Exact vs approximate Riemann solvers












1














I am trying to understand numerical methods for conservation laws. I am confused with few terminologies. I have the following doubts.




  1. When do we say that a numerical scheme for a conservation law is a Riemann solver?


  2. What is the difference between approximate and exact Riemann solvers?


  3. I read that Godunov scheme is an exact Riemann solver, but is there any other scheme which is exact Riemann solver?











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    1














    I am trying to understand numerical methods for conservation laws. I am confused with few terminologies. I have the following doubts.




    1. When do we say that a numerical scheme for a conservation law is a Riemann solver?


    2. What is the difference between approximate and exact Riemann solvers?


    3. I read that Godunov scheme is an exact Riemann solver, but is there any other scheme which is exact Riemann solver?











    share|cite|improve this question



























      1












      1








      1







      I am trying to understand numerical methods for conservation laws. I am confused with few terminologies. I have the following doubts.




      1. When do we say that a numerical scheme for a conservation law is a Riemann solver?


      2. What is the difference between approximate and exact Riemann solvers?


      3. I read that Godunov scheme is an exact Riemann solver, but is there any other scheme which is exact Riemann solver?











      share|cite|improve this question















      I am trying to understand numerical methods for conservation laws. I am confused with few terminologies. I have the following doubts.




      1. When do we say that a numerical scheme for a conservation law is a Riemann solver?


      2. What is the difference between approximate and exact Riemann solvers?


      3. I read that Godunov scheme is an exact Riemann solver, but is there any other scheme which is exact Riemann solver?








      pde numerical-methods terminology hyperbolic-equations






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      edited Dec 18 '18 at 13:58









      Harry49

      6,00121031




      6,00121031










      asked Dec 17 '18 at 11:58









      RosyRosy

      1045




      1045






















          2 Answers
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          0














          To make everything clear, let us go back to Godunov's method for scalar conservation laws $u_t + f(u)_x = 0$. Godunov's method reads
          $$
          u_i^{n+1} = u_i^n - frac{Delta t}{Delta x}(f_{i+1/2} - f_{i-1/2})
          $$

          where $u_i^n simeq u(x_i, t_n)$, $x_{i+1} = x_i+Delta x$, $t_{n+1} = t_n+Delta t$, and $f_{i+1/2}$ is the numerical flux at $x_{i+1/2}$. The latter is given by
          $f_{i+1/2} = f (u^*)$,
          where $u^*$ is obtained by evaluating the solution to the Riemann problem
          $$
          u(x,t_n) = leftlbrace
          begin{aligned}
          & u_i^n & & text{if}quad x<x_{i+1/2}\
          & u_{i+1}^n & & text{if}quad x>x_{i+1/2}
          end{aligned}
          right.
          $$

          at $(x_{i+1/2}, t_{n+1})$ (see Sec. 4.11 of [1]). If this computation does not require all the Riemann solution, it requires a full knowledge of its structure, i.e. what we call an exact Riemann solver. This notion is intrinsically linked to the Godunov method.



          In some cases it may be very expensive to evaluate $u^*$ exactly as defined above. Thus, approximate Riemann solvers are sometimes preferred. For instance, one can name the Roe, HLLE, and HLLC solvers (see Sec. 15.3 of [1]). Those methods introduce approximations of $u^*$ which are easier to compute than the exact $u^*$. However, one should be careful since approximate Riemann solvers can introduce artifacts for particular solutions (e.g. transsonic rarefactions and slow-moving shocks).





          [1] R.J. LeVeque, Finite Volume Methods for Hyperbolic Problems, Cambridge University Press, 2002, doi:10.1017/CBO9780511791253






          share|cite|improve this answer































            0














            In addition to Harry49's answer, I would recommend you a book to read if you want to know more about Riemann solvers from basic to advanced things:



            E.F. Toro, Riemann solvers and numerical methods for fluid dynamics, 3rd edition, 2009



            I know it helped me a lot.






            share|cite|improve this answer





















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              2 Answers
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              2 Answers
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              0














              To make everything clear, let us go back to Godunov's method for scalar conservation laws $u_t + f(u)_x = 0$. Godunov's method reads
              $$
              u_i^{n+1} = u_i^n - frac{Delta t}{Delta x}(f_{i+1/2} - f_{i-1/2})
              $$

              where $u_i^n simeq u(x_i, t_n)$, $x_{i+1} = x_i+Delta x$, $t_{n+1} = t_n+Delta t$, and $f_{i+1/2}$ is the numerical flux at $x_{i+1/2}$. The latter is given by
              $f_{i+1/2} = f (u^*)$,
              where $u^*$ is obtained by evaluating the solution to the Riemann problem
              $$
              u(x,t_n) = leftlbrace
              begin{aligned}
              & u_i^n & & text{if}quad x<x_{i+1/2}\
              & u_{i+1}^n & & text{if}quad x>x_{i+1/2}
              end{aligned}
              right.
              $$

              at $(x_{i+1/2}, t_{n+1})$ (see Sec. 4.11 of [1]). If this computation does not require all the Riemann solution, it requires a full knowledge of its structure, i.e. what we call an exact Riemann solver. This notion is intrinsically linked to the Godunov method.



              In some cases it may be very expensive to evaluate $u^*$ exactly as defined above. Thus, approximate Riemann solvers are sometimes preferred. For instance, one can name the Roe, HLLE, and HLLC solvers (see Sec. 15.3 of [1]). Those methods introduce approximations of $u^*$ which are easier to compute than the exact $u^*$. However, one should be careful since approximate Riemann solvers can introduce artifacts for particular solutions (e.g. transsonic rarefactions and slow-moving shocks).





              [1] R.J. LeVeque, Finite Volume Methods for Hyperbolic Problems, Cambridge University Press, 2002, doi:10.1017/CBO9780511791253






              share|cite|improve this answer




























                0














                To make everything clear, let us go back to Godunov's method for scalar conservation laws $u_t + f(u)_x = 0$. Godunov's method reads
                $$
                u_i^{n+1} = u_i^n - frac{Delta t}{Delta x}(f_{i+1/2} - f_{i-1/2})
                $$

                where $u_i^n simeq u(x_i, t_n)$, $x_{i+1} = x_i+Delta x$, $t_{n+1} = t_n+Delta t$, and $f_{i+1/2}$ is the numerical flux at $x_{i+1/2}$. The latter is given by
                $f_{i+1/2} = f (u^*)$,
                where $u^*$ is obtained by evaluating the solution to the Riemann problem
                $$
                u(x,t_n) = leftlbrace
                begin{aligned}
                & u_i^n & & text{if}quad x<x_{i+1/2}\
                & u_{i+1}^n & & text{if}quad x>x_{i+1/2}
                end{aligned}
                right.
                $$

                at $(x_{i+1/2}, t_{n+1})$ (see Sec. 4.11 of [1]). If this computation does not require all the Riemann solution, it requires a full knowledge of its structure, i.e. what we call an exact Riemann solver. This notion is intrinsically linked to the Godunov method.



                In some cases it may be very expensive to evaluate $u^*$ exactly as defined above. Thus, approximate Riemann solvers are sometimes preferred. For instance, one can name the Roe, HLLE, and HLLC solvers (see Sec. 15.3 of [1]). Those methods introduce approximations of $u^*$ which are easier to compute than the exact $u^*$. However, one should be careful since approximate Riemann solvers can introduce artifacts for particular solutions (e.g. transsonic rarefactions and slow-moving shocks).





                [1] R.J. LeVeque, Finite Volume Methods for Hyperbolic Problems, Cambridge University Press, 2002, doi:10.1017/CBO9780511791253






                share|cite|improve this answer


























                  0












                  0








                  0






                  To make everything clear, let us go back to Godunov's method for scalar conservation laws $u_t + f(u)_x = 0$. Godunov's method reads
                  $$
                  u_i^{n+1} = u_i^n - frac{Delta t}{Delta x}(f_{i+1/2} - f_{i-1/2})
                  $$

                  where $u_i^n simeq u(x_i, t_n)$, $x_{i+1} = x_i+Delta x$, $t_{n+1} = t_n+Delta t$, and $f_{i+1/2}$ is the numerical flux at $x_{i+1/2}$. The latter is given by
                  $f_{i+1/2} = f (u^*)$,
                  where $u^*$ is obtained by evaluating the solution to the Riemann problem
                  $$
                  u(x,t_n) = leftlbrace
                  begin{aligned}
                  & u_i^n & & text{if}quad x<x_{i+1/2}\
                  & u_{i+1}^n & & text{if}quad x>x_{i+1/2}
                  end{aligned}
                  right.
                  $$

                  at $(x_{i+1/2}, t_{n+1})$ (see Sec. 4.11 of [1]). If this computation does not require all the Riemann solution, it requires a full knowledge of its structure, i.e. what we call an exact Riemann solver. This notion is intrinsically linked to the Godunov method.



                  In some cases it may be very expensive to evaluate $u^*$ exactly as defined above. Thus, approximate Riemann solvers are sometimes preferred. For instance, one can name the Roe, HLLE, and HLLC solvers (see Sec. 15.3 of [1]). Those methods introduce approximations of $u^*$ which are easier to compute than the exact $u^*$. However, one should be careful since approximate Riemann solvers can introduce artifacts for particular solutions (e.g. transsonic rarefactions and slow-moving shocks).





                  [1] R.J. LeVeque, Finite Volume Methods for Hyperbolic Problems, Cambridge University Press, 2002, doi:10.1017/CBO9780511791253






                  share|cite|improve this answer














                  To make everything clear, let us go back to Godunov's method for scalar conservation laws $u_t + f(u)_x = 0$. Godunov's method reads
                  $$
                  u_i^{n+1} = u_i^n - frac{Delta t}{Delta x}(f_{i+1/2} - f_{i-1/2})
                  $$

                  where $u_i^n simeq u(x_i, t_n)$, $x_{i+1} = x_i+Delta x$, $t_{n+1} = t_n+Delta t$, and $f_{i+1/2}$ is the numerical flux at $x_{i+1/2}$. The latter is given by
                  $f_{i+1/2} = f (u^*)$,
                  where $u^*$ is obtained by evaluating the solution to the Riemann problem
                  $$
                  u(x,t_n) = leftlbrace
                  begin{aligned}
                  & u_i^n & & text{if}quad x<x_{i+1/2}\
                  & u_{i+1}^n & & text{if}quad x>x_{i+1/2}
                  end{aligned}
                  right.
                  $$

                  at $(x_{i+1/2}, t_{n+1})$ (see Sec. 4.11 of [1]). If this computation does not require all the Riemann solution, it requires a full knowledge of its structure, i.e. what we call an exact Riemann solver. This notion is intrinsically linked to the Godunov method.



                  In some cases it may be very expensive to evaluate $u^*$ exactly as defined above. Thus, approximate Riemann solvers are sometimes preferred. For instance, one can name the Roe, HLLE, and HLLC solvers (see Sec. 15.3 of [1]). Those methods introduce approximations of $u^*$ which are easier to compute than the exact $u^*$. However, one should be careful since approximate Riemann solvers can introduce artifacts for particular solutions (e.g. transsonic rarefactions and slow-moving shocks).





                  [1] R.J. LeVeque, Finite Volume Methods for Hyperbolic Problems, Cambridge University Press, 2002, doi:10.1017/CBO9780511791253







                  share|cite|improve this answer














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                  edited Dec 18 '18 at 14:21

























                  answered Dec 18 '18 at 13:46









                  Harry49Harry49

                  6,00121031




                  6,00121031























                      0














                      In addition to Harry49's answer, I would recommend you a book to read if you want to know more about Riemann solvers from basic to advanced things:



                      E.F. Toro, Riemann solvers and numerical methods for fluid dynamics, 3rd edition, 2009



                      I know it helped me a lot.






                      share|cite|improve this answer


























                        0














                        In addition to Harry49's answer, I would recommend you a book to read if you want to know more about Riemann solvers from basic to advanced things:



                        E.F. Toro, Riemann solvers and numerical methods for fluid dynamics, 3rd edition, 2009



                        I know it helped me a lot.






                        share|cite|improve this answer
























                          0












                          0








                          0






                          In addition to Harry49's answer, I would recommend you a book to read if you want to know more about Riemann solvers from basic to advanced things:



                          E.F. Toro, Riemann solvers and numerical methods for fluid dynamics, 3rd edition, 2009



                          I know it helped me a lot.






                          share|cite|improve this answer












                          In addition to Harry49's answer, I would recommend you a book to read if you want to know more about Riemann solvers from basic to advanced things:



                          E.F. Toro, Riemann solvers and numerical methods for fluid dynamics, 3rd edition, 2009



                          I know it helped me a lot.







                          share|cite|improve this answer












                          share|cite|improve this answer



                          share|cite|improve this answer










                          answered Jan 5 at 23:13









                          MarkMark

                          4617




                          4617






























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