Derives semiclassical orbital magnetization energy in non-Hermitian periodic systems and defines a non-Hermitian angular momentum operator compatible with the real part of the orbital magnetic moment, with imaginary part linked to a generalized Aharonov-Bohm effect.
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2 Pith papers cite this work. Polarity classification is still indexing.
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Families of nonlinear skin modes emerge from linear ones in the Hatano-Nelson model with Kerr nonlinearity, exhibiting enhanced localization for focusing and reduced localization for defocusing nonlinearity.
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Non-Hermitian magnetic moment
Derives semiclassical orbital magnetization energy in non-Hermitian periodic systems and defines a non-Hermitian angular momentum operator compatible with the real part of the orbital magnetic moment, with imaginary part linked to a generalized Aharonov-Bohm effect.
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Skin modes in a nonlinear Hatano-Nelson model
Families of nonlinear skin modes emerge from linear ones in the Hatano-Nelson model with Kerr nonlinearity, exhibiting enhanced localization for focusing and reduced localization for defocusing nonlinearity.