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Critical fluctuations and pseudogap observed in the microwave conductivity of Bi2Sr2CaCu2O8+delta, Bi2Sr2Ca2Cu3O10+delta, and YBa2Cu3O7-delta thin films (CROSBI ID 109570)

Prilog u časopisu | izvorni znanstveni rad | međunarodna recenzija

Peligrad, D.-N. ; Mehring, M. ; Dulčić, Antonije Critical fluctuations and pseudogap observed in the microwave conductivity of Bi2Sr2CaCu2O8+delta, Bi2Sr2Ca2Cu3O10+delta, and YBa2Cu3O7-delta thin films // Physical review. B, Condensed matter and materials physics, 69 (2004), 14; 144516, 12. doi: 10.1103/PhysRevB.69.144516

Podaci o odgovornosti

Peligrad, D.-N. ; Mehring, M. ; Dulčić, Antonije

engleski

Critical fluctuations and pseudogap observed in the microwave conductivity of Bi2Sr2CaCu2O8+delta, Bi2Sr2Ca2Cu3O10+delta, and YBa2Cu3O7-delta thin films

Critical fluctuations have been studied in the microwave conductivity of Bi2Sr2CaCu2O8+delta, Bi2Sr2Ca2Cu3O10+delta, and YBa2Cu3O7-delta thin films above T-c. It is found that a consistent analysis of the real and imaginary parts of the fluctuation conductivity can be achieved only if an appropriate wave vector or energy cutoff in the fluctuation spectrum is taken into account. In all of the three underdoped superconducting films one observes strong fluctuations extending far above T-c. The coherence length inferred from the imaginary part of the conductivity exhibits the static critical exponent nu=1 very close to T-c, and a crossover to the region with nu=2/3 at higher temperatures. In parallel, our analysis reveals the absence of the normal conductivity near T-c, i.e., fully opened pseudogap. Following the crossover to the region with nu=2/3, the normal conductivity is gradually recovered, i.e., the closing of the pseudogap is monitored.

short-wavelength cutoff ; single-crystals ; t-c ; thermodynamic fluctuations ; thermal fluctuations ; phase fluctuations ; superconductors ; transitions ; frequency ; behavior

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Podaci o izdanju

69 (14)

2004.

144516

12

objavljeno

1098-0121

1550-235X

10.1103/PhysRevB.69.144516

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Fizika

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