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Exponentially decreasing or steady-state orbital motions can appear under specific conditions.
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From the present simulations, the critical current density is obtained as jcri =6.4× 106 A/ cm2 for STT only, jcri =6.8× 106 A/ cm2 for STT+OH (P), and 6.1× 106 A/ cm2 for STT+OH (AP). These deviations for the case of additional OH effect are within ±5% of that for STT only.
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From the present simulations, the critical current density is obtained as jcri =6.4× 106 A/ cm2 for STT only, jcri =6.8× 106 A/ cm2 for STT+OH (P), and 6.1× 106 A/ cm2 for STT+OH (AP). These deviations for the case of additional OH effect are within ±5% of that for STT only.
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