246 research outputs found

    Smoothness of the density for solutions to Gaussian rough differential equations

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    We consider stochastic differential equations of the form dYt=V(Yt)dXt+V0(Yt)dtdY_t=V(Y_t)\,dX_t+V_0(Y_t)\,dt driven by a multi-dimensional Gaussian process. Under the assumption that the vector fields V0V_0 and V=(V1,,Vd)V=(V_1,\ldots,V_d) satisfy H\"{o}rmander's bracket condition, we demonstrate that YtY_t admits a smooth density for any t(0,T]t\in(0,T], provided the driving noise satisfies certain nondegeneracy assumptions. Our analysis relies on relies on an interplay of rough path theory, Malliavin calculus and the theory of Gaussian processes. Our result applies to a broad range of examples including fractional Brownian motion with Hurst parameter H>1/4H>1/4, the Ornstein-Uhlenbeck process and the Brownian bridge returning after time TT.Comment: Published in at http://dx.doi.org/10.1214/13-AOP896 the Annals of Probability (http://www.imstat.org/aop/) by the Institute of Mathematical Statistics (http://www.imstat.org

    A dual algorithm for stochastic control problems : Applications to Uncertain Volatility Models and CVA

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    We derive an algorithm in the spirit of Rogers [SIAM J. Control Optim., 46 (2007), pp. 1116--1132] and Davis and Burstein [Stochastics Stochastics Rep., 40 (1992), pp. 203--256] that leads to upper bounds for stochastic control problems. Our bounds complement lower biased estimates recently obtained in Guyon and Henry-Labordère [J. Comput. Finance, 14 (2011), pp. 37--71]. We evaluate our estimates in numerical examples motivated by mathematical finance. Read More: http://epubs.siam.org/doi/10.1137/15M101994

    On the integration of weakly geometric rough paths

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    We close a gap in the theory of integration for weakly geometric rough paths in the in…nite-dimensional setting. We show that the integral of a weakly geometric rough path against a su¢ ciently regular one form is, once again, a weakly geometric rough path

    Gravitational wave behavior at a vacuum-matter interface

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    In classical electrodynamics, boundary conditions of the E and B fields are derived from Maxwell\u27s equations, which are used to derive the Fresnel equations describing the behavior of a wave at an interface between media with given indices of refraction. Though electrodynamics and gravity are in some instances strikingly analogous, boundary conditions in general relativity are somewhat more opaque. We will see that while while continuity of the metric must be true in general, discontinuity of the extrinsic curvature of spacetime, while allowed by the Einstein field equations, results in a singularity in the energy-momentum tensor. This singularity is interpreted as a surface mass density. Unlike in electrodynamics, there is an additional refractive effect of the spacetime metric. Its origin considered, a gravitational refractive index will be treated similarly to the electromagnetic refractive index. Attempts to derive gravitational Fresnel equations follow
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