Polarizability of D+X complex in bulk semiconductors

The electric polarizability α of ionized-donor-bound exciton D+X in bulk semiconductor is calculated for all values of the effective electron-to-hole mass ratio σ included in the range of stability (σ<σχ). The calculation is performed within the variational method by using 56-term wave function....

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Datum:2006
Hauptverfasser: Katih, M., Diouri, J., El Haddad, A.
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Sprache:English
Veröffentlicht: Інститут фізики напівпровідників імені В.Є. Лашкарьова НАН України 2006
Schriftenreihe:Semiconductor Physics Quantum Electronics & Optoelectronics
Online Zugang:http://dspace.nbuv.gov.ua/handle/123456789/121639
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spelling irk-123456789-1216392017-06-16T03:04:03Z Polarizability of D+X complex in bulk semiconductors Katih, M. Diouri, J. El Haddad, A. The electric polarizability α of ionized-donor-bound exciton D+X in bulk semiconductor is calculated for all values of the effective electron-to-hole mass ratio σ included in the range of stability (σ<σχ). The calculation is performed within the variational method by using 56-term wave function. An asymptotic behavior of α in the vicinity of the critical value σc is deduced. We have also calculated the limiting value σ for which the polarizability equals that of D− system. 2006 Article Polarizability of D+X complex in bulk semiconductors / M. Katih, J. Diouri, A. El Haddad // Semiconductor Physics Quantum Electronics & Optoelectronics. — 2006. — Т. 9, № 4. — С. 7-11. — Бібліогр.: 16 назв. — англ. 1560-8034 PACS 71.35.-y http://dspace.nbuv.gov.ua/handle/123456789/121639 en Semiconductor Physics Quantum Electronics & Optoelectronics Інститут фізики напівпровідників імені В.Є. Лашкарьова НАН України
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
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language English
description The electric polarizability α of ionized-donor-bound exciton D+X in bulk semiconductor is calculated for all values of the effective electron-to-hole mass ratio σ included in the range of stability (σ<σχ). The calculation is performed within the variational method by using 56-term wave function. An asymptotic behavior of α in the vicinity of the critical value σc is deduced. We have also calculated the limiting value σ for which the polarizability equals that of D− system.
format Article
author Katih, M.
Diouri, J.
El Haddad, A.
spellingShingle Katih, M.
Diouri, J.
El Haddad, A.
Polarizability of D+X complex in bulk semiconductors
Semiconductor Physics Quantum Electronics & Optoelectronics
author_facet Katih, M.
Diouri, J.
El Haddad, A.
author_sort Katih, M.
title Polarizability of D+X complex in bulk semiconductors
title_short Polarizability of D+X complex in bulk semiconductors
title_full Polarizability of D+X complex in bulk semiconductors
title_fullStr Polarizability of D+X complex in bulk semiconductors
title_full_unstemmed Polarizability of D+X complex in bulk semiconductors
title_sort polarizability of d+x complex in bulk semiconductors
publisher Інститут фізики напівпровідників імені В.Є. Лашкарьова НАН України
publishDate 2006
url http://dspace.nbuv.gov.ua/handle/123456789/121639
citation_txt Polarizability of D+X complex in bulk semiconductors / M. Katih, J. Diouri, A. El Haddad // Semiconductor Physics Quantum Electronics & Optoelectronics. — 2006. — Т. 9, № 4. — С. 7-11. — Бібліогр.: 16 назв. — англ.
series Semiconductor Physics Quantum Electronics & Optoelectronics
work_keys_str_mv AT katihm polarizabilityofdxcomplexinbulksemiconductors
AT diourij polarizabilityofdxcomplexinbulksemiconductors
AT elhaddada polarizabilityofdxcomplexinbulksemiconductors
first_indexed 2025-07-08T20:15:49Z
last_indexed 2025-07-08T20:15:49Z
_version_ 1837111180818120704
fulltext Semiconductor Physics, Quantum Electronics & Optoelectronics, 2006. V. 9, N 4. P. 7-11. © 2006, V. Lashkaryov Institute of Semiconductor Physics, National Academy of Sciences of Ukraine 7 PACS 71.35.-y Polarizability of D+X complex in bulk semiconductors M. Katih, J. Diouri and A. El Haddad* Faculté des sciences, Département de Physique, B.P. 2121, Tétouan, Morocco *Correspondent address: a_haddad01@yahoo.fr Abstract. The electric polarizability α of ionized-donor-bound exciton D+X in bulk semiconductor is calculated for all values of the effective electron-to-hole mass ratio σ included in the range of stability (σ<σχ). The calculation is performed within the variational method by using 56-term wave function. An asymptotic behavior of α in the vicinity of the critical value σc is deduced. We have also calculated the limiting value σ for which the polarizability equals that of D− system. Keywords: exciton, polarizability, wave function, variational method. Manuscript received 02.10.06; accepted for publication 23.10.06. 1. Introduction The existence of ionized-donor-bound exciton in semiconductors was first predicted by Lampert [1] and confirmed later by experimental works [2-4]. For direct gap semiconductors with isotropic bands, the calculation of the ground state energy of such a complex is reduced in the effective mass approximation, to solve the Hamiltonian of three bodies system formed by one electron-hole pair (e,h) trapped by one donor centre D+. This system is labelled D+X. It is clear that when the energy XD E + is less than the neutral donor energy 0D E , the excitonic complex forms and may affect, to some extent, the optical spectra of the host material. The stability of such a complex depends on the electron-hole mass ratio he mm /=σ . Several works have been devoted to this question [5-9]. Particularly, Skettrup et al. [8] have shown that the D+X complex stabilizes for all σ values lying lower than a critical point 426.0=cσ . Recently, dos Santos et al. [10] have reconsidered again the question and calculated σc by an original adiabatic approach using hyperspherical coordinates and obtained 431.0=cσ . In the particular case of 2D system, Stauffer and Stébé [9] have shown that the range of stability extends to 88.02 =D cσ . However, if one reviews the literature in the area, one is surprised by the insufficiency of works carrying on the effect of the electric field on D+X complex, in particular, the calculation of polarizability. To our knowledge, the unique work dealing with this question is that of Essaoudi et al. [11] in which the specific case of GaAs/Ga1−xAlxAs quantum well with the electric field applied parallel to the growth direction is studied. It has been shown in this work that the D+X complex is sensitive to the action of the field only for well widths higher than 10 nm. The numerical method used in this calculation cannot be generalized to the bulk limiting case because of the axial character of the used trial function inherent in the specific case of the 2D symmetry. Let’s recall that in a previous paper, we have calculated the polarizability of −X and + 2X complexes [12, 13]. But for these systems, the range of stability covers all σ-values whereas for D+X, the range of stability is limited. This is why we were interested in the present study. In what follows we calculate the electric polarizability of D+X complex in the framework of the variational method by using a trial function including 56 terms which gives an accurate numerical result. This paper is organized as follows: in section II we outline our method to determine the polarizability of D+X, in section III we explain our numerical method using a 56 terms trial wave function. Finally, in the last section we discuss our results. 2. The model In the effective mass approximation, the Hamiltonian of an ionized donor bound to an exciton in the presence of a constant electric field F directed along to the z-axis can be written as: H = H0 + W , (1) where H0 is given by H0 = T + V . (2) Semiconductor Physics, Quantum Electronics & Optoelectronics, 2006. V. 9, N 4. P. 7-11. © 2006, V. Lashkaryov Institute of Semiconductor Physics, National Academy of Sciences of Ukraine 8 Here, T is the kinetic energy and V is the Coulomb interaction between the particles of the system heT Δ−Δ−= 22 1 σ , (3) ehhe rrr V 111 −+−= , (4) and W is the electric energy operator FzzW he )( −= . (5) Note that in the previous expressions, we have used the atomic units (a.u.); 22 / ema eD hε= as the unit of length, DD aeE ε/2= as the unit of energy and DD eaEF /0 = as the unit of electric field strength. ε is an appropriate dielectric constant taking into account possible polarization effects. The parameter he mm /=σ defines the electron-to-hole effective mass ratio. re and rh are the distances from the ionized donor to the electron and the hole, respectively, while reh is the distance between the electron and the hole. ze and zh denote the coordinates of the electron and the hole along the electric field direction, respectively. eΔ and hΔ are the Laplacian operators with respect to the hole and electron coordinates. In order to calculate the polarizability α of the system, we develop the wave function Ψ and the energy E of the system in power series with respect to the electric field intensity. So we have ...2 210 +Ψ+Ψ+Ψ=Ψ FF , (6) ...2 210 +++= ΨΨ ΨΨ = FEFEE H E , (7) where Ψ0, Ψ1 and Ψ2 are F-independent functions, Ψ0 and E0 being the wave function and the energy of D+X in the absence of the field. Substituting H and Ψ in equation (7) and taking into account the spherical symmetry of the ground state in absence of electric field (F=0), we obtain: ⎪⎩ ⎪ ⎨ ⎧ −= = α 2 1 0 2 1 E E (8) where the polarizability α is given by .8 )(422 2 00 2 10 0 00 10110101 ΨΨ ΨΨ + + ΨΨ Ψ−Ψ−ΨΨ+ΨΨ− = E zzEH he α (9) One may ensure, as established in the appendix, that this entity is essentially positive for all σ values, what proves the stability of the complex for any weak electric field. Furthermore, equation (9) shows that the polarizability α depends only on E0, Ψ0 and Ψ1, the terms including Ψ2 simplify. E0 and Ψ0 are the well- known energy and wave function of the ground state of D+X in absence of electric field which are determined variationally by several authors [5-9]. As we can remark, the determination of the polarizability requires the knowledge of the wave function part Ψ1. On the other hand, since we are interested with the calculation of the polarizability, we consider that the electric field is sufficiently low, so, we can restrict the development of the energy to its quadratic form: E = E0 + E2F2. (10) Then it is convenient to use the variational method for calculating the energy E of the ground state of the system. With account of the symmetry of the problem, the trial function Ψ is chosen in the following way [12]: ),,(),,,,(1 ehheheehhe rrrfzzzrrr =Ψ , (11) where z = ze – zh , (12) f is a function that contains the variational parameters. Hence, ΨΨ ΨΨ = H E min . (13) Such a choice allows considerable simplifications. First, we can ensure that the integral 10 ΨΨ vanishes. In addition, we may establish the following relations whatever the choice of the function f(re,rh,reh): ,)1()( )()( 0 00 f z fzHf zz fHzzfzzH eh hehe ∂ ∂ +−= ∂ ∂ − ∂ ∂ + +−=− σσ (14) fHrffHzf eh 0 2 0 2 3 1 = , (15a) , 3 1 . 3 1 f r rf frff z zf eh eh eheh ∂ ∂ = =∇= ∂ ∂ rr (15b) frffzf eh 22 3 1 = , (15c) frfz eh 2 0 2 0 3 1 Ψ=Ψ . (15d) Semiconductor Physics, Quantum Electronics & Optoelectronics, 2006. V. 9, N 4. P. 7-11. © 2006, V. Lashkaryov Institute of Semiconductor Physics, National Academy of Sciences of Ukraine 9 In these conditions, the expected value of E2 is written as: 00 2 0 3 2 min ΨΨ Ψ+ = frfGf E eh , (16) where the operator G is given by eh eheheh r rrEHrG ∂ ∂ +−−= )1(2 00 2 σ . (17) The expression (16) shows that the calculation of E2 involves only the distances re, rh, reh. Next we use for Ψ0 the expression given by Stauffer and Stébé [9] : ∑ −=Ψ ++ nml nmlnml lmn ks tuskCuts ,, 0 ) 2 exp(),,( . (18) The exponents l, m, n are positive or zero integers and the elliptical coordinates s, t, u are given by s = re + reh, t = re – reh, u = rh . (19) The scaling factor k and the linear coefficients Clmn are determined variationaly for each σ value in the range of stability. We choose the function f in the following form: ∑ −= ++ nml nmlnml lmnehhe ks tuskArrrf ,, ) 2 exp(),,( , (20) where Almn are the linear variational parameters. Following the Hasse variational method [15], we use the values of k and Clmn that we obtain by minimizing the mean values of the Hamiltonian H0 in the absence of electric field. The variational parameters Almn are obtained by minimising the following expression (21) obtained after substituting equations (18) and (20) into (16). CSCk ARCAGA E ~~~ 3 ~~~ 2 ~~~ min 22 + ++ + = , (21) where A ~ ( C ~ ) denotes the column matrix of the coefficients Almn(Clmn) and +A ~ ( +C ~ ) its transposed matrix. G ~ , R ~ and S ~ are the squared matrices of the coefficients defined by: ,'''))1( )(( 2 0 22''' nml r rk EkVTkrlmnG eh eh eh nml lmn ∂ ∂ +− −−+= σ (22a) '''2''' nmlrlmnR eh nml lmn = , (22b) '''''' nmllmnS nml lmn = . (22c) The basic functions lmn are given by ) 2 exp( s tuslmn nml −= . (23) Equalling to zero the derivative of the expression involved in equation (21) with respect to A ~ , we find the following secular equation for Almn, CRAGG ~~~ ) ~~ ( 2 1 −=++ , (24) which yields CSC ARC k ~~~ ~~~ 3 2 0 2 + + − =α , (25) where 0 ~ A is the solution of the equation (24). 3. Numerical steps The calculation of the scaling factor k, the coefficients Clmn and the energy E0 is derived from the solution of the generalized eigenvalue problem [9] CQkCP ~~~~ = (26) with STQnmlVlmnP nml lmn ~~~ and'''''' β+=−= , (27) where CSC CTC nmlTlmnT nml lmn ~~~ ~~~ and'''''' + + == β . (28) Starting from 4/)2/1(0 σβ += that corresponds to the asymptotic behavior, we calculate the upper eigenvalue k, and then we deduce the corresponding vector C ~ which gives the next value of β and so on until the desired convergence on β, k and C ~ . Consequently, the energy E0 is deduced from the relation 2 0 kE β−= [9]. Let’s note in passing that the solution of equation (26) requires to solve the eigenvalue problem of the real symmetric matrix 2/12/1 ~~~~ −−= QPQM . This calculation is performed by using the Jacobi numerical method [14]. The system of linear equations (24) is solved numerically by using the LU-decomposition method [14]. Practically, we have limited the development of the functions Ψ0 and Ψ1 to 56 terms corresponding to the condition 5≤++ nml . Within this approximation, we obtain a rather good value of the critical mass ratio σc= 0.367. 4. Results The variations of the polarizability of D+X versus the mass ratio σ is presented in Fig. 1 (solid line). It is seen Semiconductor Physics, Quantum Electronics & Optoelectronics, 2006. V. 9, N 4. P. 7-11. © 2006, V. Lashkaryov Institute of Semiconductor Physics, National Academy of Sciences of Ukraine 10 that the polarizability increases with increasing σ up to the critical value σc in the vicinity of which an asymptotic behaviour is observed. Such a result may be interpreted physically by the weak bonding of the hole to the neutral donor in this point. Indeed, it is well known that the binding energy of D+X decreases with increasing σ in the absence of the electric field [8]. In the presence of a weak field, the hole is removed far from the electron along the direction of the field. This behaviour is confirmed by the variations of the electron polarizability (αe) and the hole polarizability (αh) defined by 〈ze,h〉 = αe,hF for weak electric field. This result is illustrated in Fig. 1 (dashed lines). The polarizability of D+X is then given by α = αh − αe. This asymptotic trend attests the consistency of our method because it is compatible with physics of such systems. After calculating the polarizability, we have deduced the binding energy of the complex in the presence of a weak electric field, which is defined as W = E(D0) – E . (29) -500 0 500 1000 1500 2000 2500 3000 3500 4000 4500 0,0 0,1 0,2 0,3 σ Po la riz ab ili ty (a t.u ni ts ) (α) (αe) (αh) αh = hole polarizability αe = electron polrizability α = αh - αe Fig. 1. The polarizability of D+X complex (in a.u. = 3 Daε ) as a function of the electron-to-hole effective mass ratio (solid line). Electron and hole polarizabilities in D+X (dashed lines). 0,000 0,005 0,010 0,015 0,020 0,025 0,030 0,035 0,040 0,045 0,050 0,0 0,1 0,2 0,3 σ Io ni za tio n fie ld (a t.u ni ts ) Fig. 2. The variation of ionization electric field (in a.u.) versus σ. The calculation was made in the weak field approximation: F<<FI, where FI is the ionization field defined by 000 2 1 EWFr Ieh −−== . (30) As an illustration, the variations of FI versus σ are reported in Fig. 2. In this condition, the neutral donor energy can be written as follows: 20 4 9 2 1 )( FDE −−= (31) and in the same way: 2 0 2 1 FEE α−= . (32) Practically, we have restricted our calculation to the strength field value F = 0.3FI which may be considered as consistent with the quadratic approximation in calculating the binding energy. Recall that it has been shown [16] that the perturbative calculation of the binding energy of the exciton for the strength field values up to 0.5FI gives good results. In Table, we report the values (in a.u.) of α, W0, and W for the strength field value F = 0.3FI in the range of σ values between 0 and σc. Semiconductor Physics, Quantum Electronics & Optoelectronics, 2006. V. 9, N 4. P. 7-11. © 2006, V. Lashkaryov Institute of Semiconductor Physics, National Academy of Sciences of Ukraine 11 Table. Listing of α, W0, and W for the strength field value F = 0.3FI, in the range of σ values between 0 and σc (in a.u.) σ α F = 0.3FI W0 W 0 22 0.01381 0.08378 0.08545 0.05 39 0.00832 0.05767 0.05886 0.1 77 0.00496 0.03946 0.04035 0.15 143 0.00285 0.02618 0.02674 0.2 289 0.00153 0.01645 0.01678 0.25 630 0.00074 0.00941 0.00958 0.3 1488 0.00029 0.00444 0.00450 0.35 4483 0.00005 0.00096 0.00096 σc ∞ 0 0 0 As an indication, we have calculated the value σD of σ for which the polarizability equals that of D− system. To do that, analogy of D− with the negative hydrogen ion [17] is made and gives 1765.0=Dσ with the corresponding polarizability α = 206 (a.u.). That means that for this limiting value of σ, the shift of both D− and D+X lines in the optical spectra when a weak electric field is applied is the same. Hence, for semiconductors with Dσσ < , the D+X shift is lower than that of D− while the situation is inverted for Dσσ > . In summary, we have presented a variational calculation of the polarizability of D+X as well as the binding energy in the presence of a weak electric field. This study shows an asymptotic behaviour of the polarizability in the vicinity of σc. This behaviour is principally due to the contribution of the hole which is weakly bound to the neutral donor D0. It has been established also that the effect of a weak electric field is more pronounced for σ values lower that σ = 0.3. As a comparison, confrontation of the polarizability of D+X with D− system is made and shows that it is possible to range the semiconductors in two classes following the relative shift of D+X and D− lines. Appendix We establish in what follows the effect of the stabilization of D+X complex in the presence of weak electric field. The expansion in power series of the dipolar electric moment in terms of the electric field strength yields: ....... )(2 )( 00 10 +=+ ΨΨ Ψ−Ψ = = ΨΨ Ψ−Ψ FF zz zz eh eh α (A1) By identifying to α as given by Eq. (9), we obtain: .4 )( 00 2 10 0101 11010 ΨΨ ΨΨ +ΨΨ− −ΨΨ=Ψ−Ψ EH Ezz he (A2) Substituting then (A2) in (9) gives .8 2 2 00 2 10 0 00 110101 ΨΨ ΨΨ − − ΨΨ ΨΨ−ΨΨ = E EH α (A3) It is evident that the first term in (A3) is positive because of the variational principle, and regarding to the negative value of E0, the sign of α is always positive which asserts the property of the stability of the complex as advanced above. References 1. M.A. Lampert // Phys. Rev. Lett. 1, p. 450 (1958). 2. D.G. Thomas and J.J. Hopfield // Phys. Rev. 128, p. 2135 (1962). 3. D.C. Reynolds and T.C. Collins, Excitons: their properties and uses. Academic, New York, 1981. 4. R.A. Mair, J. Li, S.K. Duan, J.Y. Lin, and H.X. Jiang // Appl. Phys. Lett. 74, p. 513 (1999). 5. J.J. Hopfield // Proc. 7-th Intern. Conf. on the Physics of Semiconductors, Paris, 1964 (Dunod Cie, Paris, 1964), p. 725. 6. R.R. Sharma and Sergio Rodriguez // Phys. Rev. 153, p. 823 (1967). 7. M. Suffczynski, W. Gorzkowski, and R. Kowal- czyk // Phys. Lett. 24A, p. 453 (1967). 8. T. Skettrup, M. Suffczynski and W. Gorzkowski // Phys. Rev. B 4, p. 512 (1971). 9. L. Stauffer and B. Stebe // Phys. Rev. B 39, p. 5345 (1989). 10. A.S. dos Santos, Mauro Masili, and J.J. De Groote // Phys. Rev. B 64, 195210 (2001). 11. I. Essaoudi, B. Stébé, and A. Ainane // Phys. Rev. B 64, 235311 (2001). 12. M. Katih, J. Diouri and E. Feddi // Phys. status solidi (b) 175, p. 349 (1993). 13. E. Feddi, F. Dujarding, J. Diouri, A. Elhassani, M. Katih and B. Stébé // Phys. status solidi (b) 201, 512 (1997). 14. H. Press William, P. Flannery Brian, A. Teukolsky Saul and T. Vetterling William, Numerical Recipes, Fortran Version (1989). 15. H.R. Hasse // Proc. Camb. Phil. Soc. 27, p. 66 (1932). 16. Daniel F. Blossey // Phys. Rev. B 2, p. 3976 (1970).