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We numerically calculate the magnetization by applying the magnetic field () perpendicular to two-dimensional corbino disk system without electron spin. We obtain that the period of the Aharonov-Bohm (AB) oscillations of magnetization exhibit , and almost as a function of , depending on numbers of electrons (), where is a unit flux and is the magnetic flux through the hollow of the disk. The oscillations of are classified into five patterns at investigated in this study. These are expected to be observed in the two-dimensional semiconductor corbino disk with the hollow radius of about 10 nm and small electron numbers at the high magnetic field.

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