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This article was downloaded by: [Nezbeda, Ivo]On: 28 January 2011Access details: Access Details: [subscription number 932744087]Publisher Taylor & FrancisInforma Ltd Registered in England and Wales Registered Number: 1072954 Registered office: Mortimer House, 37-41 Mortimer Street, London W1T 3JH, UK
Molecular PhysicsPublication details, including instructions for authors and subscription information:http://www.informaworld.com/smpp/title~content=t713395160
Vapour/liquid coexistence in long-range Yukawa fluids determined bymeans of an augmented van der Waals approachRoman Melnyka; Ivo Nezbedabc; Andrij Trokhymchukad
a Institute for Condensed Matter Physics, National Academy of Sciences of Ukraine, Lviv, 79011,Ukraine b Faculty of Science, J.E. Purkinje University, 400 96 Ústí nad Labem, Czech Republic c E. HalaLab. of Thermodynamics, Institute of Chemical Process Fundamentals, Academy of Sciences, 165 02Prague 6, Czech Republic d Department of Chemistry and Biochemistry, Brigham Young University,Provo, UT 84602, USA
Online publication date: 24 January 2011
To cite this Article Melnyk, Roman , Nezbeda, Ivo and Trokhymchuk, Andrij(2011) 'Vapour/liquid coexistence in long-range Yukawa fluids determined by means of an augmented van der Waals approach', Molecular Physics, 109: 1, 113 —121To link to this Article: DOI: 10.1080/00268976.2010.542034URL: http://dx.doi.org/10.1080/00268976.2010.542034
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Molecular PhysicsVol. 109, No. 1, 10 January 2011, 113–121
INVITED ARTICLE
Vapour/liquid coexistence in long-range Yukawa fluids determined
by means of an augmented van der Waals approach
Roman Melnyka, Ivo Nezbedabc and Andrij Trokhymchukad*
aInstitute for Condensed Matter Physics, National Academy of Sciences of Ukraine, Lviv,79011, Ukraine; bFaculty of Science, J.E. Purkinje University, 400 96 Ustı nad Labem,
Czech Republic; cE. Hala Lab. of Thermodynamics, Institute of Chemical Process Fundamentals,Academy of Sciences, 165 02 Prague 6, Czech Republic; dDepartment of Chemistry and Biochemistry,
Brigham Young University, Provo, UT 84602, USA
(Received 8 August 2010; final version received 15 November 2010)
The vapour–liquid phase diagram of long-range Yukawa fluids with the decay parameter z�� 1 is calculated bymeans of an augmented van der Waals theory based on the reference system that includes both the repulsive andshort-range attractive interaction. Comparison with Monte Carlo simulation data, as well as with the traditionalvan der Waals approach based on a purely repulsive hard-sphere reference system and other semi-analyticaltheoretical approaches, is made.
Keywords: Yukawa fluid; perturbation theory; augmented van der Waals approach; vapour–liquid coexistence
1. Introduction
Because of its versatility the attractive hard-sphere
Yukawa (AHSY) potential has become one of the most
popular fluid models studied in the last decade
intensively both by molecular simulations [1–3] and
theory [4–9]. In their recent paper [10] Caillol et al.
have reported an extensive computer simulation
study of the vapour–liquid (VL) coexistence in the
long-range attractive Yukawa fluids. In the same
study these authors have also shown that two
rather sophisticated theoretical approaches, namely,
the self-consistent Ornstein–Zernike equation
(SCOZA) and the hierarchical reference theory
(HRT) perform extremely well in reproducing these
computer simulation data while an optimized mean
field theory (OMF), while yielding the exact result in
the limit of an infinite range of the potential, still
deteriorates when the interaction is long ranged but yet
finite. Very recently the same systems were studied [11]
also by means of the numerical solution of the
Ornstein–Zernike integral equation using Sarkisov’s
closure [12].As an alternative to the above numerically demand-
ing methods we have recently proposed a transparent
perturbation theory approach [13,14] built upon the
Yukawa (Y) models as a sort of reference and which
makes use of the availability of both approximate
analytic [4] and accurate empirical [7–9] results for the
Y fluid. The use of the Y reference considerably
improves accuracy of the perturbation methods: the
more features are captured by the reference, the less
important become perturbation correction terms and,
consequently, all considerations are confined to a
first-order expansion or further even to an augmented
van der Waals (the simplified first-order expansion)
theory only [15]. This approach can be viewed as a
counterpart of the common augmented van der Waals
(vdW) theory based on the purely repulsive hard-
sphere (HS) reference; we will refer to these two
theories as the vdW/Y and vdW/HS approaches,
respectively. The vdW/Y approach has been applied
already to the medium range (Lennard-Jones-like)
attractive hard-core Yukawa potential [14] and to the
Sutherland potential [15] made up of a hard-core
repulsion and a power law attractive tail, while
potentially it is applicable to any simple fluid.
The determining feature for such a claim is the
flexibility of the Y model to mimic short-range
interactions of various kinds that usually are achieved
by employing several Yukawa terms (e.g. see equations
that have been developed by Guerin [16] for the sum of
two Yukawa (2Y) potentials and by Tang [17] for the
multi-Yukawa potentials). Quite recently [18] we
reported 2Y representation of the short-range inter-
action in the EXP6 fluids and examined it using
molecular simulations.
*Corresponding author. Email: [email protected]
ISSN 0026–8976 print/ISSN 1362–3028 online
� 2011 Taylor & Francis
DOI: 10.1080/00268976.2010.542034
http://www.informaworld.com
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The aim of the present paper is twofold. First, we
will show that the simple vdW-like theory may perform
as well as the advanced theoretical approaches like
SCOZA and HRT. Secondly, we will emphasize that a
natural way to improve the traditional vdW theory lies
in an improvement of the reference system contribu-
tion rather than in a modernizing the perturbation
contribution. We proceed presenting first the model
and theoretical basis of the vdW/Y approach in the
following section. The original results obtained for
selected model long-range Yukawa fluids are then
shown and discussed in Section 3.
2. Model and theory
The attractive hard sphere Yukawa (AHSY) potential
is defined by
uðrÞ ¼1, if r5 �,
��ð�=rÞ exp �zðr� �Þ� �
, if r � �,
�ð1Þ
where r is the distance between two particles, � is the
hard-core diameter of the particles and � is the potentialdepth, both set to unity henceforth. The exponent z
determines the range of the interaction and in this
study will consider it within the range 0.1� z�� 1.
Specifically, the long-range AHSY potential functions
for the case of z�¼ 1, 0.5 and 0.1 are shown in
Figure 1. We have chosen these values of parameter z
for the possibility to compare the results with extensive
Monte Carlo (MC) computer simulation data for the
VL coexistence reported by Caillol et al. [10].The augmented vdW theory employed in this study
results as a simplified byproduct when deriving a
general perturbation theory based on the attractive
Yukawa (Y) reference system [14]. Specificity of such a
perturbation theory is that it is built upon the reference
fluid that, besides the HS repulsion, includes also some
portion of the attraction within the spirit of a unified
view of fluids [19]. To be more specific, the basic idea is
that in the (dense) fluid phase the pair interaction u can
be separated into two parts,
u ¼ u0 þ Du, ð2Þ
where u0, referred to as a reference, is responsible for
the local ordering in the system while Du plays the role
of a perturbation that has only little effect on this local
structure. The important point is that the reference
part need not be only repulsive, as it is usually thought,
but may (should) incorporate also a piece of the
attractive interactions at short interparticle separa-
tions. A route toward the thermodynamic properties of
the original u-fluid at hand goes then via the expansion
of the Helmholtz free energy,
�A ¼ �A0 � 2p��NZ
g0ðrÞDuðrÞr2 drþ . . . , ð3Þ
where � ¼ 1=kBT, kB is Boltzmann’s constant, N is the
number of molecules, �¼N/V is the number density,
and g0 is the radial distribution function of the
–1.0
–0.8
–0.6
–0.4
–0.2
0.0
0.2
0.4
Pai
r in
tera
ctio
n, u
(r)/
Distance, r/s
(a)
zs=0.1
zs=0.5
zs=1
0 1 2 3 4 5 6 7 8 9 10 1 2 3 4
–1.0
–0.8
–0.6
–0.4
–0.2
0.0
0.2
0.4
Distance, r/s
(b)
Perturbation Δu
AHSY fluid (zs=1)
Reference Y–fluid (z0s=3)
Pai
r in
tera
ctio
n, u
(r)/
Figure 1. Part (a): the long-range AHSY potential at different values of the range parameter, z, as shown in the figure. Part (b):the decomposition of the long-range Yukawa potential with the range parameter z�¼ 1 into the reference and perturbationcontributions.
114 R. Melnyk et al.
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reference system. The degree of similarity of the
short-range structure of the parent u-fluid and that of
the reference u0-fluid determines then the magnitude
of the difference A�A0 and governs the convergence of
expansion (3).For the approach based on expansion (3) to be of a
practical use it is necessary that it converges fast and
can be considered only with the first-order vdW-like
correction,
aðT, �Þ ¼ �2pZ
g0ðrÞDuðrÞr2 dr: ð4Þ
Higher order corrections are both only approximate
and time consuming, and defy any analytic treatment.
At this point it also worth noting that the simple
vdW-like term correction in the expansion for A is also
a prerequisite for obtaining other thermodynamic
functions in a tractable form. For instance, by deriving
the equation for pressure, P, we have to deal with the
density derivative @a/@�. To obtain the equation of
state (EOS) in a closed form, an approximation
aðT, �Þ ! a0 ¼ �2pZ
DuðrÞr2 dr, ð5Þ
is then very often used. Following the traditional
approach, i.e. to operate with the HS reference fluid,
u0ðrÞ � uHSðrÞ ¼1, if r5 �,
0, if r � �,
�ð6Þ
it is easy to show that such an approximation is too
crude. This is discernible from Figure 2: the vdW
correction term a being evaluated via definition,Equation (4), with the HS radial distribution functionfor g0, strongly depends on density and significantlydiffers from the constant a0 given by approximation,Equation (5). Consequently, the density derivative@a/@� cannot be neglected in the case of the HSreference fluid. On the other hand, following oursuggestion [13,14] and using as the reference the short-range (z0�¼ 3) attractive Y fluid,
u0ðrÞ � uYðrÞ ¼1, if r5 �,
��ð�=rÞ exp �z0ðr� �Þ� �
, if r � �,
�
ð7Þ
we see in Figure 2 that a(T, �) practically does notchange with a density having a magnitude nearly thatof a0. It means that using the Y reference system theassumption (5) becomes fully justified and leads thento the augmented vdW theory that reads as
�A
N¼�A0
N� ��a0,
�P
�¼�P0
�� ��a0,
�U
N¼�U0
N� ��a0: ð8Þ
To understand the phenomenon of the Y reference wefirst note that for both reference systems, HS and Y,the radial distribution functions g0� gHS or g0� gY arevery similar and both depend on density. But it is theperturbation term, Du, that differs significantly withdependence on the choice of the reference system.Indeed, when the HS fluid is employed as the reference
0
2
4
6
8(a)
T*=1.5
T*=2
T*=1
HS reference system
vdW
coe
ffici
ent,
ba
Density, rs30.0 0.2 0.4 0.6 0.8 1.0 0.0 0.2 0.4 0.6 0.8 1.0
0
2
4
6
8(b)
T*=2
T*=1.5
T*=1
Y reference system
vdW
coe
ffici
ent,
ba
Density, rs3
Figure 2. An example of the vdW correction term �a(T, �) evaluated for the Lennard-Jones-like hard-core Yukawa fluidwith z�¼ 1.8. Part (a) shows the results for the case of a traditional HS reference system while part (b) shows the results in thecase of a proposed Y reference system characterized by z0�¼ 3. The thick solid lines in both parts correspond to a0 given byEquation (5); the thin lines represent a(T, �) from Equation (4) using for the radial distribution function g0 of the HS and Yreference systems the PY and MSA results, respectively; the symbols in part (b) have the same meaning but obtained by using forthe radial distribution function g0 the ‘exact’ computer simulation data.
Molecular Physics 115
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system then the perturbation term Du(r) incorporatesthe entire interaction energy u(r) which is the strongest
at the hard-core contact r¼ �. However, hard-core
contact distance is the most density sensitive region in
the HS radial distribution function gHS. Conversely, as
we can see from Figure 1b, inclusion into the reference
part of the short-range attraction of the same energy
minimum � as in the parent fluid, makes the pertur-
bation term Du(r) very weak in the most important
region of small separations between the molecules.
In particular, the perturbation term is exactly zero at
the hard-core contact, i.e. Du(r¼ �)¼ 0. It means that
in the case of the Y reference system the contribution
to a(T, �) from the range of small r in g0� gY is
practically killed by the value of Du, and an approx-
imation g0� 1 within the framework of the augmented
vdW/Y theory becomes then well grounded.The Y reference system defined by Equation (7) is
characterized by a so far unspecified range parameter z0.
One obvious restriction imposed on z0 is that the rangeof the attraction for the reference fluid pair potential
u0(r) must be shorter than that of u(r). Moreover, the
perturbation theory may be intuitively expected to
perform the better the closer the reference fluid is to theparent fluid. Before attempting to be more specific one
should always realize reasons why the HS reference has
been so successful. Not only because availability of
results for both the structure and thermodynamics but
primarily because of its flexibility. The lack of thecritical point in the HS fluid makes it possible to change
the HS diameter (and hence the packing density) over a
large range of values without imposing serious restric-
tions on the properties of the considered system and
thus tune the results to the wished outcome. Recentcomputer simulation studies [1–3,6] of the short-rangeY
fluid showed that: (i) the VL critical temperature
decreases in this system and is approaching the triple
point temperature when the range of attraction
2.0
2.1
2.2
2.3
2.4
2.5 zs=1
vdW/HS
vdW/Y
Density, rs3
Tem
pera
ture
, Tk B
/
(a)
0.0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.0 0.1 0.2 0.3 0.4 0.5 0.6 0.7
6.0
6.5
7.0zs=0.5
Density, rs3
Tem
pera
ture
, Tk B
/
(b)
0.0 0.1 0.2 0.3 0.4 0.5 0.6 0.7
110
115
120
125 zs=0.1
Density, rs3
Tem
pera
ture
, Tk B
/
(c)
Figure 3. Vapour–liquid coexistence curve for the long-range AHSY fluids with different values of the range parameter(a) z�¼ 1, (b) 0.5 and (c) 0.1 obtained by means of augmented vdW theory with HS (dashed line) and with Y (solid line) referencesystems. The symbols stand for MC computer simulation data (filled spheres) and the hierarchical reference theory (triangle)results, both due to Caillol et al. [10].
116 R. Melnyk et al.
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Table 1. Coexistence densities, internal energy and chemical potential at vapour–liquidcoexistence in the long-range AHSY fluid with z�¼ 1 obtained by means of augmented vdWtheory with two different reference systems and those from MC computer simulations due toCaillol et al. [10].
kBT/� �v�3 �l�
3 (U/NkBT )v (U/NkBT )l �/kBT
2.460 MC 0.183(2) 0.395(10) �1.025(50) �2.19(5) �2.77(1)vdW/Y 0.178 0.391 �0.951 �2.13 �2.73
2.392 MC 0.135(2) 0.439(5) �0.78(2) �2.52(2) �2.87(1)vdW/Y 0.139 0.448 �0.76 �2.52 �2.82
2.338 MC 0.112(2) 0.474(4) �0.67(1) �2.79(2) �2.95(1)vdW/Y 0.117 0.484 �0.652 �2.80 �2.90
2.283 MC 0.096(2) 0.508(5) �0.59(2) �3.07(3) �3.04(2)vdW/Y 0.099 0.515 �0.565 �3.068 �2.98
2.229 MC 0.085(3) 0.543(6) �0.54(2) �3.37(3) �3.11(2)vdW/Y 0.084 0.544 �0.492 �3.332 �3.071vdW/HS 0.177 0.330 �1.000 �1.860 �2.835
2.175 MC 0.070(2) 0.564(4) �0.447(15) �3.60(3) �3.21(1)vdW/Y 0.071 0.572 �0.428 �3.598 �3.169vdW/HS 0.139 0.383 �0.804 �2.213 �2.908
2.120 MC 0.062(2) 0.594(6) �0.420(15) �3.89(3) �3.30(2)vdW/Y 0.060 0.597 �0.373 �3.868 �3.274vdW/HS 0.114 0.423 �0.677 �2.507 �2.986
2.066 MC 0.050(2) 0.612(3) �0.344(5) �4.120(15) �3.43(1)vdW/Y 0.051 0.622 �0.324 �4.146 �3.387vdW/HS 0.095 0.457 �0.579 �2.782 �3.071
2.012 MC 0.042(2) 0.634(4) �0.30(1) �4.440(25) �3.55(1)vdW/Y 0.043 0.645 �0.280 �4.432 �3.510vdW/HS 0.080 0.488 �0.498 �3.050 �3.163
Table 2. The same as in Table 1 but with z�¼ 0.5.
kBT/� �v�3 �l�
3 (U/NkBT )v (U/NkBT )l �/kBT
6.892 MC 0.169(8) 0.355(8) �0.93(3) �1.99(2) �2.82(1)vdW/Y 0.171 0.360 �0.945 �2.01 �2.81
6.859 MC 0.160(8) 0.370(8) �0.89(4) �2.05(4) �2.84(1)vdW/Y 0.163 0.371 �0.903 �2.08 �2.82
6.727 MC 0.130(6) 0.400(6) �0.75(2) �2.31(4) �2.90(1)vdW/Y 0.137 0.408 �0.775 �2.34 �2.88vdW/HS 0.192 0.312 �1.077 �1.75 �2.82
6.595 MC 0.118(4) 0.439(4) �0.689(15) �2.58(2) �2.96(1)vdW/Y 0.118 0.440 �0.678 �2.570 �2.94vdW/HS 0.153 0.362 �0.876 �2.07 �2.88
6.463 MC 0.103(4) 0.467(4) �0.62(1) �2.74(2) �3.02(1)vdW/Y 0.102 0.467 �0.598 �2.79 �3.01vdW/HS 0.129 0.399 �0.752 �2.33 �2.94
6.331 MC 0.085(4) 0.485(4) �0.52(1) �2.99(1) �3.11(1)vdW/Y 0.089 0.493 �0.531 �3.01 �3.08vdW/HS 0.110 0.430 �0.657 �2.56 �3.00
6.199 MC 0.076(2) 0.512(2) �0.468(5) �3.21(1) �3.17(2)vdW/Y 0.077 0.517 �0.472 �3.22 �3.16vdW/HS 0.095 0.457 �0.579 �2.78 �3.07
6.067 MC 0.068(2) 0.539(3) �0.43(1) �3.46(2) �3.27(3)vdW/Y 0.067 0.539 �0.420 �3.44 �3.24vdW/HS 0.083 0.482 �0.513 �3.00 �3.14
5.935 MC 0.058(2) 0.556(3) �0.375(10) �3.64(2) �3.34(1)vdW/Y 0.058 0.561 �0.374 �3.66 �3.33vdW/HS 0.072 0.506 �0.456 �3.21 �3.22
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decreases, and (ii) the short-range Y fluid with z0�¼ 3has its critical temperature nearly the same asthe triple point temperature of the Lennard-Jonesfluid. If one chooses, for instance, z0 larger than butclose to 3, then for the whole family of the medium-and long-range fluids such a defined Y referencesystem will be always closer to the parent fluid thanany HS reference, and yet it will enjoy the sameflexibility.
As regards available equations for the properties ofthe short-range Y reference fluids, they are comparablewith those for the HS reference fluid. An analyticaltreatment of the Y model is available within the meanspherical approximation (MSA) [4] that can be viewedas a counterpart of the common Percus–Yevick theoryin the case of the HS reference system. There are alsoanalytic results developed within the high temperatureexpansions (HTE) [7–9] that make it possibleto evaluate the thermodynamic properties for the Yreference fluid. By comparison with computer simula-tion data for a set of the range parameter valuesranging from z0�¼ 3 up to 6, which are typical for theY reference system, it has been already shown [9] thatthe HTE equations work well over wide density andtemperature windows.
3. Results
The main result of this study concerns the vapour–liquid (VL) phase diagram of the long-range attractivehard-sphere Yukawa (AHSY) fluid that follows fromthe augmented vdW approach built on the Y referencefluid and is given by Figure 3. Independently of thereference system, the VL coexistence within the vdWapproach is obtained by finding the intersection of theP�� surfaces for both the liquid and vapour branchesalong the same isotherm. For this purpose the chemicalpotential � was obtained from
�� ¼�A0
Nþ�P0
�� 2��a: ð9Þ
Figure 3 shows the VL coexistence curves for allthree cases of the long-range AHSY fluid considered inthis study, namely, z�¼ 1, 0.5 and 0.1. For each case theresults of the augmented vdW theory based on bothreference systems, HS and Y, are shown and comparedagainst MC computer simulation data due to Caillolet al. [10]. All the vdW/Y calculations were performedusing for the Y reference fluid the range parametervalue, z0�¼ 3. The equations to evaluate the thermo-dynamic properties A0, P0 and U0 of the Y reference
Table 3. The same as in Table 1 but with z�¼ 0.1.
kBT/� �v�3 �l�
3 (U/NkBT )v (U/NkBT )l �/kBT
121.57 MC 0.17(1) 0.340(15) �0.96(2) �1.96(5) �2.86(2)vdW/Y 0.159 0.356 �0.904 �2.03 �2.86vdW/HS 0.162 0.351 �0.920 �1.99 �2.86
120.46 MC 0.145(10) 0.360(15) �0.82(1) �2.05(1) �2.89(1)vdW/Y 0.146 0.374 �0.838 �2.15 �2.89vdW/HS 0.148 0.370 �0.851 �2.12 �2.89
119.36 MC 0.136(5) 0.380(5) �0.79(2) �2.21(2) �2.92(2)vdW/Y 0.135 0.391 �0.781 �2.27 �2.92vdW/HS 0.137 0.387 �0.793 �2.24 �2.91
118.25 MC 0.126(2) 0.393(3) �0.73(1) �2.32(2) �2.95(1)vdW/Y 0.125 0.406 �0.732 �2.38 �2.95vdW/HS 0.127 0.402 �0.742 �2.35 �2.94
117.15 MC 0.121(4) 0.416(4) �0.716(15) �2.46(2) �2.97(1)vdW/Y 0.117 0.420 �0.688 �2.48 �2.98vdW/HS 0.118 0.416 �0.697 �2.46 �2.97
116.05 MC 0.109(2) 0.425(3) �0.65(1) �2.54(2) �3.000(15)vdW/Y 0.109 0.434 �0.648 �2.59 �3.01vdW/HS 0.110 0.430 �0.656 �2.56 �3.00
114.94 MC 0.102(1) 0.439(2) �0.641(5) �2.64(1) �3.04(1)vdW/Y 0.102 0.446 �0.612 �2.69 �3.04vdW/HS 0.103 0.443 �0.619 �2.66 �3.03
112.73 MC 0.091(1) 0.466(2) �0.555(5) �2.86(1) �3.10(1)vdW/Y 0.089 0.470 �0.546 �2.89 �3.10vdW/HS 0.090 0.467 �0.555 �2.88 �3.10
110.52 MC 0.077(3) 0.483(5) �0.48(1) �3.028(25) �3.17(1)vdW/Y 0.078 0.493 �0.490 �3.09 �3.17vdW/HS 0.079 0.489 �0.498 �3.08 �3.17
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fluid are taken from [15]. One can see that over the rangeof z values considered, the vdW/Y theory reproducesthe MC data for the VL coexistence extremely well.Conversely, the vdW/HS theory can be applicable onlyin the case of very small values of z�� 0.1. This isexpected, since increasing the range of attraction(decreasing the values of z) results in an increase ofthe critical point temperature (e.g. T �c for z�¼ 0.1 isapproximately of two orders larger than that for z�¼ 1)and role of the attraction becomes rather small. Forz�4 0.1 the critical temperature in the AHSY fluid isgetting lower and the vdW/HS theory rapidly deterio-rates: the coexistence curve of vdW/HS is found to benarrower and the critical point significantly lower thanthat of vdW/Y theory. The study due to Hendersonet al. [5] has shown that to describe the VL coexistencein the AHSY fluid with z�¼ 1.8 by using the HSreference one needs to take into account the secondcorrection term in expansion (3).
The vapour and liquid coexistence density, �vand �l, that result from the augmented vdW/Y theoryand those due to Caillol et al. [10] from MC computer
simulations are for convenience collected in Tables 1to 3 for z�¼ 1, 0.5 and 0.1, respectively. The sametables also consist of the theoretical results andcomputer simulation data for the coexistence internalenergies and excess chemical potential along thecoexistence curve. For the sake of clarity, the compar-ison of the coexistence internal energies and excesschemical potential that result from vdW/Y, vdW/HStheories and from MC computer simulations areshown in Figures 4 and 5. The tendency is quite thesame as we already have seen for the VL phasediagrams presented in Figure 3.
As can be noted from Figure 3, there are no MCcomputer simulation data for the critical point param-eters since those were not computed by Caillol et al.[10]. Instead, these authors reported for the criticalpoint parameters the results of the SCOZA and HRTtheories. The comparison between different theoreticalpredictions for the critical point parameters can bemade from Table 4. It can be seen that the agree-ment between the vdW/Y and the two theories isquite good.
2.0
2.1
2.2
2.3
2.4
2.5
2.6
zs=1
vdW/HS
vdW/Y
Internal energy, U/NkBT
Tem
pera
ture
, Tk B
/
(a)
6.0
6.4
6.8
zs=0.5
Internal energy, U/NkBT
Tem
pera
ture
, Tk B
/
(b)
–4 –3 –2 –1 0 –4 –3 –2 –1 0
–4 –3 –2 –1 0
110
115
120
125zs=0.1
Internal energy, U/NkBT
Tem
pera
ture
, Tk B
/
(c)
Figure 4. Internal energy U/NkBT along the vapour–liquid coexistence curve for the long-range AHSY fluids with (a) z�¼ 1,(b) 0.5 and (c) 0.1. The symbols are MC computer simulation data of Caillol et al. [10].
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4. Conclusion
We have shown that recently proposed augmentedvdW/Y theory, built upon the short-range attractiveYukawa (Y) reference system, being applied to thelong-range AHSY fluid agrees well with computersimulation data due to Caillol et al. [10] and iscomparable with advanced theoretical approaches,namely, the SCOZA and HRT. At first glance thisresult may look rather trivial. However, being com-pared with the traditional augmented vdW theory thatuses the HS reference system (vdW/HS theory)it highlights the importance of the inclusion of theshort-range correlations and, consequently, the short-range attraction between molecules into the referencesystem. In particular, we note that the presence of theshort-range attraction in a reference system is a naturalway to provide the systematic and self-consistentimprovement of the traditional vdW theory. Indeed,the inclusion of the short-range attraction intoa reference fluid modifies both the contribution ofthe perturbation term and the contribution of thereference system. This novel reference system becomes
2.0
2.1
2.2
2.3
2.4
2.5
2.6
zσ=1
vdW/HS
vdW/Y
Tem
pera
ture
, Tk B
/ε
Chemical potential, m/kBT
(a)
6.0
6.2
6.4
6.6
6.8
7.0
–3.6 –3.4 –3.2 –3.0 –2.8 –2.6 –3.4 –3.2 –3.0 –2.8
zσ=0.5
Tem
pera
ture
, Tk B
/ε
Chemical potential, m/kBT
(b)
110
115
120
125
–3.4 –3.2 –3.0 –2.8
zσ=0.1
Tem
pera
ture
, Tk B
/ε
Chemical potential, m/kBT
(c)
Figure 5. Chemical potential �/kBT along the vapour–liquid coexistence curve for the long-range AHSY fluids with (a) z�¼ 1,(b) 0.5 and (c) 0.1. The meaning of symbols are the same as in Figure 4.
Table 4. Critical point temperature T�c ¼ kBTc=� and den-sity ��c ¼ �c�
3 of the long-range AHSY fluid with differentvalues of the range parameter z�¼ 1, 0.5 and 0.1 as resultingfrom the SCOSA and HRT both due to Caillol et al. [10] andfrom augmented vdW theory with two different referencesystems.
z� T�c ��c
0.1 SCOZA 124.82 0.2495HRT 124.77 0.250vdW/Y 124.76 0.248vdW/HS 124.52 0.248
0.5 SCOZA 7.068 0.259HRT 7.076 0.260vdW/Y 7.047 0.258vdW/HS 6.795 0.247
1 SCOZA 2.518 0.279HRT 2.514 0.279vdW/Y 2.521 0.275vdW/HS 2.263 0.246
120 R. Melnyk et al.
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quantitatively and, what is even more important,qualitatively very different from the HS referencesystem exhibiting important new features, like depen-dence on the temperature, etc. Importantly, despitesuch progress in the formulation of the referencesystem, the contribution of the Y reference system toboth the thermodynamics as well as the structure is stillavailable in the form of closed analytical equations(within the MSA or HTE approximations).
To evaluate the perturbation interaction contribu-tion a(T, �), we are using a simplified expression (5) thatusually is obtained from an exact expression (4) byassuming that the radial distribution function of thereference system is uniform, i.e. g0(r)¼ 1. We haveshown (see Figure 2) that the assumption aðT, �Þ ! a0,being a rather crude approximation in the case of theHS reference system, is quite accurate in the case of theY reference system. The small discrepancies that stillcould be observed between a(T, �) and a0 are negligiblein describing the VL coexistence, being comparable tothe accuracy of the description of the radial distributionfunction gY(r) of the Y reference system (the MSAtheory) and to the accuracy of the description ofthe thermodynamics of the reference system itself(the MSA or HTE approximations). Summarizing, theproposed Y reference system may play a role similar tothat played in the liquid state theories by the HS system.Although in the present study this has been illustratedusing the long-range AHSY fluid, it can be implementedwith any other kind of long-range interaction potential.
Acknowledgements
This work was supported by the Grant Agency of theAcademy of Sciences of the Czech Republic (Grant No.
IAA400720710) and Czech–Ukrainian Bilateral CooperativeProgram.
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