Characteristic length for pinning force density in $Nb{_3}Sn$
Abstract
The pinning force density (where is the critical current density and is the magnetic field) is one of the main parameters that characterize the resilience of a superconductor to carry a dissipative-free transport current in an applied magnetic field. Kramer (1973 J.Appl.Phys. 44 1360), and Dew-Hughes (1974 Phil.Mag. 30 293) proposed a widely used scaling law for the pinning force density amplitude: , where , , , and are free-fitting parameters. Since the late 1970-s till now, several research groups have reported experimental data on the dependence of on the average grain size, , in -based conductors. Godeke (2006 Superc.Sci.Techn. 19 R68) proposed that the dependence obeys the law . However, this scaling law has several problems, for instance, the logarithm is taken from a non-dimensionless variable, and for large grain sizes and for . Here we reanalysed the full inventory of publicly available data for conductors and found that the dependence can be described by law, where the characteristic length, , varies within a remarkably narrow range, that is, , for samples fabricated by different technologies. The interpretation of the result is based on the idea that the in-field supercurrent flows within a thin surface layer (thickness of ) near the grain boundary surfaces. An alternative interpretation is that represents characteristic length of the exponential decay flux pinning potential from the dominant defects in superconductors, which are grain boundaries.
Cite
@article{arxiv.2306.13071,
title = {Characteristic length for pinning force density in $Nb{_3}Sn$},
author = {E. F. Talantsev and E. G. Valova-Zaharevskaya and I. L. Deryagina and E. N. Popova},
journal= {arXiv preprint arXiv:2306.13071},
year = {2023}
}
Comments
27 pages, 12 figures