<?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">JFRM</journal-id><journal-title-group><journal-title>Journal of Financial Risk Management</journal-title></journal-title-group><issn pub-type="epub">2167-9533</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jfrm.2015.43010</article-id><article-id pub-id-type="publisher-id">JFRM-59341</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Business&amp;Economics</subject></subj-group></article-categories><title-group><article-title>
 
 
  Operational Risk Modelling in Insurance and Banking
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>gnjen</surname><given-names>Vukovic</given-names></name><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><author-notes><corresp id="cor1">* E-mail:<email>ognjen.vukovic@uni.li, oggyvukovich@gmail.com</email>;<email>Department for Finance, University of Liechtenstein, Vaduz, Liechtenstein</email>;</corresp></author-notes><pub-date pub-type="epub"><day>01</day><month>09</month><year>2015</year></pub-date><volume>04</volume><issue>03</issue><fpage>111</fpage><lpage>123</lpage><history><date date-type="received"><day>20</day>	<month>June</month>	<year>2015</year></date><date date-type="rev-recd"><day>accepted</day>	<month>29</month>	<year>August</year>	</date><date date-type="accepted"><day>1</day>	<month>September</month>	<year>2015</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 author of the presented paper is trying to develop and implement the model that can mimic the state of the art models of operational risk in insurance. It implements generalized Pareto distribution and Monte Carlo simulation and tries to mimic and construct operational risk models in insurance. At the same time, it compares lognormal, Weibull and loglogistic distribution and their application in insurance industry. It is known that operational risk models in insurance are characterized by extreme tails, therefore the following analysis should be conducted: the body of distribution should be analyzed separately from the tail of the distribution. Afterwards the convolution method can be used to put together the annual loss distribution by combining the body and tail of the distribution. Monte Carlo method of convolution is utilized. Loss frequency in operational risk in insurance and overall loss distribution based on copula function, in that manner using student-t copula and Monte Carlo method are analysed. The aforementioned approach represents another aspect of observing operational risk models in insurance. This paper introduces: 1) Tools needed for operational risk models; 2) Application of R code in operational risk modeling;3) Distributions used in operational risk models, specializing in insurance; 4) Construction of operational risk models.
 
</p></abstract><kwd-group><kwd>Insurance</kwd><kwd> Operational Risk</kwd><kwd> Monte Carlo</kwd><kwd> Statistical Distributions</kwd><kwd> Modeling</kwd><kwd> Copula</kwd><kwd>  Convolution</kwd><kwd> Loss Frequency</kwd><kwd> Severity</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Operational risk is defined according to Basel II  (Nicolas &amp; Firzli, 2011)  as well as according to European Solvency II which adopted for insurance industry is defined in the following way  (Nicolas &amp; Firzli, 2011) .</p><p>Operational risk is the risk of change in value caused by the fact that actual losses, incurred for inadequate or failed internal processes, people and systems, or from external events (including legal risk), and differs from the expected losses.</p><p>In order to analyse operational risk in insurance, Solvency II Directive  (Mittnik, 2011)  must be discussed. Solvency II Directive is an EU Directive that codifies and harmonises the EU insurance regulation. This concerns the amount of capital that EU insurance companies must hold to reduce the risk of insolvency. Solvency II  (Mittnik, 2011)  is called “Basel for insurers”  (Nicolas &amp; Firzli, 2011) . Solvency II is somewhat similar to the banking regulations of Basel II. The proposed Solvency II framework has three main areas (pillars)  (Accords, 2006) :</p><p>・ Pillar 1―quantitative requirements</p><p>・ Pillar 2―requirements for the governance and risk management of insurers and their supervision</p><p>・ Pillar 3―disclosure and transparency requirements</p><p>In order to analyse the operational risk in insurance  (CEA―Groupe Consultatif, 2005) , the attention towards pillar 2 and pillar 1 should be directed. Ernst &amp;Young reports that most of the insurance companies in 2016 will manage to implement the Solvency II requirement until January 2016  (PWC Financial Services Regulatory Practice, 2014) . One of the major new features of Solvency II is that insurance companies must now devote a portion of their equity to covering their exposure to operational risks. There are approaches to calculate the capital requirement: a standard and more advance approach. The advanced approach uses an internal model of risk that corresponds to the company’s real situation. Quantitative impact study (QIS 5) has encouraged insurance companies to adopt the internal model by structuring the standard approach such that it uses up much more equity  (Solvency―European Commission, 2012) . In order to analyse the operational risk in this frame, the following assumption will be made: risk will be divided between frequency and severity risk  (Doerig, 2000) . They will be modeled by Loss Distribution approach  (Power, 2005) . Severity risk represents the risk of large but rare losses. Bayesian networks are used to model severity risk.</p><sec id="s1_1"><title>1.1. Bayesian Networks</title><p>Bayesian networks are defined as a probabilistic graphical model that represents a set of random variables and their conditional dependencies via a directed acyclic graph (DAG). For example, a Bayesian network could represent the probabilistic relationships between the cause and result. If we are aware of the causes, the probabilities of results can be calculated.</p><p>In order to define the Bayesian network, the following definition will be used. <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x5.png" xlink:type="simple"/></inline-formula>is a Bayesian network with respect to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x6.png" xlink:type="simple"/></inline-formula> if its joint probability density function (with respect to a product measure) can be written as a product of the individual density functions, conditional on their parent variables:</p><disp-formula id="scirp.59341-formula85"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2410129x7.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x8.png" xlink:type="simple"/></inline-formula> is the set of parents of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x9.png" xlink:type="simple"/></inline-formula>.</p><p>The probability of any member of a joint distribution can be calculated from the conditional probabilities using the chain rule, taking into consideration at the same topological ordering of X.</p><disp-formula id="scirp.59341-formula86"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2410129x10.png"  xlink:type="simple"/></disp-formula><p>Equation (2) can be written as:</p><disp-formula id="scirp.59341-formula87"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2410129x11.png"  xlink:type="simple"/></disp-formula><p>(for each <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x12.png" xlink:type="simple"/></inline-formula> which is a parent of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x13.png" xlink:type="simple"/></inline-formula>).</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x14.png" xlink:type="simple"/></inline-formula>is a Bayesian network with respect to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x15.png" xlink:type="simple"/></inline-formula> if it satisfies the local Markov property, each variable is conditionally independent of its non-descendants given its parent variables.</p><disp-formula id="scirp.59341-formula88"><label>(4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2410129x16.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x17.png" xlink:type="simple"/></inline-formula> is the set of descendants and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x18.png" xlink:type="simple"/></inline-formula> is the set of non-descendants of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x19.png" xlink:type="simple"/></inline-formula>.</p><p>The aforementioned thing can also be expressed in terms similar to the first definition, as:</p><disp-formula id="scirp.59341-formula89"><label>(5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2410129x20.png"  xlink:type="simple"/></disp-formula><p>For each <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x21.png" xlink:type="simple"/></inline-formula> which is not a descendant of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x21.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x22.png" xlink:type="simple"/></inline-formula> is</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x23.png" xlink:type="simple"/></inline-formula>For each <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x23.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x24.png" xlink:type="simple"/></inline-formula> which is a parent of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x23.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x24.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x25.png" xlink:type="simple"/></inline-formula>.</p><p>Note that the set of parents is a subset of the set of non-descendants because the graph is acyclic.</p></sec><sec id="s1_2"><title>1.2. Developing Bayesian Networks</title><p>To develop a Bayesian network, we often first develop a <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x26.png" xlink:type="simple"/></inline-formula> (directed acyclic graph) <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x26.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x27.png" xlink:type="simple"/></inline-formula>such that we believe <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x26.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x27.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x28.png" xlink:type="simple"/></inline-formula> satisfies the local Markov property with respect to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x26.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x27.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x28.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x29.png" xlink:type="simple"/></inline-formula>. Sometimes this is done by creating a casual<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x26.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x27.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x28.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x29.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x30.png" xlink:type="simple"/></inline-formula>. We then ascertain the conditional probability distribution of each variable given its parents in<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x26.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x27.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x28.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x29.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x30.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x31.png" xlink:type="simple"/></inline-formula>. In many cases and in particular in the case where the variables are discrete, we define the joint distribution of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x26.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x27.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x28.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x29.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x30.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x31.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x32.png" xlink:type="simple"/></inline-formula> to be the product of these conditional distributions, then X is a Bayesian network with respect to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x26.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x27.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x28.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x29.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x30.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x31.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x32.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x33.png" xlink:type="simple"/></inline-formula>.</p><p>In order to model loss severity, since it can be difficult to model operational risk losses of a risk class using only one probability distribution, we analyse severity at two levels: body and tail of the distribution delimited by a high threshold value<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x34.png" xlink:type="simple"/></inline-formula>.</p><p>The central body can be modeled by using a parametric distribution. One of the distributions that can be used is lognormal. Body is usually estimated on internal data, since the sample size is sufficient below the threshold<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x35.png" xlink:type="simple"/></inline-formula>.</p><p><xref ref-type="fig" rid="fig1">Figure 1</xref> demonstrates the body of the distribution, it is assumed that the body of the distribution embraces lognormal value, therefore we assume the lognormal distribution. In order to analyse the tail, it can be modeled applying extreme value theory  (Embrechts, Kluppelberg, &amp; Mikosch, 1997)  the distribution above the threshold, we are talking about Generalized Pareto distribution (GPD). Tail is usually estimated on internal data integrated with external data and scenario generated data above<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x36.png" xlink:type="simple"/></inline-formula>. Data are real scarce above threshold<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x36.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x37.png" xlink:type="simple"/></inline-formula>.</p><p>Generalized Pareto distribution is used to capture the tail of severity distribution. <xref ref-type="fig" rid="fig2">Figure 2</xref> shows the Genera-</p><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> Lognormal distribution</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-2410129x38.png"/></fig><fig id="fig2"  position="float"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> Generalized Pareto distribution</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-2410129x39.png"/></fig><p>lized Pareto distribution, its density as well as its cumulative function.</p><p>The commonly used approach to quantify operational risk is the Loss Distribution Approach  (Embrechts, Kluppelberg, &amp; Mikosch, 1997)  where frequency and severity of operational risk losses are modeled separately. The yearly potential loss <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x40.png" xlink:type="simple"/></inline-formula> is based on the sum of the yearly losses <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x40.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x41.png" xlink:type="simple"/></inline-formula> related to the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x40.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x42.png" xlink:type="simple"/></inline-formula> risk classes.</p><p>The yearly potential loss <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x43.png" xlink:type="simple"/></inline-formula> related to risk class<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x43.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x44.png" xlink:type="simple"/></inline-formula>, is affected by two sources of uncertainty:</p><p>・ The number of losses <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x45.png" xlink:type="simple"/></inline-formula> in one year time horizon</p><p>・ The impact of each single loss <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x46.png" xlink:type="simple"/></inline-formula></p><p>If the following procedure is to be applied to mathematical modeling of operational risk in insurance, the only thing that should be changed is the distribution that it is to be used. Therefore, the methods of copula and convolution will be explained as well as the possible distribution that could be applied in insurance.</p></sec><sec id="s1_3"><title>1.3. Convolution</title><p>In mathematics, convolution is a mathematical operation on two functions <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x47.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x47.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x48.png" xlink:type="simple"/></inline-formula>, producing a third function that is typically viewed as a modified version of one of the original functions, giving the area overlap between the two functions as a function of the amount that one of the original functions is translated  (Bracewell, 1986; Damelin &amp; Miller, 2011) . Convolution is presented in the following manner:</p><p>It is defined as the integral of the product of the two functions after one is reversed and shifted. It is a particular kind of integral transform:</p><disp-formula id="scirp.59341-formula90"><label>(6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2410129x49.png"  xlink:type="simple"/></disp-formula><p>Although the symbol <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x50.png" xlink:type="simple"/></inline-formula> is used above, it need not represent the time domain. However formula can be interpreted as a weighted average of the function <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x50.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x51.png" xlink:type="simple"/></inline-formula> at the moment <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x50.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x51.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x52.png" xlink:type="simple"/></inline-formula> where the weighting is given by <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x50.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x51.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x52.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x53.png" xlink:type="simple"/></inline-formula> simply shifted by amount<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x50.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x51.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x52.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x53.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x54.png" xlink:type="simple"/></inline-formula>. As <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x50.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x51.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x52.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x53.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x54.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x55.png" xlink:type="simple"/></inline-formula> changes, the weighting function emphasizes different part of the input function  (Bracewell, 1986; Damelin &amp; Miller, 2011) .</p></sec><sec id="s1_4"><title>1.4. Copula</title><p>A copula is a multivariate probability distribution for which the marginal probability distribution of each variable is uniform. Copulas are used to describe the dependence between random variables.</p><p>One important theorem for copulas is Sklar’s theorem. We will now define the copula:</p><p>Copula  (Nelsen, 1999)  is a multivariate distribution function, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x56.png" xlink:type="simple"/></inline-formula>, with marginal functions distributed uniformly in [0,1] (U(0,1)) such that</p><p>1) <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x57.png" xlink:type="simple"/></inline-formula></p><p>2) <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x58.png" xlink:type="simple"/></inline-formula>has marginal functions <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x58.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x59.png" xlink:type="simple"/></inline-formula> such that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x58.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x59.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x60.png" xlink:type="simple"/></inline-formula> <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x58.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x59.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x60.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x61.png" xlink:type="simple"/></inline-formula></p><p>Sklar’s theorem  (Sklar, 1959)  provides the theoretical foundation for the application of copula. Sklar’s theorem states that every multivariate cumulative distribution function</p><disp-formula id="scirp.59341-formula91"><label>(7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2410129x62.png"  xlink:type="simple"/></disp-formula><p>Of a random vector <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x63.png" xlink:type="simple"/></inline-formula> with marginal <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x63.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x64.png" xlink:type="simple"/></inline-formula> and it can be written as:</p><disp-formula id="scirp.59341-formula92"><label>(8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2410129x65.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x66.png" xlink:type="simple"/></inline-formula> is copula.</p><p>The copula that will be used is Gaussian copula and Gumbel copula. They will be presented shortly.</p><p>The Gaussian copula:</p><p>Gaussian copula  (Nelsen, 1999)  is a distribution over the unit cube<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x67.png" xlink:type="simple"/></inline-formula>. It is constructed from a multivariate normal distribution over <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x67.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x68.png" xlink:type="simple"/></inline-formula> using the probability integral form.</p><p>The Gaussian copula for<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x69.png" xlink:type="simple"/></inline-formula>, it can be written with parameter matrix <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x69.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x70.png" xlink:type="simple"/></inline-formula> can be written as:</p><disp-formula id="scirp.59341-formula93"><label>(9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2410129x71.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x72.png" xlink:type="simple"/></inline-formula> is the inverse cumulative distribution function of a standard normal and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x72.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x73.png" xlink:type="simple"/></inline-formula> is the joint cumulative distribution function of a multivariate normal distribution with mean vector zero and covariance matrix equal to the correlation matrix<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x72.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x74.png" xlink:type="simple"/></inline-formula>.</p><p>The density matrix can be written as</p><disp-formula id="scirp.59341-formula94"><label>(10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2410129x75.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x76.png" xlink:type="simple"/></inline-formula> is the identity matrix.</p><p>Other famous copulas are Archimedean copulas.</p></sec><sec id="s1_5"><title>1.5. Archimedean Copulas</title><p>Archimedean copulas  (Nelsen, 1999)  are an associative class of copulas. Archimedean copulas are popular because they allow modeling dependence in arbitrarily high dimensions with only one parameter, governing the strength of dependence.</p><p>A copula <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x77.png" xlink:type="simple"/></inline-formula> is called Archimedean if it admits the representation</p><disp-formula id="scirp.59341-formula95"><label>(11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2410129x78.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x79.png" xlink:type="simple"/></inline-formula> is a continuous, strictly decreasing and convex function such that<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x79.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x80.png" xlink:type="simple"/></inline-formula>. <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x79.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x80.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x81.png" xlink:type="simple"/></inline-formula>is a parameter within some parameter space<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x79.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x80.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x81.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x82.png" xlink:type="simple"/></inline-formula>. <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x79.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x80.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x81.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x82.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x83.png" xlink:type="simple"/></inline-formula>is the so-called generator function and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x79.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x80.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x81.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x82.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x83.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x84.png" xlink:type="simple"/></inline-formula> is the pseudo-inverse defined by:</p><disp-formula id="scirp.59341-formula96"><label>(12)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2410129x85.png"  xlink:type="simple"/></disp-formula><p>Moreover, the above formula for C yields a copula for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x86.png" xlink:type="simple"/></inline-formula> if and only if <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x86.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x87.png" xlink:type="simple"/></inline-formula> is d-monotone on<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x86.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x87.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x88.png" xlink:type="simple"/></inline-formula>. That is, if it is <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x86.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x87.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x88.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x89.png" xlink:type="simple"/></inline-formula> times differentiable and the derivatives satisfy</p><disp-formula id="scirp.59341-formula97"><label>(13)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2410129x90.png"  xlink:type="simple"/></disp-formula><p>for all <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x91.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x91.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x92.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x91.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x92.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x93.png" xlink:type="simple"/></inline-formula> is nonincreasing and convex.</p><p>The copula that we will also introduce is Gumbel copula.</p><p>It has the following bivariate form:</p><disp-formula id="scirp.59341-formula98"><label>(14)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2410129x94.png"  xlink:type="simple"/></disp-formula><p>After giving the definition of two most important techniques of aggregating operational risk, we will introduce the distributions that we will be using as well as the definition of value at risk and expected shortfall.</p></sec><sec id="s1_6"><title>1.6. Statistical Distributions</title><p>To analyse severity in that sense pertaining to body of the distribution, following distributions can be used, given their densities:</p><p>Lognormal distribution density  (Hazewinkel, 2001) :</p><disp-formula id="scirp.59341-formula99"><label>(15)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2410129x95.png"  xlink:type="simple"/></disp-formula><p>Weibull density distribution:</p><p>The probability density function of a Weibull random variable  (Hazewinkel, 2001)  is:</p><disp-formula id="scirp.59341-formula100"><label>(16)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2410129x96.png"  xlink:type="simple"/></disp-formula><p>where k &gt; 0 is the shape parameter and λ &gt; 0 is the scale parameter of the distribution. Its complementary cumulative distribution function is a stretched exponential function. The Weibull distribution is related to a number of other probability distributions; in particular, it interpolates between the exponential distribution (k = 1)</p><p>and the Rayleigh distribution (k = 2 and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x97.png" xlink:type="simple"/></inline-formula>)</p><p>Loglogistic probability density function is defined in the following way:</p><disp-formula id="scirp.59341-formula101"><label>(17)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2410129x98.png"  xlink:type="simple"/></disp-formula><p>The parameter <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x99.png" xlink:type="simple"/></inline-formula> is a scale parameter and is also the median of the distribution. The parameter <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x99.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x100.png" xlink:type="simple"/></inline-formula> is a shape parameter. The distribution is unimodal when <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x99.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x100.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x101.png" xlink:type="simple"/></inline-formula> and its dispersion decreases as <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x99.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x100.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x101.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x102.png" xlink:type="simple"/></inline-formula> increases.</p><p>The following functions are shown in the graphs below:</p><p><xref ref-type="fig" rid="fig3">Figure 3</xref> shows probability density functions of Loglogistic, Weibull and lognormal distributions.</p><p>At the same time, we will introduce Champernowne distribution  (Hazewinkel, 2001)  that we will also be using, its probability density function is given in the graph below:</p><disp-formula id="scirp.59341-formula102"><label>(18)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2410129x103.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x104.png" xlink:type="simple"/></inline-formula> are positive parameters, and n is the normalizing constant, which depends on the parameters.</p><fig-group id="fig3"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> Loglogistic, Weibull and lognormal probability density functions respectively.</title></caption><fig id ="fig3_1"><label>(b)</label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-2410129x105.png"/></fig><fig id ="fig3_2"><label> (c)</label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-2410129x106.png"/></fig><fig id ="fig3_3"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-2410129x107.png"/></fig></fig-group><p>When obtaining copula, Monte Carlo method will be used, so we will introduce it shortly.</p><p>One is interested in the expectation of a response function <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x108.png" xlink:type="simple"/></inline-formula> applied to some random vector</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x109.png" xlink:type="simple"/></inline-formula>. If we denoted the cumulative distribution function of this random vector with<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x109.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x110.png" xlink:type="simple"/></inline-formula>, the quantity of interest can thus be written as:</p><disp-formula id="scirp.59341-formula103"><label>(19)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2410129x111.png"  xlink:type="simple"/></disp-formula><p>If <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x112.png" xlink:type="simple"/></inline-formula> is given by a copula model, example:</p><disp-formula id="scirp.59341-formula104"><label>(20)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2410129x113.png"  xlink:type="simple"/></disp-formula><p>Then expectation can be written as:</p><disp-formula id="scirp.59341-formula105"><label>(21)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2410129x114.png"  xlink:type="simple"/></disp-formula><p>In case the copula <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x115.png" xlink:type="simple"/></inline-formula> is absolutely continuous, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x115.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x116.png" xlink:type="simple"/></inline-formula>has density c, the equation can be written as</p><disp-formula id="scirp.59341-formula106"><label>(22)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2410129x117.png"  xlink:type="simple"/></disp-formula><p>If copula and margins are known (or if they have been estimated), then the following Monte Carlo algorithm can be used:</p><p>1) Draw a sample <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x118.png" xlink:type="simple"/></inline-formula> of size n from the copula C</p><p>2) By applying the inverse marginal cdf’s, produce a sample of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x119.png" xlink:type="simple"/></inline-formula> by setting</p><disp-formula id="scirp.59341-formula107"><graphic  xlink:href="http://html.scirp.org/file/1-2410129x120.png"  xlink:type="simple"/></disp-formula><p>3) Approximate <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x121.png" xlink:type="simple"/></inline-formula> by its empirical value:</p><disp-formula id="scirp.59341-formula108"><label>(23)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2410129x122.png"  xlink:type="simple"/></disp-formula></sec><sec id="s1_7"><title>1.7. VAR and Expected Shortfall</title><p>After having introduced all the necessary tools for operational risk model in insurance, we will just provide the VAR and expected shortfall definition  (Longin, 1997)  and then we are going to present the modeling results.</p><disp-formula id="scirp.59341-formula109"><label>(24)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2410129x123.png"  xlink:type="simple"/></disp-formula><p>Confidence level<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x124.png" xlink:type="simple"/></inline-formula>, the VaR  (Longin, 1997)  of the portfolio at the confidence level <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x124.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x125.png" xlink:type="simple"/></inline-formula> is given by the smallest number <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x124.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x125.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x126.png" xlink:type="simple"/></inline-formula> such that the probability that the loss <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x124.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x125.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x126.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x127.png" xlink:type="simple"/></inline-formula> exceeds <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x124.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x125.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x126.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x127.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x128.png" xlink:type="simple"/></inline-formula> is at most<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x124.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x125.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x126.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x127.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x128.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x129.png" xlink:type="simple"/></inline-formula>. Mathematically, if <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x124.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x125.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x126.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x127.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x128.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x129.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x130.png" xlink:type="simple"/></inline-formula> is the loss of a portfolio, then <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x124.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x125.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x126.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x127.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x128.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x129.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x130.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x131.png" xlink:type="simple"/></inline-formula> is the level <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x124.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x125.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x126.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x127.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x128.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x129.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x130.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x131.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x132.png" xlink:type="simple"/></inline-formula> quantile.</p><p>In order to model tails, Generalized Pareto distribution will be used.</p><p>The standard cumulative distribution function (cdf) of the GPD is defined by<sup> </sup></p><disp-formula id="scirp.59341-formula110"><label>(25)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2410129x133.png"  xlink:type="simple"/></disp-formula><p>where the support is <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x134.png" xlink:type="simple"/></inline-formula> for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x134.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x135.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x134.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x135.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x136.png" xlink:type="simple"/></inline-formula> for<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x134.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x135.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x136.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x137.png" xlink:type="simple"/></inline-formula>.</p><disp-formula id="scirp.59341-formula111"><label>(26)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2410129x138.png"  xlink:type="simple"/></disp-formula><p>Expected shortfall</p><p>Expected shortfall is defined as</p><disp-formula id="scirp.59341-formula112"><label>(27)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2410129x139.png"  xlink:type="simple"/></disp-formula><p>Or equivalently can be written as:</p><disp-formula id="scirp.59341-formula113"><label>(28)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2410129x140.png"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.59341-formula114"><label>(29)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2410129x141.png"  xlink:type="simple"/></disp-formula><p>is the lower <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x142.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x142.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x143.png" xlink:type="simple"/></inline-formula> is the indicator function.</p></sec></sec><sec id="s2"><title>2. Experimental Results</title><p>After having introduced all the necessary tools, the experimental results will be presented. As we are considering operational risk models in insurance, we will use the following tools. The procedure is the following. As we don’t have enough data, we will use random number generator, let it simulate the events, but at the same defining that extreme events don’t occur frequently. Afterwards we will implement the distribution for body and tail of the severity of distribution. Frequency of events was modeled by using Poisson distribution. A standard choice to estimate annual frequency of operational risk loss is performed by using Poisson distribution. On the basis of extreme value theory, the distribution function of loss data above a high threshold <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x144.png" xlink:type="simple"/></inline-formula> is supposed to follow a Generalized Pareto distribution. Lognormal distribution will be used for modeling body of severity distribution. Afterwards, we use the convolution method using frequency and severity distribution and we obtain annual loss distribution. Convolution is performed by using Monte-Carlo method.</p><p>Following steps are performed:</p><p>1) Extract one random number <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x145.png" xlink:type="simple"/></inline-formula> from frequency distribution</p><p>2) Extract <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x146.png" xlink:type="simple"/></inline-formula> random numbers <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x146.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x147.png" xlink:type="simple"/></inline-formula> from severity distribution</p><p>3) Obtain a possible figure of yearly op. loss <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x148.png" xlink:type="simple"/></inline-formula></p><p>Repeat <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x149.png" xlink:type="simple"/></inline-formula> times and we obtain annual loss distribution. In order to obtain overall annual loss distribution, we use the following procedure:</p><p>・ Extract one random value <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x150.png" xlink:type="simple"/></inline-formula> from copula function</p><p>・ Extract n random numbers from loss distributions related to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x151.png" xlink:type="simple"/></inline-formula> risk classes</p><p>・ Sum yearly losses to obtain overall annual loss distribution</p><p>If the real data is used, then to estimate the parameters maximum likelihood, method of moments, probability weighted method of moments should be used.</p><p>The simulation results are given below:</p><disp-formula id="scirp.59341-formula115"><graphic  xlink:href="http://html.scirp.org/file/1-2410129x152.png"  xlink:type="simple"/></disp-formula><p>The body of distribution is considered to be lognormal. The first fit value is the mean and the other one is standard deviation. The gradient of the function demonstrates where the function is 0.</p><p>In <xref ref-type="fig" rid="fig4">Figure 4</xref>, optimisation values are given for different theta 1 and theta 2 that represent optimal values. Goodness of fit can also be performed, if the real data is used. <xref ref-type="fig" rid="fig7">Figure 7</xref> shows negative log-likelihood method for fitting log-normal distribution. In that direction, Kolmogorov-Smirnov and Anderson-Darling test statistics are used, but this is left for further research.</p><p>To estimate the tail of the severity distribution, we have to set a high threshold<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x153.png" xlink:type="simple"/></inline-formula>: the parameters are estimated on excess over threshold using probability weighted moments, maximum likelihood method etc. Mean excess function is defined in the following way:</p><disp-formula id="scirp.59341-formula116"><label>(30)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2410129x154.png"  xlink:type="simple"/></disp-formula><p>What should be noticed is that if the mean excess function for Generalized Pareto distribution is a linear function of u, if the empirical mean excess function is a straight line above a threshold, it is an indication that the excess over <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410129x155.png" xlink:type="simple"/></inline-formula> follows a generalized Pareto distribution, which is shown in the <xref ref-type="fig" rid="fig8">Figure 8</xref>.</p><p>It is obvious that <xref ref-type="fig" rid="fig5">Figure 5</xref> demonstrates that the tail of severity distribution is following Generalized Pareto distribution. QQ plots of the Generalized Pareto distribution using maximum likelihood method and probability weighted method of moments.</p><p>Q-Q plots in <xref ref-type="fig" rid="fig6">Figure 6</xref> demonstrate that the tail of severity distribution is characterised by generalized Pareto distribution. Results are the following. Using the aforementioned methods, the following results are obtained:</p><fig-group id="fig4"><label><xref ref-type="fig" rid="fig4">Figure 4</xref></label><caption><title> Neg-log likelihood for fitting log-normal distribution with random number generator.</title></caption><fig id ="fig4_1"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-2410129x156.png"/></fig><fig id ="fig4_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-2410129x157.png"/></fig></fig-group><fig id="fig5"  position="float"><label><xref ref-type="fig" rid="fig5">Figure 5</xref></label><caption><title> Mean excess function</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-2410129x158.png"/></fig><p>To analyse the loss frequency, we assume Poisson process and obtain the following results:</p><p><xref ref-type="fig" rid="fig7">Figure 7</xref> shows loss frequency distribution for Poisson case.</p><p>After having introduced the severity and loss frequency distribution, we use the convolution method to obtain annual loss distribution. The code will be given in the appendix, so that the calculation can be performed.</p><p>The annual loss distributions are obtained in <xref ref-type="fig" rid="fig8">Figure 8</xref>.</p><p><xref ref-type="fig" rid="fig8">Figure 8</xref> shows annual loss distribution as a result of convolution method, it is the combination of lognormal and generalized Pareto distribution.</p><p>It is the combination of lognormal and generalized Pareto distribution, therefore because they differ and vary from sample to sample, the copula method should be used to obtain overall annual loss distribution  (Hazewinkel, 2001) .</p><p>Using Student t-copula, overall loss distribution is calculated and code that can be replicated is given, together with the VaR  (Longin, 1997)  results which are shown in <xref ref-type="fig" rid="fig9">Figure 9</xref>.</p><p>The code given in appendix demonstrates how to calculate VaR and copula for overall loss distribution. At the same time, some results are given for Value at Risk, expected loss and capital requirements. The given calculations and results demonstrate how to model risk in insurance by using lognormal and generalized Pareto distribution. At the same time distribution can be changed depending of the situation. This approach introduces modeling of operational risk in insurance and financial institutions and represents a review of the state of art techniques.</p></sec><sec id="s3"><title>3. Conclusion</title><p>This paper introduces the state of the art techniques in operational risk modeling. It begins by presenting Solvency II and Basel II criteria. Afterwards it introduces statistical and mathematical techniques. Consequently, it presents modeling techniques by introducing Generalized Pareto distribution which is used in operational risk models in insurance and banking. The aforementioned paper represents a review in operational risk models in</p><fig-group id="fig6"><label><xref ref-type="fig" rid="fig6">Figure 6</xref></label><caption><title> QQ plots with maximum likelihood method and probability weighted moments.</title></caption><fig id ="fig6_1"><label> (b)</label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-2410129x160.png"/></fig><fig id ="fig6_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-2410129x159.png"/></fig></fig-group><fig id="fig7"  position="float"><label><xref ref-type="fig" rid="fig7">Figure 7</xref></label><caption><title> Loss frequency distribution Results: lambda Sample 532 &gt; lambda 791.7354</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-2410129x161.png"/></fig><fig id="fig8"  position="float"><label><xref ref-type="fig" rid="fig8">Figure 8</xref></label><caption><title> Annual loss distribution</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-2410129x162.png"/></fig><fig id="fig9"  position="float"><label><xref ref-type="fig" rid="fig9">Figure 9</xref></label><caption><title> Copula method for obtaining overall annual loss distribution</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-2410129x163.png"/></fig><p>insurance. It introduces techniques that can be used in modeling operational risk in insurance and banking, and it can be immediately applied. Hopefully, this review will provide further research in risk models and provide new ideas that can be applied to operational risk in whole.</p></sec><sec id="s4"><title>Acknowledgements and Declaration of Interest Section</title><p>The authors report no conflicts of interest. The authors alone are responsible for the content and writing of the paper. I would like to thank my family for the immense support.</p></sec><sec id="s5"><title>Cite this paper</title><p>OgnjenVukovic, (2015) Operational Risk Modelling in Insurance and Banking. Journal of Financial Risk Management,04,111-123. doi: 10.4236/jfrm.2015.43010</p></sec><sec id="s6"><title>Appendix</title>Convolution Method Code in R to Obtain Overall Annual Loss Distribution<p>install.packages(‘evir’)</p><p>library(evir)</p><p># Quantile function of lognormal-GPD severity distribution</p><p>qlnorm.gpd = function(p, theta, theta.gpd, u)</p><p>{</p><p>Fu = plnorm(u, meanlog=theta[<xref ref-type="bibr" rid="scirp.59341-ref1">1</xref>], sdlog=theta[<xref ref-type="bibr" rid="scirp.59341-ref2">2</xref>])</p><p>x = ifelse(p</p><p>qlnorm( p=p, meanlog=theta[<xref ref-type="bibr" rid="scirp.59341-ref1">1</xref>], sdlog=theta[<xref ref-type="bibr" rid="scirp.59341-ref2">2</xref>] ),</p><p>qgpd( p=(p - Fu) / (1 - Fu) , xi=theta.gpd[<xref ref-type="bibr" rid="scirp.59341-ref1">1</xref>], mu=theta.gpd[<xref ref-type="bibr" rid="scirp.59341-ref2">2</xref>], beta=theta.gpd[<xref ref-type="bibr" rid="scirp.59341-ref3">3</xref>]) )</p><p>return(x)</p><p>}</p><p># Random sampling function of lognormal-GPD severity distribution</p><p>rlnorm.gpd = function(n, theta, theta.gpd, u)</p><p>{ r = qlnorm.gpd(runif(n), theta, theta.gpd, u)}</p><p>set.seed(1000)</p><p>nSim = 10000# Number of simulated annual losses</p><p>H = 1500 # Threshold body-tail</p><p>lambda = 791.7354 # Parameter of Poisson body</p><p>theta1 = 2.5 # Parameter mu of lognormal (body)</p><p>theta2 = 2 # Parameter sigma of lognormal (body)</p><p>theta1.tail = 0.5 # Shape parameter of GPD (tail)</p><p>theta2.tail = H # Location parameter of GPD (tail)</p><p>theta3.tail = 1000 # Scale parameter of GPD (tail)</p><p>sj = rep(0,nSim) # Annual loss distribution inizialization</p><p>freq = rpois(nSim, lambda) # Random sampling from Poisson</p><p>for(i in 1:nSim) # Convolution with Monte Carlo method</p><p>sj[i] = sum(rlnorm.gpd(n=freq[i], theta=c(theta1,theta2), theta.gpd=c(theta1.tail, theta2.tail, theta3.tail), u=H))</p><p>sj[i]</p>Code to Calculate Overall Loss Distribution with VAR Results<p>&gt;library(QRM)</p><p>&gt;set.seed(1000)</p><p>&gt;nSim = 1000000 # Number of simulated overall annual losses</p><p>&gt;s1 = rlnorm(n=nSim, meanlog=4.5, sdlog=2.3) # Loss distribution risk class 1</p><p>&gt;s2 = rlnorm(n=nSim, meanlog=5, sdlog=2.5) # Loss distribution risk class 2</p><p>&gt;VaR.s1 = quantile(s1, 0.999) # VaR risk class 1</p><p>&gt;VaR.s2 = quantile(s2, 0.999) # VaR risk class 2</p><p>&gt;corr = 0.6 # Correlation among risk classes</p><p>&gt;corrMatrix = matrix(data=c(1,corr,corr,1), nrow=2) # correlation matrix</p><p>&gt;dof = 5 # degrees of freedom</p><p>&gt;simCopulaT = rcopula.t(n=nSim, df=dof, Sigma=corrMatrix) # Simulations from Student-t copula</p><p>&gt;s = quantile(s1, simCopulaT[,1]) + quantile(s2, simCopulaT[,2]) # overall annual loss distribution</p><p>&gt;VaR.s = quantile(s, 0.999)</p><p>&gt;divEff = (VaR.s1+VaR.s-VaR.s)/(VaR.s1+VaR.s) # diversification effect</p><p>&gt;EL = quantile(s, 0.5) # Expected loss</p><p>&gt;capReq = VaR.s - EL # Capital requirement</p><p>&gt;VaR.s1; VaR.s2; VaR.s; divEff; EL; capReq</p><p>99.9%</p><p>111300.8</p><p>99.9%</p><p>339577.2</p><p>99.9%</p><p>410748.6</p><p>99.9%</p><p>0.2131997</p><p>50%</p><p>355.3662</p><p>99.9%</p><p>410393.2</p></sec></body><back><ref-list><title>References</title><ref id="scirp.59341-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">(2012). 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