Magnetoconductivity of Bi2Sr2Ca1−xYxCu2O8+δ in fluctuation regime C. P. Dhard, S. N. Bhatia, P. V. P. S. S. Sastry, J. V. Yakhmi, and A. K. Nigam Citation: J. Appl. Phys. 76, 6944 (1994); doi: 10.1063/1.358082 View online: http://dx.doi.org/10.1063/1.358082 View Table of Contents: http://jap.aip.org/resource/1/JAPIAU/v76/i10 Published by the American Institute of Physics. Related Articles Frequency dependent dielectric properties of Cu0.5Tl0.5Ba2Ca2(Cu3-yMy)O10-δ superconductor J. Appl. Phys. 111, 013920 (2012) Enhancement of superconducting properties in FeSe wires using a quenching technique J. Appl. Phys. 111, 013912 (2012) Transport properties of superconducting MgB2 composites with carbon-encapsulated Fe nanospheres J. Appl. Phys. 110, 123921 (2011) Organization of flux line system and voltage oscillations in superconducting MgB2 J. Appl. Phys. 110, 113917 (2011) Magnetic pinning of flux lattice in superconducting-nanomagnet hybrids Appl. Phys. Lett. 99, 182509 (2011) Additional information on J. Appl. Phys. Journal Homepage: http://jap.aip.org/ Journal Information: http://jap.aip.org/about/about_the_journal Top downloads: http://jap.aip.org/features/most_downloaded Information for Authors: http://jap.aip.org/authors Downloaded 01 Mar 2012 to 14.139.97.76. Redistribution subject to AIP license or copyright; see http://jap.aip.org/about/rights_and_permissions Magnetoconductivity of BipSr2Cal +JxCu20s+s in fluctuation regime C. P. Dhard and S. N. Bhatia Department of Physics, Indian Institate of Technology, Bombay 400 076, India P. V. P. S. S. Sastty and J. V. Yakhmi Chemistry Division, Bhabha Atomic Research Centre, Bombay 400 085, India A. K. Nigam Tata Institute of Fundamental Research, Bombay 400 005 India The magnetoconductivity of polycrystalline Bi,Sr,Ca,-,Y,Cu,Os+& x=0,0.05 and 0.20 samples in the magnetic field of 4 T was measured. The excess conductivity has been analyzed in the light of Aronov-Hikami-Larkin and Bieri-Maki formalisms together with Thompson’s correction of the Zeeman term of both theories. The later theory was found within the clean limit to describe the data adequately and yielded the estimate for the phase braking time r+=lX10-13 s. The Maki-Thompson-Zeeman contribution (Aot,,rrJ in these samples is found to be negligible. The short coherence length coupled with the high transition temperature provide an excellent opportunity to study the rounding of the transition in the oxide superconductors. The fluctuation enhanced conductivity, i.e., excess conductivity (Aaj in zero field is representable by the AslamazovLarkin (AL) and Maki-Thompson (MT) terms.’ The magnetic field affects the excess conductivity through the orbital angular momentum giving rise to AL-orbital (AUK) and MT-orbital (ho,) terms and through the spin angular momentum yielding ALZeeman (ho& and MT-Zeeman (AC& terms. Aronov, Hikami, and Larkina (,AHL) have derived the expressions for these terms from the standard theory in the dirty limit. However this theory is not applicable to high T, superconducting (HTSC) materials as they fall within the clean limit with the mean free path Z*&,(O) [Z-100 A and tab(O)=15 A for YBa,Cu,O, (YBCO)]. Later Bieri and Maki3 (BM) proposed another theory of ha(H) which was valid for the clean limit but it gave results identical to the AHL theory. Both AL contributions are not sensitive to the mean free path of the electrons. Therefore, their values remain essentially unchanged in both dirty and clean limits. However the MT contribution depends sensitively on I since the vertex renormalization is essentially controlled by I in the clean limit. The expressions obtained by Bieri and Maki3 in this limit for all the four terms are identical to the AHL expressions with the difference that the terms AoALz and Ao,, had (o,/4~-kT)~ instead of ( w,/~&T,)~ as their prefactors and S was defined by S=1.203[1/&,(0)] S&, where S,, is given by (Ref. 2) SAHL=16&O)kT7,$rrd2~. Later it was pointed out by Thompson4 that both these theories were wrong in treating the Zeeman splitting energy, correction to this leaves the three terms, viz., Au,,, AC-, and Aotiz unchanged but modifies the fourth Au,. Experimentally almost all the attention appears to have been focused on YBCO only and to the best of our knowledge no attempt has been made to study the Bi,Sr,CaCu,Os+, (BSCCO) system in this light. Earlier Matsuda et aL5 analyzed the magnetoconductivity of YBCO thin t%ns in terms of AHL formalism without Thompson correction. All four contributions were required giving the value of the phase breaking time ~-+=10-‘~ s at 100 K. However Semba et al.” found no evidence for the hoin their 6944 J. Appl. Phys. 76 (lo), 15 November 1994 data on single crystals of YBCO. They found 7+==5X lo-r4 s which is the shortest time reported so far. Sugawara et al.’ have analyzed their Au(H) data measured on chemical vapor deposition (CVD) films of YBCO in BM theory with Thompson’s correction’ (BMT), and find the bow, term to be essential in both the ho-(H) vs E [= (T- T’ff)/TFf, TFf is the mean field transition temperature] as well as Au(H) vs H data. In polycrystalline YBCO Matsuda et aZ.’ also found vanishing values of ACT,, using uncorrected AHL expressions. And our recent analysis on similar samples in the light of corrected AHLJBM expressions support these results.” We have measured the magnetoconductivity of polycrystalline Bi,Sr&a, -,Y,Cu20s+ 6 samples with x =O, 0.05, and 0.20 and find the ACT,, contribution to be negligible. The samples were prepared by the matrix precursor method by reacting B&O, with a Sr,CaCu20s precursor in the presence of O2 at 900-950 “C. All the samples were confirmed to be of single phase by x-ray diffraction (XRD). dc conductivity was measured by the four probe method on bar shaped samples.’ The current density used was typically 0.1 A/cm’. Samples were so oriented that the measuring current was perpendicular to the applied field. The sample temperature was measured with a Si diode/CGR thermometer, placed in contact with the sample in a copper holder, and was raised at the rate of 2 K/h. The data were taken at the interval of 20 mK within the transition region. At high temperatures (T&2T,) the zero field and the field data coincide for all the samples implying negligible magnetoresistance to be present in the normal state and below TFf the transition broadens in the field. A field of 4 T was used because for the higher fields the orbital terms show deviations from the H2 behavior predicted by the above theories.“73 In zero field, a single sharp peak in dp/dT is symmetrical about the temperature T,, of its maximum, whereas in the field this curve spreads towards lower temperatures. This spread is around 35 K for x=0 and increases further with the Y concentration. We have analyzed the total fluctuation conductivity where A q(H) = [ 4H, T> - g,(H, VI aAH, T) = lIp,(H,T) is the background conductivity. Agf(H) contains the zero field conductivity (Ref. 11) Ao-(O) and the modifications produced in it by the magnetic field. The estiQ 1994 American Institute of Physics Downloaded 01 Mar 2012 to 14.139.97.76. Redistribution subject to AIP license or copyright; see http://jap.aip.org/about/rights_and_permissions Bi2SrZCa TAJ3LB I. Various fitted physical parameters for BSCCO samples in the clean and dirty limit. r+, r, and I are calculated at 100 K. In BM, L(O) and &b(O) are constants, whereas in BMT-d(dirty) and BMT-c(clean) these are temperature dependent. E,(O) i& &b(O) (4 7 1 (lo-14 9) t-4 3 (lo-‘3 s) x=0 AHL. BM BMT-d BMTc 1.9 2.3 1.8 1.8 10.0 9.1 9.9 8.9 1.0 1.3 0.81 0.11 1.0 5.3 0.13 5.3 9.8 52.5 x=0.05 AHL BM BMT-d BMT-c 2.5 2.6 1.8 1.8 11.4 10.2 9.9 8.6 4.0 1.7 0.86 0.12 1.1 5.3 0.16 5.3 11.0 58.6 x=0.20 AI-E BM BMTd BMlk CU,O,+~ h6t 10000 MT AL h ‘E ALZ MTZ 3.2 3.1 1.9 1.9 12.8 11.8 10.4 10.4 6.0 2.0 0.86 0.12 1.3 5.3 0.18 5.3 1994 \\ \ 11.5 61.2 mation of background conductivity u,(H,T) have been discussed in detail in Ref. 1. The experimental data of AnAH, T) of x=0 was first fitted to the combined expressions of zero field AL and MT terms and field dependent AHL expressions of AL and MT terms with Thompson’s correction by taking &(O), ,$,(O), and Q-$as the adjustable parameters. r+ was assumed to vary as r#=r&T where 7fl is a constant. The values of fitted parameters are shown in Table I. Good agreement can be obtained with &(0)=1.9 & &,(O)=lO.O A, and r4=1X10-r3 s. The value of E,(O) agreed with that obtained from the zero field data.’ The agreement further improved when BM equations with Thompson’s correction were used and the mean free path 1 was allowed to vary with temperature as I= lo/T where 1, is a constant. Here in the clean limit &(O), .&CO), and Z,,T~ were taken as the free parameters. &(O) slightly increased to 2.3 A and &(O) decreased to 9.1 A. We obtained Zo7~=6.8X10-8 A s. To get an estimate of r+ from this product, we note that I= mF= r,,uF/T (i.e., Ia= rOuF) where r is the transport relaxation time and bF the Fermi velocity of the carriers. The later is estimated as (0.6-1.6)X107 cm/s from the relation &,(O) =fiu,JaA with the in-plane energy gap parameter givenr’ by 2A.ikT,=3.5-8. Now assuming r$=~ this product yields r+ (100 K)-1.3X10-r3 s for the lowest estimate of uF, i.e., uF=O.SX~O~ cm/s. This compares well with the value obtained by Sugawara et aL7 Batlogg,‘” from the resistivity data, has obtained r=fifl.35kT=5.4X 10-12fT. With ~~-10~ cm/s, this yields r+( 100 K)-5X10-14 s from our estimates of ZOrfl and the rdr comes out to be -2.3. BMT? have further also assumed E(O) and tab(O) to be temperature dependent along with I, for both dirty and clean limits. Assuming these temperature variations, values of the parameters obtained are listed in Table I. Both the limits give identical values of &(O) as 1.8 A whereas &,(O) works out to be =9 A and 210 A for the dirty and clean limits, respecJ. Appl. Phys., Vol. 76, No. 10, 15 November \ 4 sr2cao95 y,.,, cu, 0, +A I 1000 1 ‘c: F t MT0 kk 100 b a 10 :/ , eps FIG. 1. Fluctuation and magnetoconductivity of BSCCO n=O and 0.05 in (a) and (b). In (a) &(O) and cob(O) are temperature dependent while in (b) they are constants. Note the change in relative order of AJ-Z and MT0 contributions in (a) and (b). All the four contributions to Ao((N,T), i.e., AL.0, MTO, ALZ, and MTZ and the excess magnetoconductivity Au,,, displayed here, are negative in magnitude. tively, at 100 K. These values agree with those obtained by BMT on single crystals of YBCO. Our analysis yields r+fFO.2 and uF= 7X106 cm/s for the clean limit using the Batlogg’s” value of r. This is the clean limit r and therefore Dhard et al. Downloaded 01 Mar 2012 to 14.139.97.76. Redistribution subject to AIP license or copyright; see http://jap.aip.org/about/rights_and_permissions 6945 cannot be used in the dirty limit as has been used conventionally. To estimate 7 in the dirty limit we assumed vF=1X107 cm/s. We get r+=1X10-r3 and r in this Iimit=~~=1.3X10-‘5 s. Thus r,Jrd=62. This ratio is too large. rd appears to be too small, its reasonable value should be a smaller fraction of Q-.If uF is reduced further the ratio rdr also gets reduced but it still remains too high. In the case of AHL r is also very small. As this theory is valid for the dirty case, 1 wilI be -&,(O). With ~~-10~ cm/s this yields r6-lX10-r4 s and rdrd=lO. Two points are to be noted about this analysis. The data has been fitted over the range O.OlGeGO.2 and the nonlocal effects have not been included. These effects apparently become visible at eaO.25 as shown by BMT. The magnetoconductivity obtained by subtracting hum(O) and AU-~(O) from Auf(H,T) is displayed in Fig. l(a) along with the calculated values of the four field depenhas the smallest value over the dent contributions. Arm entire E range, being less than 1% of the total Au-~(H,T). The fit does not deteriorate when the term Auis dropped altogether. However the rms deviation jumps when the next is dropped. This result is in conformity larger term Au,, with our previous conclusionlo on polycrystalline YBCO (measured at 4 T) and with Semba et aL6 and Matsuda et al.’ who also found ACT- to be negligible in their magnetoconductivity of single crystal and polycrystalline YBCO, respectively, measured at 1 T. However Sugawara et al.’ found this term to be present as a substantial fraction of the total magnetoconductivity at 13 T. Since the BMT equations predict each of the four contributions to be proportional to -H2, the Au-, i.e., the ratio relative magnitude of Au~(Au~,+Au,,+Au~+Aumz) will not increase with H and will be a function of E and r6, only. In actual practice since Aum and Aumo show some saturation at high fields near T,(at 60.015) the ratio may increase at such fields. For the present data the equations predict the ratio to be less than 1% over the entire E range of the data, i.e., for 0.05~~GO.2, and to remain at negligible levels even when r+ is increased to =10-t3 s. The anisotropy ratio (AuM~+Au,)/(Aum+Aum+Au~-t-AumJ works out to be 5.6 at e=O.O5 and AuMTz forms 10% of this ratio. The magnetoconductivity of the x=0.05 and 0.20 6946 samples behaves identically. The plot for x =0.05 is shown in Fig. l(b). Aumz here is also negligible and the neglect of this term does not alter the fits in any of these samples. Though the AHL theory gives reasonable estimates of r$, it underestimates r thus yielding a very large value for the ratio rdr. This ratio is similarly overestimated in the BMT dirty limit and underestimated in its clean limit. Only when E(O) and &,(O) are taken as temperature independent does this theory yield reasonable estimates of rdr. The values are listed in Table I. All the parameters, viz., r+, t,(O) and .E&,(O)~etc., increase systematically with Y concentration. r4 shows a slight increase with Y doping but still Aa,, remains negligible. However this increase in r+ increases the magnitude of the Aa,, relative to those of the other two. Instead of being the smallest term as in the Y-free sample, it and becomes the second largest term. over takes AuIn summary our analysis of the magnetoconductivity of Y-doped polycrystalline BSCCO suggests the absence of Aucontributions for the fields up to 4 T. The other three terms Au,, , Au,, , and Au, all contribute significantly. Due to the absence of AaM,, the validity of the Thompson correction could not be verified. Though BMT theory appears to agree with experiments, for a better estimate of r+ prior knowledge of some of the parameters, E(O), &(O), or VF, will be useful. Data further appear to favor the temperature independent value of c,(O) and &(O) and discard their functional forms given by the BMT equations. ’S. N. Bhatia and C. P. Dhard, Phys. Rev. B 49, 12206 (1994). 2A. G. Aronov, S. Hikami, and A. I. Iarkin, Phys. Rev. Lett. 62, 965 (1989); 62, 2336(E) (1989). 3J. B. Bieri and K. Maki, Phys. Rev. B 42,4854 (1990). 4R. S. Thompson, Phys. Rev. Lett. 66, 2280 (1991). ‘Y. Matsuda, T. Hiiai, S. Komiyama, T. Terashima, Y. Bando, K. Iijima, K. Yamamoto, and K Hirata, Phys. Rev. B 40, 5176 (1989). 6K. Semba, T. Ishii, and A. Matsuda, Phys. Rev. L&t. 67, 769 (1991). ‘5. Sugawara, H. Iwasaki, N. Kobayashi, H. Yamane, and T. Hirai, Phys. Rev. B 46, 14 818 (1992). ‘J. B. Bieri, K. Maki, and R. S. Thompson, Phys. Rev. B 44,4709 (1991). “A. Matsuda and K. Semba, Physica C 185189,797 (1991). taS. N. Bhatia and C. P. Dhard, Physica C (to be published). US. Hikami and A. I. Larkin, Mod. Phys. Lett. B 2, 693 (1988). tzB. Batlogg, in High Temperature Superconductors, edited by K. S. Bedell ef al. (Addison-Wesley, Redwood City, 1990), p. 37. J. Appl. Phys., Vol. 76, No. IO, 15 November 1994 Downloaded 01 Mar 2012 to 14.139.97.76. Redistribution subject to AIP license or copyright; see http://jap.aip.org/about/rights_and_permissions Dhard et al.
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