In Dirac semimetals, interband mixing has been known theoretically to give rise to a giant orbital diamagnetism when the Fermi level is close to the Dirac point. In Bi_1−xSb_x and other Dirac semimetals, an enhanced diamagnetism in the magnetic susceptibility χ has been observed and interpreted as a manifestation of such giant orbital diamagnetism. Experimentally proving their orbital origin, however, has remained challenging. The cubic antiperovskite Sr₃PbO is a three-dimensional Dirac electron system and shows the giant diamagnetism in χ as in the other Dirac semimetals. ²⁰⁷Pb NMR measurements are conducted in this study to explore the microscopic origin of diamagnetism. From the analysis of the Knight shift K as a function of χ  and the relaxation rate T₁^–1 for samples with different hole densities, the spin and the orbital components in K are successfully separated. The results establish that the enhanced diamagnetism in Sr₃PbO originates from the orbital contribution of Dirac electrons, which is fully consistent with the theory of giant orbital diamagnetism.

See below for more information.

• Aritcle URL : https://journals.aps.org/prb/abstract/10.1103/PhysRevB.103.115117
• Takagi-Kitagawa Lab. : http://park.itc.u-tokyo.ac.jp/takagi_lab/en/
• Ogata Lab. : https://sites.google.com/hosi.phys.s.u-tokyo.ac.jp/homepage/english