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Unit 23: Differentiation of Integrals




                                                                                                Notes
                                         1
                                   lim       ò   f(y)d  n (y) =  f(x)
                                   r   n (B (x))  r B (x)
                                     0
                                          r
          for  -almost all points x  R . It is important to note, however, that the measure zero set of
                                  n
              n
          “bad” points depends on the function f.
          Borel Measures on R n
          The result for Lebesgue measure turns out to be a special case of the following result, which is
          based on the Besicovitch covering theorem: if  is any locally finite Borel measure on R  and
                                                                                  n
          f : R   R is locally integrable with respect to , then
             n
                                         1
                                                     
                                   lim       ò   f(y)d (y) =  f(x)
                                    r  (B (x))  r B (x)
                                     0
                                         r
                                 n
          for -almost all points x R .
          Gaussian Measures
          The problem of the differentiation of integrals is much harder in an infinite-dimensional setting.
          Consider a separable Hilbert space (H, ,) equipped with a Gaussian measure . As stated in the
          article on the Vitali covering theorem, the Vitali covering theorem fails for Gaussian measures
          on infinite-dimensional Hilbert spaces. Two results of David Preiss (1981 and 1983) show the
          kind of difficulties that one can expect to encounter in this setting:

              There is a Gaussian measure  on a separable Hilbert space H and a Borel set M  H so that,
               for -almost all x  H,

                                             (M B (x))
                                               Ç
                                        lim       r   =  1
                                         r  0   (B (x))
                                                r
                                                                                1
              There is a Gaussian measure  on a separable Hilbert space H and a function f  L (H, ; R)
               such that
                                  ì   1                        ü
                                                 
                                                      
                                                               r - +¥
                                                            s
                            lim inf í     ò Ds(x)  f(y)d (y) x II, 0 < < ý
                            r  0   (B (x))
                                  ï î  s                       ï þ
          However, there is some hope if one has good control over the covariance of . Let the covariance
          operator of  be S : H  H given by
                                                  
                                                  
                                      Sx, y =  H ò   x, z y, z d (z)
                                                        
                                                      
          or, for some countable orthonormal basis (e )   of H,
                                              i iN
                                                2
                                                     
                                         Sx =  å s  x, e e .
                                                    i
                                                1
                                                       i
                                             i N
                                             
          In 1981, Preiss and Jaroslav Tišer showed that if there exists a constant 0 < q < 1 such that
                                            s  2 i 1  £ qs  2 i  ,
                                              +
          then, for all f  L (H, ; R),
                        1
                                      1                
                                                 
                                         ò   f(y)d (y) ¾¾¾ f(x)
                                    (B (x))  r B (x)  r  0
                                      r
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