Magnetic properties of high-T[subscript c] superconductors

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1992
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Gohng, Junho
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Douglas K. Finnemore
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Physics and Astronomy
Physics and astronomy are basic natural sciences which attempt to describe and provide an understanding of both our world and our universe. Physics serves as the underpinning of many different disciplines including the other natural sciences and technological areas.
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Abstract

Magnetic properties of high-T[subscript] c superconductors have been studied in order to determine the free-energy surface, the characteristic critical fields, order parameters structure, and the grain size effect on magnetization. Studies of the thermodynamic reversibility for YBa[subscript]2Cu[subscript]3O[subscript]7-[delta] show the rounding in magnetization vs. temperature curves is a reflection of the thermodynamic fluctuations near T[subscript] c. Specific heat jump C(0)-C(H) values that have been calculated from the free-energy surfaces show good agreement with the direct calorimetric measurements;Comparative studies of the free-energy surfaces, flux creep and critical currents for both melt-textured and grain-aligned YBa[subscript]2Cu[subscript]3O[subscript]7-[delta] samples have been undertaken in order to evaluate the difference caused by different micro structures in these samples. The free energy per unit length of a vortex is found to be essentially the same in the melt-textured sample as for the single crystals in the grain-aligned sample, suggesting that the line energy is the same for these rather different samples. The specific heat jump values calculated from the free-energy surfaces also show close agreement between the two samples;Magnetic field and temperature dependence of the average Ginzburg-Landau order parameter \langle f\rangle is evaluated by fitting the magnetization data of grain-aligned YBa[subscript]2Cu[subscript]3O[subscript]7-[delta] to the Hao-Clem model in the region of thermodynamic reversibility. H[subscript] c(T) and H[subscript] c2(T) were also determined from the fitting along with the [kappa][subscript] c(T) values. The study reveals that [kappa][subscript] c is a slowly decreasing function of temperature near T[subscript] c. Fittings of the same model to Bi[subscript]2Sr[subscript]2Ca[subscript]2Cu[subscript]3O[subscript]10 have been carried out. The 2-D nature of bismuth family superconductors introduces some difficulties in applying Hao-Clem model and it is discussed in comparison with YBa[subscript]2Cu[subscript]3O[subscript]7-[delta] results;Lastly, studies on the grain size effect on free energy and specific heat jump in grain aligned YBa[subscript]2Cu[subscript]3O[subscript]7-[delta] samples show that the free energy is reduced by about 15% as the average grain size changes from 37.5 to 12.7 [mu]. The twin spacing d is related to the average grain size D by d∝√D and is thought to be the major factor that causes the decrease in the free energy.

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Wed Jan 01 00:00:00 UTC 1992