<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">WJCMP</journal-id><journal-title-group><journal-title>World Journal of Condensed Matter Physics</journal-title></journal-title-group><issn pub-type="epub">2160-6919</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/wjcmp.2013.31015</article-id><article-id pub-id-type="publisher-id">WJCMP-28346</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  Mathematical Modelling of Bloch NMR to Explain the Rashba Energy Features
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>oses</surname><given-names>E. Emetere</given-names></name><xref ref-type="aff" rid="aff1"><sub>1</sub></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff1"><label>1</label><addr-line>Department of Physics, Federal University of Technology Minna, Minna, Nigeria</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>emetere@yahoo.com</email></corresp></author-notes><pub-date pub-type="epub"><day>27</day><month>02</month><year>2013</year></pub-date><volume>03</volume><issue>01</issue><fpage>87</fpage><lpage>94</lpage><history><date date-type="received"><day>September</day>	<month>7th,</month>	<year>2012</year></date><date date-type="rev-recd"><day>October</day>	<month>22nd,</month>	<year>2012</year>	</date><date date-type="accepted"><day>November</day>	<month>9th,</month>	<year>2012</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
   The Bloch NMR as an analytical tool was able to address the fundamental features in the learning of spintronics. Beside confirming past assertions on the Rashba spin-orbit interaction, thermal motion of hole and electron spin and features of the quantum well, it was also able to explain the condition necessary for Rashba splitting within the quantum well. When the Rashba energy is 43 meV, it modified the Ehrenfest’s theorem to hold for an external magnetic field. The confinement potential which is the strength of the Rashba spin-orbit interaction was shown to be controlled magnetically. 
 
</p></abstract><kwd-group><kwd>Bloch NMR; Rashba Energy; Rashba Parameter; Quantum Well; Spin-Plit; Hole Spin Velocity</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>The Bloch NMR model has over the years proven to be a good diagnostic tool for investigating properties of known quantities. For example, the Bloch NMR equations has shown good success in the study biological and physiological properties of living tissue [1,2]. Besides medical applications, the Bloch NMR equations were used to investigate the thermodynamic properties of system e.g. the Wegner distribution function [<xref ref-type="bibr" rid="scirp.28346-ref3">3</xref>]. Recently, the Bloch NMR was used to analyse the magnetic penetration depth of superconducting material and was also applied to explain the muon-spin [<xref ref-type="bibr" rid="scirp.28346-ref4">4</xref>].</p><p>The technological and computational prospects of semiconductor spintronics have been explored in various researches [5-10]. One of the notable works in the semiconductor spintronics is the Rashba term [11-13]. One of the major successes of the Rashba term is the measurement of the strength of spin splitting using the Rashba energy of split state and coupling parameter. The Rashba energies can be tuned by changing the composition parameters of the surface alloy [14,15] while the Rashba coupling parameter (α<sub>R</sub>) was calculated as 10<sup>−1</sup> eV&#197; for conventional narrow-gap semiconductor structures. Unfortunately, low Rashba coupling parameter do not supports the 2 d spintronics device. Early this year, a layered semiconductor (bismuth tellurohalides) was found to exhibit a large spin splitting [<xref ref-type="bibr" rid="scirp.28346-ref16">16</xref>] which was about 4.8 eV. The improvements on the spin-split extended to nonmagnetic material where the Rashba-Bychkov effect shows the possibility of producing spin-split energy bands in nonmagnetic materials without the application of any external magnetic field [<xref ref-type="bibr" rid="scirp.28346-ref17">17</xref>]. The Rashba splitting was believed to have been absent in quantum wells because quantum well states are standing waves [<xref ref-type="bibr" rid="scirp.28346-ref18">18</xref>], but was opposed by Stanley et al. [<xref ref-type="bibr" rid="scirp.28346-ref19">19</xref>]. The later proved that Rashba splitting occurs in the quantum well states II-V semiconductors. The giant spin splitting in semiconductor is dependent on the spin-orbit interaction [17,20] which is now referred to as the Rashba spin-orbit interaction [<xref ref-type="bibr" rid="scirp.28346-ref12">12</xref>]. The gaint spin splitting was first demonstrated on a noble metal [21,22] and further improved on in thin-film [23,24].</p><p>In this paper, the Bloch NMR equations were used as a diagnostic tool to analyze the Rashba energies state in a rotating magnetic frame. Derivations of operational equations were used to solve the Rashba energy with the mind set of investigating the conditions necessary for the presence of Rashba splitting in quantum wells and the possibility of controlling the confinement potential magnetically.</p></sec><sec id="s2"><title>2. Theoretical Derivations</title><p>The following theoretical assumptions were made in order to incorporate the Bloch NMR into the spintronics device 1) The Rashba parameter was substituted for the spin coupling in the Bloch NMR because they both are synonymous in operation.</p><p>2) Let the excitation frequencies in each concept be the same <img src="15-4800143\a3e276f6-fef0-4487-8d37-3fb6f5971703.jpg" /></p><p>3) The macroscopic magnetization of the localized was equated with the equilibrium magnetization of the Bloch model.</p><p>4) Semiconductors have various electron-hole recombination rates [25,26]. The speed of the holes and electrons is assumed<img src="15-4800143\1a1fb34f-2198-4393-94e0-9fc2048e71ed.jpg" />.</p><p>5) Both the g tends to 1, likewise the frequency difference between Larmor frequencies.</p><sec id="s2_1"><title>2.1. Spin Splitting Derivations</title><p>The Rashba energy and Rashba parameter are related in the equations shown below</p><disp-formula id="scirp.28346-formula38307"><label>(1)</label><graphic position="anchor" xlink:href="15-4800143\2a25c862-964c-40bf-a1c3-63a01fef5f6c.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.28346-formula38308"><label>(2)</label><graphic position="anchor" xlink:href="15-4800143\e1b9f8af-feea-4442-99f4-24b83a0968c1.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.28346-formula38309"><label>(3)</label><graphic position="anchor" xlink:href="15-4800143\0a918b95-05df-4edf-ac29-9b422a463abf.jpg"  xlink:type="simple"/></disp-formula><p>The magnetic potential introduced by Zeeman term</p><disp-formula id="scirp.28346-formula38310"><label>(4)</label><graphic position="anchor" xlink:href="15-4800143\074bbf23-ad18-44a6-92ca-9fbec4d00bd2.jpg"  xlink:type="simple"/></disp-formula><p>The resulting spin-splitting of s-type electron states is given by</p><disp-formula id="scirp.28346-formula38311"><label>(5)</label><graphic position="anchor" xlink:href="15-4800143\41c1438a-8e4f-4718-85c9-d935cd6add18.jpg"  xlink:type="simple"/></disp-formula><p>From Equations (1)-(5), Equation (6) was derived</p><disp-formula id="scirp.28346-formula38312"><label>(6)</label><graphic position="anchor" xlink:href="15-4800143\8b1ec4d9-e3cd-4f30-be80-8601c9451ea1.jpg"  xlink:type="simple"/></disp-formula><p>where E<sub>R</sub> = Rashba energy, α<sub>B</sub> = Rashba parameter, m<sup>*</sup> = effective mass, u = magnetic potential, σ = spin index, Pauli spin matrices, for electric spin, it is given as</p><p><img src="15-4800143\fc5fd7e2-e911-4c70-88f8-7ba9d8593f1d.jpg" /></p><p>where a = lattice constant, g = g-factor. μ<sub>B</sub> = mobility.</p></sec><sec id="s2_2"><title>2.2. Bloch NMR Derivation Model</title><p>In this section, a mathematical algorithm to describe in detail the translational mechanical properties of the Bloch NMR equation was developed. A sample of atomic crystal structure is analyzed by the x, y, z component (in the rotating frame) of magnetization given by the Bloch equations which may be written as follows</p><disp-formula id="scirp.28346-formula38313"><label>(7)</label><graphic position="anchor" xlink:href="15-4800143\12eaccad-e23b-4a95-8eff-e3e1646e1280.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.28346-formula38314"><label>(8)</label><graphic position="anchor" xlink:href="15-4800143\c2e3fb1a-8f8d-4ba5-8405-dfc4d6f822fb.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.28346-formula38315"><label>(9)</label><graphic position="anchor" xlink:href="15-4800143\c9e8d956-aaaf-48d1-97a3-0a55e1f83c8f.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="15-4800143\54cf360d-5ac5-49c4-bcfd-afd8a466524f.jpg" /> the frequency difference between Larmor frequency and frame of reference, <img src="15-4800143\94471d3a-c62b-4292-b564-65ae8f94b604.jpg" />is the Rabi frequency, <img src="15-4800143\625d7b62-1731-47e3-88f7-21cf71142084.jpg" />is the Larmor frequency, M<sub>x</sub>, M<sub>y</sub> are the transverse magnetization, M<sub>z</sub> is the longitudinal magnetization, M<sub>o</sub> is the equilibrium magnetization. The movement of the holes and electrons is assumed to move at a velocity V<sub>e</sub> and V<sub>h</sub> and at distances L<sub>h</sub> &amp; L<sub>e</sub> from the conduction and valence bands.</p><disp-formula id="scirp.28346-formula38316"><label>(10)</label><graphic position="anchor" xlink:href="15-4800143\04fb6829-f97b-4118-8b7f-a84d9d237caf.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.28346-formula38317"><label>(11)</label><graphic position="anchor" xlink:href="15-4800143\600b4fda-2bb4-42a4-a21c-4985c56f9ad0.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.28346-formula38318"><label>(12)</label><graphic position="anchor" xlink:href="15-4800143\76794d99-bcd6-47a0-b3ae-04b5ea15396b.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="15-4800143\2ad6bbac-fbfc-49df-93e4-285314446153.jpg" /> and <img src="15-4800143\d3570d85-c9a4-480d-8e69-c69c99721770.jpg" /></p><disp-formula id="scirp.28346-formula38319"><label>(13)</label><graphic position="anchor" xlink:href="15-4800143\8b38e2a2-ade2-4100-a931-c9ddccaa57b6.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.28346-formula38320"><label>(14)</label><graphic position="anchor" xlink:href="15-4800143\b51de0f0-c982-4d30-8f29-eeba087a1122.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.28346-formula38321"><label>(15)</label><graphic position="anchor" xlink:href="15-4800143\a2cc3d01-2ce3-4d9d-b167-9b25253eeb1c.jpg"  xlink:type="simple"/></disp-formula><p>The solution of the above equations can be arranged in matrix form as shown below</p><disp-formula id="scirp.28346-formula38322"><label>(16)</label><graphic position="anchor" xlink:href="15-4800143\ef086a1b-a88f-408e-acc2-e0a28d649b6b.jpg"  xlink:type="simple"/></disp-formula><p>The matrix multiplication as shown below leads to the steady solutions of the Bloch equations in the rotating frame of reference are shown below</p><disp-formula id="scirp.28346-formula38323"><label>(17)</label><graphic position="anchor" xlink:href="15-4800143\9535cc02-3107-49bf-955b-ff3b3b456cd4.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.28346-formula38324"><label>(18)</label><graphic position="anchor" xlink:href="15-4800143\bc5d1c44-2873-4550-9ee7-d360ad7b1988.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.28346-formula38325"><label>(19)</label><graphic position="anchor" xlink:href="15-4800143\21e33db2-9d0d-440c-8b95-11e03c1fab76.jpg"  xlink:type="simple"/></disp-formula><p>These solutions directly give the frequency response of the magnetization. This idea gives the possibilities of quantitatively calculating the measured signal if a spin system is characterized by relaxation times T<sub>1</sub> and T<sub>2</sub>. The term <img src="15-4800143\6fc5961e-6822-454a-83e8-9aa2fc80a129.jpg" /> is proportional to the radio frequency power P. At the state of no saturation i.e. for low power P, this term <img src="15-4800143\317a6352-c556-4a7e-b1fb-4bb71a5f3c5a.jpg" /> is small <img src="15-4800143\787e75b2-2ca2-4885-a5f2-db002b012e12.jpg" />.</p><disp-formula id="scirp.28346-formula38326"><label>(20)</label><graphic position="anchor" xlink:href="15-4800143\8b76ce95-b8c5-45d2-8c14-517539e4f737.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.28346-formula38327"><label>(21)</label><graphic position="anchor" xlink:href="15-4800143\da300d31-66ed-4406-8182-f24168f5ac7a.jpg"  xlink:type="simple"/></disp-formula></sec><sec id="s2_3"><title>2.3. Operational Equations</title><p>The operational equations used for the simulations were worked out and systems of equations were generated. Equations (6), (20) and (21) yield</p><disp-formula id="scirp.28346-formula38328"><label>(22)</label><graphic position="anchor" xlink:href="15-4800143\d30b29f3-4159-4e2b-b76d-b87177716cde.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.28346-formula38329"><label>(23)</label><graphic position="anchor" xlink:href="15-4800143\af8517a8-00b9-4ce1-a5c0-15e5c7278c5e.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="15-4800143\cea18b14-8194-4795-87c8-7803d972f2cc.jpg" /></p><disp-formula id="scirp.28346-formula38330"><label>(24)</label><graphic position="anchor" xlink:href="15-4800143\bb02cf6e-adbb-432f-a91c-9c8c9f34cb08.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="15-4800143\616f5cc2-d267-48c9-8318-77b98a575f87.jpg" /></p><p>Equations (17)-(19) yield when <img src="15-4800143\2a0732fd-b815-4026-8935-af3f81288a99.jpg" /></p><disp-formula id="scirp.28346-formula38331"><label>(25)</label><graphic position="anchor" xlink:href="15-4800143\1c6448f8-c3aa-462a-810d-9e8fb0a5b236.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.28346-formula38332"><label>(26)</label><graphic position="anchor" xlink:href="15-4800143\fc66cb8e-6aff-40f7-bfee-6d50ece92303.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.28346-formula38333"><label>(27)</label><graphic position="anchor" xlink:href="15-4800143\b472b7b6-b281-47c2-b4e1-d96ee32205c2.jpg"  xlink:type="simple"/></disp-formula><p>Applying Equations (23)-(27)</p><disp-formula id="scirp.28346-formula38334"><label>(28)</label><graphic position="anchor" xlink:href="15-4800143\53611939-526e-4cfb-8541-c1e7f093fa5f.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.28346-formula38335"><label>(29)</label><graphic position="anchor" xlink:href="15-4800143\bb759aac-fe44-470c-803c-2f4eefbd1512.jpg"  xlink:type="simple"/></disp-formula><p>Ploting the first and second term of Equations (28) and (29) where <img src="15-4800143\709b1a3e-97ba-4d6b-8cd6-21a1b5fee4db.jpg" /></p><p>The Rashba energy along the vertical and horizontal axes are represented diagrammatically (shown in <xref ref-type="fig" rid="fig1">Figure 1</xref>) which satisfies the mathematical expression <img src="15-4800143\e91a9967-c79e-401e-bf56-fbf247cf403a.jpg" />.</p></sec></sec><sec id="s3"><title>3. Simulations of Derivations</title><p>In this section, the simulations of Equations (22)-(24) under various conditions e.g. the time relaxations and magnetic moments. Time relaxations of 9 ns was applied (Laura Fanea et al., 2011) to investigate the behavior of the Rashba energy with respect to its longitudinal and transverse component.</p></sec><sec id="s4"><title>4. Results and Discussion</title><p>Thermal motion of the hole was investigated in <xref ref-type="fig" rid="fig2">Figure 2</xref> where the hole velocity was plotted against the angle of propagation at a relaxation time 9 &#215; 10<sup>−9</sup> s. Its results was in accordance with past papers [27,28] which was interpreted that the stochastic modulation of the interaction between the heavy and light hole sub-bands may induce a nonadiabatic transitions between them, which may eventually lead to J-relaxation and dephasing. In <xref ref-type="fig" rid="fig3">Figure 3</xref>, the focus was to which type of character is dominant among the subbands. In accordance to the graphical expression given by Winkler [<xref ref-type="bibr" rid="scirp.28346-ref29">29</xref>] it was discovered that the features of <xref ref-type="fig" rid="fig3">Figure 3</xref> is a heavy hole character. <xref ref-type="fig" rid="fig4">Figure 4</xref> investigated the relationship between the potential and the spin mobility within the system. The direction of the wavelike structure gives an asymmetric double peak structure which shows that energy exist between the peaks which was as a result of the perpendicular magnetic field. An in-plane inversion asymmetry can induce a contribution from an in-plane potential gradient, which can strongly enhance the spin splitting [<xref ref-type="bibr" rid="scirp.28346-ref22">22</xref>]. Figures 5 and 6 explain more on effect of the external magnetic fields on the holes or electron in the quantum well. Actually, <xref ref-type="fig" rid="fig5">Figure 5</xref> supports the idea that quantum well states are standing waves and should therefore show no Rashba splitting while <xref ref-type="fig" rid="fig6">Figure 6</xref> supports that the Rashba splitting occurs in the quantum well state (two strange events). One of the objectives of this paper was to investigate the conditions necessary for the Rashba splitting within the quantum well. Figures 7 and 8 are similar in shape i.e. showing the strength of the splitting. Figures 9 and 10 show the Rashba energies at ground state (in which was calculated at about ≥43 meV) which have two branches synonymous to the spin up state and the spin down state.</p><p>Unlike the findings of Eerdunchaolu et al. [<xref ref-type="bibr" rid="scirp.28346-ref30">30</xref>] an increase in the Rashba energy makes no significant change in χ<sub>1</sub> &amp; χ<sub>2</sub> (which is described as the height). More importantly, it reveals that Rashba split of orbit interaction effect is not dependent on the height in the y direction. This is because the effective magnetic field which is produced by spin-orbit coupling (due to the lack of structure inversion symmetry) is approximately perpendicular to the electron momentum in the quantum ring. <xref ref-type="fig" rid="fig1">Figure 1</xref>1 shows that electron wave function bound in a quantum well in the presence of an external (or built-in) field e.g. M<sub>x</sub>, M<sub>y</sub> or M<sub>z</sub>. Very much like the reaction of the electric</p><p>fields in the quantum well, the behavioral features of the effective magnetic field in the conduction band (upper part of <xref ref-type="fig" rid="fig1">Figure 1</xref>1) and valence band (lower part of <xref ref-type="fig" rid="fig1">Figure 1</xref>1)) is the sum of the magnetic field and the contributions due to the position dependence of the conduction band. In other words, the modification of Ehrenfest’s theorem becomes necessary because it is the magnetic field in the valence band that controls the Rashba spin splitting of electron states. <xref ref-type="fig" rid="fig1">Figure 1</xref>2 gives a joint feature of Figures 5 and 6 which may suggest the possibility of the ideas of Petersen et al. [<xref ref-type="bibr" rid="scirp.28346-ref18">18</xref>] and Stanley et al. [<xref ref-type="bibr" rid="scirp.28346-ref19">19</xref>] occurring simultaneously within the quantum well.</p></sec><sec id="s5"><title>5. Conclusion</title><p>The Bloch NMR model has been proven to be efficient in analyzing the fundamentals of spintronics. It was discovered that an increase in the Rashba energy makes no sig-</p><p>nificant changes in χ<sub>1</sub> &amp; χ<sub>2</sub> (which was described as height). This result, makes the Rashba split of orbit interaction effect independent on the height along the y direction as shown in Figures 9 and 10. Furthermore, this led to the alteration of Ehrenfest’s theorem (which originally applies to the external electric fields), but now applies to the external magnetic field. Therefore, the confinement potential which is the strength of the Rashba spin-orbit interaction can also be controlled magnetically. This idea may be expatiated upon based on further research. Also the Bloch NMR was also effective to analyze the quantum well i.e. even though it is a standing wave, it could still experience Rashba splitting when the quantized electron energy E<sub>e</sub> ≥ 1 meV and the length of the quantum well is 6 nm.</p></sec><sec id="s6"><title>6. Appreciation</title><p>This work is self-funded. I appreciate Mrs. Jennifer Emetere for editing the script. I appreciate the Head of Physics Department of the above named institution.</p></sec><sec id="s7"><title>REFERENCES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.28346-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">O. B. Awojoyogbe, “A Mathematical Model of Bloch NMR Equations for Quantitative Analysis of Blood Flow in Blood Vessels with Changing Cross-section II,” Physica A: Statistical Mechanics and Its Applications, Vol. 323, 2003, pp. 534-550.  
doi:10.1016/S0378-4371(02)02025-3</mixed-citation></ref><ref id="scirp.28346-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">O. B. Awojoyogbe, “Analytical Solution of the Time Dependent Bloch NMR Equations: A Translational Mechanical Approach,” Physica A: Statistical Mechanics and Its Applications, Vol. 339, No. 3-4, 2004, pp. 437-460. doi:10.1016/j.physa.2004.03.061</mixed-citation></ref><ref id="scirp.28346-ref3"><label>3</label><mixed-citation publication-type="other" xlink:type="simple">E. P. Wigner, “On the Quantum Correction for Thermodynamic Equilibrium,” Physical Review, Vol. 40, No. 5, 1932, pp. 749-759. doi:10.1103/PhysRev.40.749</mixed-citation></ref><ref id="scirp.28346-ref4"><label>4</label><mixed-citation publication-type="other" xlink:type="simple">U. E. Uno and M. E. Emetere, “Analysis of the High Temperature Superconducting Magnetic Penetration Depth Using the Bloch NMR Equations,” Global Engineers and Technologist Review, Vol. 2, No. 1, 2012, pp. 14-21.</mixed-citation></ref><ref id="scirp.28346-ref5"><label>5</label><mixed-citation publication-type="other" xlink:type="simple">C. Benett and D. Di Vincenzo, “Quantum Information and Computation,” Nature, Vol. 404, 2000, pp. 247253. doi:10.1038/35005001</mixed-citation></ref><ref id="scirp.28346-ref6"><label>6</label><mixed-citation publication-type="other" xlink:type="simple">S. Yuasa, T. Nagahama, A. Fukushima, Y. Suzuki and K. Ando, “Giant Room-Temperature Magnetoresistance in Single-Crystal Fe/MgO/Fe Magnetic Tunnel Junctions,” Nature Materials, Vol. 3, No. 12, 2004, pp. 868-871.  
doi:10.1038/nmat1257</mixed-citation></ref><ref id="scirp.28346-ref7"><label>7</label><mixed-citation publication-type="other" xlink:type="simple">S. Parkin, C. Kaiser, A. Panchula, P. Rice, B. H. M. Samant and S. H. Yang, “Giant Tunnelling Magnetoresistance at Room Temperature with MgO(100) Tunnel Barriers,” Nature Materials, Vol. 3, 2004, pp. 862-867. doi:10.1038/nmat1256</mixed-citation></ref><ref id="scirp.28346-ref8"><label>8</label><mixed-citation publication-type="other" xlink:type="simple">T. Dietl, “Magnetic Anisotropy and Domain Structure in Carrier-Controlled Ferromagnetic Semiconductors,” Journal of Physics: Condensed Matter, Vol. 16, No. 48, 2004, p. S5471. doi:10.1088/0953-8984/16/48/001</mixed-citation></ref><ref id="scirp.28346-ref9"><label>9</label><mixed-citation publication-type="other" xlink:type="simple">T. Dietl, “Magnetic Anisotropy and Domain Structure in Carrier-Controlled Ferromagnetic Semiconductors,” Proceedings 27th International Conference on Physics of Semiconductors, Flagstaff, 2004, pp. 56-60.</mixed-citation></ref><ref id="scirp.28346-ref10"><label>10</label><mixed-citation publication-type="other" xlink:type="simple">F. H. L. Koppens, et al., “Driven Coherent Oscillations of a Single Electron Spin in a Quantum Dot,” Nature, Vol. 442, 2006, pp. 766-771. doi:10.1038/nature05065</mixed-citation></ref><ref id="scirp.28346-ref11"><label>11</label><mixed-citation publication-type="other" xlink:type="simple">Z. Wilamowski, W. Jantsch, N. Sandersfeld, M. Muhlberger, F. Schaffler and S. Lyon, “Spin Relaxation and g-Factor of Two-Dimensional Electrons in Si/SiGe Quantum Wells,” Physica E: Low-Dimensional Systems and Nanostructures, Vol. 16, No. 2, 2003, pp. 111-115.  
doi:10.1016/S1386-9477(02)00582-9</mixed-citation></ref><ref id="scirp.28346-ref12"><label>12</label><mixed-citation publication-type="other" xlink:type="simple">Y. Bychkov and E. I. Rashba, “Oscillatory Effects and the Magnetic Susceptibility of Carriers in Inversion Layers,” Journal of Physics C: Solid State Physics, Vol. 17, No. 33, 1984, pp. 6039-6045.</mixed-citation></ref><ref id="scirp.28346-ref13"><label>13</label><mixed-citation publication-type="other" xlink:type="simple">E. I. Rashba, “Theory of Electrical Spin Injection: Tunnel Contacts as a Solution ofthe Conductivity Mismatch Problem,” Physical Review B, Vol. 62, No. 24, 2000, pp. R16267-R16270. doi:10.1103/PhysRevB.62.R16267</mixed-citation></ref><ref id="scirp.28346-ref14"><label>14</label><mixed-citation publication-type="other" xlink:type="simple">F. Meier, V. Petrov, S. Guerrero, C. Mudry, L. Patthey, J. Osterwalder and J. H. Dil, “Unconventional Fermi Surface Spin Textures in the BixPb1-x/Ag(111) Surface Alloy,” Physical Review B, Vol. 79, No. 24, 2009, pp. 241408-241412. doi:10.1103/PhysRevB.79.241408</mixed-citation></ref><ref id="scirp.28346-ref15"><label>15</label><mixed-citation publication-type="other" xlink:type="simple">J. Nitta, T. Akazaki and H. Takayanagi, “Gate Control of Spin-Orbit Interaction in an Inverted In0.53Ga0.47As/ In0.52Al0.48As Heterostructure,” Physical Review Letters, Vol. 78, No. 7, 1997, pp. 1335-1338.  
doi:10.1103/PhysRevLett.78.1335</mixed-citation></ref><ref id="scirp.28346-ref16"><label>16</label><mixed-citation publication-type="other" xlink:type="simple">S. V. Eremeev, I. A. Nechaev, Y. M. Koroteev, P. M. Echenique and E. V. Chulkov, “Ideal Two-Dimensional Electron Systems with a Giant Rashba-Type Spin Splitting in Real Materials: Surfaces of Bismuth Tellurohalides,” Physical Review Letters, Vol. 108, No. 24, 2012, pp. 246802-246807. doi:10.1103/PhysRevLett.108.246802</mixed-citation></ref><ref id="scirp.28346-ref17"><label>17</label><mixed-citation publication-type="other" xlink:type="simple">Y. A. Bychkov and E. I. Rashba, “Properties of a 2D Electron Gas with Lifted Spectral Degeneracy,” JETP Letters, Vol. 39, No. 2, 1984, pp. 78-83.</mixed-citation></ref><ref id="scirp.28346-ref18"><label>18</label><mixed-citation publication-type="other" xlink:type="simple">L. Petersen and P. Hedegard, “A Simple Tight-Binding Model Of Spin-Orbit Splitting Of Sp-Derived Surface States,” Surface Science, Vol. 459, No. 1-2, 2000, pp. 49-56. doi:10.1016/S0039-6028(00)00441-6</mixed-citation></ref><ref id="scirp.28346-ref19"><label>19</label><mixed-citation publication-type="other" xlink:type="simple">J. P. Stanley, N. Pattinson, C. J. Lambert and J. H. Jefferson, “Rashba Spin-Splitting in Narrow Gap III-V Semiconductor Quantum Wells,” Physica E: Low-Dimensional Systems and Nanostructures, Vol. 20, No. 3-4, 2004, pp. 433-435. doi:10.1016/j.physe.2003.08.052</mixed-citation></ref><ref id="scirp.28346-ref20"><label>20</label><mixed-citation publication-type="other" xlink:type="simple">M. I. Dyakonov and V. Y. Kachorovskii, “Spin Relaxation of Two Dimensional Electrons in Noncentrosymetric Semiconductors,” Soviet Physics: Semiconductors, Vol. 20, 1986, pp. 110-116.</mixed-citation></ref><ref id="scirp.28346-ref21"><label>21</label><mixed-citation publication-type="other" xlink:type="simple">D. Pacilé, C. R. Ast, M. Papagno, C. Da Silva, L. Moreschini, M. Falub, A. P. Seitsonen and M. Grioni, “Electronic Structure of an Ordered Pb∕Ag(111) Surface Alloy: Theory and Experiment,” Physical Review B, Vol. 73, No. 24, 2006, pp. 245429-245435.  
doi:10.1103/PhysRevB.73.245429</mixed-citation></ref><ref id="scirp.28346-ref22"><label>22</label><mixed-citation publication-type="other" xlink:type="simple">C. R. Ast, K. Kern and M. Grioni, “Giant Spin Splitting through Surface Alloying,” Physical Review Letters, Vol. 98, No. 18, 2007, pp. 186807-186811.  
doi:10.1103/PhysRevLett.98.186807</mixed-citation></ref><ref id="scirp.28346-ref23"><label>23</label><mixed-citation publication-type="other" xlink:type="simple">K. He, T. Hirahara, T. Okuda, S. Hasegawa, A. Kakizaki and I. Matsuda, “Spin Polarization of Quantum Well States in Ag Films Induced by the Rashba Effect at the Surface,” Physical Review Letters, Vol. 101, No. 10, 2008, pp. 107604-107608.  
doi:10.1103/PhysRevLett.101.107604</mixed-citation></ref><ref id="scirp.28346-ref24"><label>24</label><mixed-citation publication-type="other" xlink:type="simple">E. Frantzeskakis, S. Pons, H. Mirhosseini, J. Henk, C. R. Ast and M. Grioni, “Tuning of Spin-Gaps at Silicon Interfaces,” Physical Review Letters, Vol. 101, No. 19, 2008, pp. 196805-196809.  
doi:10.1103/PhysRevLett.101.196805</mixed-citation></ref><ref id="scirp.28346-ref25"><label>25</label><mixed-citation publication-type="other" xlink:type="simple">R. F. Pierret, “Semiconductor Device Fundamentals,” Prentice Hall, New York, 1995.</mixed-citation></ref><ref id="scirp.28346-ref26"><label>26</label><mixed-citation publication-type="other" xlink:type="simple">P. Harrison, “Quantum Wells, Wires and Dots,” Wiley, New York, 2005. doi:10.1002/0470010827</mixed-citation></ref><ref id="scirp.28346-ref27"><label>27</label><mixed-citation publication-type="other" xlink:type="simple">Y. A. Serebrennikov, “Single-Hole Spin Dephasing in Bulk Crystals,” Physical Review B, Vol. 71, No. 23, 2005, pp. 233202-233206. doi:10.1103/PhysRevB.71.233202</mixed-citation></ref><ref id="scirp.28346-ref28"><label>28</label><mixed-citation publication-type="other" xlink:type="simple">D. Culcer and R. Winkler, “Spin Polarization Decay in Spin-1/2 and Spin-3/2 Systems,” Physical Review B, Vol. 76, No. 19, 2007, pp. 195204-195210.  
doi:10.1103/PhysRevB.76.195204</mixed-citation></ref><ref id="scirp.28346-ref29"><label>29</label><mixed-citation publication-type="other" xlink:type="simple">R. Winkler, “Spin-Orbit Coupling Effects in Two-Dimensional Electron and Hole Systems,” Springer-Verlag Berlin Heidelberg, New York, 2003.  
doi:10.1007/b13586</mixed-citation></ref><ref id="scirp.28346-ref30"><label>30</label><mixed-citation publication-type="other" xlink:type="simple">Eerdunchaolu, W. Xin and Y.-W. Zhao, “Influence of Rashba SOI and Polaronic Effects on the Ground-State Energy of Electrons in Semiconductor Quantum Rings,” Chinese Physics Letters, Vol. 27, No. 1, 2010, pp. 017201-017201. doi:10.1088/0256-307X/27/1/017201</mixed-citation></ref></ref-list></back></article>