Spin-density enhancement in a 119 Sn implanted 110Cr single crystal as evidenced by Mo ¨ ssbauer spectroscopy S. M. Dubiel,* J. Cies ´ lak, and J. Z ˙ ukrowski Faculty of Physics and Nuclear Techniques, The University of Mining and Metallurgy (AGH), aleja Mickiewicza 30, PL-30-059 Krako ´w, Poland H. Reuther Institut fuer Ionenstrahlphysik und Materialforschung, Forschungszentrum Rossendorf, Postfach 510119, D-01314 Dresden, Germany Received 22 November 2000; published 19 January 2001 Magnetic properties of a presurface zone of the bulk, single-crystal 110Cr, implanted with 119 Sn ions were studied by means of conversion electron Mo ¨ssbauer spectroscopy. A strong enhancement of the magnetic hyperfine field, B, was found. The increase is by a factor of 2.7 in the average value of B and by a factor of 2.3 in the most probable value of B the amplitude of the spin-density waves, SDW’s. The observed effects are explained in terms of the interference of two spin-density waves having the same amplitude phase but various polarizations. The relative contributions of the interfering SDW’s was estimated as equal to 60% for those with mutual perpendicular and 40% for those with mutual parallel polarization. DOI: 10.1103/PhysRevB.63.060406 PACS numbers: 75.30.Fv, 75.50.Ee, 76.80.+y The antiferromagnetism of metallic chromium has been attracting great scientific interest since the discovery that it is constituted by incommensurate spin-density waves I-SDW’s. 1–3 The importance of SDW’s stems mainly from the fact that they are related to the density of electrons at the Fermi surface and its topology. SDW’s set in as linearly polarized I-SDW structure at the Ne ´ el temperature which for bulk chromium is equal to 313 K. 4 The structure consists of a sinusoidal modulation of the magnetic moments, : r = 0 sinQ r , 1 where r is the position vector, 0 is the amplitude of the SDW equal to 0.6 B at 4.2 K Ref. 5and Q is the wave vector, given by: Q =2 / a -2 / 001, 2 where a is the lattice constant and is the periodicity of the SDW’s. The latter is a continuous function of temperature with a value of 7.8 nm at RT. SDW’s can exist along any of the 001crystallographic axes, i.e., three different do- mains can coexist in an equilibrium state so-called 3 Q state. The SDW’s are polarized transversely TSDW’s down to the temperature of 123 K where the polarization changes to longitudinal LSDW’s. The transition, known as the spin-flip, is a first-order one with a wide hysteresis. 6 Theoretical calculations predict that the surface properties of chromium are different. In particular, the magnetic mo- ment should be enhanced in comparison to its bulk value. According to the tight binding calculations of Allan, the 001Cr surface has a moment of 2.8 B . 7 Self-consistent tight-binding calculations by Victora and Falicov predict the value of 3 B Ref. 8whereas ab initio full-potential linear- ized augmented-plane-wave FLAPWcalculations by Fu and Freeman give the value of 2.5 B for the top layer of bulk chromium. 9 Enhanced magnetic moment was also pre- dicted for a 001Cr monolayer on substrates other than Cr, 10,11 as well as for Cr monolayers sandwiched between Fe on one side and a vacuum on the other. 12 Experimental evidence in favor of such enhancement was recently obtained from studying epitaxial Cr/Sn multilayers by 119 Sn Mo ¨ ssbauer spectroscopy. 13 The authors found a magnetic hyperfine hffield of 1113 T which is twice as much as in a single-crystal bulk Cr. 14 However, there is still no evidence that such enhancement exists on the surface or in the presurface zone of bulk Cr. To obtain this kind of information 100 m thick foil of a single-crystal 110Cr was implanted at 65 keV with the dose of 10 16 119 Sn ions per cm 2 . According to the TRIM code the mean projected range for the ions is 15.6 nm with a longitudinal straggling of 5.8 nm. This corresponds to 2 at RT. As a reference sample, a 100 m thick single-crystal 110Cr foil doped with 0.1 at. % 119 Sn by diffusion was used. Two Mo ¨ ssbauer spectra were recorded at RT on this sample: one in the transmission mode using a standard spec- trometer and a scintillation detector for the -rays supplied by a Ca 119m SnO 3 source, and another one in conversion elec- trons mode CEMSusing a gas-flow detector. The spectra, which were fitted in terms of the hf field distribution method described in details elsewhere, 15 assuming the value of 1.0 mm/s for the full linewidth at half maximum FWHM. The line intensities ratio was fixed at the value of 3:2:1 for the spectrum recorded in the transmission mode and at 3:4:1 for those recorded in the CEMS mode. The corresponding his- tograms of the hf field distribution, P ( B ), can be seen in Fig. 1. As can be noticed there is some small difference in the shape of the two spectra. The one recorded in the transmis- sion mode is characteristic of the I-SDW structure; 14 it is symmetric and has a well-defined dip in the central part. On the other hand, the spectrum obtained in the CEMS mode is RAPID COMMUNICATIONS PHYSICAL REVIEW B, VOLUME 63, 060406R 0163-1829/2001/636/0604064/$15.00 ©2001 The American Physical Society 63 060406-1