Page 230 - Characterization and Properties of Petroleum Fractions - M.R. Riazi
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            AT029-Manual
  AT029-05
                        AT029-Manual-v7.cls
                                           August 16, 2007
         210 CHARACTERIZATION AND PROPERTIES OF PETROLEUM FRACTIONS
                                       TABLE 5.3—Recommended BIPs for SRK and PR EOS [19].
                                               PR EOS     17:42                 SRK EOS
                         Comp.       N 2        CO 2       H 2 S       N 2        CO 2       H 2 S
                         N 2        0.000      0.000       0.130      0.000      0.000      0.120
                         CO 2       0.000      0.000       0.135      0.000      0.000      0.135
                         H 2 S      0.130      0.135       0.000      0.120      0.120      0.000
                         C 1        0.025      0.105       0.070      0.020      0.120      0.080
                         C 2        0.010      0.130       0.085      0.060      0.150      0.070
                         C 3        0.090      0.125       0.080      0.080      0.150      0.070
                         iC 4       0.095      0.120       0.075      0.080      0.150      0.060
                         nC 4       0.090      0.115       0.075      0.800      0.150      0.060
                         iC 5       0.100      0.115       0.070      0.800      0.150      0.060
                         nC 5       0.110      0.115       0.070      0.800      0.150      0.060
                         C 6        0.110      0.115       0.055      0.800      0.150      0.050
                                    0.110      0.115       0.050      0.800      0.150      0.030
                         C 7+
                         Values recommended for PR EOS by Ref. [6] are as follows: N 2 /CO 2 : −0.013; N 2 /C 1 : 0.038; C 1 /CO 2 : 0.095; N 2 /C 2 :
                         0.08; C 1 /C 2 : 0.021.
         hydrocarbon systems, k ij = 0; however, for the key hydrocar-  of Eq. (5.59) for a ternary gas mixture (N = 3) becomes
         bon compounds in a mixture where they differ in size value  2     2      2
         of k ij is nonzero. For example, for a reservoir fluid that con-  a mix = y a 11 + y a 22 + y a 33 + 2y 1 y 2 a 12 + 2y 1 x 3 a 13 + 2y 2 y 3 a 23
                                                                                 3
                                                                           2
                                                                     1
         tains a considerable amount of methane and C 7+ the BIP for  (5.64)
         C 1 and C 7 fractions cannot be ignored. For nonhydrocarbon–
         hydrocarbon pairs k ij values are nonzero and have a signif-  where a 11 = a 1 , a 22 = a 2 , and a 33 = a 3 . Interaction coefficients
         icant impact on VLE calculations [20, 35]. Values of k ij for  such as a 12 can be found from Eq. (5.61): a 12 =  √ a 1 a 2 (1 − k 12 )
         a particular pair may be determined from matching exper-  where k 12 may be taken from Table 5.3 or estimated from Eq.
         imental data with predicted data on a property such as va-  (5.63). a 13 and a 23 can be calculated in a similar way.
         por pressure. Values of k ij are specific to the particular EOS
         being used. Some researchers have determined k ij for SRK
         or PR equations. Values of BIP for N 2 ,CO 2 , and methane  5.6 NONCUBIC EQUATIONS OF STATE
         with components in reservoir fluids from C 1 to C 6 and three
         subfractions of C 7+ for PR and SRK are tabulated by Whit-  The main reason for wide range application of cubic EOS is
         son [19]. Values that he has recommended for use with SRK  their application to both phases of liquids and vapors, math-
         and PR equations are given in Table 5.3. There are some gen-  ematical simplicity and convenience, as well as possibility
         eral correlations to estimate BIPs for any equation [36, 37].  of calculation of their parameters through critical constants
         The most commonly used correlation for estimating BIPs  and acentric factor. However, these equations are mainly use-
         of hydrocarbon–hydrocarbon (HC–HC) systems is given by  ful for density and phase equilibrium calculations. For other
         Chueh and Prausnitz [37]:                            thermodynamic properties such as heat capacity and en-
                         ⎧                    ⎫
                                              B               thalpy, noncubic equations such as those based on statistical

                         ⎨       2(V ci V c j ) 1/6  ⎬
        (5.63)      k ij = A 1 −          1/3                 associating fluid theory (SAFT) or perturbed hard chain the-
                               (V ci ) 1/3  + V
                         ⎩               c j  ⎭               ory (PHCT) may be used. Some of these equations have been
                                                              particularly developed for special mixtures, polar molecules,
         where V ci and V c j are critical molar volume of components  hard sphere molecules, and near critical regions. Summary
                    3
         i and j in cm /mol. Originally A = 1 and B = 3; however, in  of these equations is given by Poling et al. [8]. In this sec-
         practical cases B is set equal to 6 and A is adjusted to match  tion three important types of noncubic EOS are presented:
         saturation pressure and other variable VLE data [20, 38]. For  (1) virial, (2) Carnahan–Starling, and (3) modified Benedict–
         most reservoir fluids, A is within 0.2–0.25; however, as is seen  Webb–Rubin.                                 --`,```,`,``````,`,````,```,,-`-`,,`,,`,`,,`---
         in Chapter 9 for a Kuwaiti oil value of A was found as 0.18.
         As discussed by Poling et al. [8], Tsonopoulos recommends
         the original Chueh–Prausnitz relation (A = 1 and B = 3) for  5.6.1 Virial Equation of State
         nonpolar compounds. Pedersen et al. [39] proposed another
         relation for calculation of BIPs for HC–HC systems. Their cor-  The most widely used noncubic EOS is the virial equation or
         relation is based on data obtained from North Sea reservoir  its modifications. The original virial equation was proposed
         fluids and it is related to molecular weights of components  in 1901 by Kammerlingh–Onnes and it may be written either
         i and j as k ij = 0.001M i /M j where M i > M j . Another corre-  in the form of polynomial series in inverse volume (pressure
                    ∼
         lation was proposed by Whitson [40] for estimation of BIPs  explicit) or pressure expanded (volume explicit) as follows:
         of methane and C 7+ fraction components based on the data               B   C    D
         presented by Katz and Firoozabadi [36] for use with PR EOS.  (5.65)  Z = 1 +  V  +  V 2  +  V 3  + ···
         His correlation is as: k 1 j = 0.14 SG j – 0.0688, where 1 refers                      2
         to methane and j refers to the C 7+ ( j) fraction, respectively.  Z = 1 +  B  P +  C − B 2  P 2
                                                                                             2
          Equations (5.59)–(5.62) can be applied to either liquid or              RT        R T
         vapor mixtures. However, for the case of vapor mixtures with             D − 3BC + 2B 3     3
         N components, mole fraction y i should be used. Expansion  (5.66)   +       R T 3     P + ···
                                                                                      3













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