Energy loss and noise by chaotic motion of magnetic spin
Energy loss and noise by chaotic motion of magnetic spin
批准号:
10650269
负责人:
OKUNO Hikaru
金额:
$1.6万
依托单位:
依托单位国家:
日本
项目类别:
Grant-in-Aid for Scientific Research (C)
财政年份:
1998
资助国家:
日本
项目状态:
已结题
起止时间:
1998 至 2000
中文摘要
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英文摘要
The energy loss caused by the domain-wall motion is calculated by integrating damping term. The value of the energy loss is discussed in connection with the bifurcation diagram. The energy loss jumps to a high value at the first transition to chaos. The energy loss in the periodic window is larger than the value in the neighboring chaotic region in spite of their having the same damping coefficient.A chaotic region of domain wall motion is calculated as a function of the amplitude and frequency of the external magnetic drive field. It shows an intricate pattern composed of regular and chaotic regions. An energy loss and the Lyapunov exponent of domain wall motion are calculated. A frequency at the peak of the energy loss versus frequency curve, namely a nonlinear resonance frequency, is different from a resonance frequency in the linear theory as it shifts toward a lower frequency with increasing amplitude of the external magnetic drive field. This peak shift is explained by the effect … More of the higher order term in the nonlinear restoring force. The energy loss versus frequency curve becomes irregular and the energy loss decreases in the chaotic region where the Lyapunov exponent is positive.The two-step Ott-Grebogi-Yorke (OGY) method and the prediction OGY method for controlling chaos of magnetic domain-wall motion are proposed to improve the long settling time in the original OGY method. In the two-step OGY method, a magnetic domain wall is first moved on a periodic orbit and the OGY method is used when the orbit approaches a saddle point. In the prediction OGY method, the motion of the domain wall is predicted before the OGY method is applied. An attractor in the state space can be reconstructed by using the time series of the domain-wall motion. The near future can be predicted even in the chaotic system, because the short time developments of the neighborhood system of a predictee in the attractor are not so different from each other. The settling time of the improved OGY methods is 1/5-1/30 times as long as that of the original OGY method. Less
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H.Okuno, Y.Okada and H.Takeda: "Chaos of domain wall and OGY controlling with method of predicting"Digest of the 22 annual conference on Magnetics in Japan. 22. 141 (1998)
H.Okuno、Y.Okada 和 H.Takeda:“用预测方法控制磁畴壁的混沌和 OGY”第 22 届日本磁学年会摘要。
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通讯作者:
奥野 光: "非線形磁壁共鳴のピークシフトとカオス"日本応用磁気学会学術講演概要集. 23. 321 (1999)
Hikaru Okuno:“非线性畴壁共振中的峰移和混沌”日本应用磁学学会学术讲座摘要 23. 321 (1999)。
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Hikaru Okuno: "Controlling chaos of nonlinear domain-wall motion"Journal of Applied Physics. 85・8. 5083-5085 (1999)
奥野光:“非线性域壁运动的混沌控制”应用物理学杂志85・8(1999)。
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奥野光: "非線形磁壁共鳴のピークシフトとカオス"第23回日本応用磁気学会学術講演概要集. 321 (1999)
Hikaru Okuno:“非线性畴壁共振中的峰移和混沌”日本应用磁学学会第 23 届年会摘要 321(1999)。
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通讯作者:
奥野 光: "磁壁のカオス運動とエネルギー損失"東北大学電気通信研究所スピニクス研究会. MS6 (1999)
Hikaru Okuno:“畴壁的混沌运动和能量损失”东北大学电气通信研究所 Spinics 研究小组 MS6(1999)。
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共 23 条
Power stabilization control in large-scale power generation system linked with small-scale local power generation sysytem
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批准号:26420882
-
项目类别:Grant-in-Aid for Scientific Research (C)
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资助金额:$3.24万
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财政年份:2014
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负责人:OKUNO Hikaru
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依托单位:
Development of nano-meter multilayered magnetic film with super low energy loss and application for electric motor
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批准号:15560269
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项目类别:Grant-in-Aid for Scientific Research (C)
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资助金额:$2.56万
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财政年份:2003
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负责人:OKUNO Hikaru
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依托单位:
海外基金