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Article: Modeling defaults with nested Archimedean copulas

TitleModeling defaults with nested Archimedean copulas
Authors
Issue Date2010
Citation
Blaetter der DGVFM, 2010, v. 31, n. 2, p. 213-224 How to Cite?
AbstractIn 2001, Schönbucher and Schubert extended Li's well-known Gaussian copula model for modeling dependent defaults to allow for tail dependence. Instead of the Gaussian copula, Schönbucher and Schubert suggested to use Archimedean copulas. These copulas are able to capture tail dependence and therefore allow a standard intensity-based default model to have a positive probability of joint defaults within a short time period. As can be observed in the current financial crisis, this is an indispensable feature of any realistic default model. Another feature, motivated by empirical observations but rarely taken into account in default models, is that modeled portfolio components affected by defaults show significantly different levels of dependence depending on whether they belong to the same industry sector or not. The present work presents an extension of the model suggested by Schönbucher and Schubert to account for this fact. For this, nested Archimedean copulas are applied. As an application, the pricing of collateralized debt obligations is treated. Since the resulting loss distribution is not analytical tractable, fast sampling algorithms for nested Archimedean copulas are developed. Such algorithms boil down to sampling certain distributions given by their Laplace-Stieltjes transforms. For a large range of nested Archimedean copulas, efficient sampling techniques can be derived. Moreover, a general transformation of an Archimedean generator allows to construct and sample the corresponding nested Archimedean copulas. © 2010 DAV / DGVFM.
Persistent Identifierhttp://hdl.handle.net/10722/325215
ISSN

 

DC FieldValueLanguage
dc.contributor.authorHofert, Marius-
dc.date.accessioned2023-02-27T07:30:40Z-
dc.date.available2023-02-27T07:30:40Z-
dc.date.issued2010-
dc.identifier.citationBlaetter der DGVFM, 2010, v. 31, n. 2, p. 213-224-
dc.identifier.issn1864-0281-
dc.identifier.urihttp://hdl.handle.net/10722/325215-
dc.description.abstractIn 2001, Schönbucher and Schubert extended Li's well-known Gaussian copula model for modeling dependent defaults to allow for tail dependence. Instead of the Gaussian copula, Schönbucher and Schubert suggested to use Archimedean copulas. These copulas are able to capture tail dependence and therefore allow a standard intensity-based default model to have a positive probability of joint defaults within a short time period. As can be observed in the current financial crisis, this is an indispensable feature of any realistic default model. Another feature, motivated by empirical observations but rarely taken into account in default models, is that modeled portfolio components affected by defaults show significantly different levels of dependence depending on whether they belong to the same industry sector or not. The present work presents an extension of the model suggested by Schönbucher and Schubert to account for this fact. For this, nested Archimedean copulas are applied. As an application, the pricing of collateralized debt obligations is treated. Since the resulting loss distribution is not analytical tractable, fast sampling algorithms for nested Archimedean copulas are developed. Such algorithms boil down to sampling certain distributions given by their Laplace-Stieltjes transforms. For a large range of nested Archimedean copulas, efficient sampling techniques can be derived. Moreover, a general transformation of an Archimedean generator allows to construct and sample the corresponding nested Archimedean copulas. © 2010 DAV / DGVFM.-
dc.languageeng-
dc.relation.ispartofBlaetter der DGVFM-
dc.titleModeling defaults with nested Archimedean copulas-
dc.typeArticle-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1007/s11857-010-0123-1-
dc.identifier.scopuseid_2-s2.0-78649792805-
dc.identifier.volume31-
dc.identifier.issue2-
dc.identifier.spage213-
dc.identifier.epage224-
dc.identifier.eissn1864-0303-

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