2012/05/29 by Mirko D’Ovidio, Mirko D'Ovidio, D'Ovidio, Mirko +2
Mathematics · Physics and Astronomy · #Advanced Mathematical Theories and Applications #FOS: Mathematics #Fractional Differential Equations Solutions #Geometric Analysis and Curvature Flows #Probability (math.PR) #math.PR
paper · pdf · doi:10.48550/arxiv.1205.6280
37 pages
openalex publication_date 2012/05/29 · arxiv created 2012/10/05 · arxiv updated 2012/10/08 · openalex created_date 2019/06/27 · openalex updated_date 2026/07/28
We introduce a class of isotropic time dependent random fields on the non-homogeneous sphere represented by a time-changed spherical Brownian motion of order ν∈ (0,1] with which some anisotrophies can be captured in Cosmology. This process is a time-changed rotational diffusion (TRD) or the stochastic solution to the equation involving the spherical Laplace operator and a time-fractional derivative of order ν. TRD is a diffusion on the non-homogeneous sphere and therefore, the spherical coordinates given by TRD represent the coordinates of a non-homogeneous sphere by means of which an isotopic random field is indexed. The time dependent random fields we present in this work is therefore realized through composition and can be viewed as isotropic random field on randomly varying sphere.