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19th Discrete Simulation                POLITECNICO DI TORINO
   of Fluid Dynamics                    DEPARTMENT OF ENERGETICS




    Radiative lattice Boltzmann method
     applied to combustion simulation
      and reduced chemical kinetics

            A. F. Di Rienzo, E. Chiavazzo, P. Asinari


                  July 5-9, 2010 – Rome, Italy

                                                             1
POLITECNICO DI TORINO             Introduction
GOAL OF THE TALK
To point out (a) the derivation of the lattice Boltzmann model for
solving radiative heat transfer in an absorbing and emitting
medium and (b) how this model can be coupled with combustion
simulation via lattice Boltzmann and reduced chemical kinetics.

KEY POINTS
    Combustion: to decouple fast and slow dynamics.
    Radiation: to compute radiative source term to be used
    in combustion model.
    Coupling:     to   investigate   radiative   contribution   to
    combustion for a reactive gas mixture of hydrogen and
    air.
                                                                 2
POLITECNICO DI TORINO                                     Combustion 1/2
ASSUMPTIONS:
1. Flow field is incompressible and not affected by chemical reaction.
2. Transport properties are constant.
3. Fick’s law applies to diffusion
4. Viscous energy dissipation is neglected and radiative heat transfer is
    discussed next.

Evolution equations for enthalpy and mass concentration of species i are:




    H2+Air             9 species         ([1], [2])                   9+1 equations to be solved!
[1] J. Li, Z. Zhao, A. Kazakov. F. L. Dryer, Int. J. Chem. Kinet., 2004
[2] K. Yamamoto et al., J. Stat. Phys. 107 (2002) 367–383                                      3
POLITECNICO DI TORINO                                Combustion 2/2
  ISSUES:
  • Solution of a large number of conservation equations

  • Stiffness: high computational time



REDUCTION TECHNIQUES, FAST-SLOW MOTION DECOMPOSITION ([3],[4])

                                                     Primitive variables are re-parameterized
                                                     in terms of new slow quantities

                                                     The dynamics of                is expected to be
                                                     slower than



 [3] E. Chiavazzo, I. Karlin, A. N. Gorban, K. Boulouchos, JSTAT, 2009
 [4] E. Chiavazzo, I. Karlin, A. N. Gorban, K. Boulouchos, Combust. Flame, in press, 2010               4
POLITECNICO DI TORINO                Radiation 1/3



• SCATTERING


                    Rayleigh scattering
                    theory


Participating medium is absorbing and emitting. RTE reduces:




                                                               5
POLITECNICO DI TORINO              Radiation 2/3
• ABSORPTION

NARROW BAND MODELS and WIDE BAND MODELS rigorously
describe absorption of gases. Drawback: more time consuming than the
solution of the RTE itself.

PLANCK-MEAN ABSORPTION COEFFICIENT: less sophisticated and
easy to incorporate in the RTE numerical scheme.




                     H2O




                                                                 6
POLITECNICO DI TORINO                                      Radiation 3/3


PSEUDO-TRANSIENT RTE




2-D PSEUDO-TRANSIENT RTE




                                                                                                              [5]


[5] P. Asinari, S. C. Mishra, R. Borchiellini, A lattice Boltzmann formulation to the analysis of radiative
heat transfer problems in a participating medium, NHT-B, in press, 2010                                       7
POLITECNICO DI TORINO               Coupling 1/2
DISTRIBUTION FUNCTION FOR MIXTURE AVERAGE TOTAL
ENTHALPY



RADIATIVE SOURCE TERM



                   Radiative heat flux   Incident radiation




                                                              8
POLITECNICO DI TORINO                                     Coupling 2/2
REGIONS OF INFLUENCE ([6])




                  D2Q8
[6]A. F. Di Rienzo, P. Asinari, R. Borchiellini, S. C. Mishra, Improved angular discretization and error
analysis of the lattice Boltzmann method for solving radiative heat transfer in a participating medium,
submitted to JNMH&FF, 2010                                                                                 9
POLITECNICO DI TORINO            Example
2-D LAMINAR BURNER

                         REACTIVE MIXTURE
                         Premixed hydrogen/air
                         mixture at Tin=300 K.

                         DOMAIN SIZE
                         Lx = 1.4 mm
                         Ly = 7.3 mm

                         NUMERICAL RESOLUTION
                         Nx = 65
                         Ny = 330




                                                 10
POLITECNICO DI TORINO            Case 1- Dry H2
TEMPERATURE FIELD

  Time = 1.11 ms       Time = 2.22 ms           Time = 4.44 ms




Comb.    Comb.+ Rad   Comb.      Comb.+ Rad   Comb.    Comb.+ Rad
                                                                 11
POLITECNICO DI TORINO       Case 1- Dry H2

Time = 2.22 ms
                             TRANSPARENT MEDIUM:
                                   H2+AIR




                         NO EFFECT OF RADIATIVE
                         HEAT TRANSFER !!!
                                             12
POLITECNICO DI TORINO        Case 2- Wet H2
FRESH MIXTURE: H2+Air+H2O     Non-reactive

                                  Comb.      Comb.+ Rad




                                                          13
POLITECNICO DI TORINO          Case 2- Wet H2


Even though the fresh mixture (H2+Air+H2O) is opaque,
contribution of radiative heat transfer is so small that it can be
neglected.




                                                             14
POLITECNICO DI TORINO                  Conclusions

1. Radiative   LBM        can   be   effectively   coupled   with
  combustion model, by providing it the enthalpy rate
  (radiative source term).
2. For transparent reactive mixture (H2+Air), radiative
  contribution is null:


3. For opaque fresh mixture (H2+Air+H2O), radiative
  contribution can be neglected as well:


                                                               15
POLITECNICO DI TORINO




THANKS FOR YOUR
   ATTENTION!


                         16

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Radiative lattice Boltzmann method applied to combustion simulation and reduced chemical kinetics

  • 1. 19th Discrete Simulation POLITECNICO DI TORINO of Fluid Dynamics DEPARTMENT OF ENERGETICS Radiative lattice Boltzmann method applied to combustion simulation and reduced chemical kinetics A. F. Di Rienzo, E. Chiavazzo, P. Asinari July 5-9, 2010 – Rome, Italy 1
  • 2. POLITECNICO DI TORINO Introduction GOAL OF THE TALK To point out (a) the derivation of the lattice Boltzmann model for solving radiative heat transfer in an absorbing and emitting medium and (b) how this model can be coupled with combustion simulation via lattice Boltzmann and reduced chemical kinetics. KEY POINTS Combustion: to decouple fast and slow dynamics. Radiation: to compute radiative source term to be used in combustion model. Coupling: to investigate radiative contribution to combustion for a reactive gas mixture of hydrogen and air. 2
  • 3. POLITECNICO DI TORINO Combustion 1/2 ASSUMPTIONS: 1. Flow field is incompressible and not affected by chemical reaction. 2. Transport properties are constant. 3. Fick’s law applies to diffusion 4. Viscous energy dissipation is neglected and radiative heat transfer is discussed next. Evolution equations for enthalpy and mass concentration of species i are: H2+Air 9 species ([1], [2]) 9+1 equations to be solved! [1] J. Li, Z. Zhao, A. Kazakov. F. L. Dryer, Int. J. Chem. Kinet., 2004 [2] K. Yamamoto et al., J. Stat. Phys. 107 (2002) 367–383 3
  • 4. POLITECNICO DI TORINO Combustion 2/2 ISSUES: • Solution of a large number of conservation equations • Stiffness: high computational time REDUCTION TECHNIQUES, FAST-SLOW MOTION DECOMPOSITION ([3],[4]) Primitive variables are re-parameterized in terms of new slow quantities The dynamics of is expected to be slower than [3] E. Chiavazzo, I. Karlin, A. N. Gorban, K. Boulouchos, JSTAT, 2009 [4] E. Chiavazzo, I. Karlin, A. N. Gorban, K. Boulouchos, Combust. Flame, in press, 2010 4
  • 5. POLITECNICO DI TORINO Radiation 1/3 • SCATTERING Rayleigh scattering theory Participating medium is absorbing and emitting. RTE reduces: 5
  • 6. POLITECNICO DI TORINO Radiation 2/3 • ABSORPTION NARROW BAND MODELS and WIDE BAND MODELS rigorously describe absorption of gases. Drawback: more time consuming than the solution of the RTE itself. PLANCK-MEAN ABSORPTION COEFFICIENT: less sophisticated and easy to incorporate in the RTE numerical scheme. H2O 6
  • 7. POLITECNICO DI TORINO Radiation 3/3 PSEUDO-TRANSIENT RTE 2-D PSEUDO-TRANSIENT RTE [5] [5] P. Asinari, S. C. Mishra, R. Borchiellini, A lattice Boltzmann formulation to the analysis of radiative heat transfer problems in a participating medium, NHT-B, in press, 2010 7
  • 8. POLITECNICO DI TORINO Coupling 1/2 DISTRIBUTION FUNCTION FOR MIXTURE AVERAGE TOTAL ENTHALPY RADIATIVE SOURCE TERM Radiative heat flux Incident radiation 8
  • 9. POLITECNICO DI TORINO Coupling 2/2 REGIONS OF INFLUENCE ([6]) D2Q8 [6]A. F. Di Rienzo, P. Asinari, R. Borchiellini, S. C. Mishra, Improved angular discretization and error analysis of the lattice Boltzmann method for solving radiative heat transfer in a participating medium, submitted to JNMH&FF, 2010 9
  • 10. POLITECNICO DI TORINO Example 2-D LAMINAR BURNER REACTIVE MIXTURE Premixed hydrogen/air mixture at Tin=300 K. DOMAIN SIZE Lx = 1.4 mm Ly = 7.3 mm NUMERICAL RESOLUTION Nx = 65 Ny = 330 10
  • 11. POLITECNICO DI TORINO Case 1- Dry H2 TEMPERATURE FIELD Time = 1.11 ms Time = 2.22 ms Time = 4.44 ms Comb. Comb.+ Rad Comb. Comb.+ Rad Comb. Comb.+ Rad 11
  • 12. POLITECNICO DI TORINO Case 1- Dry H2 Time = 2.22 ms TRANSPARENT MEDIUM: H2+AIR NO EFFECT OF RADIATIVE HEAT TRANSFER !!! 12
  • 13. POLITECNICO DI TORINO Case 2- Wet H2 FRESH MIXTURE: H2+Air+H2O Non-reactive Comb. Comb.+ Rad 13
  • 14. POLITECNICO DI TORINO Case 2- Wet H2 Even though the fresh mixture (H2+Air+H2O) is opaque, contribution of radiative heat transfer is so small that it can be neglected. 14
  • 15. POLITECNICO DI TORINO Conclusions 1. Radiative LBM can be effectively coupled with combustion model, by providing it the enthalpy rate (radiative source term). 2. For transparent reactive mixture (H2+Air), radiative contribution is null: 3. For opaque fresh mixture (H2+Air+H2O), radiative contribution can be neglected as well: 15
  • 16. POLITECNICO DI TORINO THANKS FOR YOUR ATTENTION! 16