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PROF. DR.-ING. HABIL. JADRAN VRABEC ThET
Fluid phase coexistence for the oxidation
of cyclohexane in CO2 expanded liquids:
COSMO-SAC vs. molecular simulation
International Workshop Molecular Modeling an Simulation:
Natural Science meets Engineering
Frankfurt, 12 March, 2013
C.-M. Hsieh1, T. Merker2, S.-T. Lin3, H. Hasse2, J. Vrabec1
1Thermodynamics and Energy Technology, University of Paderborn, Germany 2 Lab. of Engineering Thermodynamics, University of Kaiserslautern, Germany 3 Department of Chemical Engineering, National Taiwan University, Taiwan
PROF. DR.-ING. HABIL. JADRAN VRABEC ThET
Oxidation of cyclohexane to KA-oil (mixture of and )
Cyclohexane oxidation: industrial application
Use of supercritical carbon dioxide expanded media to improve
the rates of conversion and selectivity (enhance the mobility of
reactants and products)
Usually, contact cyclohexane with air low conversion rates (~10%)
for high selectivity (~ 85%)
= O
Air (O2) OH
+ COOH
COOH COOH HOOC
Used for the production of adipic acid / Nylon 6.6
PROF. DR.-ING. HABIL. JADRAN VRABEC ThET
Molecular models for investigated compounds
Cyclohexane
Cyclohexanol
CO2
Cyclohexanone
O2
Experimental measurements
VLE
Henry’s law constant
Molecular simulations
ms2
Thermodynamic models
COSMO-SAC
Peng-Robinson EOS
=O OH
Mixtures investigated:
10 (10) binary, 6 (10) ternary,
2 (5) quaternary, 1 pentenary
[1] T. Merker, et al.: J. Chem. Eng. Data, 56: 2477 (2011)
[2] T. Merker, J. Vrabec, H. Hasse: J. Chem. Thermodyn., 49: 114 (2012)
[3] S. Deublein, et al.: Comput. Phys. Commun., 182: 2350 (2011)
q: point charge, m : point dipole, Q: point quadrupole
+
H
-
O
+
CH
6 LJ-site
7LJ-site + 3 q 7 LJ- site + m
3 LJ-site + Q
2 LJ-site + Q
PROF. DR.-ING. HABIL. JADRAN VRABEC ThET 4
DIPPR correlation Equation of state (EOS) Simulation
Development of molecular pure fluid models
CO2
0.4%
0.4%
0.9%
0.8% p 1.6%
p 3.0%
p 2.7% p 3.0%
[1] T. Merker, J. Vrabec, H. Hasse: J. Chem. Phys., 129: 087101 (2008)
[2] T. Merker, C. Engin, J. Vrabec, H. Hasse: J. Chem. Phys., 132: 234512 (2010)
[3] T. Merker, J. Vrabec, H. Hasse: Fluid Phase Equilib., 315: 77-83 (2012)
[4] T. Merker, J. Vrabec, H. Hasse: Soft Mater., 10: 3-25 (2012)
=O
OH CO2
=O
OH
PROF. DR.-ING. HABIL. JADRAN VRABEC ThET
A A
B B σB, εB
σAB, εAB
Interaction between A and B:
Polar interaction: laws of electrostatics
Lennard-Jones parameters: combination rule
Molecular model of mixtures
AB A B+= / 2σ σ σ
AB A B=ε ε ε
or
Fitting to ONE experimental
datum of p(T,x) or H(T)
ξ = 1 Prediction
Modified
Lorentz-Berthelot
combining rule
σA, εA
PROF. DR.-ING. HABIL. JADRAN VRABEC ThET
COSMO-SAC (Gex model)
The activity coefficient of species i in mixture S is determined from:
[1] S.-T. Lin, S. I. Sandler: Ind. Eng. Chem. Res., 41: 899 (2002) [2] C.-M. Hsieh, et al.: Fluid Phase Equilib. 297, 90
(2010).
combSG,
/
*
/
*
// lnln Si
res
ii
res
SiSi
RT
GG
Combinatorial contribution:
Size and shape effect (Staverman−Guggenheim)
Residual contribution: Molecular interactions
water
hexane
1-octanol
Geometry opt.
-0.025 0.025 (e/Å2) (e/Å2)
COSMO
Quantum mechanics Statistical mechanics
Å2
Å2
s-profile
Å2
)(ln)(
*
/mSmii
res
Si
m
pnRT
Gss
s
Segment Activity Coefficient
PROF. DR.-ING. HABIL. JADRAN VRABEC ThET
Cyclohexane
(C6H12)
Cyclohexanol
(C6H12O)
CO2
Cyclohexanone
(C6H10O) Oxygene
Carbon dioxide
Cyclohexane
Cyclohexanone
Cyclohexanol
O2
-0.025 0.025 (e/Å2) (e/Å2)
s-profiles of investigated compounds
[1] C.-M. Hsieh, S.I. Sandler, S.-T. Lin: Fluid Phase Equilib.: 297, 90-97 (2010).
[2] T. Merker, C.-M. Hsieh, S.-T. Lin, J. Vrabec, H. Hasse: AIChE J. in press, (2013)
i
iimix pxp )()( sss-profiles for mixture:
PROF. DR.-ING. HABIL. JADRAN VRABEC ThET
COSMO-SAC
Gex
Prediction: kij = 0 and lij =0.
Or fitting to ONE experimental datum of p(T,x) or H(T)
VDW mixing rule
a(T,x),
b(x)
PR EOS
1i j ii jj ij
i j
a x x a a k
i i
i
b x b
Van der Waals mixing rule
kij
MHV1 mixing rule
a(T,x), b(x)
PRSV EOS VLE, H(T)
calculation
Peng-Robinson equation of state (PR EOS)
( ) ( )
RT ap
v b v v b b v b
E1ln
0.53
ii
i ii i
a a g bx
bRT b RT RT b
12
i j
i j ij
i j
b bb x x l
Modified Huron-Vidal 1st order
lij
[1] D.Y. Peng, D.B. Robinson: Ind. Eng. Chem Fundam., 15: 59 (1976) [2] M.L. Michelsen: Fluid Phase Equilib., 60: 47 (1990)
[3] R. Stryjek, J.H. Vera: Can. J. Chem. Eng., 64: 323 (1986)
PROF. DR.-ING. HABIL. JADRAN VRABEC ThET
Experiment
Simulation (Prediction)
Simulation (with ij)
+
O2
[1] T. Merker, et al.: J. Chem. Thermodyn., 49: 114 (2012) [2] T. Merker, et al.: Fluid Phase Equilib., 315: 77 (2012)
COSMO-SAC (Prediction)
COSMO-SAC (with lij)
PR EOS (with kij)
Henry‘s law constant CO2
OH
=O
OH
=O
.....
- - -
PROF. DR.-ING. HABIL. JADRAN VRABEC ThET
O2 + CO2
Experiment
Simulation (Prediction)
+
Simulation (with ij)
COSMO-SAC (Prediction)
COSMO-SAC (with lij)
PR EOS (with kij)
+ OH
CO2 + =O
.....
- - -
Selected binary VLE (I)
PROF. DR.-ING. HABIL. JADRAN VRABEC ThET
+ OH =O Experiment
Simulation (Prediction)
+
Simulation (with ij)
COSMO-SAC (Prediction)
COSMO-SAC (with lij)
PR EOS (with kij) .....
- - -
Selected binary VLE (II)
PROF. DR.-ING. HABIL. JADRAN VRABEC ThET
Analysis of all 10 binary systems
Rating from - - (0 points, very bad) to ++ (4 points, very good)
Mixture Molecular Simulation COSMO-SAC Peng-Robinson EOS
Prediction with ij Prediction with lij Prediction with kij
O2 + CO2 ++ ++ - ++ - ++
O2 + - ++ - ++ - - ++
O2 + - ++ - ++ - - ++
O2 + - ++ - ++ - - ++
CO2 + - + - + - - 0
CO2 + + ++ + ++ 0 ++
CO2 + - + 0 + - - 0
+ 0 ++ 0 ++ - ++
+ ++ ++ ++ ++ - - 0
+ ++ ++ 0 + - - - -
Overall 22 38 18 37 5 30
=O
OH
=O
OH
=O OH
=O
OH
[1] T. Merker, C.-M. Hsieh, S.-T. Lin, J. Vrabec, H. Hasse: AIChE J. in press, (2013)
PROF. DR.-ING. HABIL. JADRAN VRABEC ThET
Henry‘s law constant for three ternary subsystems
313 K Experiment
Simulation (with ij)
+
COSMO-SAC (with lij)
O2
CO2
=O
OH
[1] T. Merker, C.-M. Hsieh, S.-T. Lin, J. Vrabec, H. Hasse: AIChE J. in press, (2013)
PROF. DR.-ING. HABIL. JADRAN VRABEC ThET
Experiment
Simulation (with ij)
( and are in equal-molar concentration)
313 K
COSMO-SAC (with lij)
Henry‘s law constant for two quaternary subsystems
=O OH
O2
CO2 =O
OH
[1] T. Merker, C.-M. Hsieh, S.-T. Lin, J. Vrabec, H. Hasse: AIChE J. in press, (2013)
PROF. DR.-ING. HABIL. JADRAN VRABEC ThET
xi / mol mol
-1
0,0 0,2 0,4 0,6 0,8 1,0
p /
MP
a
0
2
4
6
8
Pure O2
CO2 (with constant molar fraction
0.04 of O2 in the mixture)
Pure CO2
CO2 (with constant molar fraction
0.02 of O2 in the mixture)
Experiment
Simulation (with ij)
+
COSMO-SAC (with lij)
VLE of quaternary subsystems and pentenary system
The composition (without O2 and CO2) of the fluid is constant: : 0.325 mol/mol, : 0.35 mol/mol, : 0.325 mol/mol =O OH
313 K
[1] T. Merker, C.-M. Hsieh, S.-T. Lin, J. Vrabec, H. Hasse: AIChE J. in press, (2013)
PROF. DR.-ING. HABIL. JADRAN VRABEC ThET
Conclusions
• Models can be used in industrial process design
• Good predictions from molecular simulation and
COSMO-SAC
• Capable to predict multi-component VLE
• Excellent accuracy achieved with binary parameters
• Molecular models can be used for atomistic simulations of
e.g. fluid behavior in nanostructured catalysts
PROF. DR.-ING. HABIL. JADRAN VRABEC ThET
Thank You for Your Attention!
PROF. DR.-ING. HABIL. JADRAN VRABEC ThET
Mixture (i + j) ij lij kij
O2 + CO2 1 -0.0526 0.132
O2 + C6H12 0.90 -0.0547 0.22
O2 + C6H10O 0.93 -0.0342 0.355
O2 + C6H12O 0.91 -0.0266 0.345
CO2 + C6H12 0.95 -0.0523 0.217
CO2 + C6H10O 0.985 -0.0082 0.049
CO2 + C6H12O 0.918 -0.0418 0.225
C6H12+ C6H10O 0.982 -0.0228 0.065
C6H12+ C6H12O 0.982 -0.0035 0.07
C6H10O+C6H12O 1 -0.0027 0
Values of binary interaction parameters in this work
PROF. DR.-ING. HABIL. JADRAN VRABEC ThET
PROF. DR.-ING. HABIL. JADRAN VRABEC ThET
CO2 +
Experiment
Simulation (Prediction)
+
Simulation (with ij)
COSMO-SAC (Prediction)
COSMO-SAC (with lij)
PR EOS (with kij)
CO2 + OH
+ =O
PROF. DR.-ING. HABIL. JADRAN VRABEC ThET
Contribution of molecular simulation
• powerful predictive capabilities (thermodynamic data)
• works under any physical conditions
• low cost
Why is molecular simulation not a mainstream solution for
thermodynamic data retrieval?
• suitable molecular models
• today’s MS software: only a few independent properties
• new properties require implementation
• development is impossible for an inexperienced user
PROF. DR.-ING. HABIL. JADRAN VRABEC ThET
Peng-Robinson Equation of State (PR EOS)
( ) ( )
RT ap
v b v v b b v b
22 2
,
, ,
0.45724 1 1c i
i i
c i c i
R T Ta
p T
,
,
0.0778 c i
i
c i
R Tb
p
Peng-Robinson-Stryjek-Vera EOS
E1ln
0.53
ii
i ii i
a a g bx
bRT b RT RT b
12
i j
i j ij
i j
b bb x x l
2
3
1,
, ,
0.378893 1.4897153 0.17131848
0.0196654 1 0.7
i i i
i i
c i c i
T T
T T
PRSV EOS + MHV1 + COSMOSAC
Original Peng-Robinson
1i j ii jj ij
i j
a x x a a k
i i
i
b x b
21 0.37464 1.54226 0.26992i i i
PR EOS + VDW
Modified Huron-Vidal 1st-order Mixing Rule
Prediction: kij = 0 and lij =0.
Or fitting to ONE experimental datum of p(T,x) or H(T)
Van der Waals Mixing Rule
[1] D. Y. Peng, D.B. Robinson: Ind. Eng. Chem. Fundam., 15: 59-64 (1976)
[2] R. Stryjek, J.H. Vera: Can. J. Chem. Eng., 64: 323-333 (1986)
[3] M. L. Michelsen: Fluid Phase Equilib., 60: 213-219 (1990)