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生态系统的热力学稳定性。

Thermodynamic stability of ecosystems.

作者信息

Michaelian K

机构信息

Instituto de Física, Universidad Nacional Autónoma de México, A.P. 20-364, 01000 México D.F., Mexico.

出版信息

J Theor Biol. 2005 Dec 7;237(3):323-35. doi: 10.1016/j.jtbi.2005.04.019. Epub 2005 Jun 22.

Abstract

The stability of ecosystems during periods of stasis in their macro-evolutionary trajectory is studied from a non-equilibrium thermodynamic perspective. Individuals of the species are considered as units of entropy production and entropy exchange in an open thermodynamic system. Within the framework of the classical theory of irreversible thermodynamics, and under the condition of constant external constraints, such a system will naturally evolve toward a globally stable thermodynamic stationary state. It is thus suggested that the ecological steady state, or stasis, is a particular case of the thermodynamic stationary state, and that the evolution of community stability through natural selection is a manifestation of non-equilibrium thermodynamic directives. Furthermore, it is argued that punctuation of stasis leading to ecosystem succession, may be a manifestation of non-equilibrium "phase transitions" brought on by a change of external constraints through a thermodynamic critical point.

摘要

从非平衡热力学的角度研究了生态系统在宏观进化轨迹停滞期的稳定性。物种个体被视为开放热力学系统中熵产生和熵交换的单位。在经典不可逆热力学理论的框架内,并且在外部约束恒定的条件下,这样的系统将自然地朝着全局稳定的热力学稳态演化。因此有人认为,生态稳态或停滞是热力学稳态的一种特殊情况,并且通过自然选择实现的群落稳定性演化是非平衡热力学指令的一种表现。此外,有人认为导致生态系统演替的停滞间断可能是通过热力学临界点的外部约束变化引起的非平衡“相变”的一种表现。

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