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P. 342

7.5. Maximum Principle for the One-Step-Theta Method  325


        where
                                                             
                         I + τΘA h
                                    .
                                    .                  0     
                      −I + τΘA h     .                       
                                                             
                                    .       .
                                    .       .                
                C h =                .       .                ,
                                                             
                            0              .       .
                                         .       .           
                                           .       .         
                                        −I + τΘA h   I + τΘA h
        again with Θ:=1 − Θ,
                                                      
                               τq (Θτ)+(I − τΘA h )u 0
                                 h
                                   τq ((1 + Θ)τ)      
                                     h                
                                                      
                                         .            
                        p =              . .           .
                         h
                                                      
                                          .
                                                      
                                          .
                                         .            
                                  τq (N − 1+Θ)τ)
                                     h
        Since the spatial discretization is performed as in the stationary case, and
        in the nth step the discretization relates to t = t n−1 +Θτ and also the
        approximation
                     A h u(t n−1 +Θτ) ∼ ΘA h u(t n−1 )+ΘA h u(t n )
        enters the formulation (7.66), we can assume to have the following structure
        of the right-hand side of (7.66):
                           ˆ
                                         n
        q ((n−1+Θ)τ)= −A h (Θˆ u n−1  +Θˆ u )+f((n−1+Θ)τ)for n =1,...,N.
         h
                                         h
                                 h
                                                                    (7.98)
                  n
        Here the ˆ u ∈ R M 2  are the known spatial boundary values on time level
                  h
        t n , which have been eliminated from the equation as explained, e.g., in
        Chapter 1 for the finite difference method. But as noted, we allow also for
        the case where such values do not appear (i.e., M 2 = 0) then (7.98) reduces
        to
               q ((n − 1+Θ)τ)= f((n − 1+Θ)τ)     for  n =1,... ,N .
                h
        For the continuous problem, data are prescribed at the parabolic boundary
                                                            i
        Ω ×{0}∪ ∂Ω × [0,T ]; correspondingly, the known values ˆ u are collected
                                                            h
        with the initial data u 0 ∈ R M 1  to a large vector
                                            
                                         u 0
                                       ˆ u 0  
                                           h
                                          1  
                                         ˆ u h  ,
                                            
                                 ˆ u h = 
                                          .
                                         .  
                                         .  
                                         ˆ u N
                                          h
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