Heat capacity: Difference between revisions
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Carl McBride (talk | contribs) m (Added a reference.) |
m (→Debye: Added a formula.) |
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====Einstein==== | ====Einstein==== | ||
====Debye==== | ====Debye==== | ||
A low temperatures on has | |||
:<math>c_v = \frac{12 \pi^4}{5} n k_B \left( \frac{T}{\Theta_D} \right)^3</math> | |||
where <math>k_B</math> is the [[Boltzmann constant]], <math>T</math> is the [[temperature]] and <math>\Theta_D</math> is an empirical parameter known as the Debye temperature. | |||
==See also== | ==See also== | ||
*[[Ideal gas: Heat capacity | Heat capacity of an ideal gas]] | *[[Ideal gas: Heat capacity | Heat capacity of an ideal gas]] | ||
==References== | ==References== | ||
[[category: classical thermodynamics]] | [[category: classical thermodynamics]] |
Revision as of 15:31, 21 January 2009
The heat capacity is defined as the differential of heat with respect to the temperature ,
where is heat and is the entropy.
At constant volume
From the first law of thermodynamics one has
thus at constant volume, denoted by the subscript , then ,
At constant pressure
At constant pressure (denoted by the subscript ),
where is the enthalpy. The difference between the heat capacity at constant pressure and the heat capacity at constant volume is given by
Liquids
Solids
Dulong and Petit
Einstein
Debye
A low temperatures on has
where is the Boltzmann constant, is the temperature and is an empirical parameter known as the Debye temperature.