For what temperature is the Joule-Thomson coefficient for a gas zero?

1 Answer
Sep 9, 2017

For what kind of gas?


The Joule-Thomson experiment essentially pushes a gas through a porous plug at constant enthalpy (insulated so that no heat is exchanged with the environment). This is done in such a way that all of the expansion work goes into changing the internal energy:

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Any gas is then described by the Joule-Thomson coefficient

#mu_(JT) = ((delT)/(delP))_H#,

that is, it is the change in temperature brought about by a change in pressure at constant enthalpy.

(This may be weird... but if you can perform the expansion slowly enough, the pressure can re-equilibrate and constant enthalpy is then possible with perfect insulation.)

A Joule-Thomson coefficient for any gas is given by:

#mu_(JT) = ((delT)/(delP))_H = V/C_P(alphaT - 1)#

An ideal gas always has a Joule-Thomson coefficient #mu_(JT)# of zero. Note that for ideal gases:

#alpha = 1/V ((delV)/(delT))_P = (nR)/(PV) = 1/T#

And thus, #alphaT = 1# and #mu_(JT) = 0# for an ideal gas, regardless of temperature (as long as #T ne "0 K"#).

For real gases, when #mu_(JT)# is zero, it is known to be at the inversion temperature #T_"inv"#:

#0 = V/C_P(alphaT_"inv" - 1)#

Since the volume of any gas is never zero and since assuming we don't need to reach #T = "0 K"# for the sign change to occur, the heat capacity does not reach zero:

#color(blue)(T_"inv" = 1/alpha)#


DISCLAIMER: LONG DERIVATION BELOW!

To derive this, begin at the cyclic rule of partial derivatives:

#((delT)/(delP))_H((delH)/(delT))_P((delP)/(delH))_T = -1# #" "" "bb((1))#

By definition, the constant-pressure heat capacity is:

#C_P = ((delH)/(delT))_P#, #" "" "bb((2))#

which is an experimentally-determined quantity. Next, note that, as with all derivatives:

#((delP)/(delH))_T = 1/((delH)/(delP))_T# #" "" "bb((3))#

The Gibbs' free energy is a function of #T# and #P#, so consider the ubiquitous relation in a constant-temperature system:

#dG = dH - TdS# #" "" "bb((4))#

By taking the partial derivative with respect to #P# at constant #T# of #(4)#, we get:

#((delG)/(delP))_T = ((delH)/(delP))_T - T((delS)/(delP))_T# #" "" "bb((5))#

For a similar reason, we then consider the Gibbs' free energy Maxwell Relation:

#dG = -SdT + VdP# #" "" "bb((6))#

Since for state functions, cross-derivatives are equal, we have:

#((delS)/(delP))_T = -((delV)/(delT))_P# #" "" "bb((7))#

By definition, the coefficient of thermal expansion is:

#alpha = 1/V ((delV)/(delT))_P# #" "" "bb((8))#

which is experimentally-determined. So, using #(7)# and #(8)#,

#((delS)/(delP))_T = -Valpha#. #" "" "bb((9))#

Next, from the Maxwell Relation #(6)#,

#((delG)/(delP))_T = V#. #" "" "bb((10))#

As a result, we so far have, by combining #(9)# and #(10)# into #(5)#:

#V = ((delH)/(delP))_T + TcdotValpha#

Therefore:

#((delH)/(delP))_T = V - ValphaT = -V(alphaT - 1)#

Lastly, plug this back into the cyclic rule #(1)# to find:

#((delT)/(delP))_HC_P/(-V(alphaT - 1)) = -1#

And so, the Joule-Thomson coefficient is found as:

#color(blue)(barul|stackrel(" ")(" "mu_(JT) = ((delT)/(delP))_H = V/C_P(alphaT - 1)" ")|)#