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pdf, 9 MiB - Infoscience - EPFL

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Chapter 1<br />

Introduction<br />

1.1 History of high temperature superconductivity<br />

In 1986 superconductivity was found in a range of temperature which was well<br />

above all previous signature: Bednorz and Müller found a transition temperature<br />

of about 30K [1] in the layered copper-oxide material La 2−x Ba x CuO 4 ,forwhich<br />

they won the Nobel Prize in Physics. The psychological barrier of the liquid<br />

Nitrogen condensation temperature was crossed shortly after with YBaCu 3 O 7<br />

and the hope was growing that one might find an increasing number of every-day<br />

life applications.<br />

Since then, copper-oxide superconductors, which are structural derivatives of<br />

the class of perovskites, have been at the center of a tremendous scientific activity.<br />

A number of high-temperature superconducting compounds has been reported.<br />

Starting out at T c =30K for La 2−x Ba x CuO 4 in 1986 the transition temperatures<br />

have climbed to T c = 156K in members of the HgBa 2 CuO 4+x family which are<br />

among the recently discovered compounds. Moreover, new materials found more<br />

recently like the mercury-type copper-oxides still increased accessible transition<br />

temperatures without any obvious upper bound, and a critical temperature as<br />

high as 164K was reported [2], though it was obtained for a compound under<br />

pressure. In the meantime, progress in the preparation of high-quality single<br />

crystals has allowed to remove many of the uncertainties in the interpretation of<br />

experimental data obtained from polycrystals. In Fig. 1.1 we show the lattice<br />

structure of an YBCO perovskite structure. Despite the apparent complexity of<br />

the structures of the different cuprates compounds, they all have two dimensional<br />

CuO 2 planes. In essence all the high-temperature superconductors (HTCS) consist<br />

of two-dimensional CuO 2 planes which are sandwiched between intervening<br />

atomic layers. These layers are composed mostly out of alkaline-earths, rareearths,<br />

oxygen and halogenides. Depending on the number of CuO 2 planes per<br />

unit cell the materials have a single , a double-, or a triple-plane form as in<br />

15

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