Abstract. This work presents a molecular dynamics simulation (MDS) of CaSiO3 glass
using Born–Mayer–Huggins potentials. The structural organization and structural phase
transition under compression as well as network structure of CaSiO3 are clarified through
analysis and visualization of molecular dynamics simulation data. The short-range order
structure, intermediate-range order structure are investigated in detail through analysis the
pair of radial distribution function, the coordination number distribution in TOn polyedra
and OTm linkages (n = 4 ÷ 11; m = 2 ÷ 5; T = Si, Ca). Topology structure of TOn and OTm
is also clarified by investigating bond angle and bond length distribution in TOn polyhedra
and OTm linkages.
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JOURNAL OF SCIENCE OF HNUE DOI: 10.18173/2354-1059.2016-0046
Mathematical and Physical Sci., 2016, Vol. 61, No. 7, pp. 165-175
This paper is available online at
PRESSURE-DEPENDENT STRUCTURAL HETEROGENEITY
IN CALCIUM SILICATE GLASS
Mai Thi Lan1, Nguyen Thi Thanh Ha1, Tran Thuy Duong1, Nguyen Thi Thao2
and Nguyen Van Hong1
1School of Engineering Physics, Hanoi University of Science and Technology
2Hanoi University of Education
Abstract. This work presents a molecular dynamics simulation (MDS) of CaSiO3 glass
using Born–Mayer–Huggins potentials. The structural organization and structural phase
transition under compression as well as network structure of CaSiO3 are clarified through
analysis and visualization of molecular dynamics simulation data. The short-range order
structure, intermediate-range order structure are investigated in detail through analysis the
pair of radial distribution function, the coordination number distribution in TOn polyedra
and OTm linkages (n = 4÷ 11; m = 2÷ 5; T = Si, Ca). Topology structure of TOn and OTm
is also clarified by investigating bond angle and bond length distribution in TOn polyhedra
and OTm linkages.
Keywords: Structure, phase transition, polymerization, molecular dynamics simulation,
CaSiO3.
1. Introduction
Calcium silicate (CaSiO3) is one of the members of Pyroxene, which is the main component
of Basalt. The CaSiO3 is one of main components of the Earth’s lower mantle. It is the
important component in the glass and ceramic materials [1-4]. Knowledge of structure of CaSiO3
system in both glass and liquid states under high pressure is necessary for understanding about
volcanic activity, the physicochemical and thermal change of the Earth, as well as controlling
and completing the process of new material fabrication technology. CaSiO3 system has widely
been studied for a long time by both theoretical and experimental methods [1, 5-9]. However,
experiment is usually difficult to do at high temperature and pressure due to the high melting
temperature of CaSiO3 [5]. Available experimental data are mainly measured at the ambient
condition [10-13]. The density functional theory-based molecular dynamics simulation of Silicate
liquids [1] showed that the liquid CaSiO3 structure changes significantly under compression. At
ambient pressure, the Ca-O coordination number is mainly 5, 6 and 7; Si-O coordination number
is 4. However, at high pressure (120 GPa) the Ca-O coordination number increases to 8, 9, 10; Si-O
coordination number increases to 6. The Ab-initio molecular dynamics calculation for CaSiO3
perovskite at high pressure and temperature [6] showed the existence of three stable structural
Received October 2, 2016. Accepted October 28, 2016.
Contact Mai Thi Lan, e-mail address: lan.maithi@hust.edu.vn
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Mai Thi Lan, Nguyen Thi Thanh Ha, Tran Thuy Duong, Nguyen Thi Thao and Nguyen Van Hong
phases: orthorhombic, tetragonal and cubic. The MDS results about local structure of CaSiO3
in [5] are in agreement with experimental Raman spectra. The Si-O mean coordination number
is 4. It builds up the stable SiO4 tetrahedra in CaSiO3. Although it has been studied extensively
for a long time but topology structure of Si-O network as well as the local environment of Ca2+,
Si4+, O2+ ions and their change under compression are still in debate and it need to be studied
more. This is also the motivation of our study in this work.
2. Content
2.1. Calculation method
The Born-Mayer-Huggins interatomic potential for CaSiO3 glass
Table 1. The potential parameters for CaSiO3 glass MDS
Aij (eV) Bij (A˚−1) Cij (eVA˚)
Si-Si 5006070.785 12.5 0.00
Si-O 7363.700 5.2632 0.00
O-O 1621.734 3.3333 30.22
Si-Ca 39991599.000 10.8696 0.00
Ca-O 29353.157 4.7619 0.00
Ca-Ca 200790000.000 9.6154 0.00
The atomic interaction potential is employed in MDS significantly affect to calculation
results. The pair interaction potential has still widely been used because of its simplicity as building
atomic model. Up to now, there have some evaluated potentials to study structure and dynamical
properties of oxide silicate systems with high reliability [7, 14-18]. All of these used two-body
Born-Mayer-Huggins form that is given by: Uij (r) =
(
qiqj
rij
)
+
(
Aije
−Bij∗rij − Cij
r6ij
)
.
Where U(ij) (r) is the potential that consists of the long-range Coulomb part and the
short-range repulsion part; qi, qj is the effective charge of the atom i, j respectively. Aij, Bij, Cij are
potential parameters. These parameters for CaSiO3 glass MDS are displayed in table 1 [14]; rij is
distance between atom i and j.
The MD model building for CaSiO3 glass
The molecular dynamic (MD) initial configuration of the CaSiO3 sample is built by
randomly placing N atoms in a cubic box with periodic boundary condition (N = 5000 atoms
consist of 1000 Si, 1000 Ca, 3000 O atoms). Then, the sample is heated up to 6000K to remove
the effect of remembering initial configuration and reaches to the equilibrium after 106 MD
steps. Next, the sample is cooled down to the temperature of 600K at ambient pressure with
the cooling rate of about 2.5K/ps after 2.105 MD steps to obtain the best equilibrium state (M1
model). We continue construct the M2, M3, M4, M5, M6 models by compressing model M1
to different pressures (corresponding to from 5 to 35 GPa) and then relaxed for a long time to
reach equilibrium. After that, the structural characteristic such as radial distribution function,
coordination number, bond-angle and bond-length distributions. . . are determined by mean over
2000 configurations in the last 103 MD steps.
166
Pressure-dependent structural heterogeneity in calcium silicate glass
2.2. Results of structural properties of CaSiO3 glass
In this section, the structural properties of CaSiO3 glass in the short-range order (SRO) and
intermediate-range order (IRO) will be investigated in detail.
The pair radial distribution functions (RDFs) in CaSiO3 glass at different pressures
are showed in Figure 1. The results present the height of first peak decrease and the wide
becomes broader with compression. Moreover, the next peak height rapidly decrease and finally
approaching unity at larger distances. These features demonstrate that the degree of structural
order decrease with increasing pressure. In particular, the RDF of Si-O pair is much shaper peak
and deeper minimum than Ca-O pair. The position of the first peak increase as increasing pressure.
It means that the average Ca-O and Si-O bond length increase with compression.
Figure 1. The pair radial distribution functions in CaSiO3 glass at different pressures.
Figure 2. The coordination number distribution in SiOx (x = 4 ÷ 6) and CaOy
(y = 5 ÷ 11) polyhedra at different pressures.
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Mai Thi Lan, Nguyen Thi Thanh Ha, Tran Thuy Duong, Nguyen Thi Thao and Nguyen Van Hong
Figure 3. The O-Si-O bond angle and Si-O bond length distribution
in SiOx polyhedra at different pressures
Conversely, for the RDF of Si-Si, Si-Ca, Ca-Ca and O-O pairs, the position of the first peak
decreases with pressure. So the mean bond distance of Si-Si, Si-Ca, Ca-Ca and O-O pairs decrease
as the pressure increases. In particular, the Si-O and Ca-O bond length that relates to SRO increases
from 1.61, 2.36 A˚ to 1.64 A˚, 2.38 A˚, respectively. Whereas, the bond length of Si-Si, Si-Ca, Ca-Ca
and O-O pairs which relate to IRO decreases from 3.12, 3.54, 3.64 A˚ to 2.60, 3.12, 3.28 and
2.46 A˚, respectively. This result is in good agreement with the works in [1, 9, 12]. Figure 2 shows
the coordination number distribution in SiOx and CaOy polyhedra (x = 4 ÷ 6; y = 5 ÷ 11) under
compression. This result is also in good agreement with the work [1]. The results show that, at
ambient pressure, most of Si atoms (97.7%) have four coordinated oxygen atoms forming the SiO4
polyhedra. Most of Ca atoms have from five to seven coordinated oxygen atoms forming CaO5,
CaO6 and CaO7 polyhedra. As increasing pressure, the percentage of SiO4 polyhedra decreases
meanwhile the percentage of SiO5 and SiO6 polyhedra increases. At high pressure (35GPa),
the percentage of SiO5 (43.52%) and SiO6 (53.38%) is mainly. This clearly illustrates that
under compression, there is transformation from SiO4- to SiO6-network through SiO5 polyhedra.
Similarly, as increasing pressure, the percentage of CaO5, CaO6 polyhedra strongly decreases, the
percentage of CaO9, CaO10, CaO11 polyhedra strongly increases, meanwhile the percentage of
CaO7, CaO8 increase and reach a maximum value 38.43%, 39.48% at 5, 10 GPa, respectively,
168
Pressure-dependent structural heterogeneity in calcium silicate glass
then rapidly decreases. At 35 GPa, the percentage of CaO9, CaO10, CaO11 is dominant. It means
that under compression, most of CaOy polyhedra are CaO5, CaO6 and CaO7 at low pressure and
CaO9, CaO10 CaO11 at high pressure.
Figure 4. The O-Ca-O bond angle O-Ca-O and Ca-O bond length distribution
in CaOy polyhedra (y = 5, 6, 7) at different pressures
The T-O coordination number increasing leads to T-O-T and O-T-Omean bond angle as well
as the T-T and O-O mean bond length decrease (T = Si, Ca). This make the Coulomb repulsion
between cation and cation (Ca2+ - Ca2+, Si4+ - Si4+, Si4+-Ca2+), anion and anion (O2− - O2−)
increases lead to elongation of the T-O bond length. Thus we can summary that network structure
of CaSiO3 glass is built up SiOx polyhedra (x = 4 ÷ 6) and CaOy polyhedra (y = 5 ÷ 11) with the
percentage of SiO4, CaO5, CaO6 and CaO7 is mainly at low pressure and the percentage of SiO5,
SiO6, CaO9, CaO10, CaO11 is dominant at high pressure. To clarify the SRO in CaSiO3 glass,
we continue to study the topology structure of TOn polyhedra. Figure 3 presents the O-Si-O bond
angle and Si-O bond length distribution in SiOx polyhedra (x = 4 ÷ 6) at different pressures. It
shows that, these distributions are not dependent on pressure. It means that the size and shape of
SiOx polyhedra are identical and not rely on pressure. The Coulomb repulsive force between O2−
and O2− in SiO5 and SiO6 polyhedra is stronger than the one in SiO4, so the Si-O bond length in
SiO5 and SiO6 increase. Specially, the Si-O bond length distribution in SiO4, SiO5 and SiO6 has
a peak at 1.6, 1.66 and 1.72 A˚, respectively.
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Mai Thi Lan, Nguyen Thi Thanh Ha, Tran Thuy Duong, Nguyen Thi Thao and Nguyen Van Hong
Figure 5. The O-Ca-O bond angle and Ca-O bond length distribution CaOy polyhedra
(y = 8, 9, 10, 11) at different pressures.
Similarly, Figures 4 and 5 display O-Ca-O bond angle and Ca-O bond length in CaOy
(y = 5 ÷ 11). The result shows that the bond angle distribution in CaO5, CaO6, CaO7, CaO8
undergoes a slightly change as increasing pressure in the 0 ÷ 15 GPa pressure range because of
the significant change of percentage of CaO5, CaO6, CaO7, CaO8 in the 0 ÷ 15 GPa. At upper
15 GPa, the O-Ca-O bond angle distribution in CaO5, CaO6, CaO7, CaO8 are almost not rely on
pressure. The O-Ca-O bond angle distribution in CaO9, CaO10, CaO11 are almost unchanged in
a whole considered pressure. So the shape and size of CaO5, CaO6, CaO7, CaO8 is only slightly
distorted in about under 15GPa, meanwhile the shape and size of CaO9, CaO10, CaO11 are almost
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Pressure-dependent structural heterogeneity in calcium silicate glass
not change and not depend on the range of considered pressure. These mean that SRO structure of
CaSiO3 glass is almost unchanged and not dependent on compression.
Figure 6. The distribution of OTm (m = 2 ÷ 6) linkages at different pressures.
Now, we focus on clarify IRO structure that regard to the linkage among the TOn polyhedra
in network structure of CaSiO3 glass. The distribution of OTm linkages (m = 2 ÷ 6) under
compression are showed in Figure 6. At low pressure (0 GPa), the percentage of OT2, OT3 and
OT4 linkages is 9.7%, 52.63% and 35.23%, respectively. Meanwhile the percentage of OT5 and
OT6 is almost zero. When the pressure increases, the percentage of OT2, OT3 linkages decrease,
in contrast the percentage of OT5 and OT6 linkages increase. At high pressure (35 GPa), the
percentage of OT4, OT5 and OT6 is 30%, 46.6% and 26,6% respectively. Note that, the percentage
of OTm(m = 2 ÷ 6) is k%, it means k% oxygen atoms link between m TOn polyhedra.
Figures 7 and 8 displays the T-O-T bond angle (it can be Si-O-Si, Ca-O-Ca or Si-O-Ca
bond angle) and O-T bond length (O-Si or O-Ca bond length) in OTm. The results show that, for
OT2 linkages with T is mainly Si atoms, number of Ca atoms is small so exists one peak at 145◦
corresponding to T-O-T bond angle distribution and at 1.7 A˚ corresponding to O-T bond length
distribution. The appearance two peaks in bond angle, bond length distribution of OT3, OT4, OT5
and OT6 linkages due to T consist of both Si and Ca. For example, OT3 is not only OSi3 or
OCa3 but also Si2-O-Ca or Si-O-Ca2 meanwhile Si2-O-Ca and Si-O-Ca2 is dominant. Besides,
the T-O-T bond angle distribution in OT2 and OT3 linkages has change under compression. In
contrast, the T-O-T bond angle distribution in OT4, OT5 and OT6 linkages is almost unchanged
under compression so the shape and size is unchanged and not dependent on pressure. Thus, IRO
structure in CaSiO3 glass changes due to the change of OT2 and OT3 linkages.
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Mai Thi Lan, Nguyen Thi Thanh Ha, Tran Thuy Duong, Nguyen Thi Thao and Nguyen Van Hong
Figure 7. The T-O-T bond angle and O-T bond length distribution
in OT2, OT3 linkages at different pressures.
The existence of OTm linkages in CaSiO3 glass as well as a significant percentage of O
atoms that only link among SiOx polyhedra (forming OSin linkages) or only link among CaOy
polyhedra (forming OCan linkages) (n = 2, 3, 4) is origin of structural heterogeneity and micro
phase separation. By visualizing, we show that OSin and OCan linkages (n = 2, 3, 4) tend to
building up cluster to forming Si-rich regions (SiOx phase) and Ca-rich (CaOy phase) regions in
network structure of CaSiO3 glass, see Figure 9. This is origin of structural heterogeneity and
micro phase separation. Moreover, we see that SiOx polyhedra link together forming Si-O network
in whole model, see Figure 10. It is the reason lead to polymerization on CaSiO3 glass.
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Pressure-dependent structural heterogeneity in calcium silicate glass
Figure 8. The T-O-T bond angle and O-T bond length distribution
in OT4, OT5, OT6 linkages at different pressures.
Figure 9. Spatial distribution of OSin and OCan (n = 2, 3, 4, 5) at 0 and 30 GPa.
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Mai Thi Lan, Nguyen Thi Thanh Ha, Tran Thuy Duong, Nguyen Thi Thao and Nguyen Van Hong
Figure 10. Network structure of CaSiO3 system and Si-O network that is extracted
from CaSiO3 system at ambient pressure
3. Conclusion
We have simulated CaSiO3 glass using MDS method to investigate their structure in the
range of pressure from 0 to 35 GPa. Our results are in agreement with Neutron diffraction
experiment and simulated works [1,9,12]. The network structure of CaSiO3 glass is built up the
SiOx polyhedra (x = 4 ÷ 6) and CaOy polyhedra (y = 5 ÷ 11). At ambient pressure, SiOx and
CaOy polyhedra are mainly SiO4 and CaO5, CaO6, CaO7, respectively. At high pressure, SiO5,
SiO6 and CaO9, CaO10, CaO11 polyhedra are dominant. The O-T-O bond angle and T-O bond
length distribution (T is Si or Ca) are almost not dependent on the change of pressure. It means
that the SRO structure is almost unchanged and not dependent on compression. Regarding to the
IRO structure, most of OTn linkages are OT2 and OT3 at low pressure and OT4, OT5, OT6 at
high pressure. Moreover, OSin and OCan linkages (n=2,3,4) tend to building up cluster to forming
Si-rich region (phase SiOx) and Ca-rich (phase CaOy) in network structure of CaSiO3 glass. This
is an organization of microstructure phase separate and structural heterogeneity in CaSiO3 glass.
Beside, we show that, SiOx polyhedra link together to become to Si-O network in a whole model.
It is the reason lead to polymerization in CaSiO3 glass.
Acknowledgement. This research is funded by Hanoi University of science and Technology
project number: T2016-PC-218.
REFERENCES
[1] Suraj, K. Bajgain, DiptaB. Ghosh, Bijaya B. Karki, 2015. First principles simulations of
CaO and CaSiO3 liquids: structure, thermodynamics and diffusion. Physics and Chemistry
of Minerals, Volume 42, Issue 5, pp. 393-404.
[2] Darwish H, Ibrahim S, Gomaa M, 2013. Electrical and physical properties of
Na2O-CaO-MgO-SiO2 glass doped with NdF3. Journal of Materials Science: Materials in
Electronics, 24(3):1028-1036.
174
Pressure-dependent structural heterogeneity in calcium silicate glass
[3] Matsushita T, Watanabe T, Hayanabe T, Hayashi M, Mukai K, 2011. Thermal, optical
and surface/interfacial properties of molten slagsystems. International Materials Reviews,
56(5-6):287-323.
[4] Fowler SJ, Spera F, Bohrson W, Belkin H E, de Vivo B, 2007. Phase equilibria constraints
on the chemical and physical evolution of the campanian ignimbrite. Journal of Petrology,
48(3):459-493.
[5] Yong-quan Wu, Chen Dai, Guo-chang Jiang, 2014. Local structure of calcium silicate melts
from classical molecular dynamics simulation and a newly constructed thermodynamic
model. Trans. Nonferrous Met. Soc. China 4, 1488-1499.
[6] Li Li, Donald J. Weidner, John Brodholt, Dario Alf‘e, G. David Price, Razvan Caracas,
RenataWentzcovitch, 2006. Phase stability of CaSiO3 perovskite at high pressure and
temperature: Insights from ab initio molecular dynamics. Physics of the Earth and Planetary
Interiors 155, 260-268.
[7] Robert N. Mead and Gavin Mountjoy, 2006. A Molecular Dynamics Study of the Atomic
Structure of (CaO)x(SiO2)1−x Glasses. J. Phys. Chem. B, 110, 14273-14278.
[8] R. N. Mead, G.Mountjoy, 2005. The structure of CaSiO3 glass and the modified random
network model. Phys. Chem. Classes., 46 (4), 311-314.
[9] Huang Shi-Ping, You Jing-Pin, Jiang Guo-Chang, 2000. A molecular dynamics simulation of
CaSiO3 melt under an electric field. Chin. phys. lett, Vol.17, No. 4, 279.
[10] Lange RA, Carmichael IS, 1987.Densities of Na2O–K2O–MgO–FeO–Fe2O3–Al2O3-TiO2-SiO2
liquids: new measurements and derived partial molar properties.
GeochimCosmochimActa51:2931-2946.
[11] Lange R, Carmichael IS, 1990. Thermodynamic properties of silicate liquids with emphasis
on density, thermal expansion and compressibility. Rev Mineral Geochem 24:25-64.
[12] Skinner LB et al., 2012. Structure of molten CaSiO3: neutron diffraction isotope
substitution with aerodynamic levitation and molecular dynamics study. J. PhysChem B
116:13439-13447.
[13] Benmore C, Weber J, Wilding M, Du J, Parise J., 2010. Temperature dependent structural
heterogeneity in calcium silicate liquids. Phys Rev B 82:224202.
[14] Huang Shi-Ping, You Jing-Pin, Jiang Guo-Chang, F. Yoshida, Xu Kuang-Di, 2000. A
molecular dynamic simulation of CaSiO3 melt under an electric field. Chin. Phys. Lett, Vol.
17, No. 4, 279.
[15] N. A. Morgan and F. J. Spera, 2001. A Molecular Dynamics Study of the Glass Transition in
Ca Al2Si2O8, AmericanMineralogist. Vol. 86, No. 4, pp. 915-926.
[16] T. Matsumiya, A. Nogami and Y. Fukuda, 1993. Applicability of Molecular Dynamics to
Analyses of Refining Slags. ISIJ International, Vol. 33, No. 1, pp. 210-217.
[17] F. J. Spera, D. Nevins, M. Ghiorso and I. Cutler, 2009. Structure, Thermodynamic and
Transport Properties of CaAl2Si2O8 Liquid. Part I: Molecular Dynamics Simulations.
Geochimica et Cosmochimica Acta, Vol. 73, No. 22, pp. 6918-6936.
[18] Wu Y Q, Jiang G C, You J L, Hou H Y, Chen H, Xu K D., 2004. Theoretical study of
the local structure and Raman spectra of CaO-SiO2 binary melts [J]. Journal of Chemical
Physics, 121(16): 7883-7895.
175