We have used scanning SQUID magnetometry to image vortices in ultrathin Ba0:9Nd0:1CuO2xm= CaCuO2n high temperature superconductor samples, with as few as three superconducting CuO2 planes. The Pearl lengths ( 22 L=d, L the London penetration depth, d the superconducting film thickness) in these samples, as determined by fits to the vortex images, agree with those by local susceptibility measurements, and can be as long as 1 mm. The in-plane penetration depths ab inferred from the Pearl lengths are longer than many bulk cuprates with comparable critical temperatures.We speculate on the causes of the long penetration depths, and on the possibility of exploiting the unique properties of these superconductors for basic experiments.

Penetration depths of artificially layered [Ba0.9Nd0.1CuO2+x]m/[CaCuO2]n systems / Tafuri, Francesco; Kirtley, J. R.; Medaglia, P. G.; Orgiani, P.; Balestrino, G.. - In: PHYSICAL REVIEW LETTERS. - ISSN 0031-9007. - 92:(2004), pp. 157006-157009. [10.1103/PhysRevLett.92.157006]

Penetration depths of artificially layered [Ba0.9Nd0.1CuO2+x]m/[CaCuO2]n systems

Tafuri, Francesco;
2004

Abstract

We have used scanning SQUID magnetometry to image vortices in ultrathin Ba0:9Nd0:1CuO2xm= CaCuO2n high temperature superconductor samples, with as few as three superconducting CuO2 planes. The Pearl lengths ( 22 L=d, L the London penetration depth, d the superconducting film thickness) in these samples, as determined by fits to the vortex images, agree with those by local susceptibility measurements, and can be as long as 1 mm. The in-plane penetration depths ab inferred from the Pearl lengths are longer than many bulk cuprates with comparable critical temperatures.We speculate on the causes of the long penetration depths, and on the possibility of exploiting the unique properties of these superconductors for basic experiments.
2004
Penetration depths of artificially layered [Ba0.9Nd0.1CuO2+x]m/[CaCuO2]n systems / Tafuri, Francesco; Kirtley, J. R.; Medaglia, P. G.; Orgiani, P.; Balestrino, G.. - In: PHYSICAL REVIEW LETTERS. - ISSN 0031-9007. - 92:(2004), pp. 157006-157009. [10.1103/PhysRevLett.92.157006]
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11588/662795
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