</p><p>It seems clear that the BetaMax and Burr Type XI distributions are better than both the usual Beta approximation model and Triangular distribution since for these</p><p>two distributions the variability is substantially lower as one moves away from the middle of the modal range. If one was worried about the ambiguity of the term “most likely value”, then one would use the Burr Type XI distribution instead of the Usual PERT model based on <xref ref-type="fig" rid="fig5">Figure 5</xref> which shows the closeness of the median and mode of the Burr Type XI distribution. If this was not a concern then the choice would depend on one’s conception of variability. However, if one wanted to keep variability at a reasonable level, again one is led to the Burr Type XI distribution with a standard deviation which is between 0.36 and 0.39 the value of the mode (when the mode is below 0.5).</p><p>Perhaps the most useful application of these one parameter distributions is to allow experts with limited backgrounds in probability to more accurately specify their uncertainties about the situations they are working with. For example consider the problem of estimating the chances of a failure in a power system. The expert needs only to come up with one estimate, say 0.001, and the distributions discussed in this paper would automatically generate a plausible distribution for the uncertainty in this figure. Given that many risk assessment studies and complicated projects consist of hundreds to thousands of uncertain steps, the reduction in difficulty by using one parameter families should greatly ease the problem of assigning reasonable uncertainty to the myriad steps.</p></sec><sec id="s7"><title>REFERENCES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.30367-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">S. Kotz and J. R. van Dorp, “Beyond Beta, Other Continuous Families of Distributions with Bounded Support and Applications,” World Scientific Publishing Co., Singapore City, 2004.</mixed-citation></ref><ref id="scirp.30367-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">A. O’Hagan, C. Buck, A. Daneshkhah, J. Eiser, P. Garth waite, D. Jenkinson, J. Oakley and T. Rakow, “Uncertain Judgements, Eliciting Experts’ Probabilities,” John Wiley and Sons, Ltd., Chichester, 2006.  
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