Relations between heat capacities
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In
thermodynamics Thermodynamics is a branch of physics that deals with heat, work, and temperature, and their relation to energy, entropy, and the physical properties of matter and radiation. The behavior of these quantities is governed by the four laws ...
, the
heat capacity Heat capacity or thermal capacity is a physical property of matter, defined as the amount of heat to be supplied to an object to produce a unit change in its temperature. The SI unit of heat capacity is joule per kelvin (J/K). Heat cap ...
at constant volume, C_, and the heat capacity at constant pressure, C_, are
extensive properties Physical properties of materials and systems can often be categorized as being either intensive or extensive, according to how the property changes when the size (or extent) of the system changes. According to IUPAC, an intensive quantity is one ...
that have the magnitude of energy divided by temperature.


Relations

The
laws of thermodynamics The laws of thermodynamics are a set of scientific laws which define a group of physical quantities, such as temperature, energy, and entropy, that characterize thermodynamic systems in thermodynamic equilibrium. The laws also use various paramet ...
imply the following relations between these two heat capacities (Gaskell 2003:23): :C_ - C_= V T\frac\, :\frac=\frac\, Here \alpha is the
thermal expansion coefficient Thermal expansion is the tendency of matter to change its shape, area, volume, and density in response to a change in temperature, usually not including phase transitions. Temperature is a monotonic function of the average molecular kinetic ...
: :\alpha=\frac\left(\frac\right)_\, \beta_ is the isothermal
compressibility In thermodynamics and fluid mechanics, the compressibility (also known as the coefficient of compressibility or, if the temperature is held constant, the isothermal compressibility) is a measure of the instantaneous relative volume change of a f ...
(the inverse of the
bulk modulus The bulk modulus (K or B) of a substance is a measure of how resistant to compression the substance is. It is defined as the ratio of the infinitesimal pressure increase to the resulting ''relative'' decrease of the volume. Other moduli descri ...
): :\beta_=-\frac\left(\frac\right)_\, and \beta_ is the
isentropic In thermodynamics, an isentropic process is an idealized thermodynamic process that is both adiabatic and reversible. The work transfers of the system are frictionless, and there is no net transfer of heat or matter. Such an idealized process ...
compressibility: :\beta_=-\frac\left(\frac\right)_\, A corresponding expression for the difference in specific heat capacities ( intensive properties) at constant volume and constant pressure is: : c_p - c_v = \frac where ρ is the
density Density (volumetric mass density or specific mass) is the substance's mass per unit of volume. The symbol most often used for density is ''ρ'' (the lower case Greek letter rho), although the Latin letter ''D'' can also be used. Mathematicall ...
of the substance under the applicable conditions. The corresponding expression for the ratio of specific heat capacities remains the same since the
thermodynamic system A thermodynamic system is a body of matter and/or radiation, confined in space by walls, with defined permeabilities, which separate it from its surroundings. The surroundings may include other thermodynamic systems, or physical systems that are ...
size-dependent quantities, whether on a per mass or per mole basis, cancel out in the ratio because specific heat capacities are intensive properties. Thus: :\frac=\frac\, The difference relation allows one to obtain the heat capacity for solids at constant volume which is not readily measured in terms of quantities that are more easily measured. The ratio relation allows one to express the isentropic compressibility in terms of the heat capacity ratio.


Derivation

If an infinitesimally small amount of heat \delta Q is supplied to a system in a reversible way then, according to the
second law of thermodynamics The second law of thermodynamics is a physical law based on universal experience concerning heat and energy interconversions. One simple statement of the law is that heat always moves from hotter objects to colder objects (or "downhill"), unle ...
, the entropy change of the system is given by: :dS = \frac\, Since :\delta Q = C dT\, where C is the heat capacity, it follows that: :T dS = C dT\, The heat capacity depends on how the external variables of the system are changed when the heat is supplied. If the only external variable of the system is the volume, then we can write: :dS = \left(\frac\right)_dT+\left(\frac\right)_dV From this follows: :C_=T\left(\frac\right)_\, Expressing dS in terms of dT and dP similarly as above leads to the expression: :C_=T\left(\frac\right)_\, One can find the above expression for C_-C_ by expressing dV in terms of dP and dT in the above expression for dS. :dV = \left(\frac\right)_dT+\left(\frac\right)_dP\, results in :dS = \left left(\frac\right)_+ \left(\frac\right)_\left(\frac\right)_\rightT+\left(\frac\right)_\left(\frac\right)_dP and it follows: :\left(\frac\right)_ = \left(\frac\right)_+ \left(\frac\right)_\left(\frac\right)_\, Therefore, :C_ - C_ = T\left(\frac\right)_\left(\frac\right)_=VT\alpha\left(\frac\right)_\, The partial derivative \left(\frac\right)_ can be rewritten in terms of variables that do not involve the entropy using a suitable
Maxwell relation file:Thermodynamic map.svg, 400px, Flow chart showing the paths between the Maxwell relations. P is pressure, T temperature, V volume, S entropy, \alpha coefficient of thermal expansion, \kappa compressibility, C_V heat capacity at constant volu ...
. These relations follow from the
fundamental thermodynamic relation In thermodynamics, the fundamental thermodynamic relation are four fundamental equations which demonstrate how four important thermodynamic quantities depend on variables that can be controlled and measured experimentally. Thus, they are essentiall ...
: :dE = T dS - P dV\, It follows from this that the differential of the Helmholtz free energy F = E - T S is: :dF = -S dT - P dV\, This means that :-S = \left(\frac\right)_\, and :-P = \left(\frac\right)_\, The
symmetry of second derivatives In mathematics, the symmetry of second derivatives (also called the equality of mixed partials) refers to the possibility of interchanging the order of taking partial derivatives of a function :f\left(x_1,\, x_2,\, \ldots,\, x_n\right) of ''n ...
of F with respect to T and V then implies :\left(\frac\right)_ =\left(\frac\right)_\, allowing one to write: :C_ - C_ = VT\alpha\left(\frac\right)_\, The r.h.s. contains a derivative at constant volume, which can be difficult to measure. It can be rewritten as follows. In general, :dV= \left(\frac\right)_dP+\left(\frac\right)_dT\, Since the partial derivative \left(\frac\right)_ is just the ratio of dP and dT for dV = 0, one can obtain this by putting dV = 0 in the above equation and solving for this ratio: :\left(\frac\right)_=-\frac=\frac\, which yields the expression: :C_ - C_= V T\frac\, The expression for the ratio of the heat capacities can be obtained as follows: :\frac = \frac\, The partial derivative in the numerator can be expressed as a ratio of partial derivatives of the pressure w.r.t. temperature and entropy. If in the relation :dP = \left(\frac\right)_dS+\left(\frac\right)_dT\, we put dP = 0 and solve for the ratio \frac we obtain \left(\frac\right)_. Doing so gives: :\left(\frac\right)_=-\frac\, One can similarly rewrite the partial derivative \left(\frac\right)_ by expressing dV in terms of dS and dT, putting dV equal to zero and solving for the ratio \frac. When one substitutes that expression in the heat capacity ratio expressed as the ratio of the partial derivatives of the entropy above, it follows: :\frac=\frac \frac\, Taking together the two derivatives at constant S: :\frac = \left(\frac\right)_\left(\frac\right)_=\left(\frac\right)_\, Taking together the two derivatives at constant T: :\frac=\left(\frac\right)_\left(\frac\right)_=\left(\frac\right)_\, From this one can write: :\frac=\left(\frac\right)_\left(\frac\right)_=\frac\,


Ideal gas

This is a derivation to obtain an expression for C_ - C_\, for an
ideal gas An ideal gas is a theoretical gas composed of many randomly moving point particles that are not subject to interparticle interactions. The ideal gas concept is useful because it obeys the ideal gas law, a simplified equation of state, and is a ...
. An
ideal gas An ideal gas is a theoretical gas composed of many randomly moving point particles that are not subject to interparticle interactions. The ideal gas concept is useful because it obeys the ideal gas law, a simplified equation of state, and is a ...
has the
equation of state In physics, chemistry, and thermodynamics, an equation of state is a thermodynamic equation relating state variables, which describe the state of matter under a given set of physical conditions, such as pressure, volume, temperature, or intern ...
: P V = n R T\, where :P = pressure :V = volume :n = number of moles :R =
universal gas constant(Gas constant) The molar gas constant (also known as the gas constant, universal gas constant, or ideal gas constant) is denoted by the symbol or . It is the molar equivalent to the Boltzmann constant, expressed in units of energy per temperature increment pe ...
:T = temperature The
ideal gas An ideal gas is a theoretical gas composed of many randomly moving point particles that are not subject to interparticle interactions. The ideal gas concept is useful because it obeys the ideal gas law, a simplified equation of state, and is a ...
equation of state In physics, chemistry, and thermodynamics, an equation of state is a thermodynamic equation relating state variables, which describe the state of matter under a given set of physical conditions, such as pressure, volume, temperature, or intern ...
can be arranged to give: : V = n R T / P\, or \, n R = P V / T The following partial derivatives are obtained from the above
equation of state In physics, chemistry, and thermodynamics, an equation of state is a thermodynamic equation relating state variables, which describe the state of matter under a given set of physical conditions, such as pressure, volume, temperature, or intern ...
: :\left(\frac\right)_\ = \frac \ = \left(\frac\right)\left(\frac\right) = \frac :\left(\frac\right)_\ = - \frac \ = - \frac \ = - \frac The following simple expressions are obtained for thermal expansion coefficient \alpha : :\alpha=\frac\left(\frac\right)_\ = \frac\left(\frac\right) :\alpha= 1 / T \, and for isothermal compressibility \beta_: :\beta_= - \frac\left(\frac\right)_\ = - \frac\left( - \frac\right) :\beta_= 1 / P \, One can now calculate C_ - C_\, for ideal gases from the previously-obtained general formula: :C_ - C_= V T\frac\ = V T\frac = \frac Substituting from the
ideal gas An ideal gas is a theoretical gas composed of many randomly moving point particles that are not subject to interparticle interactions. The ideal gas concept is useful because it obeys the ideal gas law, a simplified equation of state, and is a ...
equation gives finally: :C_ - C_ = n R\, where n = number of moles of gas in the thermodynamic system under consideration and R = universal gas constant. On a per mole basis, the expression for difference in molar heat capacities becomes simply R for ideal gases as follows: : C_ - C_ = \frac = \frac = R This result would be consistent if the specific difference were derived directly from the general expression for c_p - c_v\, .


See also

*
Heat capacity ratio In thermal physics and thermodynamics, the heat capacity ratio, also known as the adiabatic index, the ratio of specific heats, or Laplace's coefficient, is the ratio of the heat capacity at constant pressure () to heat capacity at constant vol ...


References

* David R. Gaskell (2008), ''Introduction to the thermodynamics of materials'', Fifth Edition, Taylor & Francis. {{ISBN, 1-59169-043-9. Thermodynamics