APPLIED PHYSICS LETTERS 88, 182504 共2006兲 Quasiferromagnetism in semiconductors T. Dubroca, J. Hack, and R. E. Hummela兲 Department of Materials Science and Engineering, University of Florida, Rhines Hall room 106, Gainesville, Florida 32611 A. Angerhofer Department of Chemistry, University of Florida, P.O. Box 117200, Gainesville, Florida 32611 共Received 20 January 2006; accepted 26 March 2006; published online 4 May 2006兲 Ferromagnetic hysteresis has been observed at room temperature in materials not consisting of elements commonly associated with ferromagnetism, such as Co, Ni, Fe, or Mn-containing alloys. In particular, we report on magnetic hysteresis seen in silicon prepared by two different techniques: ion implantation 共Si and Ar兲 and neutron irradiation. Because the material investigated contains no ferromagnetic elements, we tentatively call it “quasiferromagnetic.” The paramagnetic defects present in these materials were investigated using electron paramagnetic resonance. We suggest that these defects are one of the factors responsible for the observed macroscopic magnetic hysteresis loop. © 2006 American Institute of Physics. 关DOI: 10.1063/1.2198483兴 Spin-transport electronics 共“spintronics”兲 is an evolving device technology that functions using electron spins, either alone or in conjunction with electron charge. Our research focuses on understanding how certain semiconductors 共i.e., silicon, implanted with either silicon or argon ions or neutron irradiated兲 causes a ferromagneticlike hysteresis loop. Other investigators have speculated about the possibility of ferromagnetism in argon and neon implanted silicon or vapor-deposited amorphous Si but did not present a magnetic hysteresis loop.1,2 Their conclusions were based on electron paramagnetic resonance 共EPR兲 experiments yielding a g factor of 2.0055 which was interpreted as stemming from paramagnetic centers having a concentration between 1020 / cm3 and 1021 / cm3. Other investigators3–5 implanted manganese up to 23% into Si and observed a ferromagnetic hysteresis loop, which was interpreted to originate from the Mn d-shell electrons. Finally, our group and Laiho et al. observed ferromagnetic hysteresis in spark-processed Si 共Ref. 6兲 or anodically etched porous Si,7 respectively. In our current work, p-type silicon wafers having a resistivity of 3 – 5 ⍀ cm were implanted by silicon or argon ions using an energy of 50 keV, while the current density was kept at less than 10 A / cm2. The sample stage was water cooled throughout the implantation to diminish recrystallization. Another Si sample was neutron irradiated in a thermal neutron reactor with a dose of 4 ⫻ 1016 cm−2. Measurements of magnetization as a function of the applied magnetic field were conducted at various temperatures using a commercial superconducting quantum interference device 共SQUID兲 magnetometer. Figure 1 shows the magnetization response of Si implanted into silicon at doses of 1 ⫻ 1016 cm−2 共1A兲 and 5 ⫻ 1016 cm−2 共1B兲, respectively, measured at room temperature, while an insert shows the magnetization response of sample 1B at 10 K. An unprocessed silicon wafer was also measured 共not shown兲, and its known diamagnetic response was confirmed. These samples display magnetic hysteresis loops having a coercive field of 100 Oe, saturation fields of 600 Oe 共1A兲 and 700 Oe 共1B兲, and remanences of a兲 Electronic mail: [email protected]fl.edu 0.10 emu/ cm−3 共1A兲 and 0.11 emu/ cm−3 共1B兲, respectively. The comparison suggests that the magnetic response 共defined as the area within the hysteresis loop兲 may be increased by increasing the implantation dose. The insert of Fig. 1 shows that essentially the same magnetic behavior is observed when sample 1B is measured at 10 K. Figure 2 depicts the magnetization response of samples 2A and 2B, which were implanted with argon at doses of 2 ⫻ 1016 and 2 ⫻ 1017 cm−2, respectively, measured at room temperature. Sample 2A displays a magnetic hysteresis loop with a coercive field of 100 Oe, saturation field of 600 Oe, and a remanence of 0.3 emu/ cm3. Sample 2B displays a magnetic hysteresis loop with a coercive field of 100 Oe, a saturation field of 600 Oe, and a remanence of 0.4 emu/ cm3. Similar to Si into Si, a higher implantation concentration of Ar yields a larger magnetic response. Moreover, it is noted that implantation of argon into silicon causes a larger magnetic response than for Si into Si at a similar dose. Figure 3 depicts the magnetization response at 10 K of silicon irradiated by neutrons at a dose of 4 ⫻ 1016 cm−2. The magnetization response of the neutron-irradiated sample was FIG. 1. Magnetization vs magnetic field for sample 1A 共Si implanted into Si at 1016 cm−2 dose, solid line兲 and sample 1B 共Si implanted into Si at 5 ⫻ 1016 cm−2 dose with an energy of 50 keV, dashed line兲 measured and implanted at room temperature. Insert: magnetization vs magnetic field for sample 1B at 10 K. 0003-6951/2006/88共18兲/182504/3/$23.00 88, 182504-1 © 2006 American Institute of Physics Downloaded 25 Feb 2008 to 146.139.50.23. Redistribution subject to AIP license or copyright; see http://apl.aip.org/apl/copyright.jsp 182504-2 Dubroca et al. FIG. 2. Magnetization vs magnetic field for sample 2A 共Ar implanted into Si at 2 ⫻ 1016 cm−2 dose, solid line兲 and sample 2B 共Ar implanted into Si at 2 ⫻ 1017 cm−2 dose with an energy of 50 keV, dashed line兲 measured and implanted at room temperature. significantly weaker than that for either Si into Si or Ar into Si. Secondary ion mass spectroscopy 共SIMS兲 reveals the presence of silicon, oxygen, boron, and hydrocarbons 共results not shown for brevity兲. No other elements were observed within the detection limit. In particular, no iron 共limit at 0.02 ppm兲 was detected. This excludes the possibility that Fe is a contributing factor for the observed hysteresis loop. It is suggested instead that the large quantities of paramagnetic impurities should interact and produce hysteresis if not coherent ferromagnetism. Figure 4 shows an EPR spectrum of sample 1A measured at room temperature. Also included is a curve showing the sum of two model-generated Lorentzian lines, which displays the spectrum of an unprocessed silicon wafer, which shows no evidence of unpaired spins. The modeled line closely matches our data, with a correlation coefficient of 0.97. It is known that each Lorentzian line corresponds to the resonance of a single type of dangling bond. In contrast, a non-Lorentzian, such as a Gaussian line 共which is the sum of Lorentzian lines兲, corresponds to a distribution of dissimilar dangling bonds with slightly different g factors. Therefore, we conclude that the EPR signal of sample 1A results from two types of dangling bonds. The first Lorenzian line has a peak that yields a g factor of 2.0054, which has been attributed to a silicon dangling Appl. Phys. Lett. 88, 182504 共2006兲 FIG. 4. EPR spectrum of sample 1A 共Si implanted into Si at 1016 cm−2, square dots兲, its model using the sum of two Lorentzian lines’ first derivative 共solid line兲 and spectrum of an unprocessed silicon 共round dots scattered around zero兲. bond back-boned by three silicon atoms,8 consistent with Refs. 1, 2, and 7. The second Lorenzian line has a peak that yields a g factor of 2.0023. According to Tomozeiu et al.,9 this peak can be attributed to E⬘ centers typically present in SiO2. In our case, a small but measurable amount of oxygen is present, as determined by the SIMS analysis. A common feature of our quasiferromagnetic materials is the presence of a large number of paramagnetic centers 共i.e., unpaired spins兲. In addition, the EPR spectrum for ion implanted Si is strikingly similar to the EPR spectrum for spark-processed Si 共sp-Si兲, for which it was postulated that the ferromagnetic hysteresis loop originates from dangling bonds.6 It was shown that annealing sp-Si removes, in an irreversible manner, the ferromagnetic behavior while, at the same time, dramatically reducing the number of dangling bonds.6 It is therefore suggested that dangling bonds substantially contribute to the ferromagnetic behavior in the presently investigated quasiferromagnetic materials. It is further suggested that the unpaired spins of the dangling bonds interact to yield the quasiferromagnetic behavior in the currently investigated materials. The interaction that makes the exchange integral between the dangling bond wave functions positive can be described in at least two different ways. First, the distance between the dangling bonds may be large enough to avoid the formation of a covalent bond. At the same time, the distance may be small enough to permit the direct overlap of the wave functions of the two electrons. As such, the triplet state may be the most stable state, therefore inducing a positive exchange interaction at the electronic level. The second possibility is an indirect coupling of spins. For example, Talapatra et al.10 suggested that the ferromagnetic hysteresis loop observed for carbon nanostructures implanted with nitrogen requires not only unpaired spins but also double bonds. This would permit a delocalization of the electrons and would create a mediated pathway for an indirect exchange interaction between unpaired electrons. Similarities between Si and C allow us to propose that an equivalent mechanism may be possible for Si. At present, neither a direct nor an indirect exchange coupling between dangling bonds is ruled out. An analysis that connects our observations with the density of paramagnetic defects utilizing pulsed EPR and ENDOR is currently in progress. 1 A. F. Khokhlov and P. V. Pavlov, JETP Lett. 24, 211 共1976兲; Pis’ma Zh. Eksp. Teor. Fiz. 24, 238 共1976兲. FIG. 3. Magnetization vs magnetic field for sample 3 共silicon irradiated at a 2 T. R. Askew, H. J. Stapleton, and K. L. Brower, Phys. Rev. B 33, 7 dose of 4 ⫻ 1016 cm−2 with thermal neutrons兲 measured at 10 K. Downloaded 25 Feb 2008 to 146.139.50.23. Redistribution subject to AIP license or copyright; see http://apl.aip.org/apl/copyright.jsp 182504-3 共1986兲. F. M. Zhang, Y. Zeng, J. Gao, X. C. Liu, X. S. Wu, and Y. W. Du, J. Magn. Magn. Mater. 282, 216 共2004兲. 4 L. Liu, N. Chen, S. Song, Z. Yin, F. Yang, C. Chai, S. Yang, and Z. Liu, J. Cryst. Growth 273, 458 共2005兲. 5 M. Bolduc, C. Awo-Affouda, A. Stollenwerk, M. B. Huang, F. G. Ramos, G. Agnello, and V. P. Labella, Phys. Rev. B 71, 033302 共2005兲. 6 J. Hack, M. H. Ludwig, W. Geerts, and R. E. Hummel, Mater. Res. Soc. Symp. Proc. 452, 147 共1997兲. 3 Appl. Phys. Lett. 88, 182504 共2006兲 Dubroca et al. 7 R. Laiho, E. Lahderanta, L. Vlasenko, M. Vlasenko, and M. Afanasiev, J. Lumin. 57, 197 共1993兲. 8 W. L. Warren, E. H. Pointdexter, M. Offenberg, and W. Muller-Warmuth, J. Electrochem. Soc. 139, 872 共1992兲. 9 N. Tomozeiu, E. E. van Faassen, W. M. Arnoldbik, A. M. Vredenberg, and F. H. P. M. Habraken, Thin Solid Films 420–421, 382 共2002兲. 10 S. Talapatra, P. G. Ganesan, T. Kim, R. Vajtai, M. Huang, M. Shima, G. Ramanath, D. Srivastava, S. C. Deevi, and P. M. Ajayan, Phys. Rev. Lett. 95, 097201 共2005兲. Downloaded 25 Feb 2008 to 146.139.50.23. Redistribution subject to AIP license or copyright; see http://apl.aip.org/apl/copyright.jsp
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