research papers
Crystal structures of calcium hemicarboaluminate and carbonated calcium hemicarboaluminate from synchrotron powder diffraction data
aMax-Planck-Institute for Solid State Research, Heisenbergstraße 1, Stuttgart D-70569, Germany, and bInstitut für Geowissenschaften und Geographie, FG Mineralogie/Geochemie, Halle Von Seckendorff-Platz Haus 3, Halle D-06120, Germany
*Correspondence e-mail: r.dinnebier@fkf.mpg.de
One of the main phases formed at the beginning of the carbonation reaction of cementitious building materials is the calcium hemicarboaluminate (abbreviated as Hc). This AFm (shorthand for hydrated calcium aluminate phases structurally related to hydrocalumite) phase was synthesized, crystallized and then studied by synchrotron X-ray powder diffraction and micro-Raman spectroscopy. At room temperature and standard experimental conditions two major cementitious phases were detected, the Hc phase (as a major phase) and carbonated calcium hemicarboaluminate (abbreviated as cHc). By increasing the temperature the Hc form transforms into cHc. The crystal structures of these important AFm phases were successfully solved and refined in the a = 5.7757 (1) and c = 48.812 (2) Å, and cHc the unit-cell parameters a = 5.7534 (1) and c = 46.389 (1) Å. The two crystal structures are composed of positively charged main layers, [Ca4Al2(OH)12]2+, and negatively charged interlayers, [OH2n(CO3)1 − n·4H2O]2−. The structure of the main layers is typical of the AFm family. Conversely, the interlayer region has a characteristic structure built up from water molecules and statistically distributed anions. In the interlayer, the Hc carbonate and hydroxyl anions are distributed in a 0.25:0.5 ratio, whereas the ratio of the anions in the cHc interlayers is 0.4:0.2.
of the trigonal Hc has the unit-cell parameters1. Introduction
Cements are one of the most used materials in the construction industry and civil engineering. Calcium aluminate cements (also known as aluminous or high-alumina cements) are of special interest because of their ability to develop rapid strength (even at low temperatures) and high chemical resistance. On hydration, they can form AFm phases (shorthand for hydrated calcium aluminate phases structurally related to hydrocalumite) which belong to the lamellar double hydroxide family (Pöllmann, 1984; Matschei et al., 2007). Carbonate-containing AFm phases are mainly formed during the carbonation process of many different building materials. The AFm phases are composed of positively charged main layers and negatively charged interlayers. The main layers have a similar structure in all AFm phases, with the chemical formula [Ca4Al2(OH)12]2+, and are built up of aluminium octahedra and calcium capped trigonal antiprisms. Conversely, the interlayer region is characterized by pronounced diversity in the composition and structure, and can accommodate one (primary interlayer), two (binary) or three (tertiary) types of anions. In the AFm phases with a primary interlayer, [Xx·nH2O]2–, X can be carbonate (Fischer & Kuzel, 1982; François et al., 1998; Renaudin, François et al., 1999; Renaudin & François, 1999), sulfate, as in the synthesized monosulfoaluminate (Allmann, 1977) or as in the natural mineral kuzelite (Pöllmann et al., 1997), chloride as in Friedel's salt (Terzis et al., 1987; Renaudin, Kubel et al., 1999; Rapin et al., 2002), iodide (Rapin et al., 1999), nitrate (Renaudin & François, 1999) and others. Several structural studies on binary phases, [XxYy·nH2O]2−, were reported. In these structures X and Y can be sulfate and chloride as in Kuzel's salt (Mesbah, François et al., 2011), chloride and carbonate as in the synthesized phase (Mesbah, Rapin et al., 2011) or as in the natural mineral hydrocalumite (Sacerdoti & Passaglia, 1988), bromide and chloride (Rapin & Francois, 2001; Renaudin et al., 2004) or hydroxide and carbonate (Fischer & Kuzel, 1982). Also, examples of a ternary AFm phase containing sulfate, carbonate and hydroxide as anions are reported (Pöllmann et al., 1998; Pöllmann, 2006). Most of the crystal structures of the AFm phases are solved and refined using single-crystal or powder X-ray diffraction data. A list of selected AFm phases, described in the trigonal (rhombohedral) (as the crystal structures of the compounds presented in this article), is given in Table 1.
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To the best of our knowledge the
of the binary phase composed of hydroxide and carbonate anions, the calcium hemicarboaluminate (Hc) phase, has not been reported so far. This phase is important because it is the main phase formed at the beginning of carbonation reactions of building materials. The chemical formula of this compound can be written aswhere the amount of water molecules (n) can vary and have different bonding fashions. Another common way of representing the composition of the Hc phase (especially in industry) is by using the cement chemistry notation
Pioneering studies on the Hc phase were reported in the 1960s, i.e. those by Dosch & zur Strassen (1965), Ahmed et al. (1968) and Roberts (1968). Fischer & Kuzel (1982) reinvestigated the system 20 years later and indexed the powder diffraction pattern in the trigonal with the being either R3c or and lattice parameters of a = 5.77 and c = 49.16 Å. The was not solved but it was proposed that it is built of typical AFm main layers and an interlayer composed of the carbonate anion, hydroxyl anions and two types of water molecules – crystallographically bonded and space-filling water molecules. Ipavec et al. (2011) reported that the Hc phase shows high susceptibility to atmospheric carbon dioxide and when exposed to air it gradually transforms into calcium monocarboaluminate (which structure was solved by François et al., 1998; Renaudin & François, 1999).
The Hc phase does not form crystals of sufficient quality for single-crystal diffraction. Accordingly, the only method of choice for
is powder diffraction.Motivated by the importance of the Hc phase in the cement industry, structural studies on the system in the temperature range 297–1173 K were undertaken. This phase was synthesized as the (sufficiently) pure phase and was studied using synchrotron X-ray powder diffraction (XRPD). The in situ high-resolution synchrotron X-ray powder diffraction and micro-Raman spectroscopy.
of the Hc phase was solved and refined. At room temperature, together with the Hc phase, another major phase was found in the system, the carbonated calcium hemicarboaluminate (cHc) phase. Its structure was solved and refined and it was found that this phase is characterized by a larger amount of carbonate anion (at the expense of the hydroxyl anions). By heating in an atmosphere with a reduced amount of carbon dioxide, the Hc phase completely transforms into the cHc phase which thereafter is stable up to decomposition. The high-temperature behavior of the two-phase system (referred as Hc-cHc) was studied by2. Experimental
2.1. Synthesis
The Hc-cHc sample was synthesized using a paste reaction with stoichiometric quantities of monocalcium aluminate (synthesized by the laboratory reaction of CaCO3 and γ-Al2O3 with intermediate grinding at a temperature of 1623 K), CaO (synthesized by decarbonization reaction of CaCO3 at 1273 K for 1 h) and CaCO3. The reactants were mixed in polyethylene bottles with CO2-free, freshly distilled water (with a water-to-solid ratio of 10). Chemical analyses were performed using ICP-OES (HORIBA) and ICP-MS (thermo-instruments PQ Excell) and the results are given in Table 2. By using XRPD analysis two impurities (tricalcium dialuminium oxide hexahydrate and calcium carbonate) were identified, together present in less than 4 wt % of the composition. After drying in a desiccator at room temperature the Hc-cHc system crystallized as thin hexagonal uniaxial negative plates (as previously observed by Fischer & Kuzel, 1982). The scanning electron micrograph of the phase at room temperature is given in Fig. 1 (obtained by using a Jeol instrument JSM 6300).
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2.2. Powder X-ray diffraction and determination
For ) were collected using a high-resolution powder diffractometer at the I11 beamline, located at the British national synchrotron facility the Diamond Light Source. The wavelength of radiation was determined from a silicon standard to be 0.826401 (300) Å. The beamline set-up and characteristics are described in the literature (Parker et al., 2011; Thompson et al., 2009, 2011). The diffraction data were collected in the temperature range 297–1173 K. The scans at each temperature were written continuously with 2 K min−1 and 14 s per frame.
determination the powder diffraction data of Hc-cHc (Fig. 2For the diffraction measurements finely powdered samples were placed in quartz capillaries with limited contact to the atmosphere. The carbon dioxide led to the transformation of the Hc phase into the cHc phase on heating, as shown by the changes in unit-cell parameters in Fig. 2. In the case of heating the Hc-cHc system in open air, the system shows significantly different behavior, i.e. resulting in the appearance of a new phase at higher temperatures (further studies on this phase transformations are in process).
Analysis of the powder data collected at 297 K led to the identification of two major phases, Hc and cHc, and impurities of H12Al2Ca3O12 (16592-ICSD) and CaCO3 (20179-ICSD), both impurity phases present in less than 4 wt % of the total amount. Both AFm phases were indexed (Coelho, 2003) in the trigonal with slightly different unit-cell parameters, as given in Table 3.1
‡Due to the small disordered occupancies of the hydroxyl O atoms, they are not included in the final of the cHc phase. Therefore, the presented values of n and of the formula weight are calculated. §Rexp, Rp, Rwp, RBragg and S values are as defined in TOPAS4.2 (Bruker, 2007). |
The ). The peak profiles and precise lattice parameters were determined by a Pawley fit (Pawley, 1981) using the fundamental parameter approach of TOPAS4.2 (Bruker, 2007; Cheary et al., 2004; Coelho, 2000). Chebyshev polynomials were used for the modeling of the background. The same procedure was repeated on the data collected at different temperatures. By increasing the temperature, gradual changes of the parameters were noticed and above 337 K only one major phase was identified (cHc), as shown in Fig. 2.
found in the powder pattern indicated as the most probable and this was later confirmed by (Rietveld, 1969Over the course of the et al., 2011) as a starting model. In order to confirm the structure of the layers without using a starting model, the charge-flipping method was used, leading to the same The solution was completed by finding the structure of the interlayer region, performed by inspecting the difference Fourier maps.
solution the atomic coordinates of the main layer atoms were taken from the close structure (Mesbah, RapinFor the final
the profile and lattice parameters as well as the atomic positions were subjected to except of the parameters of the hydroxyl O atoms because of the low occupancies. The displacement factors were treated isotropically.The strong anisotropy of width and asymmetry of the Bragg reflections could be quite satisfactorily modeled by the phenomenological microstrain model of Stephens with four refinable parameters for the rhombohedral ). Nevertheless, in order to obtain a better fit of the peak profile for a higher quality of the symmetry-adapted spherical harmonics were applied instead to the width and shape of the Bragg peaks. No attempt was made to physically model the complex peak shape, suggesting a severe and other types of disorder. Despite the use of capillaries in Debye–Scherrer geometry, a small amount of the was detected which originates from the plate-like form of the crystallites (see Fig. 1) and was adequately described by the use of symmetry-adapted spherical harmonics. The origin of the complex peak profile is quite likely related to the simultaneous occurrence of stacking faults (h.c.p./c.c.p.) of the extreme layer structure and variations of the content of dissipated water in different domains. Rietveld refinements were carried out on the diffraction patterns collected at 297 and 347 K (Fig. 3). The data and the final agreement factors (R values) are listed in Table 3.
(Stephens, 1999The difference Fourier maps were generated using the program JANA (Petřiček et al., 2006). The structure factors for Fourier synthesis were obtained from the using the program TOPAS4.2 (Bruker, 2007).
2.3. Raman spectroscopy
The micro-Raman spectra were recorded using a Jobin Yvon Typ V 010 Labram single grating spectrometer, equipped with a double super razor edge filter and a peltier-cooled CCD camera. The resolution of the spectrometer (grating 1800 L mm−1) was 1 Raman shift (cm−1). The spectra were taken in quasi-backscattering geometry using the linearly polarized 532.0 nm line of a with power less than 1 mW, focused to a 20 µm spot through a 20× microscope objective onto the top surface of the sample. For the heating experiments, a linkam THS 600 heater was used, with a small argon gas flow rate.
3. Results and discussion
3.1. of Hc
The ) is composed of main layers and interlayers, as in the case of other AFm phases. The structure of the main layers is typical for the AFm family, where the aluminium is coordinated by six O atoms forming an octahedron. Aluminium octahedra are arranged in hexagonal primitive nets connected by the Ca atoms (Fig. 4a). The calcium cation is coordinated by seven O atoms, six belonging to the main layer and an oxygen from the water molecule placed in the interlayer region. The seven O atoms around the calcium build a polyhedron that can be regarded as a strongly deformed octahedron with one triangle expanded such that a bowl is formed and is closed by an interlayer water molecule forming a capped trigonal antiprism (Terzis et al., 1987), as shown in Fig. 4(b). Six main layers arranged perpendicular to the c-axis and divided by the interlayer regions build the packing diagram of the Hc phase, as presented in Fig. 4(c).
of the Hc phase (Fig. 4The main structural differences within the members of the AFm family are observed in their interlayer regions. In the case of the Hc phase, the interlayer is composed of carbonate and hydroxyl anions and water molecules which are bonded to the calcium cations of the main layer (Fig. 4c). On every aluminium cation in the main layer there are 0.25 carbonate and 0.5 hydroxyl anions in the interlayer region, providing electroneutrality. The carbonate anions are ordered and placed perpendicular to the threefold axis running parallel to the c axis. The hydroxyl anions are placed on a general position and are disordered around the position of the carbonate anion. Owing to the low occupancy and high level of disorder, the positions of the hydroxyl group cannot be freely refined. In order to find the most probable positions of these atoms difference Fourier maps were generated using a model of the containing the main layers, the bonded water molecules in the interlayer and the carbonate group with a fixed occupancy of 0.25. Two different sections of the map are given in Fig. 5. On closer inspection of the map neither positive nor negative electron density can be observed around the position of the C atom, implying the correctly refined occupancy of the carbonate group. Fig. 5(a) shows that the positive electron density is observed above and below the positions of the carbonate group originating by the OH− anion. By introducing the hydroxyl anions in the model, a significant reduction in the Rwp factor was noticed (dropping by a value of 2%). During the final the position and occupancy of the OH− group was fixed, as found by the difference Fourier maps. It is worth noting that the difference Fourier map calculated after introducing the OH− anion still showed a positive electron density smeared below and above the carbonate group. This electron density might originate from dissipated water, completely disordered in this interlayer's region as suggested by previous studies. Namely, Fischer & Kuzel (1982) reported different hydration stages of the Hc phase in the temperature range between 295 and 473 K. As mentioned in §1, it was suspected that in the interlayer region, beside the water molecules bonded to the calcium cations, there are space-filling water molecules. In their study the content of water is removed in three steps: the first two steps are assigned to losing the space-filling molecules, and the third step to removing the crystallographically bonded water. The space-filling water cannot be detected by X-ray diffraction, therefore it was not accounted for in the final Rietveld refinements and it was not included in the model.
Taking into account the disorder of the anionic species in the structure, and their statistical distribution, it can be said that the C1 or Ci in Schoenflies notation).
of the is significantly lower (3.2. of cHc phase
The cHc phase crystallized together with Hc giving the Hc-cHc two-phase system. On heating, the whole quantity of Hc transferred into the cHc phase (Fig. 2). Both phases have the same for the main layers, but they show a significant difference in the interlayer region. A difference Fourier map was generated using the same model as in the case of the Hc phase (containing the main layers, the interlayer water molecules and the carbonate group with fixed occupancy of 0.25). Closer inspection of the map showed pronounced positive electron density around the positions of the carbonate atoms, indicating the underestimated content of the carbonate group (Fig. 6). After refining the occupancies of the carbonate atoms to the value of 0.4 the difference Fourier map showed no significant (neither positive nor negative) electron density around the carbonate atoms. As shown in Fig. 6(b), the carbonate group is shifted up and down from the position in the center of the interlayer, which also implies that the might be as low as C1 or Ci, and the resulting trigonal structure is obtained as the superposition of all interlayers. According to the charge balance, the quantity of hydroxyl anions has to be reduced and fixed to 0.2. Taking into account the low occupancy and the fact that these hydroxyl atoms are distributed on a general position with high multiplicity, their positions cannot be found and refined from powder diffraction data. To shine light on the interlayer structure and obtain deeper knowledge on the distribution of the anionic species, additional studies using the method of maximum are in progress.
cHc can be regarded as an intermediate phase between the Hc phase and calcium monocarboaluminate (abbreviated as Mc). The Mc phase crystallizes in the triclinic et al., 1998).
and one of the main differences with the of the Hc phase is the fact that one of the O atoms from the carbonate group is directly bonded to the calcium cation (François3.3. Micro-Raman spectroscopy
A powerful tool to inspect the bonding scheme of the carbonate group in AFm phases is micro-Raman spectroscopy. As described above, in the case of the Hc and cHc phases, the carbonate group is placed in the center of the interlayer and the O atoms are not bonded to the main layer. Mesbah, Rapin et al. (2011) reported the micro-Raman spectra of some AFm phases and found that the Raman band at 1068 cm−1 is attributed to the carbonate group directly bonded to the main layer and the Raman band at 1086 cm−1 is attributed to the weakly bonded carbonate group located at the center of the interlayer. The micro-Raman spectra of the Hc-cHc system are presented in Fig. 7, where an intense band is noticed around 1086 cm−1 corresponding to the non-bonded carbonate group. The micro-Raman spectra were taken at different temperatures and a shift of the band was not observed, confirming that in the structures of both phases (Hc and cHc) the carbonate group environment is the same. It should be noted that an additional band is noticed at 1068 cm−1, corresponding to the bonded carbonate group. During the micro-Raman measurements only the surface is tested, therefore, it can be suspected that part of the surface of Hc-cHc is transformed into Mc, giving rise to this weak band. The same experiment was carried out on an open atmosphere with unlimited access to carbon dioxide and under these experimental conditions at higher temperatures the band at 1086 cm−1 completely disappeared and the band at 1068 cm−1 gained in intensity, indicating that a new phase was formed where the carbonate group is bonded to the main layer (crystal structure analysis of this phase is in progress). As shown in Fig. 7, the position of the band at 530 cm−1 remains unchanged. Knowing that this band originates by the Raman active vibrations of the Al(OH)6 group, it can be confirmed that in the temperature interval up to 388 K the structure of the main layers remains unchanged.
3.4. Decomposition products
Analysis of the powder patterns collected as a function of temperature led to the detection of two phases crystallizing after the decomposition of the Hc-cHc system. The first phase, lime (CaO, PDF file 43-1001), appeared with onset at 823 K, and the second one, mayenite (Ca12Al14O33, PDF file 48-1882), with onset at 1123 K. The decomposition is similar in the case of Kuzel's salt (Mesbah, François et al., 2011).
4. Conclusion
The ca 338 K two different hydration forms simultaneously exist, the Hc and the cHc phase. Their crystal structures are composed of positively charged main layers and negatively charged interlayers. The interlayer region accommodates statistically distributed carbonate and hydroxyl anions. In the Hc phase on every Al atom there are 0.25 carbonate anions and 0.5 hydroxyl anions. By partial carbonation of the Hc phase, the cHc phase is formed in which there are more carbonate anions (0.4) and less hydroxyl anions (0.2). On increasing the temperature in atmosphere with a reduced amount of carbon dioxide the Hc phase completely transforms into the cHc phase which is present up to decomposition at ca 393 K. The carbonate group environment was additionally studied by micro-Raman spectroscopy and it was confirmed that in both structures the carbonate group is placed in the interlayer region.
of the cementitious Hc AFm phase was solved and refined by XRPD using synchrotron radiation. It was found that up toSupporting information
10.1107/S010876811203042X/eb5017sup1.cif
contains datablocks global, cHc, Hc. DOI:Structure factors: contains datablock Hc. DOI: 10.1107/S010876811203042X/eb5017Hcsup2.hkl
Structure factors: contains datablock cHc. DOI: 10.1107/S010876811203042X/eb5017cHcsup3.hkl
Rietveld powder data: contains datablock 297K. DOI: 10.1107/S010876811203042X/eb5017297Ksup4.rtv
Rietveld powder data: contains datablock 347K. DOI: 10.1107/S010876811203042X/eb5017347Ksup5.rtv
C0.4AlCa2O9.2 | Z = 6 |
Mr = 259.14 | F(000) = 774.0 |
Trigonal, R3c | Dx = 1.942 Mg m−3 |
Hall symbol: -R 3 2"c | Synchrotron radiation, λ = 0.8264 (3) Å |
a = 5.7534 (1) Å | T = 347 K |
c = 46.389 (1) Å | white |
V = 1329.84 (4) Å3 | ?, ? × ? × ? mm |
C0.4AlCa2O9.2 | V = 1329.84 (4) Å3 |
Mr = 259.14 | Z = 6 |
Trigonal, R3c | Synchrotron radiation, λ = 0.8264 (3) Å |
a = 5.7534 (1) Å | T = 347 K |
c = 46.389 (1) Å | ?, ? × ? × ? mm |
x | y | z | Uiso*/Ueq | Occ. (<1) | |
Ca1 | 0.66667 | 0.33333 | 0.67930 (2) | 0.0231 (4)* | |
Al1 | 0 | 0 | 0 | 0.0127 (5)* | |
O1 | 0.3051 (3) | 0.0586 (3) | 0.52121 (3) | 0.0151 (5)* | |
O2 | 0.66667 | 0.33333 | 0.93091 (6) | 0.0630 (10)* | |
O3 | 0.220 (3) | 0 | 0.75 | 0.025 (2)* | 0.40 |
C1 | 0.66667 | 0.33333 | 0.083333 | 0.025 (2)* | 0.40 |
Ca1—O1i | 2.374 (2) | Al1—O1iv | 1.890 (2) |
Ca1—O1ii | 2.450 (2) | C1—O3v | 1.266 (4) |
Ca1—O2iii | 2.619 (3) | ||
O1iv—Al1—O1vi | 180.0 | O1xiii—Ca1—O1xiv | 146.32 (5) |
O1vii—Al1—O1viii | 180.0 | O1xiv—Ca1—O1xii | 117.25 (3) |
O1ix—Al1—O1x | 180.0 | O1i—Ca1—O1xiv | 117.25 (3) |
O1iv—Al1—O1vii | 95.36 (6) | O1i—Ca1—O1xii | 117.25 (3) |
O1iv—Al1—O1ix | 95.36 (6) | O1xi—Ca1—O1xiv | 86.21 (6) |
O1vii—Al1—O1ix | 95.36 (6) | O1xiii—Ca1—O1i | 86.21 (6) |
O1vi—Al1—O1viii | 95.36 (6) | O1ii—Ca1—O1xii | 86.21 (6) |
O1vi—Al1—O1x | 95.36 (6) | O1xiii—Ca1—O1xi | 83.35 (5) |
O1viii—Al1—O1x | 95.36 (6) | O1xiii—Ca1—O1ii | 83.35 (5) |
O1iv—Al1—O1viii | 84.64 (6) | O1xi—Ca1—O1ii | 83.35 (5) |
O1iv—Al1—O1x | 84.64 (6) | O1xiii—Ca1—O1xii | 63.65 (8) |
O1vii—Al1—O1vi | 84.64 (6) | O1xi—Ca1—O1i | 63.65 (8) |
O1vii—Al1—O1x | 84.64 (6) | O1ii—Ca1—O1xiv | 63.65 (8) |
O1ix—Al1—O1vi | 84.64 (6) | O1xii—Ca1—O2iii | 80.35 (4) |
O1ix—Al1—O1viii | 84.64 (6) | Al1iv—O1—Ca1xv | 104.00 (7) |
O1xi—Ca1—O1xii | 146.32 (5) | Ca1xiii—O1—Ca1xv | 93.79 (6) |
O1ii—Ca1—O1i | 146.32 (5) | O3v—C1—O3xvi | 120 |
Symmetry codes: (i) −y+1/3, −x+2/3, z+1/6; (ii) −x+4/3, −x+y+2/3, −z+7/6; (iii) −x+4/3, −y+2/3, −z+5/3; (iv) y, x, −z+1/2; (v) x+2/3, y+1/3, z−2/3; (vi) −y, −x, z−1/2; (vii) x−y, −y, −z+1/2; (viii) −x+y, y, z−1/2; (ix) −x, −x+y, −z+1/2; (x) x, x−y, z−1/2; (xi) x−y+1/3, −y+2/3, −z+7/6; (xii) x+1/3, x−y−1/3, z+1/6; (xiii) y+1/3, x−1/3, −z+7/6; (xiv) −x+y+4/3, y+2/3, z+1/6; (xv) −y+2/3, −x+1/3, z−1/6; (xvi) −y+2/3, x−y+1/3, z−2/3. |
C0.25AlCa2O9.25 | Z = 6 |
Mr = 258.13 | F(000) = 771.0 |
Trigonal, R3c | Dx = 1.824 Mg m−3 |
Hall symbol: -R 3 2"c | Synchrotron radiation, λ = 0.8264 (3) Å |
a = 5.7757 (1) Å | T = 297 K |
c = 48.812 (2) Å | white |
V = 1410.14 (7) Å3 | ?, ? × ? × ? mm |
C0.25AlCa2O9.25 | V = 1410.14 (7) Å3 |
Mr = 258.13 | Z = 6 |
Trigonal, R3c | Synchrotron radiation, λ = 0.8264 (3) Å |
a = 5.7757 (1) Å | T = 297 K |
c = 48.812 (2) Å | ?, ? × ? × ? mm |
x | y | z | Uiso*/Ueq | Occ. (<1) | |
Al1 | 0 | 0 | 0 | 0.0127 (7)* | |
Ca1 | 0.66667 | 0.33333 | 0.67796 (4) | 0.0214 (4)* | |
O1 | 0.3012 (3) | 0.0484 (4) | 0.52040 (6) | 0.0224 (5)* | |
O2 | 0.66667 | 0.33333 | 0.93875 (8) | 0.063 (2)* | |
O3 | 0.219 (2) | 0 | 0.75 | 0.025 (4)* | 0.25 |
O4 | 0.565 | 0.474 | 0.094 | 0.025 (7)* | 0.08333 |
C1 | 0.66667 | 0.33333 | 0.08333 | 0.025 (4)* | 0.25 |
Ca1—O1i | 2.346 (3) | C1—O3v | 1.265 (9) |
Ca1—O1ii | 2.467 (3) | C1—O4 | 1.324 |
Ca1—O2iii | 2.439 (4) | O3—O4vi | 0.745 (3) |
Al1—O1iv | 1.900 (3) | O4—O4vii | 1.456 |
O1iv—Al1—O1viii | 180.0 | O1i—Ca1—O1xiv | 116.50 (5) |
O1ix—Al1—O1x | 180.0 | O1i—Ca1—O1xvi | 116.50 (5) |
O1xi—Al1—O1xii | 180.0 | O1xiv—Ca1—O1xvi | 116.50 (5) |
O1xiii—Ca1—O1xiv | 148.60 (8) | O1i—Ca1—O2iii | 79.08 (8) |
O1xv—Ca1—O1xvi | 148.60 (8) | O1xiv—Ca1—O2iii | 79.08 (8) |
O1ii—Ca1—O1i | 148.60 (8) | O1xvi—Ca1—O2iii | 79.08 (8) |
O1xv—Ca1—O2iii | 128.85 (6) | O3v—C1—O3xvii | 120.0 |
O1xiii—Ca1—O1i | 86.29 (9) | O3v—C1—O3xviii | 120.0 |
O1xv—Ca1—O1xiv | 86.29 (9) | O3xvii—C1—O3xviii | 120.0 |
O1ii—Ca1—O1xvi | 86.29 (9) | O3xix—O3—O3xx | 60 |
Symmetry codes: (i) −y+1/3, −x+2/3, z+1/6; (ii) −x+4/3, −x+y+2/3, −z+7/6; (iii) −x+4/3, −y+2/3, −z+5/3; (iv) y, x, −z+1/2; (v) x+2/3, y+1/3, z−2/3; (vi) −x+y+1/3, −x+2/3, z+2/3; (vii) −x+4/3, −x+y+2/3, −z+1/6; (viii) −y, −x, z−1/2; (ix) x−y, −y, −z+1/2; (x) −x+y, y, z−1/2; (xi) −x, −x+y, −z+1/2; (xii) x, x−y, z−1/2; (xiii) y+1/3, x−1/3, −z+7/6; (xiv) −x+y+4/3, y+2/3, z+1/6; (xv) x−y+1/3, −y+2/3, −z+7/6; (xvi) x+1/3, x−y−1/3, z+1/6; (xvii) −y+2/3, x−y+1/3, z−2/3; (xviii) −x+y+2/3, −x+1/3, z−2/3; (xix) −y, x−y, z; (xx) −x+y, −x, z. |
Experimental details
(cHc) | (Hc) | |
Crystal data | ||
Chemical formula | C0.4AlCa2O9.2 | C0.25AlCa2O9.25 |
Mr | 259.14 | 258.13 |
Crystal system, space group | Trigonal, R3c | Trigonal, R3c |
Temperature (K) | 347 | 297 |
a, c (Å) | 5.7534 (1), 46.389 (1) | 5.7757 (1), 48.812 (2) |
V (Å3) | 1329.84 (4) | 1410.14 (7) |
Z | 6 | 6 |
Radiation type | Synchrotron, λ = 0.8264 (3) Å | Synchrotron, λ = 0.8264 (3) Å |
Specimen shape, size (mm) | ?, ? × ? × ? | ?, ? × ? × ? |
Data collection | ||
Diffractometer | Synchrotron Diamond I11 (Great Britain) diffractometer | Synchrotron Diamond I11 (Great Britain) diffractometer |
Specimen mounting | ? | ? |
Data collection mode | ? | ? |
Scan method | ? | ? |
2θ values (°) | 2θmin = ? 2θmax = ? 2θstep = ? | 2θmin = ? 2θmax = ? 2θstep = ? |
Refinement | ||
R factors and goodness of fit | Rp = 0.030, Rwp = 0.050, Rexp = 0.008, χ2 = 40.069 | Rp = 0.029, Rwp = 0.040, Rexp = 0.008, χ2 = 27.384 |
No. of data points | ? | ? |
No. of parameters | ? | ? |
No. of restraints | ? | ? |
Acknowledgements
The authors thank the Diamond Light Source for the synchrotron beam time and the assistance of F. Adams, Dr L. Vella-Zarb, Dr J. E. Parker and Dr C. C. Tang during the measurements. A. Schulz is gratefully acknowledged for measuring the micro-Raman spectra. TR acknowledges the PhD scholarship given by the IMPRS-AM.
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