Microscopic description of relaxation of impurity magnetic atoms in spiral magnetics

Kinetics of the impurity magnetic atoms in spiral magnetic is researched. The spectrum of the excitations of the impurity spin is obtained in approximation of weakly coupling. The equation for impurity density matrix up to second order of the perturbation theory is obtained. For impurity spin s=1/2...

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Veröffentlicht in:Вопросы атомной науки и техники
Datum:2001
1. Verfasser: Ivashin, A.P.
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Sprache:Englisch
Veröffentlicht: Національний науковий центр «Харківський фізико-технічний інститут» НАН України 2001
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Zitieren:Microscopic description of relaxation of impurity magnetic atoms in spiral magnetics / A.P. Ivashin // Вопросы атомной науки и техники. — 2001. — № 6. — С. 326-328. — Бібліогр.: 10 назв. — англ.

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author Ivashin, A.P.
author_facet Ivashin, A.P.
citation_txt Microscopic description of relaxation of impurity magnetic atoms in spiral magnetics / A.P. Ivashin // Вопросы атомной науки и техники. — 2001. — № 6. — С. 326-328. — Бібліогр.: 10 назв. — англ.
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container_title Вопросы атомной науки и техники
description Kinetics of the impurity magnetic atoms in spiral magnetic is researched. The spectrum of the excitations of the impurity spin is obtained in approximation of weakly coupling. The equation for impurity density matrix up to second order of the perturbation theory is obtained. For impurity spin s=1/2 the kinetic coefficients in terms of correlation functions are found.
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fulltext MICROSCOPIC DESCRIPTION OF RELAXATION OF IMPURITY MAGNETIC ATOMS IN SPIRAL MAGNETICS A.P. Ivashin National Science Center “Kharkov Institute of Physics and Technology”, Kharkov, Ukraine e-mail: ivashin@kipt.kharkov.ua Kinetics of the impurity magnetic atoms in spiral magnetic is researched. The spectrum of the excitations of the impurity spin is obtained in approximation of weakly coupling. The equation for impurity density matrix up to sec- ond order of the perturbation theory is obtained. For impurity spin σ=1/2 the kinetic coefficients in terms of correla- tion functions are found. PACS: 76.90.+d; 34.10.+x 1. INTRODUCTION The kinetics of impurity spin was considered in many papers [1-4]. This paper deals with the kinetics of weakly coupled impurity spin in magnetic dielectric, which is considered as a thermostat. The thermostat has a spiral structure of magnetic ordering. Objects with a spiral magnetic structure are systems with a sponta- neously broken symmetry, in which the symmetry of the statistical equilibrium state is lower than the symmetry of the Hamiltonian. Such state is not translationally in- variant and does not exhibit invariance to spin rotations around the spiral axes. The method of quasi-averages is a convenient tool for analyzing such structures [5-7]. In this paper, using the reduced description method [8], the equation for impurity spin matrix was obtained. From this equation in main approximation the energy spec- trum of impurity spin was found. In last section we de- scribe the evolution of impurity spin σ=1/2. We define the kinetic coefficients, which are expressed in terms correlation function of the thermostat. 2. KINETIC EQUATION FOR IMPURITY DENSITY MATRIX The equilibrium state of spiral magnetic is described by statistical operator −−−Ω= )(exp( 0 z Bm ShHYW νν .)).))(exp((0 сhthxpiSY Bll l +−− +∑ ν (1) where: Hm is the Hamiltonian of matrix; 1 0 −Y is the temperature; BghhB 0µ+= , h is the magnetic bias field; mceo 2=µ is a Bohr magneton; g' is the gyromagnetic ratio for matrix spin; B is the magnetic field, which is directed parallel to ax Z; p is the spiral vector; νΩ is the thermodynamic potential, which is found from the normalizing condition 1=νSpW (trace is calculated only on thermostat states). The conditions, which are assumed from the struc- ture of operator (1), are as follows [ ] 0, ≠zSW , [ ] 0, ≠mHW , [ ] 0)(, =− z Bm ShHW . It means, that statistical operator W depends on time. The statistical operator also has such space symmetry WSapiWUUSapi z aa z =−+ )exp()exp(   , where the operator of the translation aU  satisfies the fol- lowing condition alala SUSU   + + = , IUU aa =+  , a- pitch of lattice, I - unit operator. In our case the equilibrium averages of spin components of matrix are as follows  = SS z , { }))((exp thxpiSS Bl −= ⊥ ±  , where ASpWA V  νν ∞→→ ≡ limlim 0 is the quasi averages value of operator A  ; ⊥S is the module of the transversal com- ponent of spin;  S is the longitudinal component of spin. We suppose, that the impurity concentration is very low, thus the Hamiltonian of system is as follows VgBBHH z m +−= σµ 0)( , ))( 2 1( +− ⊥ ++Σ−= σσσ z l z ll zz lzll SSISIV , where VBSgHBH z mm +−= ' 0)( µ Hamiltonian of spi- ral magnetic in magnetic field, V Hamiltonian of the ex- change interaction between the magnetic matrix and the impurity; zgBσµ 0− Hamiltonian of the impurity; g is gyromagnetic ratio of the impurity; Izl, lI⊥ are the longi- tudinal and transversal integrals of interaction between impurity spin σ and matrix spin Sl. From the Liouville equation [ ]Hti t t ),()( ρρ = ∂ ∂ (2) we obtain the equation for density matrix ρSpw = ,M t w = ∂ ∂ [ ]HiSpM ,ρ= (3) where M is the impurity collision integral. The impurity matrix w satisfies equation 1=trw , tr is a trace on impurity state. We assume [8], that the sta- tistical operator is the functional of impurity density ma- trix and phase thxp B−= ϕ , when t >> 0τ (τ0 is the time of relaxation in the thermostat) { })(),( ttw ϕρρ → . 70 PROBLEMS OF ATOMIC SCIENCE AND TECHNOLOGY. 2001, № 6, p. 326-328. It means, that .),(),(),( .. w w ww t w δ ϕδ ρ+ϕ δ ϕ ϕδ ρ= ∂ ϕρ∂ (4) Substituting this equality into Liouville equation (2) and assuming Bh−≈ . ϕ in main approximation, we obtain jointly with (3) the equations set for impurity density matrix w(t). As boundary condition we use the asymp- totic condition for operator ),( ϕρ w wWiHwiH )()exp(),()exp( 0 00 ϕτϕρτ τττ  →− > >− , (5) where )exp()exp( 00 zz gBiwgBiw σµσµτ −=− , z B z m ShgBHH −−= σµ 00 . Thus the Liouville equation jointly with (4) is as follows [ ]VHiMM w w V +=+ 00 ,)(),( ρ δ ϕδ ρ , where [ ]zwiM σ,0 Ω−= , [ ]ViSpMV ,ρ≡ , gB0µ=Ω . We take into account, that [ ]z B Sihw ,),( . ρϕ δ ϕ ϕδ ρ = . As a result we obtain the integral equation for ),( ϕρ w in common with (5) [ ] ττ τ δ δ ρρτϕϕρ 00 0 ,)(),( iH ww V iH eM w ViedwWw − ∞− → ∫ −       −+= This equation and the equation (2) form the closed set of the equations for impurity density matrix w (t). The zero and the first approximation for ρ(w,ϕ) equal correspondently to wWw )(),()0( ϕϕρ = , (6a) [ ] ττ τ ϕτϕρ 00 ,)(),( 0 )1( iH ww iH eVVwWedw − → ∞− − −= ∫ , (6b) Here VSpWV )(ϕ≡ . The collision integral subject to (6a), (6b) is as follows correspondently [ ] [ ]VwiVWiSpM ,),,()0()1( == ϕρ , [ ] [ ][ ]VVVwWSpdViSpM ,,)(- , 0 )1()2( −== ∫ ∞− τϕτρ (7) ττ τ 00 iHiH VeeV −= . As a result the kinetic equation for w up to the second order on interaction take on form )2()1()0( MMMw ++= , where M(0), M(1), M(2) are defined by formulae (7). In order to calculate V we use the unitary transforma- tion += ppWUUW ~ , )exp( ∑−≡ l z llp SxpiU  . Then the calculation of the averages in spiral mag- netic can be obtained with the operator .)).)exp(()(exp(~ 00 сhtihSYShHYW Bl l z B p m +−−−−Ω= +∑νν  where +≡ pmp p m UHUH   . This statistical operator will be the space homoge- nous operator. In order to get rid of dependence on time in the statistical operator we must turn into rotating sys- tem of coordinates. It means, that we must consider the operator tSihtSih z B z B WeeW −=' , aSpWa '= . Taking these notes into account and using the reduced description method [8], the equation for impurity densi- ty matrix in the described condensed matter was ob- tained: −−= ],[0 αα σω nwiw .).]),()[(( 0 chwKd +− ∫ ∞− βαα β στσττ . (8) Frequency 0ω and ort n are defined by formulae: 2 ~ 2 0 ' 0 ~ 0 ))(())0(( ⊥⊥ ++++= SpIgBBghSI z µµω ,           +++ = ⊥⊥ 0 0 ' 0 ~ 0 ~ ))0(( ,0,)( ω µµ ω gBBghSISpIn z , )( ~ pI z , )( ~ pI ⊥ are the Fourier components of the longi- tudinal )(xI z and transversal )(xI⊥ exchange integrals; Kαβ is the spin correlation function ( )∫ ∑ ∞− −= 0 , )()()(),()()()( li eieiei xSxSxSxSxIxIdK βαβαβαα β τττ , ⊥±+= III zz ααα δδ , τ α τ α στσ 00)( iHiH ee −= . Here the averaging is performed with homogeneous and time independent statistical operator of magnetic matrix. 3. ENERGY SPECTRUM OF ANY IMPURITY SPIN IN MAGNETIC The equations (8) allow us to find the spectrum of any impurity spin in magnetic in main approximation. We perform the turn in spin space so as zUnU σσ αα =+ , where yieU α σ α = is the unit operator of turn, tan zx nn /=α . In a result we obtain the equation for impurity density matrix w~ [ ]ztwitw σω ),(~)(~ 0−= , (9) += αα UtwUtw )()(~ . The Hermit operator w~ is characterized by the set of the matrix elements nwmwmn ~~ ≡ , σσ +−= ,..., nm , where m is the eigenvector of the operator zσ , ,mmmz =σ σσ ≤≤− m . The equation (9) in terms of the matrix elements is as follows )(0 ~)()(~ tmnmn wnmitw −−= ω . From this equation we define the energy spectrum of the impurity spin. )(0 nm −= ωω , σσ +−= ,...,, nm . The spectrum we obtain has equidistant character. This spectrum is nondegenerated spectrum, when 71 σσ −== nm , and σσ =−= nm , . When nm = the repetition factor of the degenerate equals 12 +σ . 4. KINETIC COEFFICIENTS FOR IMPURI- TY SPIN 2/1=σ It is very difficult to solve equation (8) in general case. Now we pay main attention to the case, when the impurity spin is equal to 1/2. In this case: )1)(2/1( iiPw τ+= , where iτ is the Pauli matrix and P  is the polarization vector. From (8) we get the equation for a motion of polarization vector βα βγββα β γ α −−ωε−= ∂ ∂ PDP)Dn( t P S 2 1 0 (10) α βα β γα ε DD = , )DD(D S β αα βα β += 2 1 , )Re( α βλ λα βα β δ KKD −= . The first item in round brackets describes the precession of the polarization vector. The coefficients αD define the shift and the thin structure of levels, and the coeffi- cients SDα β – their width. Now we will find the solutions of the equations (10) in form t)exp(i~ ωP . In main approximation in the interaction between the matrix and the impurity spin we have obtained disper- sion equation 0)( 2 0 2 =− ωωω . From this equation we have two solutions: 0=ω and 0ωω = . Next approximation gives frequency shift δ ϖ and damping decrement γ . The solution for 0=ω is as follows: 01 =δ ω , S z S zx S x DnDnnDn 33 2 1311 2 1 2 ++=γ . And the solution for 0ωω = is 312 DnDn zx −−=δ ω , ))(2/1( 12 γγ −= S iiD . These results correspond the results obtained in [9]. Now we consider the particular case, corresponding to the case of a magnetic with “light axes” ordering type. For this case we have 0,0 ≠=± zSS . For fun- damental frequency 0=ω we have 01 =δ ω , SD331 =γ . For frequency 0ωω = correspondently 32 D−=δ ω , ))(2/1( 22112 SS DD +=γ . The results correspond the results obtained in [10]. Using the Goldstein – Primakov form for matrix spin we can find the temperature dependence of the ob- tained decrements. In quadratic approximation by f (the magnon distribution function) we have only decrement 2γ , which is not equal to zero: )1()(~)0(Re 2 2 qpqp pq qpzz ffIK +−== ∑ − εεδπγ . Performing the integration we get in spin-wave approxi- mation             = )0( ln )2( ~ 2 4 2 2 εθθπ γ kTkTI cc , where Bgapp cp '2)()( µθεε +=≡ is the energy of mag- non, θ c is the Curie energy, )0(~~ II = is the zero Fouri- er component of the longitudinal exchange integral. ACKNOWLEDGMENT The author would like to thank M.Yu. Kovalevsky for helpful discussion of the results. REFERENCES 1. T.L. Andreeva, P.L. Rubin. Dynamics of magnetic momentum in Boltzman polarized gas subject to dis- sipation // JETF. 2000, v. 118, p. 877-884. 2. A.E. Meyerovich, J.N. Naish, J.R. Overs-Bradly and A. Stepaniants. Zero-temperature relaxation in spin polarized Fermi systems // Fiz. Nizk. Temp. 1997, v. 23, № 5/6, p. 553-563 (in Russian). 3. V.F. Los. Kinetics of impurity spin in magnetic // FNT. 1981, v. 7, № 3, p. 336-349 (in Russian). 4. E.G. Petrov. Kinetic equations for dynamical sys- tem, placed in condensed matter and strong external field // TMF. 1986, v. 68, № 1, p. 117-127 (in Rus- sian). 5. N.N. Bogolubov. Quasiaverages values in problems of statistical mechanics. Preprint D-781 DUBNA, 1961. 6. M.Yu. Kovalevsky, S.V. Peletminsky, Yu.V. Slu- sarenko. Thermodynamics and kinetics of spiral magnetic structure and method of quasiaverage val- ues // TMF. 1988, v. 74, p. 281-295 (in Russian). 7. M.Yu. Kovalevsky, S.V. Peletminsky, A.A. Ro- zhkov. Green functions of spiral magnetic in hydro- dynamic and quasi-particle approximation // TMF. 1988, v. 75, p. 86-99 (in Russian). 8. A.I. Akhieser, S.V. Peletminsky. Methods of statisti- cal physics. M.: “Nauka”, 1977, p. 368. 9. A.P. Ivashin, M.Yu. Kovalevsky. Kinetics of impu- rity magnetic atoms in spiral magnetic. Preprint KPTI 89-8, M: CNIIAtominform, 1989, p. 16 (in Russian). 10.A.P. Ivashin, V.D. Tsukanov. Kinetics of spin mag- netic excitation of magnetic atoms // FTT. 1985, v. 27, № 4, p. 1032-1036 (in Russian). ВОПРОСЫ АТОМНОЙ НАУКИ И ТЕХНИКИ. 2000, №2. Серия: Ядерно-физические исследования (36), с. 3-6. 72 A.P. Ivashin National Science Center “Kharkov Institute of Physics and Technology”, Kharkov, Ukraine 2. KINETIC EQUATION FOR IMPURITY DENSITY MATRIX 4. KINETIC COEFFICIENTS FOR IMPURITY SPIN acknowledgment REFERENCES
id nasplib_isofts_kiev_ua-123456789-80043
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
issn 1562-6016
language English
last_indexed 2025-12-07T15:46:02Z
publishDate 2001
publisher Національний науковий центр «Харківський фізико-технічний інститут» НАН України
record_format dspace
spelling Ivashin, A.P.
2015-04-09T16:26:04Z
2015-04-09T16:26:04Z
2001
Microscopic description of relaxation of impurity magnetic atoms in spiral magnetics / A.P. Ivashin // Вопросы атомной науки и техники. — 2001. — № 6. — С. 326-328. — Бібліогр.: 10 назв. — англ.
1562-6016
PACS: 76.90.+d; 34.10.+x
https://nasplib.isofts.kiev.ua/handle/123456789/80043
Kinetics of the impurity magnetic atoms in spiral magnetic is researched. The spectrum of the excitations of the impurity spin is obtained in approximation of weakly coupling. The equation for impurity density matrix up to second order of the perturbation theory is obtained. For impurity spin s=1/2 the kinetic coefficients in terms of correlation functions are found.
The author would like to thank M.Yu. Kovalevsky for helpful discussion of the results.
en
Національний науковий центр «Харківський фізико-технічний інститут» НАН України
Вопросы атомной науки и техники
Kinetic theory
Microscopic description of relaxation of impurity magnetic atoms in spiral magnetics
Микроскопическое описание релаксации примесных магнитных атомов в спиральных магнетиках
Article
published earlier
spellingShingle Microscopic description of relaxation of impurity magnetic atoms in spiral magnetics
Ivashin, A.P.
Kinetic theory
title Microscopic description of relaxation of impurity magnetic atoms in spiral magnetics
title_alt Микроскопическое описание релаксации примесных магнитных атомов в спиральных магнетиках
title_full Microscopic description of relaxation of impurity magnetic atoms in spiral magnetics
title_fullStr Microscopic description of relaxation of impurity magnetic atoms in spiral magnetics
title_full_unstemmed Microscopic description of relaxation of impurity magnetic atoms in spiral magnetics
title_short Microscopic description of relaxation of impurity magnetic atoms in spiral magnetics
title_sort microscopic description of relaxation of impurity magnetic atoms in spiral magnetics
topic Kinetic theory
topic_facet Kinetic theory
url https://nasplib.isofts.kiev.ua/handle/123456789/80043
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