<?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.2017.63017</article-id><article-id pub-id-type="publisher-id">JFRM-78354</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>
 
 
  Modeling and Quantifying of the Global Wrong Way Risk
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Badreddine</surname><given-names>Slime</given-names></name><xref ref-type="aff" rid="aff1"><sub>1</sub></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff1"><label>1</label><addr-line>Financial Risk Quant from ENSAE (Ecole Nationale de la Statistique et de l’Administration Economique), Paris, France</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>badreddine.slime@gmail.com</email></corresp></author-notes><pub-date pub-type="epub"><day>11</day><month>08</month><year>2017</year></pub-date><volume>06</volume><issue>03</issue><fpage>231</fpage><lpage>246</lpage><history><date date-type="received"><day>June</day>	<month>18,</month>	<year>2017</year></date><date date-type="rev-recd"><day>Accepted:</day>	<month>August</month>	<year>8,</year>	</date><date date-type="accepted"><day>August</day>	<month>11,</month>	<year>2017</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 counterparty risk issue has become increasingly important in the world of finance. This risk is defined as the loss due to the counterparty default. The regulator uses the Credit Value Adjustment (
  
  CVA
  ) to measure this risk. However, there is the independency assumption between the default and the exposure behind the 
  
  CVA
   computation and it is not verified on the financial market. This paper presents two mathematical models for the assessment and the quantification of the counterparty risk without this assumption. This kind of risk is known as Wrong Way Risk (
  
  WWR
  ). This study focuses on t
  h
  ree approaches: empirical, copula and mixed model. The first one is based on the hazard rate modelling to express the correlation between the probability of default and the exposure. The second one is about calculating the 
  
  WWR
   effect using copulas. The last one is a combination of both. There is another assumption that makes easier the 
  
  CVA
   computation: The constant of the loss given default (
  
  LGD
  ). As we know this assumption is not verified because the 
  
  LGD
   could be deterministic or stochastic. Otherwise, it could lead to a 
  correlation effect
   between the 
  
  LGD
  , the exposure and the default, and we then obtain a Global Wrong Way Risk (
  
  GWWR
  ). Indeed, we propose a model allowing the 
  
  CVA
   quantification without these assumptions.
 
</p></abstract><kwd-group><kwd>Counterparty Risk</kwd><kwd> Credit Value Adjustment</kwd><kwd> Wrong Way Risk</kwd><kwd> Copulas</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>The credit value adjustment (CVA) computation is based on the independency assumption between the exposure and the default. However,this assumption is not verified on the market, and we although have correlation between the probability of default (PD) and the exposure at default (EAD). Therefore, we get two types of this effect: The Wrong Way Risk (WWR) when the correlation is positive and the Right Way Risk (RWR) when the correlation in this case is negative. There is another effect appears when the LGD becomes random and also depends on the default. Indeed, this could generate a correlation between the three variables that make the CVA assessment. In this case, we could call this effect as the Global Wrong Way Risk (GWWR). First, we will focus on the WWR effect and we make the difference between two kinds:</p><p>・ The systemic WWR: this kind arises at the moment where the dependency between the exposure and the default is due to a macroeconomic factor. In this case, this factor increases the EAD and the PD. If we take a put on the CAC40 index with some bank like Soci&#233;t&#233; G&#233;n&#233;ral (SG) as the issuer, then the CAC40 spot impacts both of the exposure and the counterparty rating. In fact, this index is a systemic factor in the French market and the SG is a part of the CAC40 composition.</p><p>・ The specific WWR: on the other hand, this kind comes from a specific factor. For example, we get this effect when we have a put on the stock of the issuer as underlying.</p><p>There are several models allowing the CVA computation with the WWR component. We present some of these approaches:</p><p>・ The Basel model<sup>1</sup> (  Basel Committee on Banking Supervision, 2010 ): this approach is the most straightforward one to add the correlation effect and it is used by the Basel committee to add the WWR effect in the counterparty credit risk (CCR) charge. It is based on the multiplier coefficient<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x3.png" xlink:type="simple"/></inline-formula>, to explain this effect. The exposure at default is given by the formula bellow:</p><disp-formula id="scirp.78354-formula1"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x4.png"  xlink:type="simple"/></disp-formula><p>With <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x5.png" xlink:type="simple"/></inline-formula> represents the expected effective positive exposure.</p><p>We have by default<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x6.png" xlink:type="simple"/></inline-formula>, whatever, banks could have values above 1.2. Other institutions use values bigger than the default one. The coefficient value is appreciated, on one hand, by the name concentration and that also means the portfolio granularity by counterparties. On the other hand, we have the correlation effects between assets of the same counterparty. The Basel II accords do not give details to manage the WWR. However, Basel III brings more precision to manage this kind of risk, focusing on three aspects:</p><p>&#216; Implementation of a detailed process to manage the WWR.</p><p>&#216; Advising banks to put more provision to cover the counterparty risk.</p><p>&#216; Explication of the approach to manage transactions containing the specific WWR.</p><p>The implementation of this model remains easy and could be automatically integrated to the existent model, but it has two drawbacks:</p><p>&#216; It does not give the contribution part of the WWR.</p><p>&#216; It consumes more capital requirement to cover the counterparty risk, because the standard approach is designed for the worst case.</p><p>・ The empirical approach: this approach uses the hazard rate according to the exposure. Indeed, the relation between these two quantities allows getting the diffusion of the PD, and then it could explain the correlation with the exposure. The WWR modeling progresses into three steps:</p><p>&#216; The choice of the function that gives the relation between the hazard rate and the exposure. The diffusion calculation is performed for each time step:</p><disp-formula id="scirp.78354-formula2"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x7.png"  xlink:type="simple"/></disp-formula><p>With <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x9.png" xlink:type="simple"/></inline-formula> represents the exposure. Hull and White<sup>2</sup> (  Hull &amp; White 2012 ) suggests an exponential function to implement this method.</p><p>&#216; The PD computation is done using the below formula:</p><disp-formula id="scirp.78354-formula3"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x10.png"  xlink:type="simple"/></disp-formula><p>&#216; The computation of the CVA WWR using the Monte Carlo simulation. This step is deduced directly from the exposure diffusion.</p><p>This approach allows a straight integration within the existent CVA model. In fact, it replaces the computed PDs under the independency assumption with the new one using the dependency between the default and the exposure.</p><p>・ The copula model: This approach is based on copulas to explain the relation between the default variable and the exposure. Rosen and Saunders<sup>3</sup> (  Rosen &amp; Saunders 2012 ) use the Vasicek model to make this dependency. They introduced the Gaussian copula to compute the expected exposure without the independency assumption. Their model is implemented in three steps:</p><p>&#216; The default is written as a latent variable and it is divided in two components. The first part represents the specific risk, and the second part is the systemic risk:</p><disp-formula id="scirp.78354-formula4"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x11.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x12.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x13.png" xlink:type="simple"/></inline-formula> are two independent random variables and they follow a Gaussian distribution. The counterparty is deemed in default when <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x14.png" xlink:type="simple"/></inline-formula> is lower than<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x15.png" xlink:type="simple"/></inline-formula>. The conditional probability of default regarding to the systemic variable is expressed as:</p><disp-formula id="scirp.78354-formula5"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x16.png"  xlink:type="simple"/></disp-formula><p>With <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x17.png" xlink:type="simple"/></inline-formula> represents the unconditional probability of default.</p><p>&#216; Future exposures are mapped to a market variable <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x18.png" xlink:type="simple"/></inline-formula> that also follows a Gaussian distribution. The relation between this variable and the exposure is:</p><disp-formula id="scirp.78354-formula6"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x19.png"  xlink:type="simple"/></disp-formula><p>With <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x20.png" xlink:type="simple"/></inline-formula> represents the distribution function of exposure and it is uniform.</p><p>&#216; This model supposes that the two variables <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x21.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x21.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x22.png" xlink:type="simple"/></inline-formula> are linked to a bivariate joint distribution. This relation is expressed under a Gaussian copula with the correlation <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x21.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x22.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x23.png" xlink:type="simple"/></inline-formula> between both of variables. Bocker and Brunnbauer<sup>4</sup> (  Bocker &amp; Brunnbauer, 2014 ) generalized this concept to use others copulas. This approach allows a straight integration within the existent CVA model.</p><p>The next section will be devoted to the WWR mathematical modeling using a mixed model. Indeed, we will use the empirical model to build the diffusion of PDs, and then we will explain the relation between the default and the exposure under copulas model.</p></sec><sec id="s2"><title>2. Mathematical Modeling of the WWR</title><p>The Credit Value Adjustment (CVA) is defined by the difference between the portfolio value without the counterparty default and with this component. The CVA could be written as:</p><disp-formula id="scirp.78354-formula7"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x25.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x26.png" xlink:type="simple"/></inline-formula> represents the risk free portfolio value, and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x26.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x27.png" xlink:type="simple"/></inline-formula> is the portfolio value taking in consideration the counterparty default.</p><p>Using this, we find the following formula:</p><disp-formula id="scirp.78354-formula8"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x28.png"  xlink:type="simple"/></disp-formula><p>With <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x29.png" xlink:type="simple"/></inline-formula> is the default time, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x29.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x30.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x29.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x30.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x31.png" xlink:type="simple"/></inline-formula>represents the discount factor, and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x29.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x30.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x31.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x32.png" xlink:type="simple"/></inline-formula> defines the Loss Given Default that we deem constant in this section.</p><p>We also can write:</p><disp-formula id="scirp.78354-formula9"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x33.png"  xlink:type="simple"/></disp-formula><p>where<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x34.png" xlink:type="simple"/></inline-formula>, and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x34.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x35.png" xlink:type="simple"/></inline-formula> defines the distribution of the default.</p><p>First, we begin by modeling the probability of default using the empirical model. For this, we introduce the hazard rate concept that measures the counterparty default occurrence. Giving the assumption that the default frequency follows the Poisson density, we get the formula below:</p><disp-formula id="scirp.78354-formula10"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x36.png"  xlink:type="simple"/></disp-formula><p>The relation between the<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x37.png" xlink:type="simple"/></inline-formula>, and the exposure is written as:</p><disp-formula id="scirp.78354-formula11"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x38.png"  xlink:type="simple"/></disp-formula><p>With <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x39.png" xlink:type="simple"/></inline-formula> is defined positive since<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x40.png" xlink:type="simple"/></inline-formula>.</p><p>This function should also verify the following relation under the assumption that the hazard rates curve is flat:</p><disp-formula id="scirp.78354-formula12"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x41.png"  xlink:type="simple"/></disp-formula><p>With <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x42.png" xlink:type="simple"/></inline-formula> defines the arithmetic average of simulated values until the date<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x42.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x43.png" xlink:type="simple"/></inline-formula>, and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x42.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x43.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x44.png" xlink:type="simple"/></inline-formula> is the market spread with the maturity of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x42.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x43.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x44.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x45.png" xlink:type="simple"/></inline-formula>.</p><p>We deem the following function of the hazard rate:</p><disp-formula id="scirp.78354-formula13"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x46.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x47.png" xlink:type="simple"/></inline-formula> is a function of time and determines the correlation between <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x47.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x48.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x47.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x48.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x49.png" xlink:type="simple"/></inline-formula>, and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x47.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x48.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x49.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x50.png" xlink:type="simple"/></inline-formula> is a function of time.</p><p>We can find the stochastic derivative equation (SDE) of the hazard rate by applying the It&#244;’s lemma on the<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x51.png" xlink:type="simple"/></inline-formula>, and we get:</p><disp-formula id="scirp.78354-formula14"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x52.png"  xlink:type="simple"/></disp-formula><p>With<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x53.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x53.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x54.png" xlink:type="simple"/></inline-formula>defines the volatility of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x53.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x54.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x55.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x53.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x54.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x55.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x56.png" xlink:type="simple"/></inline-formula> repre- sents the Brownian motion under the risk neutral measure.</p><p>We conclude that the hazard rate follows a log-normal distribution with parameters below:</p><disp-formula id="scirp.78354-formula15"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x57.png"  xlink:type="simple"/></disp-formula><p>In our case, we more interest about the distribution of the time integration of the<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x59.png" xlink:type="simple"/></inline-formula>. If we take the following approximation <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x59.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x60.png" xlink:type="simple"/></inline-formula> and by using the Fenton-Wilkinson<sup>5</sup> (  Fenton, 1960 ) approach, this quantity then follows a log-normal distribution with parameters below:</p><disp-formula id="scirp.78354-formula16"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x61.png"  xlink:type="simple"/></disp-formula><p>With,</p><disp-formula id="scirp.78354-formula17"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x62.png"  xlink:type="simple"/></disp-formula><p>It also supposes that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x63.png" xlink:type="simple"/></inline-formula> are independent. We get the following result by applying the Laplace transform approximation:</p><disp-formula id="scirp.78354-formula18"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x64.png"  xlink:type="simple"/></disp-formula><p>If<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x65.png" xlink:type="simple"/></inline-formula>, then <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x65.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x66.png" xlink:type="simple"/></inline-formula></p><p>The calibration is made in each time of the Monte Carlo simulation. Indeed, we minimize the distance between the PD model and the PD market basing on spreads. So, we need to do this process <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x67.png" xlink:type="simple"/></inline-formula> times using the discretization form of the hazard rate:</p><disp-formula id="scirp.78354-formula19"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x68.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x69.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x69.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x70.png" xlink:type="simple"/></inline-formula> represent the j<sup>th</sup> simulation of the exposure and the hazard rate.</p><p>The Appropriate parameters are those who minimize the following quantity:</p><disp-formula id="scirp.78354-formula20"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x71.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x72.png" xlink:type="simple"/></inline-formula> is the Monte Carlo number of simulation, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x72.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x73.png" xlink:type="simple"/></inline-formula>is the number of steps time, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x72.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x74.png" xlink:type="simple"/></inline-formula>and represents the spread with maturity<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x72.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x74.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x75.png" xlink:type="simple"/></inline-formula>.</p><p>Finally, when the parameters are computed, then the hazard rates are built sequentially at each time step. The next step allows to define the relation between the exposure and the probability of default distribution. Therefore, we use the copulas to get this relation, and we take the following definitions:</p><p>・ The value of the discount exposure <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x76.png" xlink:type="simple"/></inline-formula> at time <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x76.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x77.png" xlink:type="simple"/></inline-formula> follows a distribution<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x76.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x77.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x78.png" xlink:type="simple"/></inline-formula> with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x76.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x77.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x78.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x79.png" xlink:type="simple"/></inline-formula> her density function.</p><p>・ The default time of the counterparty <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x80.png" xlink:type="simple"/></inline-formula> is a random variable and we note his distribution function by <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x80.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x81.png" xlink:type="simple"/></inline-formula> and with the density<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x80.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x81.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x82.png" xlink:type="simple"/></inline-formula>.</p><p>・ The joint distribution of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x83.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x83.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x84.png" xlink:type="simple"/></inline-formula> is defined by:</p><disp-formula id="scirp.78354-formula21"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x85.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x86.png" xlink:type="simple"/></inline-formula> indicates the bivariate copula and we suppose <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x86.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x87.png" xlink:type="simple"/></inline-formula> is twice continuously differentiable function. The density function is written as:</p><disp-formula id="scirp.78354-formula22"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x88.png"  xlink:type="simple"/></disp-formula><p>The expected positive exposure (EPE) is equal to:</p><disp-formula id="scirp.78354-formula23"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x89.png"  xlink:type="simple"/></disp-formula><p>With <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x90.png" xlink:type="simple"/></inline-formula></p><p>We also have:</p><disp-formula id="scirp.78354-formula24"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x91.png"  xlink:type="simple"/></disp-formula><p>We then replace the value of the conditional density in the formula to get the following result:</p><disp-formula id="scirp.78354-formula25"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x92.png"  xlink:type="simple"/></disp-formula><p>By applying the strong law of large number, we obtain the following approximation of the EPE:</p><disp-formula id="scirp.78354-formula26"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x93.png"  xlink:type="simple"/></disp-formula><p>It remains one issue to complete those calculations; we are talking about the estimation of the correlation between the exposure and the probability of default. In fact, it is the requirement parameter to compute<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x94.png" xlink:type="simple"/></inline-formula>. We suggest two approaches to do this estimation:</p><p>・ The first one uses the Spearman<sup>6</sup> (  Daniel, 1990 ) correlation who is defined as:</p><disp-formula id="scirp.78354-formula27"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x96.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x97.png" xlink:type="simple"/></inline-formula> presents the ranks difference between the exposure and the probability of default, and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x97.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x98.png" xlink:type="simple"/></inline-formula> is the number of observations. We compute this correlation at each time step and we use the result of the hazard rate</p><p>diffusion for this. Finally, we can estimate the correlation by<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x99.png" xlink:type="simple"/></inline-formula>.</p><p>・ The second one is based on the minimization of the difference between the simulated survival probabilities at time <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x100.png" xlink:type="simple"/></inline-formula> using the hazard rate model and the copula at each time step:</p><disp-formula id="scirp.78354-formula28"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x101.png"  xlink:type="simple"/></disp-formula><p>We then can estimate the correlation by<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x102.png" xlink:type="simple"/></inline-formula>.</p><p>We have now all components to complete the CVA computation with the WWR effect. It remains to calculate all <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x103.png" xlink:type="simple"/></inline-formula> and apply the trapezoid integration method regarding to the PDs to get the value. The implementation of the mixed model approach will be done on the CAC40 European put option. We will use the HESTON<sup>7</sup> (  Heston, 1993 ) model to compute the put price that is based on the stochastic volatility. We then take the following assumptions:</p><p>・ The Loss Given Default <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x104.png" xlink:type="simple"/></inline-formula> is constant and equal to 60%.</p><p>・ The discretization of time space is done on 100 steps.</p><p>・ The dividends are equals to 0.</p><p>・ The credit spread of the counterparty is constant and equal to 0.8%.</p><p>・ The CAC40 put strike value is 4350.</p><p>・ The Credit Support Annex (CSA) contains a Margin Call with 10 days as Margin Dates and the calculation will be done with and without collateral.</p><p>The value of the correlation between exposures and defaults using Spearman is equal to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x105.png" xlink:type="simple"/></inline-formula>. The <xref ref-type="fig" rid="fig1">Figure 1</xref> shows the evolution of the EPE regarding to the PD with and without collateral using the Gaussian copula:</p><p>We conclude that the EPE increases with the WWR effect and the CVA will also have the same behavior. The <xref ref-type="fig" rid="fig2">Figure 2</xref> displays this effect:</p><p>The WWR increases the CVA quantity with 30%, and that proves its importance and impact on the counterparty risk measurement. The <xref ref-type="table" rid="table1">Table 1</xref> summarizes these results.</p><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> Expected positive exposure with and without WWR effect</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-2410227x106.png"/></fig><fig id="fig2"  position="float"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> CVA and WWR effect with and without collateral</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-2410227x107.png"/></fig><table-wrap id="table1" ><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> CVA WWR calculation results</title></caption><table><tbody><thead><tr><th align="center" valign="middle" ></th><th align="center" valign="middle" >Without Collateral</th><th align="center" valign="middle" >With Collateral</th></tr></thead><tr><td align="center" valign="middle" >CVA</td><td align="center" valign="middle" >0.002979613</td><td align="center" valign="middle" >0.000374312</td></tr><tr><td align="center" valign="middle" >CVA(WWR)</td><td align="center" valign="middle" >0.003501835</td><td align="center" valign="middle" >0.000521428</td></tr></tbody></table></table-wrap></sec><sec id="s3"><title>3. The Global Wrong Way Risk (GWWR)</title><p>As we saw in the last section, the compute of the CVA supposes that the LGD is constant. Furthermore, this assumption leads to the independency of this variable to the default. Nevertheless, the LGD depends to the default and automatically to the exposure, because the WWR proves that there is a dependency between the exposure and the default. We choose the word “Global” because we study the dependency between the three components that allow the calculation of the CVA. In order to model the Global Wrong Way Risk, we suggest two approaches:</p><p>・ The first approach is based on the building of a relation between the LGD and the exposure, and also, the definition of the relation between the exposure and the default. We use the same notation in the last section and we link the LGD with the exposure through the below function:</p><disp-formula id="scirp.78354-formula29"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x108.png"  xlink:type="simple"/></disp-formula><p>With<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x109.png" xlink:type="simple"/></inline-formula>.</p><p>We then replace in the CVA formula:</p><disp-formula id="scirp.78354-formula30"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x110.png"  xlink:type="simple"/></disp-formula><p>There is two ways to compute this expectation, on one hand; we can make it with empirical approach. We define the relation below:</p><disp-formula id="scirp.78354-formula31"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x111.png"  xlink:type="simple"/></disp-formula><p>With <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x112.png" xlink:type="simple"/></inline-formula> is defined positive since<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x112.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x113.png" xlink:type="simple"/></inline-formula>.</p><p>We so get the following result:</p><disp-formula id="scirp.78354-formula32"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x114.png"  xlink:type="simple"/></disp-formula><p>By applying the strong law of large number, we have at each step of time <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x115.png" xlink:type="simple"/></inline-formula> the approximation of the Global expected positive exposure (GEPE):</p><disp-formula id="scirp.78354-formula33"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x116.png"  xlink:type="simple"/></disp-formula><p>Using the trapezoid method for calculation the integral, we get:</p><disp-formula id="scirp.78354-formula34"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x117.png"  xlink:type="simple"/></disp-formula><p>On the second hand, we can use the copula approach. Given the definitions in the last section, we have:</p><disp-formula id="scirp.78354-formula35"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x118.png"  xlink:type="simple"/></disp-formula><p>Knowing that, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x119.png" xlink:type="simple"/></inline-formula></p><p>We get the following result:</p><disp-formula id="scirp.78354-formula36"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x120.png"  xlink:type="simple"/></disp-formula><p>By applying the strong law of large number, we obtain the following approximation of the GEPE:</p><disp-formula id="scirp.78354-formula37"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x121.png"  xlink:type="simple"/></disp-formula><p>We compute this quantity at each time step, and then we use the trapezoid method to compute the GWWR CVA.</p><p>The implementation of this approach needs to choose the link function between the LGD and the exposure. We then suggest the following function:</p><disp-formula id="scirp.78354-formula38"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x122.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x123.png" xlink:type="simple"/></inline-formula></p><p>The calibration of the LGD model could be done by defining the maximum and the minimum of the LGD. If we note respectively <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x124.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x124.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x125.png" xlink:type="simple"/></inline-formula> the lower and the upper bound, we thus obtain:</p><disp-formula id="scirp.78354-formula39"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x126.png"  xlink:type="simple"/></disp-formula><p>In our case, we take <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x127.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x127.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x128.png" xlink:type="simple"/></inline-formula>. We get the following values of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x127.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x128.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x129.png" xlink:type="simple"/></inline-formula></p><p>The <xref ref-type="fig" rid="fig3">Figure 3</xref> displays the evolution of the GEPE regarding to the PD with and without collateral using the Gaussian copula:</p><p>We deduce that the GEPE increases with the GWWR effect and the CVA will also have the same behavior. The GWWR grows the CVA quantity with 100%, and that proves its importance and impact on the counterparty risk measurement. The <xref ref-type="table" rid="table2">Table 2</xref> summarizes these results:</p><p>The <xref ref-type="fig" rid="fig4">Figure 4</xref> shows this effect:</p><p>・ The second approach is built around the approximation of the difference between the classical CVA, and the other one without any assumptions using a close formula. We suppose that the default is driven via a systemic factor</p><fig id="fig3"  position="float"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> Expected positive exposure with and without WWR effect</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-2410227x130.png"/></fig><table-wrap id="table2" ><label><xref ref-type="table" rid="table2">Table 2</xref></label><caption><title> CVA GWWR calculation results</title></caption><table><tbody><thead><tr><th align="center" valign="middle" ></th><th align="center" valign="middle" >Without Collateral</th><th align="center" valign="middle" >With Collateral</th></tr></thead><tr><td align="center" valign="middle" >CVA</td><td align="center" valign="middle" >0.002979613</td><td align="center" valign="middle" >0.000374312</td></tr><tr><td align="center" valign="middle" >CVA(WWR)</td><td align="center" valign="middle" >0.003535026</td><td align="center" valign="middle" >0.000540142</td></tr><tr><td align="center" valign="middle" >CVA(GWWR)</td><td align="center" valign="middle" >0.005891711</td><td align="center" valign="middle" >0.000900237</td></tr></tbody></table></table-wrap><fig id="fig4"  position="float"><label><xref ref-type="fig" rid="fig4">Figure 4</xref></label><caption><title> CVA and GWWR effect with and without collateral</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-2410227x131.png"/></fig><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x132.png" xlink:type="simple"/></inline-formula>and the default arises at time <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x132.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x133.png" xlink:type="simple"/></inline-formula> when the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x132.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x133.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x134.png" xlink:type="simple"/></inline-formula> reaches some level<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x132.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x133.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x134.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x135.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.78354-formula40"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x136.png"  xlink:type="simple"/></disp-formula><p>We can write the CVA under to the independency assumption as:</p><disp-formula id="scirp.78354-formula41"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x137.png"  xlink:type="simple"/></disp-formula><p>With <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x138.png" xlink:type="simple"/></inline-formula></p><p>We note the Global Wrong Way Risk CVA by <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x139.png" xlink:type="simple"/></inline-formula> and we define the following function:</p><disp-formula id="scirp.78354-formula42"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x140.png"  xlink:type="simple"/></disp-formula><p>For<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x141.png" xlink:type="simple"/></inline-formula>, we have<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x141.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x142.png" xlink:type="simple"/></inline-formula>.</p><p>We define the following quantities:</p><disp-formula id="scirp.78354-formula43"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x143.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.78354-formula44"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x144.png"  xlink:type="simple"/></disp-formula><p>Under the assumption of independency of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x145.png" xlink:type="simple"/></inline-formula>,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x145.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x146.png" xlink:type="simple"/></inline-formula>. Using these notations, the Global Wrong Way Adjustment (GWWA) is defined as:</p><disp-formula id="scirp.78354-formula45"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x147.png"  xlink:type="simple"/></disp-formula><p>For a<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x148.png" xlink:type="simple"/></inline-formula>.</p><p>By applying the Taylor expansion on <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x149.png" xlink:type="simple"/></inline-formula> with second order according to the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x149.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x150.png" xlink:type="simple"/></inline-formula> and by replacing the<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x149.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x150.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x151.png" xlink:type="simple"/></inline-formula>, we get:</p><disp-formula id="scirp.78354-formula46"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x152.png"  xlink:type="simple"/></disp-formula><p>By computing the first and the second derivative terms, we find the following results<sup>8</sup> (  Gourieroux, Laurent, &amp; Scaillet, 2000 ):</p><disp-formula id="scirp.78354-formula47"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x154.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.78354-formula48"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x155.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x156.png" xlink:type="simple"/></inline-formula> represents the density function of the systemic factor.</p><p>We then find the result bellow<sup>9</sup> (  Slime, 2016 ):</p><disp-formula id="scirp.78354-formula49"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x158.png"  xlink:type="simple"/></disp-formula><p>We need to define a model for computing this quantity, and we then chose the CreditRisk+<sup>10</sup> (  Credit Suisse Financial Products, 1997 ) model. This model supposes that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x159.png" xlink:type="simple"/></inline-formula> where<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x159.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x160.png" xlink:type="simple"/></inline-formula> and we obtain the following relation:</p><disp-formula id="scirp.78354-formula50"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x161.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.78354-formula51"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x162.png"  xlink:type="simple"/></disp-formula><p>Which <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x163.png" xlink:type="simple"/></inline-formula> represents the dependence factor between the counterparty and the systemic factor.</p><p>We also need to develop the derivative terms to complete the calculation, so we have:</p><disp-formula id="scirp.78354-formula52"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x164.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.78354-formula53"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x165.png"  xlink:type="simple"/></disp-formula><p>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x166.png" xlink:type="simple"/></inline-formula></p><p>The CVA assumption is the independency between the LGD, the exposure and the default, and this allows us to compute the following term:</p><disp-formula id="scirp.78354-formula54"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x167.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.78354-formula55"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x168.png"  xlink:type="simple"/></disp-formula><p>The second assumption of the CreditRisk+ model is that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x169.png" xlink:type="simple"/></inline-formula> follows a Poisson distribution with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x169.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x170.png" xlink:type="simple"/></inline-formula> as intensity. So, we deduce that:</p><disp-formula id="scirp.78354-formula56"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x171.png"  xlink:type="simple"/></disp-formula><p>We get the result bellow:</p><disp-formula id="scirp.78354-formula57"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x172.png"  xlink:type="simple"/></disp-formula><p>With <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x173.png" xlink:type="simple"/></inline-formula></p><p>And <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x174.png" xlink:type="simple"/></inline-formula></p><p>We conclude that:</p><disp-formula id="scirp.78354-formula58"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x175.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.78354-formula59"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x176.png"  xlink:type="simple"/></disp-formula><p>Subtitling in the GWWA formula, we obtain:</p><disp-formula id="scirp.78354-formula60"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x177.png"  xlink:type="simple"/></disp-formula><p>If we note the classical CVA by:</p><disp-formula id="scirp.78354-formula61"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x178.png"  xlink:type="simple"/></disp-formula><p>Then we have: <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x179.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x179.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x180.png" xlink:type="simple"/></inline-formula></p><p>Finally, we get the following formula:</p><disp-formula id="scirp.78354-formula62"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x181.png"  xlink:type="simple"/></disp-formula><p>With <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x182.png" xlink:type="simple"/></inline-formula></p><p>And <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x183.png" xlink:type="simple"/></inline-formula></p><p>Under the assumption of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x184.png" xlink:type="simple"/></inline-formula>, we obtain the simplified formula of GWWA:</p><disp-formula id="scirp.78354-formula63"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x185.png"  xlink:type="simple"/></disp-formula><p>Furthermore, the Global Wrong Way Risk CVA may be approximate using the formula bellow in the case of a symmetric distribution:</p><disp-formula id="scirp.78354-formula64"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x186.png"  xlink:type="simple"/></disp-formula><p>For non-symmetric distribution, we have:</p><disp-formula id="scirp.78354-formula65"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x187.png"  xlink:type="simple"/></disp-formula><p>As we know that the systemic factor <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x188.png" xlink:type="simple"/></inline-formula> follows the Gamma distribution, we could calibrate the factor <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x188.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x189.png" xlink:type="simple"/></inline-formula> using the Maximum Likelihood Estimation (MLE). We deem <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x188.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x189.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x190.png" xlink:type="simple"/></inline-formula> observation of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x188.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x189.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x190.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x191.png" xlink:type="simple"/></inline-formula> and the likelihood function is defined by:</p><disp-formula id="scirp.78354-formula66"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x192.png"  xlink:type="simple"/></disp-formula><p>We then should compute the maximum of the logarithmic function:</p><disp-formula id="scirp.78354-formula67"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x193.png"  xlink:type="simple"/></disp-formula><p>It remains to develop the first and the second derivative. The calculation leads to the following results:</p><disp-formula id="scirp.78354-formula68"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x194.png"  xlink:type="simple"/></disp-formula><p>We use the Stirling approximation to resolve this equation:</p><disp-formula id="scirp.78354-formula69"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x195.png"  xlink:type="simple"/></disp-formula><p>We compute the estimator, we then get<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2410227x196.png" xlink:type="simple"/></inline-formula>. This estimator must verify the second condition, and we obtain by computing the second derivative:</p><disp-formula id="scirp.78354-formula70"><graphic  xlink:href="http://html.scirp.org/file/1-2410227x197.png"  xlink:type="simple"/></disp-formula><p>The <xref ref-type="fig" rid="fig5">Figure 5</xref> and the <xref ref-type="table" rid="table3">Table 3</xref> summarize the comparison between all approaches. The approximation of the GWWR using the adjustment has a tow strong advantage. The first one, it gives us a closed formula to compute the GWWR part. The second one, his implementation is straightforward and it</p><fig id="fig5"  position="float"><label><xref ref-type="fig" rid="fig5">Figure 5</xref></label><caption><title> CVA and GWWA effect without collateral</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-2410227x198.png"/></fig><table-wrap id="table3" ><label><xref ref-type="table" rid="table3">Table 3</xref></label><caption><title> CVA GWWA calculation results</title></caption><table><tbody><thead><tr><th align="center" valign="middle" ></th><th align="center" valign="middle" >Without Collateral</th></tr></thead><tr><td align="center" valign="middle" >CVA</td><td align="center" valign="middle" >0.002979613</td></tr><tr><td align="center" valign="middle" >CVA(WWR)</td><td align="center" valign="middle" >0.003535026</td></tr><tr><td align="center" valign="middle" >CVA(GWWR)</td><td align="center" valign="middle" >0.005891711</td></tr><tr><td align="center" valign="middle" >CVA(GWWA)</td><td align="center" valign="middle" >0.004105520</td></tr></tbody></table></table-wrap><fig id="fig6"  position="float"><label><xref ref-type="fig" rid="fig6">Figure 6</xref></label><caption><title> The evolution of GWWA regarding to the correlation</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-2410227x199.png"/></fig><p>could be directly integrated on the existent framework.</p><p>We also conclude in the <xref ref-type="fig" rid="fig6">Figure 6</xref> that the conditional default probability decreases within , and the GWWA follows the same effect. This makes sense with the definition of the GWWR. Indeed, the exposure should also decrease regarding to the conditional PD, and the GWWA must be reduced.</p></sec><sec id="s4"><title>4. Conclusion</title><p>This paper was dedicated to the models allowing, on one hand, the quantifying of the Wrong Way Risk. On the other hand, we also developed two methods to integrate the Loss Given Default correlation effect. First, we began by introducing the existent approaches that give us the measurement of the WWR effect when we observe the positive correlation between the exposure and the default. We proposed a new model that combines the empirical and the copulas model. We made implementation on the European CAC40 put, and we conclude that the CVA increases potentially with the WWR effect.</p><p>Then, we generalized the concept to deem the correlation effects between the three variables. So we added the LGD correlation effect, and we proposed two models in this way. The first one is based on the definition of the function that links the LGD with the default and we also used the copula to compute the conditional expectation exposure. The second one defines a close formula to compute the difference between the classical CVA and the other one without the independency assumption.</p><p>We implemented both of these models on the European CAC40 put, and we concluded that the GWWR is more important than the WWR in term of the CVA level. Furthermore, the GWWA allows a direct integration and computation of the GWWR and we can also apply this model to the WWR. However, both of models represent some weakness. The first one needs to define and calibrate the LGD model, and the integration of the existent model is not straightforward and will cost more time calculation. The second one remains an approximation of the GWWR and requests a calibration of the systemic factor. We tried to give a close formula to allow a direct integration on the existent CVA system, because the implementation arises one of most issues in the banking platform. By the way, we suggest getting more researching on the approaches that allow a straight integration.</p></sec><sec id="s5"><title>Cite this paper</title><p>Slime, B. (2017). Modeling and Quantifying of the Global Wrong Way Risk. Journal of Financial Risk Management, 6, 231-246. https://doi.org10.4236/jfrm.2017.63017</p></sec><sec id="s6"><title>NOTES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.78354-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Basel Committee on Banking Supervision (2010). 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