Model' spinovogo stekla dlya kvantovykh yam GaAs/AlGaAs, legirovannykh nemagnitnymi primesyami, vblizi perekhoda metall–izolyator

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Resumo

In a previous report, we presented experiments which suggested that ferromagnetic ordering of the spins of localized holes in GaAs/AlGaAs quantum wells could be observed when doped with shallow (Be) acceptors at impurity concentrations near the metal-insulator transition. The compensating impurity (Si) was introduced into a narrow region at the center of the barriers [4]. In this paper, we present results from magnetotransport experiments performed on similar structures, but without the compensating impurity (Si). In these samples, the compensation degree is expected to be controlled by the background defects located at the edges of the quantum wells and within the barriers. At low temperatures T ≤ 10 K, we observed isotropic, linear magnetoresistance, anomalous behavior of the Hall effect as a function of the magnetic field, and slow relaxation of resistance after the application of a magnetic field. We explain this anomalous magnetotransport as the manifestation of a ferromagnetic transition or spin glass, originating from indirect spin exchange between localized holes on impurities near the metal-insulator transition. However, we note that perfect disorder, including signs of interspin interactions, leads to unstable configurations. In what follows, we present a model in which we start with this perfect disorder, but apply a procedure to obtain a stable configuration. We show that the resulting spin structure, a “closely packed” structure of “droplets,” can reproduce the features observed in the experiment, particularly isotropic, linear magnetoresistance.

Sobre autores

N. Agrinskaya

A.F. Ioffe Institute, Russian Academy of Sciences

Email: nina.agrins@mail.ioffe.ru
194021, St. Petersburg, Russia

V. Kozub

A.F. Ioffe Institute, Russian Academy of Sciences

Autor responsável pela correspondência
Email: nina.agrins@mail.ioffe.ru
194021, St. Petersburg, Russia

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Declaração de direitos autorais © Russian Academy of Sciences, 2023

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