<?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">JMF</journal-id><journal-title-group><journal-title>Journal of Mathematical Finance</journal-title></journal-title-group><issn pub-type="epub">2162-2434</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jmf.2012.21009</article-id><article-id pub-id-type="publisher-id">JMF-17599</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><subject> Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  The Distribution of the Value of the Firm and Stochastic Interest Rates
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>.</surname><given-names>Lakshmivarahan</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Shengguang</surname><given-names>Qian</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Duane</surname><given-names>Stock</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff2"><addr-line>Division of Finance, Michael F. Price College of Business, University of Oklahoma, Norman, USA</addr-line></aff><aff id="aff1"><addr-line>School of Computer Science, University of Oklahoma, Norman, USA</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>dstock@ou.edu(DS)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>28</day><month>02</month><year>2012</year></pub-date><volume>02</volume><issue>01</issue><fpage>75</fpage><lpage>82</lpage><history><date date-type="received"><day>September</day>	<month>14,</month>	<year>2011</year></date><date date-type="rev-recd"><day>October</day>	<month>4,</month>	<year>2011</year>	</date><date date-type="accepted"><day>October</day>	<month>30,</month>	<year>2011</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 time evolution of the value of a firm is commonly modeled by a linear, scalar stochastic differential equation (SDE) of the type where the coefficient in the drift term denotes the (exogenous) stochastic short term interest rate and is the given volatility of the value process. In turn, the dynamics of the short term interest rate are modeled by a scalar SDE. It is shown that exhibits a lognormal distribution when is a normal/Gaussian process defined by a common variety of narrow sense linear SDEs. The results can be applied to different financial situations where modeling value of the firm is critical. For example, with the context of the structural models, using this result one can readily compute the probability of default of a firm.
 
</p></abstract><kwd-group><kwd>Alue of Firm; Lognormal; Interest Rate Process</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Modeling the value of the firm is one of the more important research topics in finance. The value of an unlevered firm is the value of expected future cash flows discounted at a rate appropriate for an all-equity firm whereas the value of a levered firm is commonly expressed as the value of an unlevered firm plus the gain from leverage due to a tax shield provided by the debt. Including business disruption costs, the optimal capital structure can then be characterized as a trade-off between the interest tax shield and disruption costs. Recent analysis by Hackbarth, Hennessy and Leland [<xref ref-type="bibr" rid="scirp.17599-ref1">1</xref>] extends this line of research by examining an optimal mixture of debt; that is, the optimal mixture of bank debt and market debt (bonds).</p><p>Improved models for value of the firm are potentially useful in several contexts. For one example, consider models of credit spreads. Leland and Toft [<xref ref-type="bibr" rid="scirp.17599-ref2">2</xref>] develop an ambitious model of firm value that addresses optimal capital structure, optimal debt maturity, and the term structure of credit spreads. Recently, Qi [<xref ref-type="bibr" rid="scirp.17599-ref3">3</xref>] has modified the Leland and Toft [<xref ref-type="bibr" rid="scirp.17599-ref2">2</xref>] model by setting the lower bankruptcy boundary to be a fraction of bond face value. The importance of good structural models for credit spreads has been enhanced with the growth of credit derivatives and the credit crisis of 2007 and 2008. More specifically, notional amounts of credit derivatives grew by over 100% for every year from 2004 through 2006. At the end of 2006, there was 34.5 trillion outstanding (see Saha-Bubna and Barrett [<xref ref-type="bibr" rid="scirp.17599-ref4">4</xref>]). The weakened credit quality of many financial firms in 2007 and 2008 caused high volatility in equity markets and, also, large changes in the value of credit spreads and credit default swaps.</p><p>Our purpose is to derive distributions of <img src="9-1490033\0d0fd654-84c2-4256-b197-30507549b9b1.jpg" /> whose evolution critically depends on the models for the short term interest rate process,<img src="9-1490033\ace97b80-5f19-4717-94e0-0c4e1e477bec.jpg" />. Models for <img src="9-1490033\797d057d-a39f-4590-8684-a0f8375c61e7.jpg" /> can be broadly classified as (a) general linear and (b) non linear models. General linear models are also popularly known as affine models. In this context, we refer to Duffie, Filipovic and Schachermayer [<xref ref-type="bibr" rid="scirp.17599-ref5">5</xref>]; Duffie and Singleton [<xref ref-type="bibr" rid="scirp.17599-ref6">6</xref>]; and Lamberton and Lapeyre [<xref ref-type="bibr" rid="scirp.17599-ref7">7</xref>]. In this paper we are particularly interested in a special class of the general linear models called narrow sense linear models described by Arnold [<xref ref-type="bibr" rid="scirp.17599-ref8">8</xref>].</p><p>The next section describes the processes for value of the firm and short term interest rates. Next, we discuss a general framework for the solution of the distribution of<img src="9-1490033\9597f02f-9182-4913-bdc1-5a1b1e7dc72a.jpg" />. Then, we describe solutions in the cases where <img src="9-1490033\a5f117ff-026a-42e5-a82e-f65bf8efc318.jpg" /> processes are narrow sense linear. Such <img src="9-1490033\43b6080d-d825-402e-b32e-8800b012a6e9.jpg" /> processes are quite popular for models of credit risk. The shapes of the <img src="9-1490033\bc60305e-1744-42d3-a3d7-871fdfe58b50.jpg" /> distributions are shown to be sensitive to such parameters as the correlation between the <img src="9-1490033\2aa34e61-8955-43ae-83f5-4bf182eaed6e.jpg" /> and <img src="9-1490033\2d938274-2ac5-40d3-bc9b-74533e60ded2.jpg" /> processes. For example, a positive correlation displays a <img src="9-1490033\80ec8f86-65a4-4007-8ba1-171e2679e0df.jpg" /> distribution with fatter tails than one with negative correlation.</p></sec><sec id="s2"><title>2. The Processes for Value of the Firm and Interest Rates</title><p>The time evolution of the value, <img src="9-1490033\e5af9cfa-5284-43c1-9d25-79080564cce7.jpg" />, of a firm is routinely modeled under the risk neutral measure by a linear, scalar, stochastic differential equation (SDE)</p><disp-formula id="scirp.17599-formula148958"><label>, (1.1)</label><graphic position="anchor" xlink:href="9-1490033\59b88bc9-428f-43b4-a574-4fc6df129926.jpg"  xlink:type="simple"/></disp-formula><p>where the instantaneous drift <img src="9-1490033\4f1161c1-916c-40aa-ba5b-5be10c44ef15.jpg" /> denotes the (exogenous) stochastic variable known as the short-term interest rate process and <img src="9-1490033\01815664-53c6-43ad-8d0b-bc36a38a85fe.jpg" /> is a deterministic function representing the instantaneous volatility as in Acharya and Carpenter [<xref ref-type="bibr" rid="scirp.17599-ref9">9</xref>].</p><p>This general form of value process has been used in numerous important structural models of credit risk. For example, see Merton [<xref ref-type="bibr" rid="scirp.17599-ref10">10</xref>] and Acharya and Carpenter [<xref ref-type="bibr" rid="scirp.17599-ref9">9</xref>] where any dividends and coupon payments, outflows of γ from the firm to investors, are subtracted from the r<sub>t</sub> drift term. Many firms do not pay dividends and our model is one of zero coupon debt so that a γ of zero is reasonable. We note that Longstaff and Schwartz [<xref ref-type="bibr" rid="scirp.17599-ref11">11</xref>] similarly have a zero γ.</p><p>The <img src="9-1490033\92b6b19b-c3e8-47fa-a832-62acc0fb93f3.jpg" /> drift of <img src="9-1490033\5ac0c0c7-f57b-4b60-abbd-f6a85df2fdcf.jpg" /> indicates our model is risk neutral. We could assume different firms have different drifts due to such things as different expected returns in their industry as well as different riskiness of assets and future projects. However, such an assumption is arbitrary and yields a model that is not arbitrage free. We believe it is much more theoretically credible to posit a risk neutral, arbitrage free model.</p><p>The dynamics of the short term interest rate are modeled, under the same risk neutral measure, by a (scalar) SDE of the type</p><disp-formula id="scirp.17599-formula148959"><label>, (1.2)</label><graphic position="anchor" xlink:href="9-1490033\4b2a1f47-4f18-4ba7-be61-9b6cd169640d.jpg"  xlink:type="simple"/></disp-formula><p>where the instantaneous drift, <img src="9-1490033\77a281ec-2507-4952-ad64-b7961f85d166.jpg" />and the volatility, <img src="9-1490033\a0b71984-9b4f-4f77-92a2-094a25b21f47.jpg" />are smooth functions. It is further assumed that the Wiener increment processes <img src="9-1490033\c81e481e-bca2-4bc3-bc85-2b0a4b7c7120.jpg" /> and <img src="9-1490033\ba8853fa-9bdf-43c3-91cc-518c561f9fab.jpg" /> are correlated; that is,</p><disp-formula id="scirp.17599-formula148960"><label>(1.3)</label><graphic position="anchor" xlink:href="9-1490033\1363ff7f-c2e3-4c4e-8800-3dd788701a51.jpg"  xlink:type="simple"/></disp-formula><p>with<img src="9-1490033\c7012ca6-b550-4c4e-a16f-a25000b271b1.jpg" />. It is worth noting that in this set up the flow of information is only one way –<img src="9-1490033\edf31fa3-9741-4378-a5ce-982b2a39dfc9.jpg" />affects <img src="9-1490033\8ba5a710-2aab-4aba-9a7d-9e7f69940360.jpg" /> and not vice versa. By combining several well known results from the literature, in this paper we characterize the distribution of the value process <img src="9-1490033\dc4ffe2e-fc32-40e6-9bfb-68262114b837.jpg" /> for different choices of the <img src="9-1490033\035b3470-6e92-4727-99c9-316d94c739ee.jpg" /> processes.</p><p>All the known stochastic interest rate models can be broadly classified into two classes—single factor models (SFMs) and multi-factor models (MFMs). We refer to Cairns [<xref ref-type="bibr" rid="scirp.17599-ref12">12</xref>] and Privault [<xref ref-type="bibr" rid="scirp.17599-ref13">13</xref>] for details. In this paper, we are primarily interested in the SFMs. These SFMs can be divided into linear and nonlinear models. Following Arnold [<xref ref-type="bibr" rid="scirp.17599-ref8">8</xref>], linear models can be further subdivided into two subclasses. The SFM in (1.2) is called a narrow sense linear model if</p><disp-formula id="scirp.17599-formula148961"><label>, (1.4)</label><graphic position="anchor" xlink:href="9-1490033\bfcce6f0-f909-4abd-a241-011b96fb56a9.jpg"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.17599-formula148962"><label>. (1.5)</label><graphic position="anchor" xlink:href="9-1490033\2c1ead80-bc91-4c62-9813-95c3c3898cf8.jpg"  xlink:type="simple"/></disp-formula><p>A general linear model, on the other hand, has <img src="9-1490033\94302a95-7df6-44ba-a45e-62f033bc5a97.jpg" /> in the form (1.4) and</p><disp-formula id="scirp.17599-formula148963"><label>, (1.6)</label><graphic position="anchor" xlink:href="9-1490033\c43a5b97-b585-442e-9b8b-83330106cbb4.jpg"  xlink:type="simple"/></disp-formula><p>where<img src="9-1490033\3c4d0d2a-6c30-489b-af2b-375699934602.jpg" /> and <img src="9-1490033\8f69cd62-0504-404d-a80d-2e63638980ab.jpg" /> are smooth functions of time<img src="9-1490033\2ffc6db9-1335-45a0-bc4f-5ddd28c2c32f.jpg" />. The general linear models are also known as affine models as in Duffie, Filipovic, and Schachermayer [<xref ref-type="bibr" rid="scirp.17599-ref5">5</xref>]; Duffie and Singleton [<xref ref-type="bibr" rid="scirp.17599-ref6">6</xref>]; and Lamberton and Lapeyre [<xref ref-type="bibr" rid="scirp.17599-ref7">7</xref>]. The SFM in (1.2) is called a nonlinear model if either <img src="9-1490033\e01db7ec-5bf1-4b7c-895f-390e2d49a581.jpg" /> and/or <img src="9-1490033\cfb43f54-b5a2-49b4-b5dd-3aba89e992bb.jpg" /> are nonlinear functions of the short rate<img src="9-1490033\639df605-da12-402c-b073-6ba426de0e8b.jpg" />.</p><p>Refer to Tables 1(a)-(c) for examples of these models. The narrow sense linear models of Merton [<xref ref-type="bibr" rid="scirp.17599-ref14">14</xref>], Vasicek [<xref ref-type="bibr" rid="scirp.17599-ref15">15</xref>], Ho and Lee [<xref ref-type="bibr" rid="scirp.17599-ref16">16</xref>], and Hull and White [<xref ref-type="bibr" rid="scirp.17599-ref17">17</xref>] are special cases of the Heath, Jarrow and Morton [<xref ref-type="bibr" rid="scirp.17599-ref18">18</xref>] model and define normal/Gaussian processes.</p><p>We first solve the scalar SDE (1.2) for<img src="9-1490033\2849b049-f136-4eaf-b1d4-5af3d85359f5.jpg" />, and using it in (1.1), we then recover<img src="9-1490033\8c908097-8fe8-4a4b-8d05-94612a8b9ab8.jpg" />. It is well known that <img src="9-1490033\e63f9f3e-3866-4541-92d8-7ac0bf51d2ae.jpg" /> is a lognormal process when <img src="9-1490033\bb9a9ef1-1190-408e-95e1-492bd219aeaa.jpg" />a constant. See Kloeden and Platen [<xref ref-type="bibr" rid="scirp.17599-ref19">19</xref>]. We extend this result by first showing that <img src="9-1490033\d440a1bb-2110-47b4-a58a-3a8912379427.jpg" /> also inherits this lognormal distribution where <img src="9-1490033\139de9a6-cf25-43b6-8569-9fe2d4949c9b.jpg" /> is a normal process defined by the narrow sense linear models in <xref ref-type="table" rid="table1">Table 1</xref>.</p><p>This problem of quantifying the probability distribution of <img src="9-1490033\e301260b-004f-4f08-ad81-194f62e845e7.jpg" /> is critical to credit risk analysis. For a review of various approaches to credit risk refer to the books by Duffie and Singleton [<xref ref-type="bibr" rid="scirp.17599-ref6">6</xref>], Bielecki and Rutkowski [<xref ref-type="bibr" rid="scirp.17599-ref20">20</xref>], and Jarrow et al. [<xref ref-type="bibr" rid="scirp.17599-ref21">21</xref>]. Clearly computation of the default probability in structural models requires knowledge of the probability distribution of <img src="9-1490033\b51e8fce-b3cb-4eae-87a2-66398e1cf7ac.jpg" /> contingent on the chosen model for the interest rate.</p></sec><sec id="s3"><title>3. A framework for the Solution</title><p>In this section we develop a framework for solving (1.1)- (1.2). Setting <img src="9-1490033\484569ed-7225-40ea-b4cd-533964dcbf50.jpg" /> and applying Ito’s lemma, equation (1.1) becomes.</p><disp-formula id="scirp.17599-formula148964"><label>. (2.1)</label><graphic position="anchor" xlink:href="9-1490033\d0dcc782-0111-4bb0-8c6a-8ac5b87fa465.jpg"  xlink:type="simple"/></disp-formula><p>See Kloeden and Platen [<xref ref-type="bibr" rid="scirp.17599-ref19">19</xref>].</p><p>Setting <img src="9-1490033\6ae40220-5186-4233-b75b-82d97403b87c.jpg" /> and</p><disp-formula id="scirp.17599-formula148965"><graphic  xlink:href="9-1490033\e77a52cb-8947-4679-b3bf-99899ea9103d.jpg"  xlink:type="simple"/></disp-formula><p><xref ref-type="table" rid="table1">Table 1</xref>. Alternative Models of<img src="9-1490033\b03cffee-b2df-424b-b170-00be05f3facc.jpg" />. The single factor model in (1.2) is called a narrow sense linear model if <img src="9-1490033\9f6f7414-18a8-41fb-9c98-f1b1a65a46d6.jpg" /> and<img src="9-1490033\7acb1882-160c-4c94-b3bf-ca2ce79141d0.jpg" />. In contrast, the model is called an affine model or a general linear model if <img src="9-1490033\1ec69437-9bd3-424f-a339-3d62ff8e4ed2.jpg" /> is of the above form and<img src="9-1490033\4afcdc55-4a19-4af2-a1be-99c2ee5bc426.jpg" />. The model is called nonlinear if either <img src="9-1490033\0023f005-4e77-43fa-97cf-d7cdbfdb8d49.jpg" /> and/or <img src="9-1490033\84536ec2-16f6-47aa-a494-7cc7d8f57fa7.jpg" /> are nonlinear functions of the short rate<img src="9-1490033\38752557-d50f-4c28-9d6f-bc684698290f.jpg" />. (a) Narrow sense linear models; (b) General linear or affine models; (c) Nonlinear models.   </p><p>(Shreve [<xref ref-type="bibr" rid="scirp.17599-ref22">22</xref>]) we can rewrite the pair of equations (1.2) and (2.1) as</p><disp-formula id="scirp.17599-formula148966"><label>(2.2)</label><graphic position="anchor" xlink:href="9-1490033\da2c161f-5dc7-4880-b479-583768fb3953.jpg"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.17599-formula148967"><label>(2.3)</label><graphic position="anchor" xlink:href="9-1490033\92ee3c4b-f510-4699-aa55-f182d0188b3b.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="9-1490033\ede3716e-f94d-421a-b00e-32f621cc1516.jpg" /> and <img src="9-1490033\7a11d141-29fe-4a99-9515-817d84612c4c.jpg" /> are two independent Wiener increment processes and</p><disp-formula id="scirp.17599-formula148968"><label>. (2.4)</label><graphic position="anchor" xlink:href="9-1490033\b27792d4-ac8e-4365-930a-14b7168942e2.jpg"  xlink:type="simple"/></disp-formula><p>Integrating (2.3), we obtain</p><disp-formula id="scirp.17599-formula148969"><label>(2.5)</label><graphic position="anchor" xlink:href="9-1490033\d8cd886d-eaa8-40e9-86cf-ae6ee279f83a.jpg"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.17599-formula148970"><label>(2.6)</label><graphic position="anchor" xlink:href="9-1490033\5259bc85-ab4e-4a0b-a8b3-6adc2881833f.jpg"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.17599-formula148971"><label>. (2.7)</label><graphic position="anchor" xlink:href="9-1490033\9b2130de-bcec-482c-8205-581e21e88c1c.jpg"  xlink:type="simple"/></disp-formula><p>From the properties of the Ito integral, Mikosch [<xref ref-type="bibr" rid="scirp.17599-ref30">30</xref>] and Shreve [<xref ref-type="bibr" rid="scirp.17599-ref22">22</xref>], it follows that</p><disp-formula id="scirp.17599-formula148972"><label>(2.8)</label><graphic position="anchor" xlink:href="9-1490033\b734cae0-a00f-438d-9a14-1dedab75c642.jpg"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.17599-formula148973"><label>. (2.9)</label><graphic position="anchor" xlink:href="9-1490033\7ccc3eb6-e363-4a92-a9a4-61177a69756e.jpg"  xlink:type="simple"/></disp-formula><p>Since <img src="9-1490033\ae907495-b51f-4d01-8744-08197dad58cc.jpg" /> and <img src="9-1490033\23fe0494-e7fd-4145-9d71-42e1a6cbd1fc.jpg" /> are independent Wiener processes, it readily follows that <img src="9-1490033\461065c0-6ab9-454b-84a8-f0759060f940.jpg" />. Thus, the distribution of <img src="9-1490033\ba82ffd7-e404-4219-8616-2bcdf749cc13.jpg" /> and hence of <img src="9-1490033\6aeb9eba-b6f3-46a7-880f-1d3af3d27e4e.jpg" /> critically depend on the properties of the <img src="9-1490033\d25b3d6b-2a62-41d9-b6e5-3781005f972e.jpg" /> process in (2.2).</p><p>In closing this section consider the special case when<img src="9-1490033\e2eae25f-6fea-4586-bec7-0f911d0fa19e.jpg" />, a constant. Then,</p><disp-formula id="scirp.17599-formula148974"><label>. (2.10)</label><graphic position="anchor" xlink:href="9-1490033\c0d970ce-b066-4b2e-89a6-02b0d49837e1.jpg"  xlink:type="simple"/></disp-formula><p>Further, when<img src="9-1490033\ca6aee43-9579-4b42-a4cb-7bbdc5d7b943.jpg" />, we obtain</p><disp-formula id="scirp.17599-formula148975"><label>. (2.11)</label><graphic position="anchor" xlink:href="9-1490033\4660b589-00e0-4dd7-8c1b-32e25ed51ab8.jpg"  xlink:type="simple"/></disp-formula><p>4. Narrow Sense Linear Models for r<sub>t</sub></p><p>Setting</p><disp-formula id="scirp.17599-formula148976"><label>, (3.1)</label><graphic position="anchor" xlink:href="9-1490033\c59cfce0-d9a6-42ff-b8a3-e8c3aeca49bc.jpg"  xlink:type="simple"/></disp-formula><p>in (2.2), we get a narrow sense (time varying) linear model known as the generalized Hull and White [<xref ref-type="bibr" rid="scirp.17599-ref17">17</xref>] model given by</p><disp-formula id="scirp.17599-formula148977"><label>. (3.2)</label><graphic position="anchor" xlink:href="9-1490033\a41cf09a-1ddc-49b6-8b17-752d9295d673.jpg"  xlink:type="simple"/></disp-formula><p>Since all the other narrow sense linear models in     <xref ref-type="table" rid="table1">Table 1</xref> are special cases of (3.2), we first concentrate on solving (3.2). Defining</p><disp-formula id="scirp.17599-formula148978"><label>, (3.3)</label><graphic position="anchor" xlink:href="9-1490033\d597fe91-49f9-4e14-ae63-5ed642965471.jpg"  xlink:type="simple"/></disp-formula><p>we get</p><disp-formula id="scirp.17599-formula148979"><label>. (3.4)</label><graphic position="anchor" xlink:href="9-1490033\08b7aec4-95c7-42e2-8dd3-97744b79b97b.jpg"  xlink:type="simple"/></disp-formula><p>This is known as the fundamental solution of (3.2). Hence the solution of (3.2) is given by (Arnold [<xref ref-type="bibr" rid="scirp.17599-ref8">8</xref>], Gard [<xref ref-type="bibr" rid="scirp.17599-ref31">31</xref>], Kuo [<xref ref-type="bibr" rid="scirp.17599-ref32">32</xref>], Lamberton and Lapeyre [<xref ref-type="bibr" rid="scirp.17599-ref7">7</xref>])</p><disp-formula id="scirp.17599-formula148980"><label>, (3.5)</label><graphic position="anchor" xlink:href="9-1490033\1240ec04-fd8f-4244-8083-fff399ce99ad.jpg"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.17599-formula148981"><label>, (3.6)</label><graphic position="anchor" xlink:href="9-1490033\fd78dee7-1a4d-4449-9e4f-6216617a85a5.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.17599-formula148982"><label>, (3.7)</label><graphic position="anchor" xlink:href="9-1490033\fe219588-97a7-4bb1-8aac-48f8d11c06c0.jpg"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.17599-formula148983"><label>. (3.8)</label><graphic position="anchor" xlink:href="9-1490033\6b475d83-d40f-47e7-a4dc-cff6fa07241c.jpg"  xlink:type="simple"/></disp-formula><p>Hence,</p><disp-formula id="scirp.17599-formula148984"><label>(3.9)</label><graphic position="anchor" xlink:href="9-1490033\4ad5e96b-2c17-412a-9681-57b73da5f3de.jpg"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.17599-formula148985"><label>. (3.10)</label><graphic position="anchor" xlink:href="9-1490033\a16f7825-4d2b-4818-a1da-c616468eecfb.jpg"  xlink:type="simple"/></disp-formula><p>Now combining (3.5)-(3.10), it follows that</p><disp-formula id="scirp.17599-formula148986"><label>. (3.11)</label><graphic position="anchor" xlink:href="9-1490033\c7c7e39d-d782-4efb-b5f5-8395f8991b0c.jpg"  xlink:type="simple"/></disp-formula><p>Applying integration by parts to the second integral on the right hand side of (3.11) and using (3.7), it follows that</p><disp-formula id="scirp.17599-formula148987"><label>(3.12)</label><graphic position="anchor" xlink:href="9-1490033\31302d53-9ee0-4505-86ed-fb724f1fe35a.jpg"  xlink:type="simple"/></disp-formula><p>Is also a Gaussian process with mean zero and variance given by</p><disp-formula id="scirp.17599-formula148988"><label>. (3.13)</label><graphic position="anchor" xlink:href="9-1490033\3cea9398-511a-4455-a4b0-8a96dcca955d.jpg"  xlink:type="simple"/></disp-formula><p>Substituting (3.11)-(3.12) in (2.5), we get</p><disp-formula id="scirp.17599-formula148989"><label>(3.14)</label><graphic position="anchor" xlink:href="9-1490033\37538923-a483-425b-b56b-e68071db15f5.jpg"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.17599-formula148990"><label>(3.15)</label><graphic position="anchor" xlink:href="9-1490033\b8c1dfee-4e8b-445a-b43c-1d644290d983.jpg"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.17599-formula148991"><label>. (3.16)</label><graphic position="anchor" xlink:href="9-1490033\aa32fca9-873d-4cd0-8952-263abde0ce69.jpg"  xlink:type="simple"/></disp-formula><p>Substituting (2.6), (3.12) and (2.7) in (3.16), the latter becomes</p><disp-formula id="scirp.17599-formula148992"><label>(3.17)</label><graphic position="anchor" xlink:href="9-1490033\0d3d2ebc-e906-4de9-b93c-55cdd1668d51.jpg"  xlink:type="simple"/></disp-formula><p>Since <img src="9-1490033\1fbf41eb-1f68-4ab6-911d-e3b70e22ac91.jpg" /> and <img src="9-1490033\2d201c38-be90-43b6-8da1-32001f192817.jpg" /> are independent, it follows that <img src="9-1490033\a018c234-03c0-42c9-ae74-b4b0492793ef.jpg" /> where</p><disp-formula id="scirp.17599-formula148993"><label>(3.18)</label><graphic position="anchor" xlink:href="9-1490033\cfe88161-e1d9-4766-b2a1-1ea9268d09fb.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.17599-formula148994"><label>, (3.19)</label><graphic position="anchor" xlink:href="9-1490033\8905a6ee-82c4-496b-a6c3-8541dc2433e9.jpg"  xlink:type="simple"/></disp-formula><p>where</p><p><img src="9-1490033\7f974260-209f-435e-b331-1a7823f8976c.jpg" /></p><p>and</p><p><img src="9-1490033\175f964a-2a5f-4fc0-a09b-3c443b2a44c9.jpg" />.</p><p>Combining (3.15)-(3.18) with (3.14), we finally obtain</p><disp-formula id="scirp.17599-formula148995"><label>(3.20)</label><graphic position="anchor" xlink:href="9-1490033\3e54cc5b-32f1-4b8e-ac8b-6ba08f102631.jpg"  xlink:type="simple"/></disp-formula><p>where<img src="9-1490033\04360fce-cb0a-4012-aa11-60107da0c814.jpg" /> given by (3.16) and <img src="9-1490033\6e6f1148-ca22-409b-994b-2c820f106d83.jpg" /> given by (3.19).</p><p>We summarize the above developments in the following:</p><p>Theorem 3.1: Let the interest rate <img src="9-1490033\c0a07b31-fabf-4dde-9a08-db1f775c2b3c.jpg" /> evolve according to a narrow sense linear, scalar, SDE of the type (3.2). Then, <img src="9-1490033\8a11dacb-7f51-46b0-85ee-862c58b9acf6.jpg" />is a Gaussian process and consequently <img src="9-1490033\0826ed5f-a434-4eda-8722-e257c6097984.jpg" /> in (2.5) is also a Gaussian process given by (3.20).</p><p>Since<img src="9-1490033\9fe057b0-0d3d-440b-9f04-0026b98079cb.jpg" />, from (3.14)-(3.20), we get</p><disp-formula id="scirp.17599-formula148996"><label>(3.21)</label><graphic position="anchor" xlink:href="9-1490033\fe2d71b5-e688-4a23-ac52-319e4a93cc0b.jpg"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.17599-formula148997"><label>(3.22)</label><graphic position="anchor" xlink:href="9-1490033\7c66df72-7a2d-4d4c-b7e5-73dd75efc157.jpg"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.17599-formula148998"><label>. (3.23)</label><graphic position="anchor" xlink:href="9-1490033\5d586723-a3a3-4005-875d-007799d29c40.jpg"  xlink:type="simple"/></disp-formula><p>The following corollary is immediate.</p><p>Corollary 3.2: Since<img src="9-1490033\79191839-6b72-4d26-bed8-acbff507c89c.jpg" />,</p><p><img src="9-1490033\017ff2cb-6723-421f-a101-c72eb221a194.jpg" />is a lognormal process whose probability density function, as a function of time, is given by</p><disp-formula id="scirp.17599-formula148999"><label>. (3.24)</label><graphic position="anchor" xlink:href="9-1490033\292e4d64-1683-4fde-a402-7f27ef356edb.jpg"  xlink:type="simple"/></disp-formula><p>It can be verified (Johnson et al. [<xref ref-type="bibr" rid="scirp.17599-ref33">33</xref>]) that the time evolution of the mean and variance of the value process</p><p><img src="9-1490033\0210b26b-b3b1-45ce-8543-231b9d7f0c81.jpg" />are given by</p><disp-formula id="scirp.17599-formula149000"><label>(3.25)</label><graphic position="anchor" xlink:href="9-1490033\6be75033-7910-419d-9d7c-7e98c3ce9cab.jpg"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.17599-formula149001"><label>. (3.26)</label><graphic position="anchor" xlink:href="9-1490033\94b346e0-b5b0-4d22-9361-c7c24637eaa6.jpg"  xlink:type="simple"/></disp-formula><p>We now enlist a number of nested corollaries by considering special cases of interest rate models.</p><p>Case 1: Let<img src="9-1490033\141bdc37-5cb7-406d-9e91-f7b9b9909245.jpg" />, a constant. Then</p><p><img src="9-1490033\9105859d-ee50-4b6c-863b-ccb8c6d4802e.jpg" />, <img src="9-1490033\a49229f4-3bfe-40a6-9f0f-3db79b2e7289.jpg" />and <img src="9-1490033\3d8437d9-b3b2-47e9-8391-ad0ac979ebca.jpg" /> is given by</p><p>(3.8). From (3.15) and (3.20), the mean is</p><disp-formula id="scirp.17599-formula149002"><label>(3.27)</label><graphic position="anchor" xlink:href="9-1490033\25799bbc-d754-422c-92df-411dd76df7d0.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="9-1490033\03fedc77-6ecd-4421-a47a-3f13a29dfa0c.jpg" /> is given in (3.6). From (3.19)-(3.20), the variance is</p><disp-formula id="scirp.17599-formula149003"><label>. (3.28)</label><graphic position="anchor" xlink:href="9-1490033\1a7f6c69-be8c-46ff-951e-4472f362791c.jpg"  xlink:type="simple"/></disp-formula><p>Case 2: Hull and White [<xref ref-type="bibr" rid="scirp.17599-ref17">17</xref>] model: In this model, <img src="9-1490033\6371449b-a907-46e2-b72d-b2aaa3d57f31.jpg" /> and <img src="9-1490033\24edb811-a432-4871-acca-611610bfcc36.jpg" /> where <img src="9-1490033\ba10db52-c67e-4ead-8177-deaafd09f788.jpg" /> and <img src="9-1490033\3520e9de-8853-499f-a4cc-13096b6fc68f.jpg" /> are constants. Thus, <img src="9-1490033\b98c3a5b-bfa6-469e-88b3-d2443f9be96a.jpg" />, <img src="9-1490033\c9a66e7e-383c-4570-b09a-84d78ce58d69.jpg" />and</p><disp-formula id="scirp.17599-formula149004"><label>. (3.29)</label><graphic position="anchor" xlink:href="9-1490033\1c58f9d0-3085-45a6-8af1-0bf047da3ccc.jpg"  xlink:type="simple"/></disp-formula><p>Hence the mean is</p><disp-formula id="scirp.17599-formula149005"><label>(3.30)</label><graphic position="anchor" xlink:href="9-1490033\7f768903-25eb-469d-b827-0212db451d5a.jpg"  xlink:type="simple"/></disp-formula><p>and the variance is</p><disp-formula id="scirp.17599-formula149006"><label>(3.30a)</label><graphic position="anchor" xlink:href="9-1490033\5cdb58f8-2db3-418f-80cb-47d32c010d9d.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.17599-formula149007"><label>. (3.30b)</label><graphic position="anchor" xlink:href="9-1490033\d6ea17e2-7a8c-46b8-924a-397e395c876e.jpg"  xlink:type="simple"/></disp-formula><p>Case 3: Ho-Lee [<xref ref-type="bibr" rid="scirp.17599-ref16">16</xref>] model: In this model, <img src="9-1490033\35f53748-c810-4f4f-b801-4c032759c065.jpg" />and<img src="9-1490033\be6cc943-f299-41ee-bd8e-634677485793.jpg" />. Then</p><disp-formula id="scirp.17599-formula149008"><label>. (3.31)</label><graphic position="anchor" xlink:href="9-1490033\eeb6644d-25aa-4e61-997a-f920b1fd89b7.jpg"  xlink:type="simple"/></disp-formula><p>The mean is</p><disp-formula id="scirp.17599-formula149009"><label>(3.32)</label><graphic position="anchor" xlink:href="9-1490033\7ba83847-5efb-4a73-80f4-6cc4b83d8117.jpg"  xlink:type="simple"/></disp-formula><p>and the variance is</p><disp-formula id="scirp.17599-formula149010"><label>(3.33a)</label><graphic position="anchor" xlink:href="9-1490033\b3f23a52-c797-435c-850e-b7953942750b.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.17599-formula149011"><label>. (3.33b)</label><graphic position="anchor" xlink:href="9-1490033\f90a423a-17ee-4000-9d47-555a42441a4a.jpg"  xlink:type="simple"/></disp-formula><p>Case 4: Vasicek [<xref ref-type="bibr" rid="scirp.17599-ref15">15</xref>] model: In this model, <img src="9-1490033\60df9909-118d-4b23-8cd9-a4036b805f7e.jpg" />, <img src="9-1490033\c36189b2-f801-458d-801e-e29a29dbfd60.jpg" />and<img src="9-1490033\c027284d-03e3-4e18-857b-8417894805d2.jpg" />. Then, <img src="9-1490033\39d0c354-b043-4b25-a60d-452e4d80e39e.jpg" />and</p><disp-formula id="scirp.17599-formula149012"><label>. (3.34)</label><graphic position="anchor" xlink:href="9-1490033\650aa82f-76de-4eba-809f-1d92b8aae723.jpg"  xlink:type="simple"/></disp-formula><p>Hence, the mean is</p><disp-formula id="scirp.17599-formula149013"><label>(3.35a)</label><graphic position="anchor" xlink:href="9-1490033\0e3aec9b-e82f-4593-82b4-e88100d04ad0.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.17599-formula149014"><label>(3.35b)</label><graphic position="anchor" xlink:href="9-1490033\630ace73-c83f-4736-a79b-a7f617685a82.jpg"  xlink:type="simple"/></disp-formula><p>and the variance is</p><disp-formula id="scirp.17599-formula149015"><label>(3.36a)</label><graphic position="anchor" xlink:href="9-1490033\46126f3f-7e55-41a5-892d-955bda071ca2.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.17599-formula149016"><label>. (3.36b)</label><graphic position="anchor" xlink:href="9-1490033\ebc55b81-b227-4a1e-b034-a0923ace24c9.jpg"  xlink:type="simple"/></disp-formula><p>Case 5: Merton [<xref ref-type="bibr" rid="scirp.17599-ref14">14</xref>]: In this case, <img src="9-1490033\54d4a501-80f7-41cc-9334-67eaf0e8e916.jpg" />, <img src="9-1490033\2b3c7e87-4d0e-4769-b6a1-cb3c3162fd9e.jpg" /> and<img src="9-1490033\846033f0-8126-438c-8b6d-c202dd18f817.jpg" />. Then <img src="9-1490033\1801d602-5dcc-488f-b688-aabf5c8dcb57.jpg" /> and</p><disp-formula id="scirp.17599-formula149017"><label>. (3.37)</label><graphic position="anchor" xlink:href="9-1490033\29237035-6792-49c7-bdb0-a00ef944768f.jpg"  xlink:type="simple"/></disp-formula><p>Hence, the mean is</p><disp-formula id="scirp.17599-formula149018"><label>(3.38)</label><graphic position="anchor" xlink:href="9-1490033\416def0a-6235-46b3-9b89-112dd4230b52.jpg"  xlink:type="simple"/></disp-formula><p>and the variance is</p><disp-formula id="scirp.17599-formula149019"><label>(3.39a)</label><graphic position="anchor" xlink:href="9-1490033\e18179be-66f6-4697-b84d-cf5699fe2850.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.17599-formula149020"><label>. (3.39b)</label><graphic position="anchor" xlink:href="9-1490033\57af5660-0f9d-4796-8cd9-e38cbea988ed.jpg"  xlink:type="simple"/></disp-formula><p>Case 6: Let<img src="9-1490033\f9d89fa8-8461-49ca-9634-bec7c45455b1.jpg" />, a constant and<img src="9-1490033\e5c4deb0-1acf-4a24-86bb-25d9800f75c4.jpg" />. Then<img src="9-1490033\fad1ed3e-39a3-4469-bff4-c139ac789a72.jpg" />, <img src="9-1490033\1a4f98a2-a6bd-4585-8eba-0434886ca034.jpg" />and<img src="9-1490033\64364ae7-feac-478b-9c3d-98a668825dbd.jpg" />. The mean</p><disp-formula id="scirp.17599-formula149021"><label>(3.40)</label><graphic position="anchor" xlink:href="9-1490033\ab9abcbb-9906-499f-8b6b-4ac4f4195c27.jpg"  xlink:type="simple"/></disp-formula><p>and the variance</p><disp-formula id="scirp.17599-formula149022"><label>. (3.41)</label><graphic position="anchor" xlink:href="9-1490033\6b284ab4-ea1c-460c-8ac3-f551a09a590c.jpg"  xlink:type="simple"/></disp-formula><p>We now provide sample plots of the <img src="9-1490033\7330613d-add9-4844-8f7d-2bc278074990.jpg" /> distribution, when <img src="9-1490033\c2e5cc35-a3a9-4f36-b6bb-d6d7e55b34b4.jpg" /> follows the Vasicek [<xref ref-type="bibr" rid="scirp.17599-ref15">15</xref>] model, for three different values of the correlation (<img src="9-1490033\45855f05-21ac-4c06-8a2c-1106a0cd5934.jpg" />, 0.9 and −0.9) in Figures 1-3 respectively. In each case the distribution of <img src="9-1490033\cd9c5ebc-a821-4198-9958-4f952e8f2d7c.jpg" /> for <img src="9-1490033\8566906f-710b-4b42-b017-271a5419b4d1.jpg" /> and 20 are given. From these figures it follows that as <img src="9-1490033\90323431-584d-4c75-9fd0-06a8bd42dab8.jpg" /> increases both the mean and variance of <img src="9-1490033\db6d611e-9454-44a5-ae5d-da1e31221616.jpg" /> increases. Further, comparing Figures 1 and 2, it follows that the effect of the positive correlation (<img src="9-1490033\787a1100-499e-48c7-a676-a5e78d94fb96.jpg" />) is to reduce the peak while making the tails fatter compared to the case when<img src="9-1490033\37f58f83-2cf1-4e82-b8af-d517f9cde654.jpg" />. Similarly from Figures 1 and 3, we readily see the negative correlation has the opposite effect of increased peak and thinner tails compared to<img src="9-1490033\3b585090-872e-47ab-9a9f-089a58f12182.jpg" />.</p><p>The primary motivation for characterizing the distribution of <img src="9-1490033\baeb4cf4-5b1b-4f2b-aa2a-12fb95da63e9.jpg" /> is to compute the probability of default. Within the framework of structural models, there has been an evolution of the definition of default. In the now classic paper, Merton [<xref ref-type="bibr" rid="scirp.17599-ref10">10</xref>] defines default as the event <img src="9-1490033\58795b92-1de3-4434-874f-6670e9e4e3ee.jpg" /> bond with maturity<img src="9-1490033\b2383b5e-ff87-4e29-a55a-a12074b7f7ef.jpg" />. Using the results described above, we could readily compute the probability default according to this classical definition1.</p><p>However, Longstaff and Schwartz [<xref ref-type="bibr" rid="scirp.17599-ref11">11</xref>] define default by the event<img src="9-1490033\5384a556-b4f3-44b0-b981-d5e5c626e816.jpg" />. Recently, Giesecke [<xref ref-type="bibr" rid="scirp.17599-ref34">34</xref>] has expanded on this theme and has defined the default by the compound event <img src="9-1490033\de746f19-291f-407f-ac5c-fea93e0f05d7.jpg" />for<img src="9-1490033\021019fb-68e4-4e54-bba6-ec3877a591e9.jpg" />.</p><p>Recall that the probability of these later events can be readily calculated using the “reflection principle” if <img src="9-1490033\62d41940-f416-418c-9dde-8038d157dda8.jpg" /> is a standard Wiener process or by using the Girsanov theorem if <img src="9-1490033\53b1a11b-8094-4b66-8f78-b246cc68d29c.jpg" /> is a Wiener process with a drift. (See Elliott and Kopp [<xref ref-type="bibr" rid="scirp.17599-ref35">35</xref>] and Giesecke [<xref ref-type="bibr" rid="scirp.17599-ref34">34</xref>]). To enable computation of default probability according to Giesecke [<xref ref-type="bibr" rid="scirp.17599-ref34">34</xref>], in the following, we seek to express <img src="9-1490033\f59c0924-9c1a-45a5-b452-bd98326e540e.jpg" /> in (3.14) as the sum of a drift term and a (time changed) Wiener process.</p><p>To this end recall that every Ito integral is equivalent to a time changed Wiener process. (See Shiryaev [<xref ref-type="bibr" rid="scirp.17599-ref36">36</xref>], Oksendal [<xref ref-type="bibr" rid="scirp.17599-ref37">37</xref>], Karatzas and Shreve [<xref ref-type="bibr" rid="scirp.17599-ref25">25</xref>]). Accordingly, from (3.17) we obtain</p><disp-formula id="scirp.17599-formula149023"><label>(3.42)</label><graphic position="anchor" xlink:href="9-1490033\12464fd0-4cf8-43f9-a231-0cdf6051c4f0.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="9-1490033\d072577c-b6a1-473d-bb9c-5065f3b4e656.jpg" /> and <img src="9-1490033\bd8de3ec-8831-450a-817e-1cc8c0068962.jpg" /> are two independent Wiener process with</p><p><img src="9-1490033\f6a1f1db-543d-4868-a238-0abef71292d5.jpg" />,<img src="9-1490033\f48c3616-b134-4aa1-ad4a-c2d39a897c09.jpg" /></p><p>and <img src="9-1490033\915df32f-5c52-4728-9a44-af18b886102d.jpg" /> and <img src="9-1490033\bb0f75f8-b0c1-428b-93a5-2643cba392a1.jpg" /> are given in (3.19). Since <img src="9-1490033\fcb246ac-f167-41ae-b42a-aca8e4ed3d0e.jpg" /> and <img src="9-1490033\4e37a69a-09ae-445e-b305-17d810979c5b.jpg" /> are independent, there exists a Wiener process <img src="9-1490033\9930a81c-6eb9-4d3e-b9c1-2052f87a4031.jpg" /> such that</p><disp-formula id="scirp.17599-formula149024"><label>(3.43)</label><graphic position="anchor" xlink:href="9-1490033\cdc3a051-c4a9-4eb2-bb94-7bef4d99bc9a.jpg"  xlink:type="simple"/></disp-formula><p>where</p><p><img src="9-1490033\518d02c8-7f0e-4772-b0b4-241e4dafc51f.jpg" /></p><p>as given by (3.18)-(3.19).</p><p>Combining (3.43) with (3.14), it follows that</p><disp-formula id="scirp.17599-formula149025"><label>(3.44)</label><graphic position="anchor" xlink:href="9-1490033\e5b59b0b-659c-456c-8eda-6390dffaa1d6.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="9-1490033\f3c7e5a0-d0ee-4713-b65e-c6a5a9fea6b2.jpg" /> as in (3.20).</p><p>5. Conclusions</p><p>We have analyzed the impact of <img src="9-1490033\f8b43f52-a320-4d19-9079-9435369e6240.jpg" /> on <img src="9-1490033\5a93cf97-5f26-413f-9414-0c5539e01a7c.jpg" /> when <img src="9-1490033\d19c7be2-3f68-4cb9-9a10-f3fd8c857ee8.jpg" /> evolves according to a narrow sense linear model in <xref ref-type="table" rid="table1">Table 1</xref>(a). Consider the case when <img src="9-1490033\59448236-25ba-4004-8ecc-89a815ce6d1c.jpg" /> evolves according to a general linear model, such as for example, the Brennan-Schwartz [<xref ref-type="bibr" rid="scirp.17599-ref38">38</xref>] model in <xref ref-type="table" rid="table1">Table 1</xref>(b). In this case the explicit form of the solution for <img src="9-1490033\b932ac5c-002a-43e8-8ae0-afc22e51e2c7.jpg" /> is well known (Arnold [<xref ref-type="bibr" rid="scirp.17599-ref8">8</xref>], Gard [<xref ref-type="bibr" rid="scirp.17599-ref15">15</xref>], Lamberton and Lapeyre [<xref ref-type="bibr" rid="scirp.17599-ref7">7</xref>]) and is given by</p><p><img src="9-1490033\f0e2ea96-6307-40f3-a387-f143c4b85472.jpg" /></p><p>where the process <img src="9-1490033\fd02a13b-4191-4ae8-8ad0-cf124e79e8ca.jpg" /> is given by</p><p><img src="9-1490033\24979087-01e2-4385-90a5-7a1724133671.jpg" />with<img src="9-1490033\208548c8-f1e8-4200-97e8-9f836fc6ca07.jpg" />. Hence,</p><p><img src="9-1490033\193ad397-cf45-4998-ab7e-6b0d52b6836e.jpg" />involves a process</p><p><img src="9-1490033\f51d4c25-edf1-42c2-b566-7c39b42f8f55.jpg" /></p><p>which is an integral of the exponential functionals of the Wiener process. Processes of the type <img src="9-1490033\b7600fa0-a7a5-4ee9-8dcf-bff7d3854172.jpg" /> routinely arise in the evaluation of Asian type options (Vorst [<xref ref-type="bibr" rid="scirp.17599-ref39">39</xref>]). By relating <img src="9-1490033\0ddcb6d6-f9f5-4c3f-a0a3-c6019813d394.jpg" /> to a Bessel process, Yor [<xref ref-type="bibr" rid="scirp.17599-ref40">40</xref>] and Geman and Yor [<xref ref-type="bibr" rid="scirp.17599-ref41">41</xref>] have provided a complete characterization of the distribution of the <img src="9-1490033\f64ebb93-b5a2-494e-89c5-672c3891a53a.jpg" /> process. Combining these results with (2.5) to derive the distribution of <img src="9-1490033\73d6fe29-d83f-461b-be45-3e8e7381cf97.jpg" /> is an interesting open problem. Similarly, computing the distribution <img src="9-1490033\0ac946ee-13b7-4e30-97f1-52669585dc03.jpg" /> when <img src="9-1490033\b4155583-dd53-4f09-8548-eaa703963188.jpg" /> evolves according to the nonlinear models is <xref ref-type="table" rid="table1">Table 1</xref>(c) is also wide open. Solutions to these problem will shed further light on the impact of the choice of interest rate models on default probability and hence on credit risk analysis.</p><p>6. Acknowledgements</p><p>We are grateful to Robert J. Elliott (University of Calgary) and to Luciano Campi (Universite Paris Dauphine) for their interest and comments that improved the presentation.</p><p>REFERENCES</p></sec><sec id="s4"><title>NOTES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.17599-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">D. Hackbarth, C. A. Hennessy and H. E. 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