<?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">OJOp</journal-id><journal-title-group><journal-title>Open Journal of Optimization</journal-title></journal-title-group><issn pub-type="epub">2325-7105</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/ojop.2013.21001</article-id><article-id pub-id-type="publisher-id">OJOp-29423</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Computer Science&amp;Communications</subject><subject> Engineering</subject><subject> Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  An Epsilon Half Normal Slash Distribution and Its Applications to Nonnegative Measurements
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>enhao</surname><given-names>Gui</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Pei-Hua</surname><given-names>Chen</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Haiyan</surname><given-names>Wu</given-names></name><xref ref-type="aff" rid="aff3"><sup>3</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff2"><addr-line>Department of Management Science, National Chiao Tung University, HsinChu, Chinese Taipei</addr-line></aff><aff id="aff3"><addr-line>Department of EPLS, Florida State University, Tallahassee, USA</addr-line></aff><aff id="aff1"><addr-line>Department of Mathematics and Statistics, University of Minnesota Duluth, Duluth, USA</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>wgui@d.umn.edu(EG)</email>;<email>paulachen@g2.nctu.edu.tw(PC)</email>;<email>hw07d@fsu.edu(HW)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>29</day><month>03</month><year>2013</year></pub-date><volume>02</volume><issue>01</issue><fpage>1</fpage><lpage>8</lpage><history><date date-type="received"><day>January</day>	<month>5,</month>	<year>2013</year></date><date date-type="rev-recd"><day>February</day>	<month>4,</month>	<year>2013</year>	</date><date date-type="accepted"><day>February</day>	<month>28,</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>
 
 
   We introduce a new class of the slash distribution using the epsilon half normal distribution. The newly defined model extends the slashed half normal distribution and has more kurtosis than the ordinary half normal distribution. We study the characterization and properties including moments and some measures based on moments of this distribution. A simulation is conducted to investigate asymptotically the bias properties of the estimators for the parameters. We illustrate its use on a real data set by using maximum likelihood estimation. 
 
</p></abstract><kwd-group><kwd>Epsilon Half Normal Distribution; Slash Distribution; Kurtosis; Skewness; Maximum Likelihood Estimation</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>The epsilon half normal distribution, proposed by Castro et al. [<xref ref-type="bibr" rid="scirp.29423-ref1">1</xref>], is widely used for nonnegative data modeling, for instance, to consider the lifetime process under fatigue. We say that a random variable <img src="1-2730003\9b4c9224-703d-4348-9f98-2dd2039956e3.jpg" /> has an epsilon half normal distribution with parameters <img src="1-2730003\5184694b-2007-459c-bcf8-fc561b937095.jpg" /> and<img src="1-2730003\46d8e91c-405f-4eda-b107-6fa3b49f3b3b.jpg" />, denoted by<img src="1-2730003\ccab543f-ce6a-4c74-8287-7caf4aa12db2.jpg" />, if its density function is given by, for<img src="1-2730003\ca8d4d79-6359-4898-a8b2-ca78568976c0.jpg" />,</p><disp-formula id="scirp.29423-formula5218"><label>(1)</label><graphic position="anchor" xlink:href="1-2730003\df5d22c6-a567-430c-8cfc-a947f9db33b2.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="1-2730003\866d232b-aede-49af-84f4-b3ab42eab1f0.jpg" /> denotes the standard normal density function. When<img src="1-2730003\0b5c05e4-f294-47b1-97ce-e5d77132c5a9.jpg" />, the epsilon half normal distribution reduces to the half normal distribution investigated in [2-4].</p><p>Castro et al. [<xref ref-type="bibr" rid="scirp.29423-ref1">1</xref>] provided mathematical properties of the epsilon half normal distribution and discussed some inferential aspects related to the maximum likelihood estimation.</p><p>On the other hand, a random variable <img src="1-2730003\a20a1240-8694-4b68-be34-8f3c9cbf4822.jpg" /> has a standard slash distribution <img src="1-2730003\8154ef0b-5fae-48cb-97f1-e977ec980900.jpg" /> with parameter<img src="1-2730003\88ca3a50-28cc-4f38-8d81-9678b2312fdc.jpg" />, introduced in [<xref ref-type="bibr" rid="scirp.29423-ref5">5</xref>], if <img src="1-2730003\9e069255-6137-4087-96c0-70218d1d0439.jpg" /> can be represented as</p><disp-formula id="scirp.29423-formula5219"><label>(2)</label><graphic position="anchor" xlink:href="1-2730003\9366f1fc-74b0-4c84-a5ff-344031db8ef9.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="1-2730003\6e817114-ecae-44a1-b80e-05e16e45280e.jpg" /> and <img src="1-2730003\1584deff-7a9d-44dc-9231-a079d45e64c8.jpg" /> are independent. It generalizes normality and has been much studied in the statistical literature.</p><p>For the limit case<img src="1-2730003\b21ab7c8-b15c-40ac-be08-151dd38887df.jpg" />, <img src="1-2730003\ca3dd5ac-661d-4ee3-b072-adde30fd4b41.jpg" />yields the standard normal distribution<img src="1-2730003\81ca39eb-0b95-4568-98e6-3520766c1b1f.jpg" />. Let<img src="1-2730003\d3c68d48-6774-454b-98a3-b8764ccacf4a.jpg" />, the canonical slash distribution follows, see [<xref ref-type="bibr" rid="scirp.29423-ref6">6</xref>]. It is well known that the standard slash density has heavier tails than those of the normal distribution and has larger kurtosis. It has been very popular in robust statistical analysis and studied by some authors.</p><p>The general properties of this canonical slash distribution were studied in [5,7]. Kafadar [<xref ref-type="bibr" rid="scirp.29423-ref8">8</xref>] investigated the maximum likelihood estimates of the location and scale parameters.</p><p>G&#243;mez et al. [<xref ref-type="bibr" rid="scirp.29423-ref9">9</xref>] replaced standard normal random variable <img src="1-2730003\0aa69e50-e094-4436-a74f-ea20a3a96ca0.jpg" /> by an elliptical distribution and defined a new family of slash distributions. They studied its general properties of the resulting families, including their moments. Genc [<xref ref-type="bibr" rid="scirp.29423-ref10">10</xref>] proposed the univariate slash by a scale mixtured exponential power distribution and investigated asymptotically the bias properties of the estimators. Wang et al. [<xref ref-type="bibr" rid="scirp.29423-ref11">11</xref>] introduced the multivariate skew version of this distribution and examined its properties and inferences. They substituted the standard normal random variable <img src="1-2730003\99e17a00-196e-49f6-86e1-3e7e2d2e2d1c.jpg" /> by a skew normal distribution studied in [<xref ref-type="bibr" rid="scirp.29423-ref12">12</xref>] to define a skew extension of the slash distribution.</p><p>Olmos et al. [<xref ref-type="bibr" rid="scirp.29423-ref3">3</xref>] introduced the slashed half normal distribution by a scale mixtured half normal distribution and showed that the resulting distribution has more kurtosis than the ordinary half normal distribution. Since the epsilon half normal distribution <img src="1-2730003\df4b65a2-5254-442b-b5ae-e4ae0f2a9ba6.jpg" /> is an extension of the half normal distribution, it is naturally to define a slash distribution based on it in which skewness and thick tailed situations may exist. It leads to a new model on nonnegative measurements with more flexible asymmetry and kurtosis parameters.</p><p>The paper is organized as follows: in Section 2, we introduce the new slash distribution and study its relevant properties, including the stochastic representation etc. In Section 3 we discuss the inference, moments and maximum likelihood estimation for the parameters. Simulation studies are performed to investigate the behaviors of estimators in Section 4. In Section 5, we give a real illustrative application and report the results. Section 6 concludes our work.</p></sec><sec id="s2"><title>2. Epsilon Half Normal Slash Distribution</title><sec id="s2_1"><title>2.1. Stochastic Representation</title><p>Definition 2.1 A random variable <img src="1-2730003\19814413-c7f9-455e-b42a-fe9d728130e9.jpg" /> has an epsilon half normal slash distribution if it can be represented as the ratio</p><disp-formula id="scirp.29423-formula5220"><label>(3)</label><graphic position="anchor" xlink:href="1-2730003\c52b63b9-98a8-4bfd-9751-e59868716d7a.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="1-2730003\eb813084-03c3-41d0-9171-f046ab35fd73.jpg" /> defined in (1) and</p><p><img src="1-2730003\a4f34c81-d75e-4283-8487-a5fc9b52ed54.jpg" />are independent, <img src="1-2730003\a383be6f-0bf8-4bd8-8b1b-00092bdae0fb.jpg" />, <img src="1-2730003\9b1e31ca-486c-4637-a4e5-05fde9c8de97.jpg" />,<img src="1-2730003\61912a32-9e7e-40d8-9f93-3504debd034f.jpg" />. We denote it as<img src="1-2730003\e89000cc-509a-4f0c-a4d6-bfd2a61b4384.jpg" />.</p><p>Proposition 2.2 Let<img src="1-2730003\61226c8e-8a4f-4888-a129-73b8d54b4ae4.jpg" />. Then, the density function of <img src="1-2730003\3a4ae254-8501-4d1d-a254-7c67de0df014.jpg" /> is given by, for<img src="1-2730003\0f028086-b797-4dc9-8ec2-be11fbb876f1.jpg" />,</p><disp-formula id="scirp.29423-formula5221"><label>(4)</label><graphic position="anchor" xlink:href="1-2730003\5c38e853-2112-436d-9749-ce2f6717444b.jpg"  xlink:type="simple"/></disp-formula><p>where<img src="1-2730003\cbc13741-1f46-435e-89b7-bb7c4c67c7a9.jpg" />, <img src="1-2730003\5f644770-c51a-4ac5-8c51-4fbba1bdf8ee.jpg" />,<img src="1-2730003\7d4469f8-5df0-4de1-8fba-fb9d412adece.jpg" />.</p><p>Proof. From (1), the joint probability density function of <img src="1-2730003\3bc8f3c2-ca0f-4ef7-801b-a115e3b2ae13.jpg" /> and <img src="1-2730003\4555b863-39b2-49fd-923f-b609975ebb7f.jpg" /> is given by, for<img src="1-2730003\c44d5912-86a0-4765-95be-a300472fa8f4.jpg" />,</p><p><img src="1-2730003\1319e666-b786-4e19-ab6d-189c19f601fb.jpg" /></p><p>Using the transformation:</p><p><img src="1-2730003\f8ce4c5d-10c0-424d-ab6a-1dc3eb4dffe5.jpg" />the joint probability density function of <img src="1-2730003\8d2fc4d2-d0ae-4ed7-8425-b23d910d8b9b.jpg" /> and <img src="1-2730003\b9d00193-323b-486b-9ea0-9dd24ab7813d.jpg" /> is given by, for<img src="1-2730003\c799b880-8c35-43c6-8178-e1f9c164b963.jpg" />,</p><p><img src="1-2730003\31b78dd9-f103-493f-8a26-36965c300a8a.jpg" /></p><p>The marginal density function of <img src="1-2730003\3b4a60bb-5bc1-4680-af6c-07cbc750a5c1.jpg" /> is given by</p><p><img src="1-2730003\a4073ed5-ffb4-4cdb-a53a-354ac8700c88.jpg" /></p><p>After changing the variable into<img src="1-2730003\83352a65-93a0-43aa-b413-836c8e9592f6.jpg" />, the dendity function will be obtained as stated.</p><p>Remark 2.3 If<img src="1-2730003\c0853097-f295-45bb-b723-e6c0cfeeaa13.jpg" />, the density function (4) reduces to <img src="1-2730003\9aa186c9-c6b9-46de-b5b8-bfb0b00d388d.jpg" /></p><p>which is the density function for the slashed half normal distribution studied by [<xref ref-type="bibr" rid="scirp.29423-ref3">3</xref>]. As<img src="1-2730003\bd236921-89dc-4e2e-a7b4-73ba5e827562.jpg" />,</p><p><img src="1-2730003\62f10d0b-c880-49ef-9db1-cc96b9edd746.jpg" /></p><p>The limit case of the epsilon half normal slash distribution is the epsilon half normal distribution. For<img src="1-2730003\aa8813e5-c2d5-4387-9039-9e47ac5c3cb1.jpg" />, the canonical case follows.</p><p><xref ref-type="fig" rid="fig1">Figure 1</xref> shows some plots of the density function of the epsilon half normal slash distribution with various parameters.</p><p>The cumulative distribution function of the epsilon half normal slash distribution <img src="1-2730003\2fc4d1ce-9bec-4c1a-925a-04664a327612.jpg" /> is given as follows. For<img src="1-2730003\58f8fa31-6ca0-41ae-ab45-33cf0289253e.jpg" />,</p><disp-formula id="scirp.29423-formula5222"><label>(5)</label><graphic position="anchor" xlink:href="1-2730003\30e3d538-c676-4339-923e-b533c7333afb.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="1-2730003\1182313b-9a25-4121-a91d-bc61ea3093fc.jpg" /> is the cumulative distribution function for the standard normal random variable.</p><p>Proposition 2.4 Let <img src="1-2730003\1d271189-e37e-4b6e-9074-d28e484c94df.jpg" /> and<img src="1-2730003\037449f2-cb47-4dcc-a540-a43998c0f486.jpg" />, then<img src="1-2730003\dff3fda9-adc1-44c3-9a6b-51fc33acddb2.jpg" />.</p><p>Proof.</p><p><img src="1-2730003\7439776f-42c4-45e0-9277-a3009ab382ab.jpg" /></p><p>Remark 2.5 Proposition 2.4 shows that the epsilon half normal slash distribution can be represented as a scale mixture of an epsilon half normal distribution and uniform distribution. The result provides another way besides the definition (3) to generate random numbers from the epsilon half normal slash distribution</p><p><img src="1-2730003\56790ddb-b701-4f4d-a8de-46f7a2d7ab77.jpg" />.</p></sec><sec id="s2_2"><title>2.2. Moments and Measures Based on Moments</title><p>In this section, we derive the moment generating function,the k-th moment and some measures based on the moments.</p><p>Proposition 2.6 Let<img src="1-2730003\2f04ec99-b4e7-4a57-a98c-005ea73ad5df.jpg" />, then the moment generating function of <img src="1-2730003\a6fcea9a-7ea5-493f-8d0a-687ddaf0d0ae.jpg" /> is given by for<img src="1-2730003\15dba023-ac63-4518-814f-5c009595ea2a.jpg" />,</p><disp-formula id="scirp.29423-formula5223"><label>(6)</label><graphic position="anchor" xlink:href="1-2730003\162f6802-b2a1-45f9-aa0c-1b2f4be78ad9.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="1-2730003\42dc1496-23ca-4c31-a30c-71cee567dbf0.jpg" /> and<img src="1-2730003\4212aced-19e4-4438-8abf-cc59f86a141f.jpg" />. Proof. See [<xref ref-type="bibr" rid="scirp.29423-ref1">1</xref>].</p><p>Proposition 2.7 Let<img src="1-2730003\5710f289-f14c-4b39-8314-dd23dcdd9405.jpg" />, then the moment generating function of <img src="1-2730003\8441b125-6583-400c-8e11-f412657a74ef.jpg" /> is given by, for<img src="1-2730003\844cf0cf-6da8-49a3-ad83-c55ac365ef87.jpg" />,</p><disp-formula id="scirp.29423-formula5224"><label>(7)</label><graphic position="anchor" xlink:href="1-2730003\dcc5553f-f700-4a63-b0bb-132e5b0d2053.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.29423-formula5225"><label>(8)</label><graphic position="anchor" xlink:href="1-2730003\f6300866-aadd-4a56-be1c-d9ca49fef377.jpg"  xlink:type="simple"/></disp-formula><p>where<img src="1-2730003\a9051d05-4090-44e8-87c8-72487ddc0ce9.jpg" />, <img src="1-2730003\2cff2be0-56b9-4599-bbc9-8465c1226c0e.jpg" />and<img src="1-2730003\60b20f12-7bc4-45e6-a072-342d1c141fef.jpg" />.</p><p>Proof. From Proposition 2.4 and using properties of the conditional expectation, we have</p><p><img src="1-2730003\cdcc6fe6-5544-48b3-af53-fe1c639c71b2.jpg" /></p><p>Making the transformation <img src="1-2730003\01edcc07-d5a9-4e7d-821f-3b7b4a78a8e0.jpg" /> and the result follows.</p><p>Proposition 2.8 Let<img src="1-2730003\f4ca75e3-d401-4948-9f4c-0c30b97260a2.jpg" />, then the <img src="1-2730003\aed13b98-3551-4b5a-ba35-3fe7ac37ca85.jpg" /> non-central moments are given by</p><disp-formula id="scirp.29423-formula5226"><label>(9)</label><graphic position="anchor" xlink:href="1-2730003\347b113d-59a0-4aac-b1f9-ee05f2a7ec98.jpg"  xlink:type="simple"/></disp-formula><p>for<img src="1-2730003\fcf9329a-321c-49c2-be18-7219a6b2a989.jpg" />. where <img src="1-2730003\439e4f2e-a9ca-4f93-948f-7fda2efc961a.jpg" /> and<img src="1-2730003\9dc5f623-c168-42a8-93f2-b4ecc6b8888d.jpg" />.</p><p>Proof. See [<xref ref-type="bibr" rid="scirp.29423-ref1">1</xref>].</p><p>Proposition 2.9 Let<img src="1-2730003\efbc3cc9-d774-4c13-852d-5bdd1799dab0.jpg" />, where<img src="1-2730003\44dd25ae-caac-4043-b595-2d4ebbb5d226.jpg" />, <img src="1-2730003\a15cab36-6b57-4ef5-bbc4-f375eb3d0895.jpg" />and<img src="1-2730003\05b763ff-5449-413e-b812-547cac97d545.jpg" />. For <img src="1-2730003\016bb5fe-ab00-4731-9b26-946c88b410ea.jpg" /> and<img src="1-2730003\e3331b17-1a78-447f-9fd4-8cfff66a318e.jpg" />, the <img src="1-2730003\0e4e722c-e7a3-46f5-b9d7-ec634f484563.jpg" /> non-central moment of <img src="1-2730003\74d24c11-dfed-4a9d-915e-1978a81215de.jpg" /> is given by</p><disp-formula id="scirp.29423-formula5227"><label>(10)</label><graphic position="anchor" xlink:href="1-2730003\6563c3d7-5d8a-4838-b798-04ecfaa90a8a.jpg"  xlink:type="simple"/></disp-formula><p>Proof. From the stochastic representation defined in (3) and the results in (9), the claim follows in a straightforward manner.</p><p><img src="1-2730003\575e9011-ff4e-40d3-a85c-2f7bf87e5f6e.jpg" /></p><p>The following results are immediate consequences of (10).</p><p>Corollary 2.10 Let<img src="1-2730003\9331b536-669a-4aea-bc4c-c6deb2fa7e36.jpg" />, where<img src="1-2730003\133f0ac6-b4f0-4699-9746-48ef5bc17024.jpg" />, <img src="1-2730003\c8647b9c-074f-4d5c-af45-ef0080d7124c.jpg" />and<img src="1-2730003\7e8564e6-8612-42df-838b-44069c17e1d1.jpg" />. The mean and variance of <img src="1-2730003\ca3b4150-2d1b-4223-b117-02c60449741b.jpg" /> are given by</p><disp-formula id="scirp.29423-formula5228"><label>(11)</label><graphic position="anchor" xlink:href="1-2730003\80aec176-fd4b-439b-a89d-ddf66f94e2b9.jpg"  xlink:type="simple"/></disp-formula><p>and for<img src="1-2730003\fabc0c96-5d5d-4ece-aae2-801dbb12c8dd.jpg" />,</p><p><img src="1-2730003\6c28437d-1dea-4d7f-b2ee-e8db7aff2250.jpg" /></p><p>For the standardized skewness</p><p><img src="1-2730003\24713177-6082-4c8b-8dde-d7a40b64a1da.jpg" /></p><p>and kurtosis coefficients</p><p><img src="1-2730003\9837b1a1-2d62-4709-9b2d-9c7dce26dce5.jpg" />we have the following results.</p><p>Corollary 2.11 Let<img src="1-2730003\406107ac-bad4-4306-99b6-fef4b80c94a2.jpg" />, where<img src="1-2730003\2847f5ac-8e79-495c-8a81-72551b04121a.jpg" />, <img src="1-2730003\6f286532-846f-435c-9815-d7b5567cb0ab.jpg" />and<img src="1-2730003\c02855af-1e1c-428f-824d-d64ab93d9f71.jpg" />. The skewness and kurtosis coefficients of <img src="1-2730003\ad839862-7cde-431c-b171-67fb7610d470.jpg" /> are given by</p><disp-formula id="scirp.29423-formula5229"><label>(12)</label><graphic position="anchor" xlink:href="1-2730003\01ae0f9e-6493-4294-8dfa-41889d362b8d.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.29423-formula5230"><label>(13)</label><graphic position="anchor" xlink:href="1-2730003\8f24269b-60c0-4f21-836d-eb6476eb5445.jpg"  xlink:type="simple"/></disp-formula><p>where</p><p><img src="1-2730003\eb6e75b7-c0ac-4c56-b772-9af9bbeee9d9.jpg" /></p><p><img src="1-2730003\8c7c7992-a305-48e2-a6f3-b423e13a7f16.jpg" /></p><p><img src="1-2730003\fee4902b-f8ef-4174-ae43-6e03be133740.jpg" /></p><p>Remark 2.12 As<img src="1-2730003\d68e0ca2-6f5b-4557-9372-0698429018d7.jpg" />, the skewness coefficient converges.</p><p><img src="1-2730003\c7beb022-642a-4630-b217-bac198dc644f.jpg" /></p><p>and the kurtosis coefficient converges as well</p><p><img src="1-2730003\d224448f-fa36-47b9-b3ce-290f782499d1.jpg" /></p><p>which are the corresponding skewness and kurtosis coefficients for the epsilon half normal distribution<img src="1-2730003\e068f9da-6537-4933-abfe-9572840a6044.jpg" />.</p><p><xref ref-type="fig" rid="fig2">Figure 2</xref> shows the skewness and kurtosis coefficients with various parameters for the <img src="1-2730003\63b15c3d-806c-409b-9488-bf56c630f733.jpg" /> model. The skewness and kurtosis coefficients decrease as <img src="1-2730003\7fd47425-c4c6-4e7b-bf81-cbdadb1a7404.jpg" /> increases. The parameter <img src="1-2730003\8c70e72c-8ade-4556-943a-edbdd01fad8f.jpg" /> does not affect the two coefficents.</p></sec></sec><sec id="s3"><title>3. Maximum Likelihood Inference</title><p>In this section, we consider the maximum likelihood estimation about the parameters of the <img src="1-2730003\5f95aa26-96b1-42dc-8814-a9b0789aaa03.jpg" /> model defined in (4). For<img src="1-2730003\0d316682-eadb-47c1-bd52-0b9e847b0c60.jpg" />,</p><p><img src="1-2730003\f1a72620-60f9-4d6f-bb2e-9df7324745a5.jpg" /></p><p>where<img src="1-2730003\66ce15a4-3bae-4e28-94d1-6679e2a62551.jpg" />.</p><p>Suppose <img src="1-2730003\2ce886e8-0945-4210-82c5-9fcf7b3e318e.jpg" /> is a random sample of size <img src="1-2730003\2103f1aa-2052-49ea-aff6-0bf8107c337f.jpg" /> from the epsilon half normal slash distribution</p><p><img src="1-2730003\cf3c2922-11a7-430d-a5d6-8865fbddc5c4.jpg" />. Then the log-likelihood function can be written as</p><disp-formula id="scirp.29423-formula5231"><label>(14)</label><graphic position="anchor" xlink:href="1-2730003\958eb2c2-f2fa-4d3a-af6a-e32be2f2ed05.jpg"  xlink:type="simple"/></disp-formula><p>&#160;The estimates of the parameters maximize the likelihood function. By taking the partial derivatives of the log-likelihood function with respect to <img src="1-2730003\6c05925e-82b0-446c-9d97-7516f027873a.jpg" /> respectively and equalizing the obtained expressions to zero, we obtain the following maximum likelihood estimating equations.</p><p><img src="1-2730003\7c876151-64d6-41d4-8f33-06b29175a0f6.jpg" /></p><p><img src="1-2730003\d0f0434c-e738-4cae-bdbe-0c96d34bf147.jpg" /></p><p><img src="1-2730003\6fbcdde3-5cfe-4408-badb-d845b2982390.jpg" /></p><p>The maximum likelihood estimating equations above are not in a simple form. In general, there are no implicit expression for the estimates. The estimates can be obtained through some numerical procedures such as Newton-Raphson method. Many programs provide routines to solve such maximum likelihood estimating equations.</p><p>In this paper, all the computations are performed using software R. The MLE estimators are computed by the optim function which uses L-BFGS-B method. In the following section, a simulation is conducted to illustrate the behavior of the MLE.</p><p>For asymptotic inference of<img src="1-2730003\7a1ca4bb-db8c-4b7e-be1d-78921708040f.jpg" />, the Fisher information matrix <img src="1-2730003\fccbdc5d-f45f-42bb-808e-e384f726ef36.jpg" /> plays a key role. It is well known that its inverse is the asymptotic variance matrix of the maximum likelihood estimators. For the case of a single observation<img src="1-2730003\d1faac9f-0c8f-4dcc-93dc-0eeee93bb249.jpg" />, we take the second order derivatives of the log-likelihood function in (14) and the Fisher information matrix is defined as</p><disp-formula id="scirp.29423-formula5232"><label>(15)</label><graphic position="anchor" xlink:href="1-2730003\06d4dfdb-3f59-4bb1-9829-ec4992880a3c.jpg"  xlink:type="simple"/></disp-formula><p>for <img src="1-2730003\18ae9e65-7e78-4f04-85e9-88ebe2cb56a0.jpg" /> and<img src="1-2730003\a77c029e-adec-49e3-a2ee-acdfba2c8084.jpg" />.</p><p>Proposition 3.1 Let <img src="1-2730003\857f9caa-60ed-4145-87e3-e82b8a07b49b.jpg" /> is a random sample of size <img src="1-2730003\4e3d9010-27b6-4e47-aeb6-d21caff5d274.jpg" /> from the distribution<img src="1-2730003\98b32e6b-e354-41ab-83d4-469cf272829a.jpg" />, where <img src="1-2730003\65f8c3fc-f94f-4516-a7ea-214db15b8ff7.jpg" /> and <img src="1-2730003\286f366b-8610-4131-a714-39f7cd89de99.jpg" /> is the maximum likelihood estimator of<img src="1-2730003\935387c2-4cae-44d1-bbd3-7a3ce8ee414c.jpg" />, we have</p><disp-formula id="scirp.29423-formula5233"><label>(16)</label><graphic position="anchor" xlink:href="1-2730003\ddc46619-316c-44c9-922c-33284292580c.jpg"  xlink:type="simple"/></disp-formula><p>Proof. It follows directly by the large sample theory for maximum likelihood estimators and the Fisher information matrix given above.</p></sec><sec id="s4"><title>4. Simulation Study</title><sec id="s4_1"><title>4.1. Data Generation</title><p>In this section, we present how to generate the random numbers from the epsilon half normal slash distribution<img src="1-2730003\a2899a1a-abe5-448a-a8a5-197cee2bb1a2.jpg" />.</p><p>Proposition 4.1 Let <img src="1-2730003\200951d5-f13e-4bcd-9ec4-625695630ef0.jpg" /> be two independent random variables, where <img src="1-2730003\91fa06a3-d0e7-45c6-9103-b28a259a88db.jpg" /> and <img src="1-2730003\3d72cd6a-49a4-4f0b-ba34-5559b6001086.jpg" /> is such that</p><p><img src="1-2730003\e7cf3875-8c72-4839-89f4-b77aa7f03bc0.jpg" /></p><p>then<img src="1-2730003\d2b41d24-405a-4bf9-8f41-7cd5e0e0c433.jpg" />, where <img src="1-2730003\67eb0c69-404c-4edb-ad4b-a04e34964766.jpg" /> and <img src="1-2730003\f0233d14-7ff4-4dfe-a4c4-ded8b2e8dd68.jpg" />.</p><p>Proof. For<img src="1-2730003\a636f788-1d7e-430d-8b77-f4e6c8ae518e.jpg" />,</p><p><img src="1-2730003\f8060ea5-2876-4d83-adb5-5aafa22bb3af.jpg" /></p><p>The density function of <img src="1-2730003\87b62526-de5a-447b-80b0-7c62ddbd2114.jpg" /> is</p><p><img src="1-2730003\145a2b0f-51e2-42a9-8537-d5ba6a9d4698.jpg" /></p><p>which proves the result.</p><p>Using the definition in (3) and the results in Proposition 4.1, we can generate variates from the epsilon half normal slash distribution <img src="1-2730003\b3dbf551-05c6-491c-81fe-28329852eabe.jpg" /> with the following algorithm.</p><p>Algorithm 4.2 Using the definition in (3) to generate data</p><p>• Generate<img src="1-2730003\6d9cda62-5373-4b5a-9b5a-4ff61566c6da.jpg" />, <img src="1-2730003\15b9f54a-cb3a-43ea-8b6e-63f42799cff4.jpg" />and</p><p>• <img src="1-2730003\19d35fb5-fe69-46a4-b2f9-b8b819ad61ef.jpg" /></p><p>• Let <img src="1-2730003\213d0bf3-6200-4283-abf2-bf1724e0f86e.jpg" /> if<img src="1-2730003\bfdc853c-c434-4d5e-b308-89e4ef1fc8f3.jpg" />. Otherwise <img src="1-2730003\a00a7026-4a15-47cd-bcfa-911897d1e7c3.jpg" /></p><p>• Set <img src="1-2730003\2d8b6d3a-0432-494a-ad38-a98880522f06.jpg" /></p><p>• Set <img src="1-2730003\ff17e6ae-3e41-421a-86e5-6ab44dd589a4.jpg" /></p></sec><sec id="s4_2"><title>4.2. Behavior of MLE</title><p>In this section, we perform a simulation study to illus trate the behavior of the MLE estimators for parameters<img src="1-2730003\28f6d09f-24c7-4865-bbc3-e5792d073915.jpg" />, <img src="1-2730003\3907968b-6485-4d4a-92da-60739aab9a7d.jpg" />and<img src="1-2730003\6aaa751c-0202-46a8-8a24-31d313c7b407.jpg" />.</p><p>It is known that as the sample size increases, the distribution of the MLE tends to the normal distribution with mean <img src="1-2730003\540156ef-b804-4346-b933-3698fd96fc96.jpg" /> and covariance matrix equal to the inverse of the Fisher information matrix. However, the log-likelihood function given in (14) is a complex expression. It is not generally possible to derive the Fisher information matrix. Thus, the theoretical properties (asymptotically normal, unbiased etc) of the MLE estimators are not easily derived. We study the properties of the estimators numerically.</p><p>We first generate 500 samples of size <img src="1-2730003\3d619972-4742-4822-b742-a2b55f4ea8f2.jpg" /> and <img src="1-2730003\4a65ca3f-0079-4c21-a14f-754e18d1a895.jpg" /> from the <img src="1-2730003\a8206886-561a-48bb-8a10-524e54bc0188.jpg" /> distribution for fixed parameters. The estimators are computed by the optim function which uses L-BFGS-B method in software R. The empirical means and standard deviations(SD) of the estimators are presented in <xref ref-type="table" rid="table1">Table 1</xref>.</p><p>It can be seen from <xref ref-type="table" rid="table1">Table 1</xref> that the parameters are well estimated and the estimates are asymptotically un-</p><p><xref ref-type="table" rid="table1">Table 1</xref>. Empirical means and SD for the MLE estimators of<img src="1-2730003\416dd60b-bb07-43a5-a066-1f8bee292215.jpg" />, <img src="1-2730003\d607ac15-99fc-4e23-b35f-fb05f11449af.jpg" />and<img src="1-2730003\034886e0-fd5a-49a6-85a2-85d96e8e284b.jpg" />.</p><p><img src="1-2730003\4b19d8cf-990e-45c4-9c4d-cfddfa12333a.jpg" /></p><p><xref ref-type="table" rid="table2">Table 2</xref>. Summary for the life of fatigue fracture.</p><p><img src="1-2730003\7b582bc4-7113-4841-ab3c-f3d532b1b4a0.jpg" /></p><p><xref ref-type="table" rid="table3">Table 3</xref>. Maximum likelihood parameter estimates(with (SD)) of the HN, EHN and EHNS models for the stressrupture data.</p><p><img src="1-2730003\58d80967-08b7-49b6-80f4-94bd83190f93.jpg" /></p><p>biased. The empirical mean square errors decrease as sample size increases as expected.</p></sec></sec><sec id="s5"><title>5. Real Data Illustration</title><p>In this section, we consider the stress-rupture data set, the life of fatigue fracture of Kevlar 49/epoxy that are subject to the pressure at the 90% level. The data set has been previously studied in [1,3,13,14].</p><p><xref ref-type="table" rid="table2">Table 2</xref> summarizes descriptive statistics of the data set where <img src="1-2730003\050b79c8-fb24-4c63-bc2b-b9a380e40d94.jpg" /> and <img src="1-2730003\3f2e98d3-d702-4a80-9f00-56292a1543cb.jpg" /> are sample asymmetry and kurtosis coefficients, respectively. This data set indicates non negative asymmetry.</p><p>We fit the data set with the half normal, the epsilon half normal and the epsilon half normal slash distributions using maximum likelihood method. The results are reported in <xref ref-type="table" rid="table3">Table 3</xref>. The usual Akaike information criterion (AIC) and Bayesian information criterion (BIC) to measure of the goodness of fit are also computed. <img src="1-2730003\8f364558-a93d-4448-813d-8142570a5e85.jpg" />and<img src="1-2730003\87b6c258-644c-4769-b437-949511f676c6.jpg" />. where <img src="1-2730003\b7f72102-49bb-4e41-96c1-169d3c1ae26a.jpg" /> is the number of parameters in the distribution and <img src="1-2730003\b81d106d-49fc-4dca-87a9-2d1b8209a35c.jpg" /> is the maximized value of the likelihood function. The results indicate that <img src="1-2730003\6d6675f3-eecc-454a-ab4a-798e50b51cbf.jpg" /> model fits best. Figures 3(a) and (b) display the fitted models using the MLE estimates.</p></sec><sec id="s6"><title>6. Concluding Remarks</title><p>In this article, we have studied the epsilon half normal slash distribution<img src="1-2730003\292cad09-fa03-4214-b61e-69720224c022.jpg" />. It is defined to be the quotient of two independent random variables, an epsilon half normal random variable and a power of the uniform distribution. This nonnegative distribution extends the</p><p>epsilon half normal, the half normal distribution etc. Probabilistic and inferential properties are derived. A simulation is conducted and demonstrates the good performance of the maximum likelihood estimators. We apply the model to a real dataset and the results demonstrate that the proposed model is very useful and flexible for non negative data.</p></sec><sec id="s7"><title>7. Acknowledgements</title><p>The authors would like to thank the anonymous reviewers and the editor for their valuable comments and suggestions to improve the quality of the paper.</p></sec><sec id="s8"><title>REFERENCES</title></sec><sec id="s9"><title>NOTES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.29423-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">L. Castro, H. Gómez and M. Valenzuela, “Epsilon Half-Normal Model: Properties and Inference,” Computational Statistics &amp; Data Analysis, Vol. 56, No. 12, 2012, pp. 4338-4347. Hdoi:10.1016/j.csda.2012.03.020</mixed-citation></ref><ref id="scirp.29423-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">A. Pewsey, “Improved Likelihood Based Inference for the General Half-Normal Distribution,” Communications in Statistics—Theory and Methods, Vol. 33, No. 2, 2004, pp. 197-204. 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