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Heat and mass transfers in the context of energy geostructures  117


                      The variation of the heat transfer coefficient as a consequence of the development
                   of the boundary layers has noteworthy consequences for heat transfer analyses.
                   Varying heat transfer coefficients are associated with different heat transfer rates by
                   convection. In the context of energy geostructures, relevant heat transfer rates by con-
                   vection can take place, for instance, between the surface of the energy geostructure,
                   such as energy walls and tunnels, and adjacent underground built environments, as
                   well as between the heat carrier fluid circulating in the pipes embedded in energy
                   geostructures and the surroundings.



                   3.15 Momentum conservation equation
                   3.15.1 General

                   The momentum conservation equation expresses the principle of balance of linear
                   momentum. This conservation equation is also termed Cauchy’s first law of motion or
                   the Cauchy momentum equation. When applied to the analysis of problems of internal
                   and external flows in which due account is made of the equilibrium of the moving
                   fluid, the momentum conservation equation is typically expressed in the form of the
                   Navier Stokes equations.


                   3.15.2 Navier Stokes equations

                   The Navier Stokes equations can be derived in a similar fashion to the conservation
                   of mass (see for further details, e.g. Lewis et al. (1996)). For a viscous incompressible
                   flow they read

                                                              2
                                          dρ v rf ;i
                                            f
                                                                                         ð3:53Þ
                                                52 rp f 1 μ r v rf ;i 1 ρ b i
                                                            f         f
                                            dt
                   where b i is the vector of body forces. In indicial form
                                                                     2

                                  ρ   @v rf ;k  @v rf ;k  52  @p f  1 μ  @ v rf ;k       ð3:54Þ
                                                                       2  1 ρ b i
                                           1 v rf ;j
                                   f                               f         f
                                       @t        @x j      @x k      @x
                                                                       k
                      The Navier Stokes equations can be simplified to yield the Euler equations for
                   describing inviscid flows. Together with the mass conservation equation, the
                   Navier Stokes equations allow the describing of internal and external flow pro-
                   blems in which due account of the equilibrium of the fluid in motion is made
                   under isothermal conditions. Under nonisothermal conditions, the energy conserva-
                   tion equation must be added to the previous equations to solve the problem
                   addressed.
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