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An algorithm to characterize collective motion as the orbital instability at a macroscopic level is presented, including the introduction of “collective Lyapunov exponent." By applying the algorithm to a globally coupled map, existence of low-dimensional collective chaos is confirmed, where the scale of (high-dimensional) microscopic chaos is separated from the macroscopic motion, and the scale approaches zero in the thermodynamic limit.
収録刊行物
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- Physical Review Letters
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Physical Review Letters 81 (19), 4116-4119, 1998-11-09
American Physical Society
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詳細情報 詳細情報について
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- CRID
- 1050859215941173504
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- NII論文ID
- 120000878125
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- NII書誌ID
- AA00773679
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- 本文言語コード
- en
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- 資料種別
- journal article
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- データソース種別
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- IRDB
- CiNii Articles