Indian Journal of Pure & Applied Physics Vol. 44, January 2006, pp. 20-24 Bonding parameter, phase parameter and Ni K-edge position studies of some Ni systems Vinod K Singh Department of Applied Physics, Indian School of Mines, Dhanbad 826 004, Jharkhand Email: [email protected] Received 17 November 2004; revised 17 August 2005; accepted 9 September 2005 Extended X-ray absorption fine structure (EXAFS) phase shift studies of some nickel compounds have been carried out and the values of bonding parameter α1 and phase parameter β1 are evaluated by graphical method. α1 is then correlated with nearest neighbour distance and ionicity of the corresponding systems. It has been observed that the bonding parameter α1 decreases as bond distance decreases except in Ni3(PO4)2.XH2O and NiCl2.6H2O and decreases with increase of the ionicity except for NiBr2. The phase parameter β1 has been correlated with oxygen atoms present in a system. The nickel Kedge position in the systems under study has been correlated with ionicity. No good relation has been observed between ionicity and edge position. This has been attributed to different structure and coordination number of a system. Keywords: EXAFS, XAFS, K-edge X-ray absorption spectra IPC Code: G01J3/42 1 Introduction Extended X-ray absorption fine structure (EXAFS) observed on the high energy side of the absorption edge is attributed to the scattering of the photoelectron emitted by the absorption of the X-ray by the atoms, surrounding the emitting atom. The structures are observed in crystalline, glasses, liquids and in gases except in monoatomic gases. The structure appears over a few hundred eV on the higher side of absorption edge. In contrast, the structure close to the edge is generally dominated by strong multiple scattering process and also local atomic resonance in the absorption edge. This structure, which lies within the 30 eV of the edge, is referred to as X-ray absorption near edge structure1-3 (XANES). Originally, Kronig4,5 explained the formation of EXAFS structures. EXAFS was explained by Stern et al.6,7, Lee and Pendry8, Ashley and Doniac9 and others10-13. It has been proved to be highly useful for determination of bond length, phase parameter, bonding parameter etc. Stern, Sayer and Lytle6 have given the following expression of EXAFS function [χ (k)] of absorbing atom χ (k) = -1/k ∑Aj sin[2kR j + δj(k)] …(1) where, k is the photoelectron wave vector and Aj is an amplitude function containing the coordination number, the scattering terms, the Debye-Waller factor, the elastic loss terms, mean free path etc. The term 2kR j in sine function of Eq. (1) is due to the travel of the photoelectron from the absorbing atom to the neighbouring atom and back and δj(k) is an additional phase shift term. Lytle et al.7 in the general theory of EXAFS analysis assumed the linear form of δj(k) as δj(k) = -2kαj + 2βj …(2) where 2kαj is an absorbing atom phase shift and βj is a backscattering amplitude phase shift. We assume αj to be linear in k over the EXAFS energy range. The constants αj and βj are called bonding parameter and phase parameter, respectively. In the present paper, we have calculated the bonding parameter α1 and phase parameter β1 using a graphical method proposed by Sayer el al.7. This method has been used because of its simplicity and capability of giving good results and has also been used by many researchers14,15. We are also reporting the correlation of the bonding parameter with nearest neighbour distance and ionicity. The nearest neighbour distances have been calculated using the method proposed by Chetal et al16,17. Ionicity has been calculated using Pauling’s method18. The position of the nickel edge in the present systems has been correlated with the ionicity. SINGH: EXAFS PHASE SHIFT STUDIES OF NICKEL COMPOUNDS 2 Experimental Details A Cauchois type transmission X-ray spectrograph with diameter 40 cm was used to record K-absorption edge of Ni in the systems under study. X-ray radiation was obtained from tungsten tube operated at 13 kV and 10 mA. Mica with 2 01 planes was used for recording the X-ray spectra of the systems under study. Absorbing samples were prepared by spreading uniformly fine powder of the compounds between two cellophane tapes fixed on an aluminium frame. Microphotometer traces of the spectra were recorded using MD100 (Carl Zeiss, IRS) microphotometer. The error in the measurement of the positions of the maxima and minima in absorption spectra was of the order of ±1eV. The Ni K-edge found to split into two components K1 and K2 shown only for Ni metal in Fig. 1. The measurements of edges were made from the mid point of K1 component of the absorption edge. This point is considered to be as zero energy. 3 Results and Discussion The argument in the sinusoidal term given in Eq. (1) determines the periodicity of EXAFS arising from scattering from first co-ordination shell. From Eqs (1) and (2), we have, χ (k) = -1/k ∑Aj sin(2kR j -2kαj + 2βj) …(3) or, χ (k) = -1/k ∑Aj sin[2k(R j - αj) + 2βj] …(4) Lytle et al.7 have shown that EXAFS may be visualized as a kind of electron diffraction where the 21 source of electron originates from the atom involved in the absorbing event. The wave function of the excited photoelectron has interference between the outgoing and scattered part. The interference takes place near the origin where the overlap of the initial state occurs. Depending upon the wave number of the photoelectron, the interference is either constructive or destructive varying the dipole matrix element and hence the transition rates. Substituting into the argument of the sine function of the Eq. (4) and rearranging for the co-ordination shell, it is convenient to define n by φ1(k) = (n+1/2)π = 2k(R1 - α1)+ 2β1 …(5) where n = 0, 2, 4, ……. for the maxima and n = 1, 3, 5,……...for the minima The value of k (in Å-1) is obtained from equation k= 0.263E …(6) where, E is the energy of the peaks in EXAFS in eV. The microphotometer tracings between absorption coefficient and energy are shown in Figs 1 and 2. One can see from Eq. (5) that the value of bonding parameter (α1) and phase parameter (β1) can be determined provided we know the values of R1 and k. The value of k is determined using Eq. (6) and R1 is the crystallographic value of the nearest neighbour distance and has been calculated using the following formula developed by Mahto and Chetal16, Fig. 1 — Absorption coefficient versus energy of Ni metal Ni-As mineral, NiBr2, NiS mineral, NiS and NiCl2.6H2O INDIAN J PURE & APPL PHYS, VOL 44, JANUARY 2006 22 ⎛ π⎞ Ru = Rs + ⎜ ⎟ ⎝ 2⎠ 1/ 2 ⎡ 1 1 ⎤ − ⎢ ⎥ ⎣ Ku K s ⎦ …(7) where, Ru is the nearest neighbour distances of unknown systems, Rs, the nearest neighbour distance of standard system and K= 0.263( Er − Eb ) where, Er is the resonance energy corresponding to the peak A and Eb is the bound energy corresponding to the peak C as shown in Fig. (2) for NiSO4.6H2O. The values of Er and Eb are given in Table 1. The Ru values for the systems under study are calculated by using Eq. (7), which we shall call as R1, are given in Table 2. For calculating bonding parameter (α1) and phase parameter (β1), we have plotted φ1(k) versus k (not shown in the text). The slope of the plot is 2(R1 - α1). By substituting the values of R1 in (R1 - α1), the value of α1 of the systems under study can be calculated easily (error ± 0.01 Å). The intercept of the plot of φ1(k) and k gives 2β1 (error ± 0.01Å). The values so obtained for α1 and β1 for the systems under study are given in Table 2. From Table 2, it can be observed that as R1 decreases the value of α1 also decreases except in Ni3(PO4)2.XH2O and NiCl2.6H2O. The deviation may be attributed to the complex nature of the systems. The plot between the bonding parameter α1 and the nearest neighbour distance R1 is shown in Fig. 3. We have correlated α1 with the ionicity (I). The ionicity of the systems under study was calculated by using Pauling’s formula18 given below, ⎡ n ⎛ ( X − X a )2 ⎞ ⎤ I = ⎢1 − exp ⎜⎜ − l ⎟⎟ ⎥ 4 ⎝ ⎠ ⎦⎥ ⎣⎢ C …(8) where, Xl is the electronegativity of the ligand Xa, the electronegativity of the absorbing atom C, the Table 1 — Values of Er, resonance energy and Eb, the bound energy Sample Name of the systems No. Er (in eV) Eb (in eV) 1 NiAs-Mineral 8348.52 8332.62 2 NiBr2 8349.12 8332.62 3 NiS-Mineral 8350.62 8333.52 4 NiS compound 8350.52 8332.52 5 NiCl2.6H2O 8353.62 8334.72 6 NiO 8352.62 8334.72 7 Ni3(PO4) 2.XH2O 8353.12 8334.92 8 LaNiO3 8352.62 8334.32 9 NiCO3 8353.52 8334.82 10 Ni(NO3)2.6H2O 8355.62 8333.62 11 NiSO4.6H2O 8354.62 8332.52 Fig. 2 — Absorption coefficient versus energy of NiO, Ni3(PO4)2 xH2O, LaNiO3, NiCO3, Ni(NO3)2.6H2O and NiSO4.6H2O SINGH: EXAFS PHASE SHIFT STUDIES OF NICKEL COMPOUNDS coordination number and n is the valence of the absorbing atom. The ionicities of the systems under study calculated using Eq. (8) are given in Table 3. It can be seen from Fig. 4 that the parameter α1 decreases with the increase of ionicity of the corresponding system except for the system NiBr2. The values of phase parameter β1 in the systems under study are also given in Table 2. It can be observed from Table 2 that the Table 2 — Values of bonding parameter, nearest neighbour distance and the phase parameter for the systems under study Sample Name of the No. systems Bonding Nearest Phase parameter neighbour parameter α1 (in Å) distance β1 (in Å) R1 (in Å) 1 Ni-Metal 2.440 2.56* 0.52 2 NiAs-Mineral 2.170 2.29 0.33 3 NiBr2 2.160 2.28 0.27 4 NiS-Mineral 2.150 2.27 0.38 5 NiS compound 2.130 2.25 0.41 6 NiCl2.6H2O 2.080 2.24 0.17 7 NiO 1.990 2.09 8 Ni3(PO4) 2.XH2O 2.030 9 LaNiO3 10 23 greater the number of oxygen atoms in a system, the higher is the value for the phase parameter β1 except for the system NiCl2.6H2O. It is maximum for Ni3(PO4)2.XH2O. In the case of NiO, the value may be high due to the fact that the coordination number of Ni is six in NiO and hence Ni is surrounded by six oxygen atoms. In the case of NiCl2.6H2O, the effect of oxygen in NiCl2 perhaps is not felt as it belongs to 2nd coordination shell of water molecules. This work Table 3 — Ionicities of the systems under study Sample Name of the No. systems Ionicity Bonding parameter α1 (in Å) K-edge position (in eV) Author K-edge position (in eV) Choudhury17 1 NiAs-Mineral 0.67 2.170 8337.62 8333.70 2 NiS-Mineral 0.71 2.150 8338.62 8336.20 3 NiS compound 0.71 2.130 8340.22 8336.92 4 NiBr2 0.74 2.160 8336.82 8334.62 5 NiCl2.6H2O 0.77 2.080 8342.32 8339.52 0.68 6 Ni3(PO4) 2.XH2O 0.79 2.030 8342.92 8339.62 2.08 1.60 7 NiCO3 0.80 1.960 8341.90 8338.60 1.960 2.08 0.52 8 NiSO4.6H2O 0.81 1.917 8340.50 8339.60 NiCO3 1.960 2.07 0.53 9 Ni(NO3)2.6H2O 0.82 1.919 8342.80 8340.80 11 Ni(NO3)2.6H2O 1.919 2.03 0.63 10 NiO 0.84 1.990 8341.42 8338.32 12 NiSO4.6H2O 1.917 2.03 0.55 11 LaNiO3 0.87 1.960 8342.76 8342.62 * Crystallographic value Fig. 3 — Bonding Parameter versus nearest neighbour distance (in Å each) Fig. 4 — Bonding parameter (in Å) versuss ionicity 24 INDIAN J PURE & APPL PHYS, VOL 44, JANUARY 2006 further suggests that for arsenic, sulphur, chlorine and bromine the phase parameter β1 is less than that for oxygen atoms. The position of nickel K-edge has been studied in the systems under study. The K-edge position of nickel and corresponding ionicity are given in Table 3. We have also given the measurements of the edges carried out by Choudhury17. It can be seen from the Table 3 that as ionicity increases K-edge position also increases in the systems NiAs mineral, NiS, NiS mineral, NiSO4.6H2O, NiO and LaNiO3. However, no correlation has been observed in NiCl2.6H2O, NiBr2, Ni3(PO4)2. XH2O, NiCO3 and Ni(NO3)2.6H2O. This is due to fact that the shift of the edge does not only depend upon ionicity but also on other factors20 such as coordination number, crystal structure, valency etc. Some time X-ray scattering also affects the edge position. 4 Conclusion We conclude that the EXAFS parameters α1 and β1 can be considered as chemical parameters as they depend upon chemical parameters such as ionicity, nature of the ligand and nearest neighbour diatance etc. Acknowledgement Author is grateful to Prof A R Chetal for his constant encouragement and guidance. References 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 Rehr J J & Albers R C, Rev Mod Phys, 72 (2000) 621. R K Katare, Joshi S K, Srivastava B D, Patel R N & Mishra A, Indian J Pure& Appl Phys, 40 (2002) 908. Mishra A, Mahajan M & Johar K K, Indian J Pure & Appl Phys, 41 (2003) 232. Kronig R, Z Phys, 70 (1931) 317. Kronig R, Z Phys, 75 (1932) 468. Sayers D E, Stern E A & Lytle F W, Phys Rev Lett, 27 (1971) 1204. Stern E A, Sayers D E & Lytle F W, Phys Rev B, 11 (1975) 4825. Lee P A & Pendry J B, Phy Rev B, 11 (1975) 2795. Ashley C A & Doniac S, Phys Rev B, 11 (1975) 1279. Rehr J J et al., Phys Rev B, 44 (1991) 4146. Rehr J J et al., J Phys IV Collaq, 7 (1997) 229. Bunker B A & Stern E A, Phys Rev B, 27 (1983) 889. Murari A & Chetal A R, Phys Scripta, 50 (1994) 423. Mahto P & Chetal A R, Physica B, 158 (1989) 415. Singh V K & Chetal A R, X-ray Spectrometry, 22 (1993) 86. Pauling L, The nature of the chemical bond, (Cornell Univ Press, New York) (1960) 162. Choudhury P K, Ph. D. thesis, I S M Dhanbad (1989). Singh V K, Chetal A R & Sarode P R, Acta Physica Polonica A 6,87 (1995) 1003.
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