Theoretical studies of ⁶³Cu₂ + orbital Knight shifts of HgBa₂Ca₂Cu₃O₈+δ

The orbital Knight shifts and g factors for the tetragonal ⁶³Cu₂ + site in HgBa₂Ca₂Cu₃O₈+δ at 133 and 115 K are theoretically investigated based on the high-order perturbation formulae of these quantities for a 3d⁹ ion situated into tetragonally elongated octahedra. The theoretical results reveal go...

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Автори: Min-Quan Kuang, Shao-Yi Wu, Xian-Fen Hu
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Опубліковано: Фізико-технічний інститут низьких температур ім. Б.І. Вєркіна НАН України 2014
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Цитувати:Theoretical studies of ⁶³Cu₂ + orbital Knight shifts of HgBa₂Ca₂Cu₃O₈+δ / Min-Quan Kuang, Shao-Yi Wu, Xian-Fen Hu // Физика низких температур. — 2014. — Т. 40, № 8. — С. 869-872. — Бібліогр.: 21 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
id nasplib_isofts_kiev_ua-123456789-119586
record_format dspace
spelling Min-Quan Kuang
Shao-Yi Wu
Xian-Fen Hu
2017-06-07T15:09:37Z
2017-06-07T15:09:37Z
2014
Theoretical studies of ⁶³Cu₂ + orbital Knight shifts of HgBa₂Ca₂Cu₃O₈+δ / Min-Quan Kuang, Shao-Yi Wu, Xian-Fen Hu // Физика низких температур. — 2014. — Т. 40, № 8. — С. 869-872. — Бібліогр.: 21 назв. — англ.
0132-6414
PACS 74.25.N–, 75.10.Dg, 76.30.Fc
https://nasplib.isofts.kiev.ua/handle/123456789/119586
The orbital Knight shifts and g factors for the tetragonal ⁶³Cu₂ + site in HgBa₂Ca₂Cu₃O₈+δ at 133 and 115 K are theoretically investigated based on the high-order perturbation formulae of these quantities for a 3d⁹ ion situated into tetragonally elongated octahedra. The theoretical results reveal good agreement with the observed values. The significant anisotropies of the Knight shifts are illustrated as the considerable local tetragonal elongation distortions of the five-coordinated Cu²⁺ sites. The results at different temperatures are also discussed in view
This work was financially supported by the Sichuan Province Academic and Technical Leaders Support Fund and the Fundamental Research Funds for the Central Universities under granted No. ZYGX2012YB018.
en
Фізико-технічний інститут низьких температур ім. Б.І. Вєркіна НАН України
Физика низких температур
Свеpхпpоводимость, в том числе высокотемпеpатуpная
Theoretical studies of ⁶³Cu₂ + orbital Knight shifts of HgBa₂Ca₂Cu₃O₈+δ
Article
published earlier
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
title Theoretical studies of ⁶³Cu₂ + orbital Knight shifts of HgBa₂Ca₂Cu₃O₈+δ
spellingShingle Theoretical studies of ⁶³Cu₂ + orbital Knight shifts of HgBa₂Ca₂Cu₃O₈+δ
Min-Quan Kuang
Shao-Yi Wu
Xian-Fen Hu
Свеpхпpоводимость, в том числе высокотемпеpатуpная
title_short Theoretical studies of ⁶³Cu₂ + orbital Knight shifts of HgBa₂Ca₂Cu₃O₈+δ
title_full Theoretical studies of ⁶³Cu₂ + orbital Knight shifts of HgBa₂Ca₂Cu₃O₈+δ
title_fullStr Theoretical studies of ⁶³Cu₂ + orbital Knight shifts of HgBa₂Ca₂Cu₃O₈+δ
title_full_unstemmed Theoretical studies of ⁶³Cu₂ + orbital Knight shifts of HgBa₂Ca₂Cu₃O₈+δ
title_sort theoretical studies of ⁶³cu₂ + orbital knight shifts of hgba₂ca₂cu₃o₈+δ
author Min-Quan Kuang
Shao-Yi Wu
Xian-Fen Hu
author_facet Min-Quan Kuang
Shao-Yi Wu
Xian-Fen Hu
topic Свеpхпpоводимость, в том числе высокотемпеpатуpная
topic_facet Свеpхпpоводимость, в том числе высокотемпеpатуpная
publishDate 2014
language English
container_title Физика низких температур
publisher Фізико-технічний інститут низьких температур ім. Б.І. Вєркіна НАН України
format Article
description The orbital Knight shifts and g factors for the tetragonal ⁶³Cu₂ + site in HgBa₂Ca₂Cu₃O₈+δ at 133 and 115 K are theoretically investigated based on the high-order perturbation formulae of these quantities for a 3d⁹ ion situated into tetragonally elongated octahedra. The theoretical results reveal good agreement with the observed values. The significant anisotropies of the Knight shifts are illustrated as the considerable local tetragonal elongation distortions of the five-coordinated Cu²⁺ sites. The results at different temperatures are also discussed in view
issn 0132-6414
url https://nasplib.isofts.kiev.ua/handle/123456789/119586
citation_txt Theoretical studies of ⁶³Cu₂ + orbital Knight shifts of HgBa₂Ca₂Cu₃O₈+δ / Min-Quan Kuang, Shao-Yi Wu, Xian-Fen Hu // Физика низких температур. — 2014. — Т. 40, № 8. — С. 869-872. — Бібліогр.: 21 назв. — англ.
work_keys_str_mv AT minquankuang theoreticalstudiesof63cu2orbitalknightshiftsofhgba2ca2cu3o8δ
AT shaoyiwu theoreticalstudiesof63cu2orbitalknightshiftsofhgba2ca2cu3o8δ
AT xianfenhu theoreticalstudiesof63cu2orbitalknightshiftsofhgba2ca2cu3o8δ
first_indexed 2025-11-26T04:51:50Z
last_indexed 2025-11-26T04:51:50Z
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fulltext © Min-Quan Kuang, Shao-Yi Wu, and Xian-Fen Hu, 2014 Low Temperature Physics/Fizika Nizkikh Temperatur, 2014, v. 40, No. 8, pp. 869–872 Theoretical studies of 63 Cu 2+ orbital Knight shifts of HgBa2Ca2Cu3O8+δ Min-Quan Kuang, Shao-Yi Wu, and Xian-Fen Hu School of Physical Electronics, University of Electronic Science and Technology of China, Chengdu 610054, P.R. China E-mail: mqkuang@yeah.net Received February 17, 2014, revised March 13, 2014, published online June 23, 2014 The orbital Knight shifts and g factors for the tetragonal 63 Cu 2+ site in HgBa2Ca2Cu3O8+δ at 133 and 115 K are theoretically investigated based on the high-order perturbation formulae of these quantities for a 3d 9 ion situ- ated into tetragonally elongated octahedra. The theoretical results reveal good agreement with the observed val- ues. The significant anisotropies of the Knight shifts are illustrated as the considerable local tetragonal elonga- tion distortions of the five-coordinated Cu 2+ sites. The results at different temperatures are also discussed in view of the local structure of the Cu 2+ sites. PACS: 74.25.N– Response to electromagnetic fields; 75.10.Dg Crystal-field theory and spin Hamiltonians; 76.30.Fc Iron group (3d) ions and impurities (Ti–Cu). Keywords: g factors, Knight shifts, HgBa2Ca2Cu3O8+δ. 1. Introduction The Hg-based multilayered cuprate superconductors have become an important subject due to the unique Jo- sephson and magnetically couplings [1–3], magnetic [4] and resistivity and magnetization properties [5,6]. Usually, the Knight shifts of nuclear magnetic resonance (NMR) can demonstrate substantial information about the local structure and electronic properties of the copper-oxygen planes, which are helpful to the understandings of super- conductivity and other physical properties of this material. For instance, the Knight shifts were measured for the te- tragonal 63 Cu 2+ sites in HgBa2Ca2Cu3O8+δ with the transi- tion temperatures (Tc) (≈ 133 [7] and 115 [8] K, respec- tively), and the orbital Knight shifts K and K were obtained by extrapolation to zero temperature. However, these experimental results have not been theoretically ex- plained until now. On the other hand, the simple second- order perturbation formulae were normally utilized in the previous studies [9,10] on the Knight shifts of Cu 2+ sites in some high-Tc superconductors, while the higher (third- and fourth-) order perturbation contributions were not taken into account. Moreover, the previous calculations of Knight shifts did not connect with local structures of the magnetic sites but induced various adjusted energy separa- tions. In order to overcome the above shortcomings in the pre- vious researches and to study the Knight shifts of HgBa2Ca2Cu3O8+δ to a better extent, the high-order pertur- bation formulae of Knight shifts for a tetragonally elongated 3d 9 center are applied in this work. The theoretical calcula- tions are carried out by correlating with the local structure of the tetragonal Cu 2+ site using the superposition model. 2. Theory and calculations The Knight shifts measured at low temperatures [7,8] can be ascribed to the tetragonal 63 Cu 2+ site in HgBa2Ca2Cu3O8+δ. This site is coordinated to five oxygen ions forming a tetragonally elongated octahedron (i.e., one of the apical ligands of the octahedron is moved to infinity) [11]. For a Cu 2+ (3d 9 ) ion in a tetragonally elongated octa- hedron, the original cubic 2 Eg ground state may split into two orbital singles 2 B1g (or |ε >) and 2 A1g (or |θ >). The former is the lowest level, corresponding to the observed Knight shifts ( K K [7,8]). Meanwhile, the original cubic 2 T2g exited state can be separated into an orbital sin- glet 2 B2g (or | ζ >) and a doublet 2 Eg (or | ξ > and |η >) [12,13]. As for the previous studies on Knight shifts [9,10], the orbital contributions from the susceptibility were nor- mally insufficiently involved, and the third- and fourth- order perturbation contributions were not considered. Fur- thermore, the previous treatments failed to establish quan- titative relationships between g factors and Knight shifts. To remove the shortcoming of the previous simple se- cond-order perturbation calculations, the high (third- and Min-Quan Kuang, Shao-Yi Wu, and Xian-Fen Hu 870 Low Temperature Physics/Fizika Nizkikh Temperatur, 2014, v. 40, No. 8 fourth-) order perturbation formulae [14] are adopted here for a tetragonally elongated 3d 9 center. Despite absence of experimental g factors, the unified studies of Knight shifts and g factors are performed in this work, since g factors are also closely relevant to the local structure of the sys- tem. In view of the related investigations [7–10] on Knight shifts and g factors, one can obtain the proportionality rela- tionships between Knight shifts Ki and g shifts (gi – gs, with i = || and ). Thus, the perturbation formulae of these quantities can be expressed as follows: ____________________________________________________ 2 2 3 2 3 3 2 2 2 2 2 2 2 3 1 1 2 1 22 1 2 2 1 2 1 2 1 2 2 8 4 1 1 4 1 2 1 1 1 2 , 2 2 s s s k k k k g g g k g E E E E EE E E E E E E E E E E 22 2 3 3 1 2 2 3 2 1 2 2 1 2 2 1 2 2 12 1 2 1 2 2 22 4 2 1 2 1 1 2 1 1 1 , 2 2 2 2 s s s gk k k k g g g E E E E E E E E E E EE E E E E E 2 2 –3 3 2 2 2 2 1 1 2 1 22 1 2 2 8 4 1 1 4 1 2 2 A B d s k k k k K N r g E E E E EE E E E 2 2 2 2 2 3 1 2 1 2 1 2 2 2 1 1 1 2 2 sk g E E E E E E E , 2 2 –3 3 2 1 2 2 1 2 2 1 2 2 1 2 4 2 1 2 1 1 2 2 2 A B d k k k k K N r E E E E E E E E E E E 2 2 2 2 3 1 1 2 1 2 2 2 1 1 1 2 2 2 s s g g E E E E E E . (1) _______________________________________________ In the above expressions, gs (≈ 2.0023) is the pure spin value, k is the orbital reduction factor, is the spin-orbit coupling coefficient for the 3d 9 ion in crystals, which is usually expressed in terms of the corresponding free-ion value 0 as ≈ k 0; NA is the Avogadro’s number, and μB is the Bohr magneton. <r –3 >3d is the expectation value of inverse cube of the Cu 2+ 3d radial wave function. The denominators E1 and E2 in the above expressions are the energy separations between the excited 2 B2g and 2 Eg and the ground 2 B1g states, respectively. They can be written in terms of the cubic field parameter Dq and the tetragonal field parameters Ds and Dt using the energy ma- trices for a tetragonal 3d 9 center [15]: 1 210 , 10 – 3 5q q s tE D E D D D , (2) The structure of the Cu 2+ site in HgBa2Ca2Cu3O8+δ is characterized by one bond length R along horizontal c axis and four bond lengths R along vertical a and b axes [16]: R ≈ 2.741 and 2.786 Å and R ≈ 1.9239 and 1.9273 Å for the Hg-1223 systems with Tc (≈ 135 and 107 K, close to 133 and 115 K, respectively, for those un- der study). Then the tetragonal field parameters are de- duced from the superposition model using the local geome- try of the system [17]: 2 2 2  2 2 /7, t t s R R D A R R 4 4 4 16 2 /21 . t t t R R D A R R (3) Here t2 ≈ 3 and t4 ≈ 5 are the power-law exponents [17], 2A and 4A are the intrinsic parameters, with the reference distance of the average Cu 2+ –O 2– bond length: 4 /5.( )R R R R For octahedral 3d n ions in com- pounds, the relationships 4   3 4( )/ qA D and 2 410.8A A [17–20] have been proved suitable for many systems and are reasonably adopted here. From the optical spectral data for Cu 2+ in some oxides [13], the cubic field parameter Dq (≈ 1300 cm –1 ) and the orbital reduction factor k (≈ 0.63) can be obtained for the Cu 2+ site in HgBa2Ca2Cu3O8+δ. The free-ion value of the spin-orbit coupling coefficient is 0 ≈ 829 cm –1 [15] for Cu 2+ . Substituting these values into Eq. (1), the g factors and Knight shifts are calculated and given in Table 1. Theoretical studies of 63 Cu 2+ orbital Knight shifts of HgBa2Ca2Cu3O8+δ Low Temperature Physics/Fizika Nizkikh Temperatur, 2014, v. 40, No. 8 871 3. Discussions From Table 1, one can find that the g factors and Knight shifts based on the high-order perturbation formu- lae in this work exhibit reasonable agreement with the ex- perimental data, and these observed values are also suita- bly explained in a uniform way. 1. In the present calculations, the theoretical relationships between Knight shifts (and g factors) and the local structure of the tetragonal 63 Cu 2+ site in HgBa2Ca2Cu3O8+δ are es- tablished from the superposition model. So the imperfection of the previous treatments [9,10] based on the simple se- cond-order perturbation formulae using various adjustable energy separations is thus overcome. Notably, the positive anisotropy 0( )–K K of Knight shifts is consistent with that 0( )–g g of g factors, with the ratio – / – 6) %( ) (K K g g due to the linear relationships between g-shifts and Knight shifts. Moreover, the aniso- tropies of g factors and Knight shifts can be illustrated as the local tetragonal elongation of the 63 Cu 2+ site, characterized by one longer parallel Cu–O bond than the four perpendicu- lar ones. In fact, the local tetragonal elongation of this site can be described as the relative elongation ratios ( )– / 31R R R and 33% for the studies systems with Tc of 133 and 115 K, respectively. The highest Tc of the optimally doped Hg-1223 systems among multilayer cuprate super- conductors is attributable to the intense hybridization of the 2 2Cu(3 ) O 2 Cu(4( ) ) x y d p s electron clouds arising from the long copper-apical oxygen bond lengths R and flat CuO2 planes and remarkable antiferromagnetic spin fluctuations in the pairing mechanism [7,8]. In addition, the theoretical g factors in this work remain to be verified with further experimental measurements. 2. The g factors and orbital Knight shifts investigated here correspond to the temperatures slightly lower than Tc (≈ 133 and 115 K). The quantities used in the calculations (e.g., the energy denominators E1 and E2, the spin-orbit coupling coefficient ζ, the cubic field parameters Dq and the orbital reduction factors k (≈ N)) reflect the local ligand fields around copper sites and the Cu 2+ –O 2– orbital admix- tures (covalency) of the [CuO5] 8– clusters formed by the localized Cu 2+ (3d 9 ) and the nearest neighbour oxygen lig- ands with specific local structural data (e.g., the distinct bond lengths) at the relevant temperatures. So, the above parame- ters actually contain implicitly the respective contributions at the corresponding temperatures, and thus temperature T does not appear explicitly in the detailed calculations. 3. The errors of the present calculations may be dis- cussed as follows. First, the approximations of the theoret- ical model and formulae would bring forward some errors. Second, the errors also arise from the approximation of the relationship 2 410.8 ,A A which may affect the tetragonal field parameters and the final results. The errors for the resultant Knight shifts are estimated to be not more than 3% when the ratio 2 4/A A varies by 10%. Third, the calcu- lations of this work are performed on the basis of the con- ventional crystal-field model where the ligand orbital and spin-orbit coupling contributions are ignored. In view that the studied Cu 2+ –O 2− combination has much smaller lig- and spin-orbit coupling coefficient (≈ 151 cm –1 [21]) as compared to that (≈ 829 cm –1 [15]) of Cu 2+ , the above ligand contributions can be regarded as very small and negligible. 4. Conclusion The g factors and orbital Knight shifts are theoretically calculated for the tetragonal Cu 2+ sites in the Hg-1223 sys- tems for temperatures slightly lower than Tc (≈ 133 and 115 K). The significant anisotropies of the Knight shifts are illustrated as the considerable tetragonal elongations of the five-coordinated Cu 2+ sites. The higher Tc of the optimally doped Hg-1223 than other multilayer cuprate superconduc- tors may be attributed to the stronger hybridization of the 2 2Cu(3 ) O 2 Cu(4( ) ) x y d p s electron clouds arising from the longer copper–apical oxygen bond lengths and flatter CuO2 planes and more significant antiferromagnetic spin fluctuations in the pairing mechanism of cuprates. It appears that the present 63 Cu Knight shift analysis can be helpful to the further understandings of the electronic states and superconductivity of Hg-1223 systems. Acknowledgment This work was financially supported by the Sichuan Province Academic and Technical Leaders Support Fund and the Fundamental Research Funds for the Central Uni- versities under granted No. ZYGX2012YB018. 1. J.D. Dow and D.R. Harshman, J. Vac. Sci. Technol. B 24, 1977 (2006). 2. Y. Hirata, K.M. Kojima, S. Uchida, M. Ishikado, A. Iyo, H. Eisaki, and S. Tajima, Physica C 470, S44 (2010). 3. A. Crisan, A. Iyo, Y. Tanaka, H. Matsuhata, D.D. Shivagan, P.M. Shirage, K. Tokiwa, T. Watanabe, T.W. Button, and J.S. Abell, Phys. Rev. B 77, 144518 (2008). 4. E. Kandyel and K.M. Elsabawy, Physica C 468, 2322 (2008). 5. R. Giri, G.D. Verma, S.K. Malik, D. Kundaliya, R.S. Tiwari, and O.N. Srivastava, J. Alloy. Compd. 366, 254 (2004). 6. O. Babych, Ya. Boyko, I. Gabriel, R. Lutciv, M. Matviyiv, and M. Vasyuk, Acta. Phys. Pol. A 117, 27 (2010). Table 1. The g factors and Knight shifts (in %) for the tetra- gonal 63 Cu 2+ sites in HgBa2Ca2Cu3O8+δ T, K Ref. g g K K 133 Calc. 2.21 2.04 1.22 0.24 Exp. [7] – – 1.22(2) 0.22(2) 115 Calc. 2.20 2.04 1.14 0.22 Exp. [8] – – 1.16 0.19 Min-Quan Kuang, Shao-Yi Wu, and Xian-Fen Hu 872 Low Temperature Physics/Fizika Nizkikh Temperatur, 2014, v. 40, No. 8 7. K. Magishi, G.Q. Zheng, Y. Kitaoka, K. Asayama, K. Tokiwa, A. Iyo, and H. Ihara, Physica C 263, 375 (1996). 8. M.H. Julien, P. Carretta, M. Horvatic, C. Berthier, Y. Bert- hier, P. Ségransan, A. Carrington, and D. Colson, Phys. Rev. Lett. 76, 4238 (1996). 9. M. Itoh, S. Hirashima, and K. Motoya, Phys. Rev. B 52, 3410 (1995). 10. M. Itoh, M. Sugahara, T. Yamauchi, and Y. Ueda, Phys. Rev. B 53, 11606 (1996). 11. D.C. Johnston, A.J. Jacobson, J.M. Newsaw, J.T. Lewan- dowski, D.P. Goshorn, D. Xie, and W.B. Yelon, Am. Chem. Soc. Symposium Ser. 351, 136 (1987). 12. A. Abragam and B. 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