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The formula for Cp-Cv derived in the previous problem can also be derived starting with the definitions of these quantities in terms of U and H. Do so. Most of the derivation is very similar, but at one point you need to use the relation P=-(∂F/∂V)T.

Short Answer

Expert verified

The formula derived is CP-CV=T∂S∂VT∂V∂TP.

Step by step solution

01

Given information

Cp-Cv.

02

Explanation

The specific heat of a substance can be of two types:
(i) specific heat at constant pressure CP
(ii) specific heat at constant volume CV

They are given by

CV=∂U∂TVCP=∂H∂TP

Where, U = internal energy, H = enthalpy, V = volume and P = pressure.

Lets consider U=U(V, T), and differentiate above expression with respect to T, we get

dU=∂U∂VTdV+∂U∂TVdT

Similarly write expression for enthalpy H=U+P V.

Write the expression for d H at constant pressure d H=d U+P d V

Substitute dU=∂U∂VTdV+∂U∂TVdT

We get,

dH=∂U∂VTdV+∂U∂TVdT+pdV=∂U∂VT+PdV+∂U∂TVdT

Simplify, divide both sides of the above expression by d T,

∂H∂TP=∂U∂VT+P∂V∂TP+∂U∂TV...........................(1)

Substitute CPfor∂H∂TPandCVfor∂U∂TV, we get

CP=∂U∂VT+P∂V∂TP+CV.............................(2)

Substitute -∂F∂VTforPin equation(2)

CP=∂(U-F)∂VT∂V∂TP+CV

Now substitute TS for (U-F)

CP=T∂S∂VT∂V∂TP+CV∞

Now find CP - CV

CP-CV=T∂S∂VT∂V∂TP

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Most popular questions from this chapter

Problem 5.35. The Clausius-Clapeyron relation 5.47 is a differential equation that can, in principle, be solved to find the shape of the entire phase-boundary curve. To solve it, however, you have to know how both L and ∆V depend on temperature and pressure. Often, over a reasonably small section of the curve, you can take L to be constant. Moreover, if one of the phases is a gas, you can usually neglect the volume of the condensed phase and just take ∆V to be the volume of the gas, expressed in terms of temperature and pressure using the ideal gas law. Making all these assumptions, solve the differential equation explicitly to obtain the following formula for the phase boundary curve:

P= (constant) x e-L/RT

This result is called the vapour pressure equation. Caution: Be sure to use this formula only when all the assumptions just listed are valid.

Consider the production of ammonia from nitrogen and hydrogen,

N2+3H2→2NH3

at 298 K and 1 bar. From the values of ΔH and S tabulated at the back of this book, compute ΔG for this reaction and check that it is consistent with the value given in the table.

Derive the van't Hoff equation,

dlnKdT=ΔH°RT2

which gives the dependence of the equilibrium constant on temperature." Here ∆H°is the enthalpy change of the reaction, for pure substances in their standard states (1 bar pressure for gases). Notice that if ∆H°is positive (loosely speaking, if the reaction requires the absorption of heat), then higher temperature makes the reaction tend more to the right, as you might expect. Often you can neglect the temperature dependence of∆H°; solve the equation in this case to obtain

lnKT2-lnKT1=ΔH°R1T1-1T2

Is heat capacity (C) extensive or intensive? What about specific heat (c) ? Explain briefly.

Functions encountered in physics are generally well enough behaved that their mixed partial derivatives do not depend on which derivative is taken first. Therefore, for instance,

∂∂V∂U∂S=∂∂S∂U∂V

where each ∂/∂Vis taken with Sfixed, each ∂/∂Sis taken with Vfixed, and Nis always held fixed. From the thermodynamic identity (forU) you can evaluate the partial derivatives in parentheses to obtain

∂T∂VS=-∂P∂SV

a nontrivial identity called a Maxwell relation. Go through the derivation of this relation step by step. Then derive an analogous Maxwell relation from each of the other three thermodynamic identities discussed in the text (for H,F,andG ). Hold N fixed in all the partial derivatives; other Maxwell relations can be derived by considering partial derivatives with respect to N, but after you've done four of them the novelty begins to wear off. For applications of these Maxwell relations, see the next four problems.

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