PHYSICAL REVIEW B, VOLUME 63, 073109

K ␤ -to-K ␣ x-ray intensity ratio studies of the valence electronic structure of Fe and Ni in Fex Ni1Àx alloys S. Raj and H. C. Padhi Institute of Physics, Bhubaneswar 751005, India

M. Polasik and F. Pawłowski Faculty of Chemistry, Nicholas Copernicus University, 87-100 Torun´, Poland

D. K. Basa Department of Physics, Utkal University, Bhubaneswar 751004, India 共Received 28 June 2000; revised manuscript received 19 September 2000; published 31 January 2001兲 K ␤ -to-K ␣ x-ray intensity ratios of Fe and Ni in pure metals and in Fex Ni1⫺x alloys (x⫽0.20, 0.50, 0.58兲 exhibiting similar crystalline structure have been measured following excitation by 59.54 keV ␥ rays from a 200 mCi 241Am point source to understand why the properties of the Fex Ni1⫺x (x⫽0.2) alloy are distinct from other alloy compositions. The valence electronic structure of Fe and Ni in the samples has been evaluated by comparing the measured K ␤ -to-K ␣ intensity ratios with the results of multiconfiguration Dirac-Fock calculations. Significant changes in the 3d electron population 共with respect to the pure metal兲 are observed for Fe and Ni for certain alloy compositions. These changes can be explained by assuming rearrangement of electrons between 3d and (4s,4p) band states of the individual metal atoms. It has been found that the valence electronic structure of the Fe0.2Ni0.8 alloy is totally different from the other two alloys, which perhaps is connected to the special magnetic properties of this alloy. DOI: 10.1103/PhysRevB.63.073109

PACS number共s兲: 78.70.En, 32.30.Rj, 32.70.Fw

Fex Ni1⫺x alloys play an important role in fundamental and applied research due to the rapid advance of magnetoelectronics.1 Although the Fex Ni1⫺x alloy crystallizes in the same ␥ 共fcc兲 phase for all the compositions (x ⫽0.2, 0.5, and 0.58兲 reported here, Permalloy, a member of the family of Fex Ni1⫺x alloys 共with x⫽0.2), has some distinct physical properties of vanishingly small magnetostriction, low coercivity, and high permeability, which makes it the material of choice for magnetic recording media, sensors, and nonvolatile magnetic random access memory. The electronic density of states for 4s and 3d electrons at the Fermi surface plays a significant role for a quantitative understanding of the phenomenon of transport spin polarization.2 It is therefore very important to have a detailed knowledge of the valence electronic structure of Fe and Ni in the Fex Ni1⫺x alloys. The K ␤ -to-K ␣ x-ray intensity ratio has been reported3–21 to be a sensitive physical parameter to investigate the changes in the valence electronic structure of 3d transition metals.3 It has been found for various alloys18–21 that the change of the alloy composition may cause a change in the 3d electron population of both transition metals in the alloy, what must result in a change of the K ␤ -to-K ␣ intensity ratio of these metals 共because the change of the 3d electron population modifies the 3p orbitals more than the 2p orbitals21兲. In this paper we present the results of our study on the valence electronic structure of Fe and Ni in Fex Ni1⫺x alloys for various compositions (x⫽0.2, 0.5, and 0.58兲, exhibiting similar crystalline structure to understand why the physical properties of Fe0.2Ni0.8 alloy are drastically different from the other alloy compositions. We have used our experimental 0163-1829/2001/63共7兲/073109共4兲/$15.00

information on the valence electronic structure of both metals in the alloys to estimate the average number of 3d electrons and average number of (4s,4p) electrons of Fe and Ni. The measurements were carried out using high-purity alloys 共in powder form兲 procured from Alpha, a Johonson Mathey Company, U.K. The powder material is pelletized into the size of 10 mm diam ⫻ 3 mm thick for final use in the experiments. The experiments were performed using 59.54 keV ␥ rays from a 200 mCi 241Am point source that ionize the target atoms. The emitted x-rays were detected by a 30 mm2 ⫻3 thick Canberra Si共Li兲 detector having a 12.7 ␮ m thick beryllium window. The resolution of the Si共Li兲 detector was ⬃165 eV 关full width at half maximum 共FWHM兲兴 for a 5.9 keV x-ray peak. Pulses from the Si共Li兲 detector preamplifier were fed to an ORTEC-572 spectroscopy amplifier and then recorded in a Canberra PC based Model S-100 multichannel analyzer. The gain of the system was maintained at ⬃16 eV/channel. All the x-ray spectra were carefully analyzed with the help of a multi-Gaussian least-square fitting program22 using a nonlinear background subtraction. No low-energy tail was included in the fitting as its contribution to the ratio was shown to be quite small23. A typical K x-ray spectrum of Fex Ni1⫺x alloy corresponding to the alloy composition x ⫽0.5 is shown in Fig. 1. The K ␤ -to-K ␣ intensity ratios were determined from the fitted peak areas after applying necessary corrections to the measured data. Details regarding the experimental arrangement as well as data analysis have been reported elsewhere.18,23–26 The experimental results for the K ␤ -to-K ␣ x-ray intensity ratios of Fe and Ni in pure metals and in the Fex Ni1⫺x alloys

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©2001 The American Physical Society

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PHYSICAL REVIEW B 63 073109 TABLE II. Evaluated 3d-electron population values and total number of (4s,4p) electrons for Fe and Ni in various samples.

FIG. 1. A typical K x-ray spectrum of a Fex Ni1⫺x alloy corresponding to the alloy composition x⫽0.5. In the figure 䊊 corresponds to the experimental data, the dotted line corresponds to the fitted data, and the dashed line corresponds to the fitted background.

(x⫽0.2, 0.5, and 0.58兲 before and after corrections are presented in Table I. The errors quoted in the table are statistical only. It can be found from Table I that for all the alloy compositions the K ␤ -to-K ␣ ratios for Ni are significantly different from those of pure Ni, whereas the K ␤ -to-K ␣ ratios of Fe differ slightly from those of pure Fe. For the alloy composition x⫽0.2 the K ␤ -to-K ␣ ratio of Ni is much lower than that of pure Ni, whereas for Fe the K ␤ -to-K ␣ ratio is found to be higher than that of pure Fe. For the other two alloy compositions the K ␤ -to-K ␣ ratios of Ni are higher than those of pure Ni and for Fe they are closer to those of pure Fe. The 3d electron populations of Fe and Ni for various samples are presented in Table II. They have been evaluated by comparing the experimental values of the K ␤ -to-K ␣ intensity ratio with the results of multiconfigurational Dirac-

Kind of sample

Evaluated 3d-electron population for Fe

Total number of (4s,4p) electrons for Fe

Evaluated 3d-electron population for Ni

Total number of (4s,4p) electrons for Ni

pure Fe pure Ni Fe0.2Ni0.8 Fe0.5Ni0.5 Fe0.58Ni0.42

7.39⫾0.29 — 6.69⫾0.26 6.86⫾0.24 7.31⫾0.24

0.61⫾0.29 — 1.31⫾0.26 1.14⫾0.24 0.69⫾0.24

— 8.54⫾0.39 9.93⫾0.52 7.81⫾0.21 7.44⫾0.19

— 1.46⫾0.39 0.07⫾0.52 2.19⫾0.21 2.56⫾0.19

Fock 共MCDF兲 calculations27–29 performed for various valence electronic configurations3 of Fe and Ni. The obtained 3d electron populations for pure Fe and Ni metals 共Table II兲 are in close agreement with the results of band structure calculations of Papaconstantopoulos30 共6.93 for Fe and 8.97 for Ni兲 and Hodges et al.31 共8.82 for Ni兲. Comparison of the changes in the 3d-electron population of Fe in the Fex Ni1⫺x alloys 共with respect to pure Fe兲 with the corresponding changes for Ni indicates that these changes cannot be explained by assuming the transfer of 3d electrons from atoms of one element 共Fe or Ni兲 to atoms of the other element. However, the changes for all the alloys can easily be explained by the rearrangement of electrons between 3d and (4s,4p) band states of individual metal atoms. The approximate numbers of (4s,4p) electrons 共per one atom兲 for pure Fe and Ni have been obtained by subtracting from the total number of valence electrons of the neutral atom 共eight for Fe and ten for Ni兲 the number of 3d electrons in the pure metal from Table II (7.39⫾0.29 for Fe and 8.54⫾0.39 for Ni兲. In the case of the Fex Ni1⫺x alloys it is also possible to estimate 共in the way described above兲 the approximate numbers of (4s,4p) electrons per one atom separetly for Fe and Ni in a given alloy 共see third and fifth columns of Table II, respectively兲. Trying to answer the question why the physical properties of Fe0.2Ni0.8 alloy are distinct as compared to the other two alloys, we calculated the weighted average numbers of 3d electrons per one atom for all the Fex Ni1⫺x alloys presently studied 共the second column of Table III兲. We took in this average the numbers of 3d electrons evaluated separately for

TABLE I. Experimental K ␤ -to-K ␣ x-ray intensity ratios for Fe and Ni in Fex Ni1⫺x alloys.

Composition (x) 0 0.2 0.5 0.58 1.0

K ␤ -to-K ␣ ratio of Fe Before After correction correction — 0.1737⫾0.0010 0.1743⫾0.0009 0.1726⫾0.0008 0.1764⫾0.0009

— 0.1326⫾0.0008 0.1321⫾0.0007 0.1309⫾0.0006 0.1307⫾0.0007

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K ␤ -to-K ␣ ratio of Ni Before After correction correction 0.1808⫾0.0016 0.1723⫾0.0010 0.1808⫾0.0010 0.1822⫾0.0010 —

0.1346⫾0.0012 0.1314⫾0.0008 0.1371⫾0.0008 0.1386⫾0.0008 —

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PHYSICAL REVIEW B 63 073109

TABLE III. Comparison of estimated weighted average number of 3d and (4s,4p) electrons for various Fex Ni1⫺x alloys with the superposition values of 3d and (4s,4p) electrons obtained from the pure metal values.

Kind of sample Fe0.2Ni0.8 Fe0.5Ni0.5 Fe0.58Ni0.42

Weighted average number of 3d electrons 9.28⫾0.42 7.34⫾0.16 7.36⫾0.16

Superposition of 3d electrons obtained from pure metal values 8.31⫾0.32 7.97⫾0.24 7.87⫾0.24

Fe and Ni in a given alloy 共from Table II兲 with the weights equal to x and 1⫺x, respectively. Similarly, we evaluated the weighted average number of the (4s,4p) electrons per one atom for the examined alloys 共the fourth column of Table III兲. It can be seen from the second 共and the fourth兲 column of Table III that in the case of Fe0.2Ni0.8 alloy the weighted average number of 3d electrons is considerably larger 关and the weighted average number of (4s,4p) electrons is much smaller兴 than in the case of other two alloys. Accordingly, it is very important to find out the cause of this considerable difference of the valence electronic structure of Fe0.2Ni0.8 alloy with respect to the other two alloys. One reason that can be ascribed to the drastically different valence electronic structure of the Fe0.2Ni0.8 alloy from the other two alloys is that this is a highly asymmetric alloy with a higher concentration of nickel atoms. It is also interesting to find to what extent the valence electronic structure of the Fex Ni1⫺x alloy 共of certain composition x) differs from a superposition of the valence electronic structure of pure Fe and Ni metals. Therefore, in the third and the fifth columns of Table III we have additionally presented for every alloy composition x the superposition 共with the weights x for Fe and 1⫺x for Ni兲 of the number of 3d and (4s,4p) electrons taken from Table II for pure Fe

G. A. Prinz, Phys. Today 48 共4兲, 55 共1995兲; Science 282, 1660 共1998兲. 2 B. Nadgorny, R. J. Soulen, Jr., M. S. Osofsky, I. I. Magin, G. Laprade, R. J. M. Van de Veerdonk, A. A. Smits, S. F. Chen, E. F. Skelton, and S. B. Qadri, Phys. Rev. B 61, R3788 共2000兲, and references therein. 3 M. Polasik, Phys. Rev. A 58, 1840 共1998兲. 4 E. Lazzarini, A. L. Lazzarini-Fantola, and M. Mandelli Battoni, Radiochim. Acta 25, 21 共1978兲. 5 Y. Tamakai, T. Omori, and T. Shiokawa, Radiochem. Radioanal. Lett. 37, 39 共1979兲. 6 G. Brunner, M. Nagel, E. Hartmann, and E. Arndt, J. Phys. B 15, 4517 共1982兲. 7 T. Mukoyama, K. Taniguchi, and H. Adachi, Phys. Rev. B 34, 3710 共1986兲. 8 A. Kuckukonder, Y. Sahin, E. Buyyukkasap, and A. Kopya, J. Phys. B 26, 101 共1993兲. 1

Weighted average number of (4s,4p) electrons 0.32⫾0.42 1.66⫾0.16 1.48⫾0.16

Superposition of (4s,4p) electrons from pure metal values 1.29⫾0.32 1.03⫾0.24 0.97⫾0.24

and Ni metals. It can be seen from Table III that in the case of x⫽0.5 and 0.58 the weighted average numbers of 3d electrons in the Fex Ni1⫺x alloys 共the second column of Table III兲 are smaller than the superpositions of the number of 3d electrons of pure Fe and Ni metals 共the third column of Table III兲. However, in the case of the Fe0.2Ni0.8 alloy the weighted average number of 3d electrons is very large (9.28⫾0.42) and differs considerably from the superposition of the number of 3d electrons of pure Fe and Ni metals (8.31⫾0.32). In the case of (4s,4p) electrons the situation is opposite, i.e., the weighted average number of (4s,4p) electrons for the Fe0.2Ni0.8 alloy (0.32⫾0.42) is dramatically smaller than the superposition value (1.29⫾0.32), whereas for the other two alloys the weighted average is higher than the superposition value. The large weighted average number of 3d electrons (9.28⫾0.42) and the negligible weighted average number of (4s,4p) electrons (0.32⫾0.42) in the case of the Fe0.2Ni0.8 alloy may possibly be the reason for the high permeability and other magnetic properties of this alloy. H.C.P. and S.R. acknowledge the financial support of Council of Scientific and Industrial Research, India. This work was also partly supported by the Polish Committee for Scientific Research 共KBN兲, Grant No. 2P03B01916.

9

H. C. Padhi, C. R. Bhuinya, and B. B. Dhal, J. Phys. B 26, 4465 共1993兲. 10 C. N. Chang, S. K. Chiou, and C. L. Luo, Solid State Commun. 87, 987 共1993兲. 11 C. N. Chang, C. Chen, C. C. Yen, Y. H. Wu, C. W. Wu, and S. K. Choi, J. Phys. B 27, 5251 共1994兲. 12 E. Arndt, G. Brunner, and E. Hartmann, J. Phys. B 15, L887 共1982兲. 13 S. Raj, B. B. Dhal, H. C. Padhi, and M. Polasik, Phys. Rev. B 58, 9025 共1998兲. 14 S. Raj, H. C. Padhi, and M. Polasik, Nucl. Instrum. Methods Phys. Res. B 145, 485 共1998兲. 15 S. Raj, H. C. Padhi, M. Polasik, and D. K. Basa, Solid State Commun. 110, 275 共1999兲. 16 S. Raj, H. C. Padhi, D. K. Basa, M. Polasik, and F. Pawl”owski, Nucl. Instrum. Methods Phys. Res. B 152, 417 共1999兲. 17 S. Raj, H. C. Padhi, and M. Polasik, Nucl. Instrum. Methods Phys. Res. B 160, 443 共2000兲.

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C. R. Bhuinya and H. C. Padhi, J. Phys. B 25, 5283 共1992兲. C. R. Bhuinya and H. C. Padhi, Phys. Rev. A 47, 4885 共1993兲. 20 H. C. Padhi and B. B. Dhal, Solid State Commun. 96, 171 共1995兲. 21 S. Raj, H. C. Padhi, and M. Polasik, Nucl. Instrum. Methods Phys. Res. B 155, 143 共1999兲. 22 Computer code NSCSORT 共unpublished兲 23 V. W. Slivniski and P. J. Ebert, Phys. Rev. A 5, 1681 共1971兲. 24 B. B. Dhal, T. Nandi, and H. C. Padhi, Nucl. Instrum. Methods Phys. Res. B 101, 327 共1995兲. 25 M. J. Berger and J. H. Hubbel, XCOM programme, Center for Radition Research, National Bureau of Standards, Gaithersburg, 18 19

MD20899 共unpublished兲. J. H. Hubbel 共unpublished兲. 27 I. P. Grant, B. J. McKenzie, P. H. Norrington, D. F. Mayers, and N. C. Pyper, Comput. Phys. Commun. 21, 207 共1980兲. 28 B. J. McKenzie, I. P. Grant, and P. H. Norrington, Comput. Phys. Commun. 21, 233 共1980兲. 29 I. P. Grant, J. Phys. B 7, 1458 共1974兲. 30 D. A. Papaconstantopoulos, Handbook of Band Structure of Elemental Solids 共Plenum, New York, 1986兲. 31 L. Hodges and H. Eherenreich, N. D. Lang, Phys. Rev. 152, 505 共1966兲. 26

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Significant changes in the 3d electron population (with respect to the pure metal) are observed ... experimental arrangement as well as data analysis have been.

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