Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/16907
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dc.contributor.authorMárquez, David (Márquez Carreras)cat
dc.contributor.authorSanz-Solé, Martacat
dc.date.accessioned2011-03-08T09:48:54Z-
dc.date.available2011-03-08T09:48:54Z-
dc.date.issued1998-
dc.identifier.issn0610-0757-
dc.identifier.urihttp://hdl.handle.net/2445/16907-
dc.description.abstractWe prove a general result on asymptotic expansions of densities for families of perturbed Wiener functionals. As an application, we consider a stochastic heat equation driven by a space-time white noise εW˙ t,x, ε ∈ (0, 1]. The main theorem describes the asymptotics, as ε ↓ 0, of the density pε t,x(y) of the solution at a fixed point (t, x) for some particular value y ∈ R, which, in the diffusion case, plays the role of the diagonal.-
dc.format.extent17 p.-
dc.format.mimetypeapplication/pdf-
dc.language.isoengeng
dc.publisherUniversitat de Barcelonacat
dc.relation.isformatofReproducció del document publicat a: http://www.collectanea.ub.edu/index.php/Collectanea/article/view/3949/4789cat
dc.relation.ispartofCollectanea Mathematica, 1998, vol. 49, num. 2-3, p. 399-415cat
dc.rights(c) Universitat de Barcelona, 1998-
dc.sourceArticles publicats en revistes (Matemàtiques i Informàtica)-
dc.subject.classificationEquacions integrals estocàstiquescat
dc.subject.classificationCàlcul de Malliavincat
dc.subject.otherStochastic differential equationseng
dc.subject.otherMalliavin calculuseng
dc.titleTaylor expansion of the density in a stochastic heat equationeng
dc.typeinfo:eu-repo/semantics/article-
dc.typeinfo:eu-repo/semantics/publishedVersion-
dc.identifier.idgrec146424-
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess-
Appears in Collections:Articles publicats en revistes (Matemàtiques i Informàtica)

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