Giant orbital diamagnetism of three-dimensional Dirac electrons in SrPbO antiperovskite
arXiv:2011.13182 · doi:10.1103/PhysRevB.103.115117
Abstract
In Dirac semimetals, inter-band mixing has been known theoretically to give rise to a giant orbital diamagnetism when the Fermi level is close to the Dirac point. In BiSb and other Dirac semimetals, an enhanced diamagnetism in the magnetic susceptibility has been observed and interpreted as a manifestation of such giant orbital diamagnetism. Experimentally proving their orbital origin, however, has remained challenging. Cubic antiperovskite SrPbO is a three-dimensional Dirac electron system and shows the giant diamagnetism in as in the other Dirac semimetals. Pb NMR measurements are conducted in this study to explore the microscopic origin of diamagnetism. From the analysis of the Knight shift as a function of and the relaxation rate for samples with different hole densities, the spin and the orbital components in are successfully separated. The results establish that the enhanced diamagnetism in SrPbO originates from the orbital contribution of Dirac electrons, which is fully consistent with the theory of giant orbital diamagnetism.
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