A More General View of Temperature温度的更一般性观点
When a high temperature object is placed in contact with a low temperature object, then energy will flow from the high temperature object to the lower temperature object, and they will approach an equilibrium temperature. When the details of this common-sense scenario are examined, it becomes evident that the simple view of temperature embodied in the commonly used kinetic temperature approach has some significant problems. 当一个高温物体与一个低温物体接触时,能量会从高温物体流向低温物体,两者将趋于平衡温度。当深入考察这一常识性场景时,可以明显看出基于常用动量温度方法所体现的温度概念存在一些重大问题。
![]() The above illustration summarizes the situation when the kinetic temperature gives a reasonable general description of the nature of temperature. For monoatomic gases acting like point masses, a higher temperature simply implies higher average kinetic energy. Faster molecules striking slower ones at the boundary in elastic collisions will increase the velocity of the slower ones and decrease the velocity of the faster ones, transferring energy from the higher temperature to the lower temperature region. With time, the molecules in the two regions approach the same average kinetic energy (same temperature) and in this condition of thermal equilibrium there is no longer any net transfer of energy from one object to the other. 上述示意图总结了当动能温度能合理描述温度性质时的情况。对于像质点一样的单原子气体,温度升高仅仅意味着平均动能更高。在弹性碰撞中,快速分子撞击较慢分子时,会增加较慢分子的速度并减少较快分子的速度,将能量从较高温度区域转移到较低温度区域。随着时间推移,两个区域中的分子会接近相同的平均动能(相同的温度),在此热平衡状态下,将不再有能量从一个物体转移到另一个物体。
Complications such as these have led to the adoption of a different approach to the concept of temperature in the study of thermodynamics. Schroeder's proposal for a theoretical definition of temperature is: 这类复杂性导致了在热力学研究中对温度概念采用不同方法的必要性。Schroeder对温度的理论定义的提议是:
The kinetic temperature for monoatomic ideal gases described above is consistent with this definition of temperature for the simple systems to which it applies. In that case the equilibrium reached is one of maximum entropy, and the rate of approach to that state will be proportional to the difference in temperature between the two parts of the system. Noting that the equilibrium state of a collection of particles will be the state of greatest multiplicity, then one can define the temperature in terms of that multiplicity (entropy) as follows: 上述单原子理想气体的动能温度与它适用的简单系统的温度定义是一致的。在这种情况下,达到的平衡是一种熵最大的平衡,系统向该状态接近的速率将与系统两部分之间的温度差成正比。注意到一组粒子的平衡态将是乘积最大的状态,因此可以将温度定义为该乘积(熵)的函数,如下所示:
![]() Temperature is expressed as the inverse of the rate of change of entropy with internal energy, with volume V and number of particles N held constant. This is certainly not as intuitive as molecular kinetic energy, but in thermodynamic applications it is more reliable and more general. 温度可以表示为在体积V和粒子数N保持不变的情况下,熵与内能变化率的倒数。这显然不如分子动能直观,但在热力学应用中更为可靠和普遍。
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Index Temperature concepts Reference Schroeder Ch 1,3 索引 温度概念 参考 Schröder 第1、3章 | |||
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The Relationship of Entropy to Temperature熵与温度的关系
The definition of temperature in terms of molecular kinetic energy, the "kinetic temperature", is commonly used in introductory treatments of thermodynamics. But in view of practical difficulties with that approach, temperature is often defined in terms of two other state variables, entropy S and internal energy U. 温度以分子动能来定义,即‘动能温度’,在热力学的初等处理中被广泛使用。但考虑到该方法的实践困难,温度通常以另外两个状态变量,熵S和内能U来定义。
![]() Temperature is expressed as the inverse of the rate of change of entropy with internal energy, with volume V and number of particles N held constant. This is certainly not as intuitive as molecular kinetic energy, but in thermodynamic applications it is more reliable and more general. This form of the temperature can be obtained from the thermodynamic identity. 温度可以表示为当体积V和粒子数N保持不变时,熵与内能变化率的倒数。这显然不如分子动能直观,但在热力学应用中更为可靠和普遍。这种温度的表达形式可以从热力学恒等式中获得。
To apply this definition of temperature to a monoatomic ideal gas, we need an expression for the entropy of an ideal gas: 要将这一温度定义应用于单原子理想气体,我们需要一个理想气体的熵的表达式:
![]() Then making use of the definition of temperature in terms of entropy: 然后利用熵的定义来确定温度:
![]() This gives an expression for internal energy that is consistent with equipartition of energy. 这给出了与能量均分定理一致的内能表达式。
![]() with kT/2 of energy for each degree of freedom for each atom. 每个原子每个自由度都有kT/2的能。
Another example of this approach to temperature is the Einstein solid with q units of energy and N oscillators. The internal energy U can be represented by q times the oscillator energy unit hf = ε. The entropy can be expressed as 另一种这种温度处理方法的例子是爱因斯坦固体,其中q单位为能量,N个振子。内能U可以表示为q乘以振子能量单位hf = ε。熵可以表示为
![]() Taking the derivative gives 求导得到
![]() This is what is expected from equipartition of energy. Each oscillator has two degrees of freedom, and each should represent kT/2 of energy, giving U=NkT. 这是从能量均分定理所预期的结果。每个振子有两个自由度,每个应代表kT/2的能量,因此内能U=NkT。
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Index Temperature concepts Entropy concepts Reference Schroeder Ch 1,3 索引 温度概念 熵概念 参考 Schroeder 第1、3章 | ||
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