The Four Standard Processes in One Table

Almost every gas problem set at JEE level is one of four idealised processes, or a chain of them. Each process holds one variable fixed, and holding that variable fixed collapses the first law into a short expression you can write down without thinking.

Everything below uses the first law in the IUPAC form

ΔU=q+w\Delta U = q + w

where ΔU\Delta U is the change in internal energy of the system, qq is the heat supplied to the system, and ww is the work done on the system. Expansion work against an external pressure pexp_{ex} is w=pexΔVw = -p_{ex}\Delta V, with ΔV=V2V1\Delta V = V_2 - V_1.

Two results for an ideal gas do most of the work in this section. The internal energy of an ideal gas depends only on its temperature, because the molecules have no intermolecular potential energy to store. Enthalpy H=U+pV=U+nRTH = U + pV = U + nRT then also depends only on temperature. So for nn moles of an ideal gas,

ΔU=nCv,mΔTΔH=nCp,mΔT\Delta U = n\,C_{v,m}\,\Delta T \qquad \Delta H = n\,C_{p,m}\,\Delta T

where Cv,mC_{v,m} and Cp,mC_{p,m} are the molar heat capacities at constant volume and constant pressure.

Key Point: For an ideal gas, ΔU=nCv,mΔT\Delta U = nC_{v,m}\Delta T and ΔH=nCp,mΔT\Delta H = nC_{p,m}\Delta T hold on every path, not only at constant volume and constant pressure. The subscripts name where the heat capacities were measured, not where the formulae may be used. All you need is the temperature change.

The two molar heat capacities are tied together by

Cp,mCv,m=RC_{p,m} - C_{v,m} = R

for one mole of an ideal gas. Now the four processes, for a fixed amount nn of an ideal gas doing only pressure-volume work.

Process Held constant ww (on the gas) ΔU\Delta U qq ΔH\Delta H
Isochoric VV 00 nCv,mΔTnC_{v,m}\Delta T qv=ΔU=nCv,mΔTq_v = \Delta U = nC_{v,m}\Delta T nCp,mΔTnC_{p,m}\Delta T
Isobaric pp pΔV=nRΔT-p\,\Delta V = -nR\,\Delta T nCv,mΔTnC_{v,m}\Delta T qp=ΔH=nCp,mΔTq_p = \Delta H = nC_{p,m}\Delta T nCp,mΔTnC_{p,m}\Delta T
Isothermal, reversible TT nRTlnV2V1-nRT\ln\dfrac{V_2}{V_1} 00 w=+nRTlnV2V1-w = +nRT\ln\dfrac{V_2}{V_1} 00
Adiabatic, reversible q=0q = 0 nCv,mΔTnC_{v,m}\Delta T nCv,mΔTnC_{v,m}\Delta T 00 nCp,mΔTnC_{p,m}\Delta T

Four things in that table are worth spelling out.

In the isochoric row ΔV=0\Delta V = 0, so no expansion work is possible and every joule of heat goes into internal energy. ΔH\Delta H is still non-zero, because the temperature changed; here ΔH=ΔU+VΔp\Delta H = \Delta U + V\Delta p.

In the isobaric row, pΔV=nRΔTp\Delta V = nR\Delta T follows from writing pV=nRTpV = nRT at both states and subtracting, which is legitimate only because pp is the same at both ends.

In the isothermal row ΔT=0\Delta T = 0, so ΔU\Delta U and ΔH\Delta H are both zero and the first law reduces to q=wq = -w. Whatever work the gas does on the surroundings is replaced exactly by heat drawn in. The logarithmic expression for ww is the reversible one; for a one-step expansion against a constant pexp_{ex} the work is the smaller pexΔV-p_{ex}\Delta V instead, while ΔU\Delta U and ΔH\Delta H stay zero.

In the adiabatic row q=0q = 0 by definition, so ΔU=w\Delta U = w exactly. Work done on the gas raises its temperature; work done by the gas cools it. This row is the one that carries most of the marks, and the next block takes it apart.

Four processes drawn from one common state on a pressure volume diagram

The four processes are one family

All four curves are special cases of a single reversible path called a polytropic process, defined by

pVk=constantpV^{k} = \text{constant}

for some fixed number kk called the polytropic index, written with a letter of its own so that it is never confused with the number of moles nn. Reading off the four values of kk makes the family obvious.

kk The condition pVk=pV^k = constant becomes Process
00 p=p = constant isobaric
11 pV=pV = constant, which for an ideal gas means TT constant isothermal
γ\gamma pVγ=pV^{\gamma} = constant reversible adiabatic
kk \rightarrow \infty p1/kV=p^{1/k}V = constant, that is V=V = constant isochoric

For any k1k \ne 1 the reversible work integrates to a single expression,

w=p2V2p1V1k1w = \frac{p_2V_2 - p_1V_1}{k - 1}

Putting k=γk = \gamma gives the adiabatic work formula used later in this section. Putting k=0k = 0 gives w=(pV2pV1)/(1)=pΔVw = (pV_2 - pV_1)/(-1) = -p\,\Delta V, the isobaric result. The case k=1k = 1 has to be handled separately because the denominator vanishes, and integrating pdV-\int p\,dV with pVpV constant gives the logarithm instead. Seeing the four processes as one family stops them feeling like four unrelated formulae to memorise.

[JEE Main] A question that gives you ΔT\Delta T and asks for ΔH\Delta H is answered in one line by nCp,mΔTnC_{p,m}\Delta T, whatever the path was, provided the gas is ideal and no phase change or reaction occurs.

Adiabatic Change in an Ideal Gas

An adiabatic process is one in which no heat crosses the boundary: q=0q = 0. It is achieved either by insulating the system or by running the change so fast that heat has no time to flow. The first law then gives

ΔU=w\Delta U = w

An adiabatic expansion cools the gas; an adiabatic compression heats it.

Deriving the relation between pp and VV

Take one infinitesimal step of a reversible adiabatic change, so that the gas pressure pp and the external pressure are equal throughout. For an infinitesimal step,

dU=dq+dw=0+(pdV)=pdVdU = dq + dw = 0 + (-p\,dV) = -p\,dV

For nn moles of an ideal gas dU=nCv,mdTdU = nC_{v,m}\,dT, and p=nRT/Vp = nRT/V. Substituting both,

nCv,mdT=nRTVdVnC_{v,m}\,dT = -\frac{nRT}{V}\,dV

Divide through by nTnT to separate the variables:

Cv,mdTT=RdVVC_{v,m}\,\frac{dT}{T} = -R\,\frac{dV}{V}

Integrate from state 1 to state 2, treating Cv,mC_{v,m} as constant over the range:

Cv,mlnT2T1=RlnV2V1C_{v,m}\ln\frac{T_2}{T_1} = -R\ln\frac{V_2}{V_1}

Now define the adiabatic exponent

γ=Cp,mCv,m\gamma = \frac{C_{p,m}}{C_{v,m}}

Since Cp,mCv,m=RC_{p,m} - C_{v,m} = R for an ideal gas, dividing that relation by Cv,mC_{v,m} gives R/Cv,m=γ1R/C_{v,m} = \gamma - 1. Divide the integrated equation by Cv,mC_{v,m}:

lnT2T1=(γ1)lnV2V1=ln(V1V2)γ1\ln\frac{T_2}{T_1} = -(\gamma - 1)\ln\frac{V_2}{V_1} = \ln\left(\frac{V_1}{V_2}\right)^{\gamma-1}

Removing the logarithms,

T1V1γ1=T2V2γ1soTVγ1=constantT_1 V_1^{\gamma-1} = T_2 V_2^{\gamma-1} \qquad \text{so} \qquad TV^{\gamma-1} = \text{constant}

Replace TT by pV/nRpV/nR in that result. The constant factor 1/nR1/nR cancels from both sides and leaves

pVγ=constantpV^{\gamma} = \text{constant}

Eliminating VV instead gives the third member of the family:

p1γTγ=constantequivalentlyT2T1=(p2p1)(γ1)/γp^{1-\gamma}T^{\gamma} = \text{constant} \qquad \text{equivalently} \qquad \frac{T_2}{T_1} = \left(\frac{p_2}{p_1}\right)^{(\gamma-1)/\gamma}

Key Point: For a reversible adiabatic change of an ideal gas with constant heat capacities, pVγ=pV^{\gamma} = constant, TVγ1=TV^{\gamma-1} = constant and p1γTγ=p^{1-\gamma}T^{\gamma} = constant, where γ=Cp,m/Cv,m\gamma = C_{p,m}/C_{v,m}. Drop any one of those three conditions and the relations no longer hold.

Values of γ\gamma

For an ideal monatomic gas such as He, Ne or Ar, kinetic theory gives three translational degrees of freedom and

Cv,m=32RCp,m=Cv,m+R=52Rγ=5/23/2=531.67C_{v,m} = \frac{3}{2}R \qquad C_{p,m} = C_{v,m} + R = \frac{5}{2}R \qquad \gamma = \frac{5/2}{3/2} = \frac{5}{3} \approx 1.67

For an ideal diatomic gas such as H2\mathrm{H_2}, N2\mathrm{N_2} or O2\mathrm{O_2} at ordinary temperatures, two rotational degrees of freedom are also active and

Cv,m=52RCp,m=72Rγ=7/25/2=75=1.4C_{v,m} = \frac{5}{2}R \qquad C_{p,m} = \frac{7}{2}R \qquad \gamma = \frac{7/2}{5/2} = \frac{7}{5} = 1.4

Numerically, Cv,m=12.47 JK1mol1C_{v,m} = 12.47\ \mathrm{J\,K^{-1}\,mol^{-1}} for a monatomic gas and 20.79 JK1mol120.79\ \mathrm{J\,K^{-1}\,mol^{-1}} for a diatomic one.

These values assume the vibrational modes are not excited. At high temperature the vibrations of a diatomic molecule start to absorb energy, Cv,mC_{v,m} rises above 5R/25R/2 and γ\gamma falls below 1.41.4. For a linear triatomic or a bent triatomic molecule the count changes again. Exam problems say "monatomic" or "diatomic" precisely so that you may use 5/35/3 and 7/57/5 without worrying about this.

Work in an adiabatic process

Since q=0q = 0, the work follows directly from the internal energy change:

w=ΔU=nCv,m(T2T1)w = \Delta U = nC_{v,m}(T_2 - T_1)

Replacing Cv,m=R/(γ1)C_{v,m} = R/(\gamma - 1) gives the form most useful when temperatures are known,

w=nR(T2T1)γ1w = \frac{nR(T_2 - T_1)}{\gamma - 1}

and using pV=nRTpV = nRT at each end, nRT2=p2V2nRT_2 = p_2V_2 and nRT1=p1V1nRT_1 = p_1V_1, gives the form most useful when pressures and volumes are known:

w=p2V2p1V1γ1w = \frac{p_2V_2 - p_1V_1}{\gamma - 1}

All three expressions are the same equation. In an expansion T2<T1T_2 < T_1, so ww is negative: the gas does work on the surroundings and pays for it out of its own internal energy. In a compression T2>T1T_2 > T_1 and ww is positive.

One warning that costs marks every year is worth stating flatly. The three pVγpV^\gamma-type relations were derived for a reversible adiabatic path. An adiabatic expansion against a constant external pressure is irreversible, and those relations do not apply to it. What still applies is q=0q = 0 and

nCv,m(T2T1)=w=pex(V2V1)nC_{v,m}(T_2 - T_1) = w = -p_{ex}(V_2 - V_1)

which is solved for T2T_2 directly. Question 6 below works through exactly this case.

The two adiabatic paths differ in every quantity except qq:

Reversible adiabatic Irreversible adiabatic (constant pexp_{ex})
qq 00 00
pVγ=pV^{\gamma} = constant applies does not apply
Route to T2T_2 T2=T1(V1/V2)γ1T_2 = T_1(V_1/V_2)^{\gamma-1} solve nCv,m(T2T1)=pex(V2V1)nC_{v,m}(T_2-T_1) = -p_{ex}(V_2-V_1)
ww nCv,m(T2T1)nC_{v,m}(T_2-T_1) pex(V2V1)-p_{ex}(V_2-V_1), equal to nCv,m(T2T1)nC_{v,m}(T_2-T_1)
Cooling on expansion larger smaller
ΔS\Delta S of the gas 00 greater than 00

The last row is worth holding on to. Both processes have q=0q = 0, but only the reversible one has ΔS=0\Delta S = 0. Adiabatic and isentropic mean the same thing only when the path is also reversible.

A third adiabatic case sits at the far end of the same scale. In a free expansion the gas expands into an evacuated space, so pex=0p_{ex} = 0 and w=0w = 0. If the container is also insulated, q=0q = 0 as well, and the first law gives ΔU=0\Delta U = 0. For an ideal gas, zero ΔU\Delta U means zero ΔT\Delta T: a free expansion of an ideal gas is both adiabatic and isothermal, and neither pVγpV^\gamma nor the cooling of the ordinary adiabatic case occurs. The entropy still rises, by nRln(V2/V1)nR\ln(V_2/V_1), because the final state is the same as that reached by an isothermal expansion.

Isothermal and Adiabatic Curves Compared

Draw both processes on a pp-VV diagram starting from the same state (p1,V1)(p_1, V_1) and let the gas expand to the same final volume V2V_2. The two curves separate immediately, and the reason is temperature.

Along the isotherm the gas is held at T1T_1 by contact with a thermostat, so heat flows in to replace the energy spent as work. Along the adiabat no heat enters, so the energy spent as work comes out of the internal energy and the gas cools. A cooler gas at a given volume has a lower pressure. The adiabat therefore lies below the isotherm at every volume beyond the common starting point.

Isotherm and steeper adiabat from a common point with shaded work areas compared

The slopes

Differentiate the isothermal condition pV=pV = constant:

pdV+Vdp=0(dpdV)T=pVp\,dV + V\,dp = 0 \qquad \Rightarrow \qquad \left(\frac{dp}{dV}\right)_{T} = -\frac{p}{V}

Differentiate the adiabatic condition pVγ=pV^{\gamma} = constant by the product rule:

γpVγ1dV+Vγdp=0(dpdV)ad=γpV\gamma p V^{\gamma-1}\,dV + V^{\gamma}\,dp = 0 \qquad \Rightarrow \qquad \left(\frac{dp}{dV}\right)_{ad} = -\frac{\gamma p}{V}

Both slopes are negative, and at any common point (p,V)(p, V) they differ by exactly the factor γ\gamma.

Key Point: For an ideal gas, at any point on a pp-VV diagram the reversible adiabat is steeper than the isotherm through that point by the factor γ=Cp,m/Cv,m\gamma = C_{p,m}/C_{v,m}. Since γ>1\gamma > 1 always, the adiabat always falls away more sharply. The statement belongs to reversible paths only: an irreversible adiabatic expansion against a constant external pressure does not obey pVγ=pV^{\gamma} = constant and is not a curve of this kind at all.

For a monatomic gas the adiabat is 5/35/3 times as steep as the isotherm through the same point; for a diatomic gas, 1.41.4 times as steep.

Numbers make the separation concrete. Take 1.0 mol of an ideal monatomic gas starting at 300 K in 10.0 L, where p1=nRT/V=(0.08314)(300)/10.0=2.49 barp_1 = nRT/V = (0.08314)(300)/10.0 = 2.49\ \mathrm{bar}, and follow both paths outward.

VV / L pp on the isotherm / bar pp on the adiabat / bar Gas temperature on the adiabat / K
10.0 2.49 2.49 300
15.0 1.66 1.27 229
20.0 1.25 0.79 189
30.0 0.83 0.40 144

The isothermal pressures come from p=p1V1/Vp = p_1V_1/V and the adiabatic ones from p=p1(V1/V)5/3p = p_1(V_1/V)^{5/3}. By the time the volume has tripled, the adiabatic pressure has fallen to less than half the isothermal one, and the gas has cooled to 144 K.

Which process does more work

Work done by the gas is the area under the curve on a pp-VV diagram. Between the same two volumes, starting from the same state, the isotherm lies above the adiabat everywhere, so the area under it is larger.

wisothermal>wadiabatic(same initial state, same V2>V1)\lvert w_{isothermal} \rvert > \lvert w_{adiabatic} \rvert \qquad \text{(same initial state, same } V_2 > V_1)

The physical reading is short: in the isothermal expansion the gas is being fed heat continuously, and that borrowed energy is delivered as extra work. In the adiabatic expansion the gas spends only what it already had.

The comparison flips for a compression. Compressing from the same initial state down to the same final volume, the adiabat rises more steeply, so the area under it is larger and more work must be done on the gas adiabatically than isothermally. An adiabatic compression also leaves the gas hotter, which is why a bicycle pump warms up.

A useful ordering for a single expansion between the same two volumes, from most work delivered to least:

  1. Isothermal reversible expansion — largest.
  2. Adiabatic reversible expansion — smaller, because the gas cools on the way.
  3. Any single-step irreversible expansion against a constant external pressure — smaller still, because the opposing pressure never falls.
  4. Free expansion into a vacuum — zero, because pex=0p_{ex} = 0.

That ordering carries a condition worth stating plainly: all four paths must start from the same state and finish at the same volume. If instead the paths are made to finish at the same final pressure, the volumes reached differ, the areas are no longer being compared over the same interval, and the ranking can change. Any comparison of work has to fix what the two paths have in common before it means anything.

The same caution applies to the heat. The isothermal expansion absorbs w\lvert w \rvert of heat, the adiabatic one absorbs none, and the irreversible one absorbs whatever its smaller work demands. Only ΔU\Delta U and ΔH\Delta H are indifferent to the path, and even they are equal across these cases only when the final temperatures agree, which they do not here.

[JEE Main] A question that asks only "which is greater" can be answered from the diagram in seconds. Sketch the two curves from the common point and compare areas; no arithmetic is needed.

Cyclic Processes and Work as an Area

A cyclic process returns the system to its exact starting state. Every state function has the same value at the end as at the start, so for one complete cycle

ΔU=0ΔH=0ΔS=0ΔG=0\Delta U = 0 \qquad \Delta H = 0 \qquad \Delta S = 0 \qquad \Delta G = 0

Feeding ΔU=0\Delta U = 0 into the first law leaves the single most useful statement about cycles:

qcycle=wcycleq_{cycle} = -w_{cycle}

Net heat absorbed over a cycle equals net work done by the gas. Neither qq nor ww is a state function, so neither is zero in general; only their sum is.

Closed clockwise cycle on a pressure volume diagram with the enclosed area shaded

Reading the area

For any step, the work done on the gas is w=pexdVw = -\int p_{ex}\,dV, and on a reversible path pex=pp_{ex} = p, so the magnitude of the work is the area under that step of the curve. Around a closed loop the areas under the outward and return paths partly cancel, and what survives is the area enclosed by the loop.

Key Point: For a cyclic process the magnitude of the net work equals the area enclosed by the loop on the pp-VV diagram. A clockwise loop means net work done by the gas, so w<0w < 0 and q>0q > 0 in the IUPAC convention. An anticlockwise loop means net work done on the gas, so w>0w > 0 and q<0q < 0.

The sign rule follows from the geometry. In a clockwise loop the expansion half of the cycle happens along the upper, higher-pressure branch and the compression half along the lower branch. The gas therefore pushes out at high pressure and is pushed back in at low pressure, and it wins on the exchange. This is exactly what a heat engine does: absorb heat, deliver work, reject the rest. An anticlockwise loop is that engine run backwards, which is a refrigerator or a heat pump.

Working a cycle in practice

The reliable method is a small table. List the steps down the side and ww, ΔU\Delta U, qq across the top, fill in whichever two entries each process makes easy, and get the third from ΔU=q+w\Delta U = q + w. Then check that the ΔU\Delta U column sums to zero. That check catches almost every sign error.

Step type Which entry is easiest first Then
Isochoric w=0w = 0 ΔU=nCv,mΔT\Delta U = nC_{v,m}\Delta T, and q=ΔUq = \Delta U
Isobaric w=pΔV=nRΔTw = -p\Delta V = -nR\Delta T q=ΔH=nCp,mΔTq = \Delta H = nC_{p,m}\Delta T, and ΔU=q+w\Delta U = q + w
Isothermal reversible ΔU=0\Delta U = 0 w=nRTln(V2/V1)w = -nRT\ln(V_2/V_1), and q=wq = -w
Adiabatic q=0q = 0 w=ΔU=nCv,mΔTw = \Delta U = nC_{v,m}\Delta T

Two conversions make the arithmetic painless when pressures are in bar and volumes in litres:

1 barL=100 J1 atmL=101.3 J1\ \mathrm{bar\,L} = 100\ \mathrm{J} \qquad 1\ \mathrm{atm\,L} = 101.3\ \mathrm{J}

A rectangular cycle built from two isobars and two isochores has an area that is simply Δp×ΔV\Delta p \times \Delta V, which is the fastest area to evaluate. For a cycle containing an isothermal step the logarithmic work expression is needed for that step, and for one containing an adiabatic step the work is nCv,mΔTnC_{v,m}\Delta T for that step.

One caution about efficiency. The net work of a cycle is not the whole heat absorbed, because some steps of the cycle reject heat. The efficiency is

η=wnetqabsorbed\eta = \frac{\lvert w_{net} \rvert}{q_{absorbed}}

where qabsorbedq_{absorbed} counts only the steps in which qq is positive, not the algebraic sum. Using the net heat in the denominator gives η=1\eta = 1 for every cycle, which is the giveaway that the wrong quantity was used.

The upper limit on η\eta is set by the second law. A cycle built from two reversible isotherms at ThotT_{hot} and TcoldT_{cold} joined by two reversible adiabats — the Carnot cycle — has

ηmax=1TcoldThot\eta_{max} = 1 - \frac{T_{cold}}{T_{hot}}

with both temperatures in kelvin. No cycle working between the same two temperatures can beat it, and every real cycle falls short because its steps are irreversible. The efficiency depends only on the two temperatures, not on the gas or on how much of it there is.

Where the state functions help

The reason cycles are worth setting up carefully is that they turn hard questions into easy ones. Any quantity that is a state function can be obtained by whichever route through the cycle is simplest, because the answer does not depend on the route. If a problem asks for ΔU\Delta U from A to C and the direct path is awkward, going A to B to C gives the same number. The same freedom is what Hess's law exploits for reaction enthalpies, and it is the same principle wearing different clothes.

What cannot be moved between routes is qq and ww. Each of those belongs to the particular path taken, which is exactly why the enclosed area of a cycle is not zero even though ΔU\Delta U is.

Cycles drawn on other axes

A cycle is sometimes given on pp-TT or VV-TT axes instead, and the first job is to identify each step before any arithmetic starts. Reading the graph is a matter of knowing what each process looks like on those axes.

Process On pp-VV axes On pp-TT axes On VV-TT axes
Isochoric vertical line straight line through the origin horizontal line
Isobaric horizontal line horizontal line straight line through the origin
Isothermal rectangular hyperbola vertical line vertical line

The straight lines through the origin come from pTp \propto T at fixed VV and VTV \propto T at fixed pp, both direct readings of pV=nRTpV = nRT. Once each step is named, the work is computed on pp-VV thinking as usual, since the area rule belongs to those axes alone. An area enclosed on a pp-TT or VV-TT plot has no thermodynamic meaning at all.

Kirchhoff's Equation — How ΔrH\Delta_r H Changes with Temperature

Tables of standard enthalpies of formation are quoted at 298 K. Industrial reactions are run at 700 K or 1200 K, and the reaction enthalpy is not the same there. Kirchhoff's equation supplies the correction.

Start from the definition of heat capacity at constant pressure applied to a single substance. Warming a substance from T1T_1 to T2T_2 at constant pressure changes its enthalpy by

H(T2)=H(T1)+Cp(T2T1)H(T_2) = H(T_1) + C_p (T_2 - T_1)

when CpC_p is constant over the interval. Apply this to the products and to the reactants of a reaction separately, then subtract. The enthalpy difference between products and reactants is ΔrH\Delta_r H, and the heat capacity difference is

ΔCp=Cp(products)Cp(reactants)\Delta C_p = \sum C_{p}(\text{products}) - \sum C_{p}(\text{reactants})

each term weighted by its stoichiometric coefficient. Subtracting gives

ΔrH(T2)ΔrH(T1)=ΔCp(T2T1)\Delta_r H(T_2) - \Delta_r H(T_1) = \Delta C_p\,(T_2 - T_1)

Key Point (Definition): Kirchhoff's equation is ΔrH(T2)=ΔrH(T1)+ΔCp(T2T1)\Delta_r H(T_2) = \Delta_r H(T_1) + \Delta C_p (T_2 - T_1), where ΔCp\Delta C_p is the stoichiometric sum of the molar heat capacities of the products minus that of the reactants. It assumes ΔCp\Delta C_p is effectively constant across the temperature range and that no substance changes phase within that range.

Both conditions matter. Heat capacities themselves drift with temperature, so over a range of many hundreds of kelvin the constant-ΔCp\Delta C_p form is an approximation. The exact statement is a derivative,

(ΔrHT)p=ΔCp\left(\frac{\partial \Delta_r H}{\partial T}\right)_p = \Delta C_p

whose integrated form is

ΔrH(T2)=ΔrH(T1)+T1T2ΔCpdT\Delta_r H(T_2) = \Delta_r H(T_1) + \int_{T_1}^{T_2} \Delta C_p\,dT

and the linear equation above is what that integral becomes when ΔCp\Delta C_p is pulled out as a constant. If a reactant or product melts or boils between T1T_1 and T2T_2, the latent heat of that transition has to be added separately, because the simple linear form cannot see it. For a reaction of water, for instance, a range that straddles 373 K needs the enthalpy of vaporisation inserted at that point and the heat capacity of steam used above it.

The sign of ΔCp\Delta C_p decides the direction of the drift.

  • ΔCp>0\Delta C_p > 0: the products absorb heat faster than the reactants, so ΔrH\Delta_r H becomes more positive (less exothermic) as TT rises.
  • ΔCp<0\Delta C_p < 0: ΔrH\Delta_r H becomes more negative (more exothermic) as TT rises.
  • ΔCp=0\Delta C_p = 0: the reaction enthalpy is independent of temperature over that range.

There is a matching statement for internal energy at constant volume,

ΔrU(T2)=ΔrU(T1)+ΔCv(T2T1)\Delta_r U(T_2) = \Delta_r U(T_1) + \Delta C_v\,(T_2 - T_1)

with ΔCv\Delta C_v built the same way from constant-volume heat capacities. The two forms are consistent with each other. Differentiating ΔrH=ΔrU+ΔngRT\Delta_r H = \Delta_r U + \Delta n_g RT with respect to temperature gives

ΔCp=ΔCv+ΔngR\Delta C_p = \Delta C_v + \Delta n_g R

which is just Cp,mCv,m=RC_{p,m} - C_{v,m} = R applied to every gaseous species and summed with its stoichiometric sign. Solids and liquids contribute nothing to Δng\Delta n_g, so only the gases matter in that correction.

A worked feel for the size of the effect: for the ammonia synthesis ΔCp\Delta C_p is about 45 JK1mol1-45\ \mathrm{J\,K^{-1}\,mol^{-1}}, so raising the temperature by 200 K shifts ΔrH\Delta_r H by about 9 kJmol1-9\ \mathrm{kJ\,mol^{-1}} against a reaction enthalpy of 92.4 kJmol1-92.4\ \mathrm{kJ\,mol^{-1}}. The correction is a tenth of the value — small enough to ignore in a rough estimate, far too large to ignore in a plant design.

[JEE Main] Watch the units. Reaction enthalpies come in kJmol1\mathrm{kJ\,mol^{-1}} and heat capacities in JK1mol1\mathrm{J\,K^{-1}\,mol^{-1}}. The correction term ΔCp(T2T1)\Delta C_p(T_2-T_1) lands in joules and must be divided by 1000 before it is added.

Entropy Changes for an Ideal Gas

Entropy is a state function defined through a reversible path by dS=dqrev/TdS = dq_{rev}/T. For an ideal gas that definition can be turned into a formula in TT and VV that works for any change of state, reversible or not, because SS depends only on the endpoints.

For an infinitesimal reversible step, the first law gives dqrev=dU+pdVdq_{rev} = dU + p\,dV. For an ideal gas dU=nCv,mdTdU = nC_{v,m}\,dT and p=nRT/Vp = nRT/V, so

dS=dqrevT=nCv,mdTT+nRdVVdS = \frac{dq_{rev}}{T} = \frac{nC_{v,m}\,dT}{T} + \frac{nR\,dV}{V}

Integrating between the two states, with Cv,mC_{v,m} taken as constant,

ΔS=nCv,mlnT2T1+nRlnV2V1\Delta S = nC_{v,m}\ln\frac{T_2}{T_1} + nR\ln\frac{V_2}{V_1}

The same change expressed in TT and pp, obtained by substituting V=nRT/pV = nRT/p and using Cp,m=Cv,m+RC_{p,m} = C_{v,m} + R, is

ΔS=nCp,mlnT2T1nRlnp2p1\Delta S = nC_{p,m}\ln\frac{T_2}{T_1} - nR\ln\frac{p_2}{p_1}

Key Point: For nn moles of an ideal gas, ΔS=nCv,mln(T2/T1)+nRln(V2/V1)\Delta S = nC_{v,m}\ln(T_2/T_1) + nR\ln(V_2/V_1). Because entropy is a state function, this holds for any process joining those two states, however irreversible the actual path was. The reversible path was used only to evaluate the integral.

Three special cases fall straight out.

Isothermal change. T2=T1T_2 = T_1, so the first term vanishes:

ΔS=nRlnV2V1=2.303nRlogV2V1=2.303nRlogp1p2\Delta S = nR\ln\frac{V_2}{V_1} = 2.303\,nR\log\frac{V_2}{V_1} = 2.303\,nR\log\frac{p_1}{p_2}

Expansion raises entropy; compression lowers it. For an isothermal reversible expansion the surroundings lose exactly what the system gains, so ΔStotal=0\Delta S_{total} = 0, which is the signature of a reversible process. For an isothermal irreversible expansion ΔSsys\Delta S_{sys} is the same number, but the surroundings give up less heat, so ΔStotal>0\Delta S_{total} > 0.

Constant volume. ΔS=nCv,mln(T2/T1)\Delta S = nC_{v,m}\ln(T_2/T_1). Heating raises entropy. At constant pressure the matching result is ΔS=nCp,mln(T2/T1)\Delta S = nC_{p,m}\ln(T_2/T_1), larger for the same temperature rise because the gas also expands.

Reversible adiabatic change. Substituting T2/T1=(V1/V2)γ1T_2/T_1 = (V_1/V_2)^{\gamma-1} into the general formula gives

ΔS=nCv,m(γ1)lnV1V2+nRlnV2V1=nRlnV2V1+nRlnV2V1=0\Delta S = nC_{v,m}(\gamma-1)\ln\frac{V_1}{V_2} + nR\ln\frac{V_2}{V_1} = -nR\ln\frac{V_2}{V_1} + nR\ln\frac{V_2}{V_1} = 0

using Cv,m(γ1)=RC_{v,m}(\gamma-1) = R. A reversible adiabatic process is isentropic. An irreversible adiabatic expansion, by contrast, has q=0q = 0 but ΔS>0\Delta S > 0, so "adiabatic" and "constant entropy" are not synonyms.

The surroundings and the total

Entropy decides spontaneity only through the total, ΔStotal=ΔSsys+ΔSsurr\Delta S_{total} = \Delta S_{sys} + \Delta S_{surr}. The surroundings are treated as a reservoir so large that heat entering or leaving does not change its temperature, and any heat it exchanges is therefore exchanged reversibly:

ΔSsurr=qsurrT=qsysT\Delta S_{surr} = \frac{q_{surr}}{T} = -\frac{q_{sys}}{T}

Two isothermal expansions of the same gas between the same two states show what this buys. Take 1.0 mol expanding at 300 K from 10.0 L to 20.0 L. In both cases ΔSsys=Rln2=5.76 JK1\Delta S_{sys} = R\ln 2 = 5.76\ \mathrm{J\,K^{-1}}, because entropy is a state function.

Carried out reversibly, the gas absorbs qrev=1729 Jq_{rev} = 1729\ \mathrm{J}, so ΔSsurr=1729/300=5.76 JK1\Delta S_{surr} = -1729/300 = -5.76\ \mathrm{J\,K^{-1}} and ΔStotal=0\Delta S_{total} = 0. Carried out against a constant external pressure equal to the final pressure, the gas does less work and absorbs only q=1247 Jq = 1247\ \mathrm{J}, so ΔSsurr=1247/300=4.16 JK1\Delta S_{surr} = -1247/300 = -4.16\ \mathrm{J\,K^{-1}} and

ΔStotal=5.764.16=+1.60 JK1>0\Delta S_{total} = 5.76 - 4.16 = +1.60\ \mathrm{J\,K^{-1}} > 0

The system's entropy change is identical on the two paths; the surroundings' is not, because qq is a path function. That difference is the whole content of the second law for this process.

For a phase change at its transition temperature, where the change is reversible by construction,

ΔStrans=ΔHtransTtrans\Delta S_{trans} = \frac{\Delta H_{trans}}{T_{trans}}

with TtransT_{trans} the melting or boiling point in kelvin.

Entropy of mixing

Two ideal gases at the same temperature and pressure, separated by a partition, mix spontaneously when the partition is removed. No heat is exchanged and no work is done, yet the process runs one way only. Entropy explains it.

Each gas expands from the volume it occupied alone into the whole container. For gas A, V2/V1=Vtotal/VA=1/xAV_2/V_1 = V_{total}/V_A = 1/x_A, where xAx_A is its mole fraction. Its entropy rise is nARlnxA-n_A R\ln x_A. Adding the contribution of every component,

ΔSmix=Rinilnxior per mole of mixtureΔSmix=Rixilnxi\Delta S_{mix} = -R\sum_i n_i \ln x_i \qquad \text{or per mole of mixture} \qquad \Delta S_{mix} = -R\sum_i x_i \ln x_i

Every mole fraction is less than 1, so every logarithm is negative and ΔSmix\Delta S_{mix} is always positive. For one mole each of two gases, ΔSmix=8.314(ln0.5+ln0.5)=11.53 JK1\Delta S_{mix} = -8.314(\ln 0.5 + \ln 0.5) = 11.53\ \mathrm{J\,K^{-1}}.

Since mixing ideal gases has ΔHmix=0\Delta H_{mix} = 0, the Gibbs energy of mixing is ΔGmix=TΔSmix\Delta G_{mix} = -T\Delta S_{mix}, which is negative at every temperature. Mixing of ideal gases is spontaneous and never reverses on its own.

Gibbs Energy Away from Standard Conditions

ΔrG\Delta_r G^{\circ} is a single fixed number for a balanced equation at a stated temperature, defined with every reactant and product in its standard state — pure, at 1 bar, and at unit concentration for solutions. A real reaction vessel almost never contains that mixture. The quantity that decides which way a real mixture will move is ΔrG\Delta_r G, and the two are connected by

ΔrG=ΔrG+RTlnQ\Delta_r G = \Delta_r G^{\circ} + RT\ln Q

Here QQ is the reaction quotient: the same combination of partial pressures or concentrations that appears in the equilibrium constant, but evaluated with whatever amounts are present at that moment rather than with equilibrium amounts. For a gas reaction

aA(g)+bB(g)cC(g)+dD(g)Qp=(pC/p)c(pD/p)d(pA/p)a(pB/p)ba\mathrm{A}(g) + b\mathrm{B}(g) \rightleftharpoons c\mathrm{C}(g) + d\mathrm{D}(g) \qquad Q_p = \frac{(p_{\mathrm{C}}/p^{\circ})^{c}\,(p_{\mathrm{D}}/p^{\circ})^{d}}{(p_{\mathrm{A}}/p^{\circ})^{a}\,(p_{\mathrm{B}}/p^{\circ})^{b}}

with p=1 barp^{\circ} = 1\ \mathrm{bar}, which makes QQ dimensionless so that its logarithm is defined. In practice the partial pressures are simply entered in bar and the pp^{\circ} divisions are silent.

Two checks confirm that the equation is sensible. If the mixture happens to be in standard states, every ratio is 1, Q=1Q = 1, lnQ=0\ln Q = 0 and ΔrG=ΔrG\Delta_r G = \Delta_r G^{\circ}. And at equilibrium the mixture has no tendency to move either way, so ΔrG=0\Delta_r G = 0 while QQ has reached its equilibrium value KK. Putting both facts in,

0=ΔrG+RTlnKΔrG=RTlnK=2.303RTlogK0 = \Delta_r G^{\circ} + RT\ln K \qquad \Rightarrow \qquad \Delta_r G^{\circ} = -RT\ln K = -2.303\,RT\log K

Key Point: ΔrG=ΔrG+RTlnQ\Delta_r G = \Delta_r G^{\circ} + RT\ln Q gives the driving force of a mixture at its actual composition. Setting ΔrG=0\Delta_r G = 0 and Q=KQ = K recovers ΔrG=RTlnK\Delta_r G^{\circ} = -RT\ln K. The first equation describes a particular vessel; the second is a property of the reaction alone.

Substituting ΔrG=RTlnK\Delta_r G^{\circ} = -RT\ln K back into the first equation collapses both into one statement:

ΔrG=RTlnQK\Delta_r G = RT\ln\frac{Q}{K}

which reads off the direction of change immediately.

Condition Sign of ΔrG\Delta_r G What the mixture does
Q<KQ < K negative runs forward, making more product
Q=KQ = K zero at equilibrium, composition fixed
Q>KQ > K positive runs backward, remaking reactant

This settles a confusion that costs marks. A reaction with a large positive ΔrG\Delta_r G^{\circ} is not forbidden. It has a small KK, so it proceeds only a little way — but if the vessel starts with almost no product, QQ is smaller still, ln(Q/K)\ln(Q/K) is negative, and the reaction does run forward until QQ climbs to KK. What ΔrG\Delta_r G^{\circ} fixes is the stopping point, not whether anything happens at all.

The temperature dependence sits inside ΔrG=ΔrHTΔrS\Delta_r G^{\circ} = \Delta_r H^{\circ} - T\Delta_r S^{\circ}. Combining it with ΔrG=RTlnK\Delta_r G^{\circ} = -RT\ln K and dividing by RT-RT,

lnK=ΔrHRT+ΔrSR\ln K = -\frac{\Delta_r H^{\circ}}{RT} + \frac{\Delta_r S^{\circ}}{R}

A plot of lnK\ln K against 1/T1/T is a straight line of slope ΔrH/R-\Delta_r H^{\circ}/R and intercept ΔrS/R\Delta_r S^{\circ}/R, provided ΔrH\Delta_r H^{\circ} and ΔrS\Delta_r S^{\circ} are roughly constant over the range. An exothermic reaction has a positive slope, so KK falls as TT rises — the quantitative form of the qualitative rule that heating shifts an exothermic equilibrium backwards.

Writing that line at two temperatures and subtracting eliminates the entropy term and gives the two-point form,

lnK2K1=ΔrHR(1T11T2)\ln\frac{K_2}{K_1} = \frac{\Delta_r H^{\circ}}{R}\left(\frac{1}{T_1} - \frac{1}{T_2}\right)

which converts a value of KK at one temperature into a value at another using only the reaction enthalpy. The same caution attaches: ΔrH\Delta_r H^{\circ} must be effectively constant across the interval, which is the assumption Kirchhoff's equation exists to correct when it is not.

What ΔG\Delta G measures

At constant temperature and pressure, ΔG-\Delta G is the maximum work other than expansion work that a process can deliver:

wnonexpansion, max=ΔGw_{non-expansion,\ max} = \Delta G

in the IUPAC convention, where work done on the system is positive, so a negative ΔG\Delta G corresponds to work delivered by the system. That maximum is reached only on a reversible path; any real process delivers less, with the shortfall appearing as entropy generated. This is the quantity a galvanic cell converts into electrical work, and the reason ΔrG=nFE\Delta_r G^{\circ} = -nFE^{\circ} appears in electrochemistry rather than ΔrH\Delta_r H^{\circ}.

[JEE/NEET] A negative ΔrG\Delta_r G^{\circ} means K>1K > 1, and a positive ΔrG\Delta_r G^{\circ} means K<1K < 1. Neither says anything about how fast the reaction goes: thermodynamics fixes the destination, kinetics fixes the travelling time.

Question 1: The isochoric row, filled in

2.0 mol of an ideal monatomic gas is heated from 300 K to 500 K in a sealed rigid vessel. Find ww, ΔU\Delta U, qq and ΔH\Delta H. Take R=8.314 JK1mol1R = 8.314\ \mathrm{J\,K^{-1}\,mol^{-1}}.

Answer:

The vessel is rigid, so ΔV=0\Delta V = 0 and no expansion work is possible.

w=pexΔV=0w = -p_{ex}\Delta V = 0

The gas is monatomic, so Cv,m=32R=12.47 JK1mol1C_{v,m} = \tfrac{3}{2}R = 12.47\ \mathrm{J\,K^{-1}\,mol^{-1}} and Cp,m=52R=20.79 JK1mol1C_{p,m} = \tfrac{5}{2}R = 20.79\ \mathrm{J\,K^{-1}\,mol^{-1}}. The temperature rise is ΔT=500300=200 K\Delta T = 500 - 300 = 200\ \mathrm{K}.

ΔU=nCv,mΔT=2.0×12.47×200=4988 J\Delta U = nC_{v,m}\Delta T = 2.0 \times 12.47 \times 200 = 4988\ \mathrm{J}

From the first law with w=0w = 0, the heat is the whole of the internal energy change.

qv=ΔU=+4.99 kJq_v = \Delta U = +4.99\ \mathrm{kJ}

For the enthalpy I use the ideal-gas result that works on any path.

ΔH=nCp,mΔT=2.0×20.79×200=8316 J=+8.32 kJ\Delta H = nC_{p,m}\Delta T = 2.0 \times 20.79 \times 200 = 8316\ \mathrm{J} = +8.32\ \mathrm{kJ}

Ans: w=0w = 0, ΔU=q=+4.99 kJ\Delta U = q = +4.99\ \mathrm{kJ}, ΔH=+8.32 kJ\Delta H = +8.32\ \mathrm{kJ} Watch out: ΔH\Delta H is not zero just because the volume is fixed. The temperature changed, and for an ideal gas that alone fixes ΔH\Delta H. Here ΔH=ΔU+VΔp\Delta H = \Delta U + V\Delta p, and the pressure did rise.

Question 2: The isobaric row, filled in

3.0 mol of an ideal diatomic gas is heated from 300 K to 400 K at a constant pressure of 1.0 bar. Find ww, ΔU\Delta U, qq and ΔH\Delta H.

Answer:

For a diatomic gas Cv,m=52R=20.79 JK1mol1C_{v,m} = \tfrac{5}{2}R = 20.79\ \mathrm{J\,K^{-1}\,mol^{-1}} and Cp,m=72R=29.10 JK1mol1C_{p,m} = \tfrac{7}{2}R = 29.10\ \mathrm{J\,K^{-1}\,mol^{-1}}, and ΔT=+100 K\Delta T = +100\ \mathrm{K}.

The pressure is constant at both ends, so I can convert pΔVp\Delta V into nRΔTnR\Delta T using the gas equation at each state.

w=pΔV=nRΔT=3.0×8.314×100=2494 Jw = -p\Delta V = -nR\Delta T = -3.0 \times 8.314 \times 100 = -2494\ \mathrm{J}

The sign is negative because the gas expanded on heating and pushed the surroundings back.

ΔH=qp=nCp,mΔT=3.0×29.10×100=8730 J=+8.73 kJ\Delta H = q_p = nC_{p,m}\Delta T = 3.0 \times 29.10 \times 100 = 8730\ \mathrm{J} = +8.73\ \mathrm{kJ}

ΔU=nCv,mΔT=3.0×20.79×100=6237 J=+6.24 kJ\Delta U = nC_{v,m}\Delta T = 3.0 \times 20.79 \times 100 = 6237\ \mathrm{J} = +6.24\ \mathrm{kJ}

I check with the first law: q+w=87302494=6236 Jq + w = 8730 - 2494 = 6236\ \mathrm{J}, which matches ΔU\Delta U.

Ans: w=2.49 kJw = -2.49\ \mathrm{kJ}, ΔU=+6.24 kJ\Delta U = +6.24\ \mathrm{kJ}, q=ΔH=+8.73 kJq = \Delta H = +8.73\ \mathrm{kJ}

Question 3: The isothermal row, filled in

2.0 mol of an ideal gas expands reversibly and isothermally at 300 K from 5.0 L to 25.0 L. Find ww, qq, ΔU\Delta U and ΔH\Delta H.

Answer:

The temperature is constant, so for an ideal gas both ΔU\Delta U and ΔH\Delta H are zero straight away.

ΔU=nCv,mΔT=0ΔH=nCp,mΔT=0\Delta U = nC_{v,m}\Delta T = 0 \qquad \Delta H = nC_{p,m}\Delta T = 0

For the reversible isothermal work,

w=2.303nRTlogV2V1w = -2.303\,nRT\log\frac{V_2}{V_1}

2.303nRT=2.303×2.0×8.314×300=11488 J2.303\,nRT = 2.303 \times 2.0 \times 8.314 \times 300 = 11488\ \mathrm{J}

log25.05.0=log5=0.699\log\frac{25.0}{5.0} = \log 5 = 0.699

w=11488×0.699=8030 J=8.03 kJw = -11488 \times 0.699 = -8030\ \mathrm{J} = -8.03\ \mathrm{kJ}

With ΔU=0\Delta U = 0 the first law gives q=wq = -w.

q=+8.03 kJq = +8.03\ \mathrm{kJ}

Suppose the same expansion is instead carried out in one step against a constant external pressure equal to the final pressure of the gas. The final pressure is

p2=nRTV2=2.0×0.08314×30025.0=2.00 barp_2 = \frac{nRT}{V_2} = \frac{2.0 \times 0.08314 \times 300}{25.0} = 2.00\ \mathrm{bar}

w=pexΔV=(2.00)(25.05.0)=40.0 barL=4.00 kJw = -p_{ex}\Delta V = -(2.00)(25.0-5.0) = -40.0\ \mathrm{bar\,L} = -4.00\ \mathrm{kJ}

ΔU\Delta U and ΔH\Delta H are still zero, because the end states are the same, and qq is still w-w, now +4.00 kJ+4.00\ \mathrm{kJ}.

Ans: Reversible: w=8.03 kJw = -8.03\ \mathrm{kJ}, q=+8.03 kJq = +8.03\ \mathrm{kJ}. Irreversible one-step: w=4.00 kJw = -4.00\ \mathrm{kJ}, q=+4.00 kJq = +4.00\ \mathrm{kJ}. In both, ΔU=ΔH=0\Delta U = \Delta H = 0 Watch out: ΔU=0\Delta U = 0 does not mean nothing happened. It also does not fix ww: the same pair of end states gave two different amounts of work, because work is a path function while internal energy is not.

Question 4: Reversible adiabatic expansion of a monatomic gas

1.0 mol of an ideal monatomic gas at 300 K expands reversibly and adiabatically until its volume doubles. Find the final temperature, ww, ΔU\Delta U and ΔH\Delta H.

Answer:

The gas is monatomic, so γ=5/3\gamma = 5/3 and γ1=2/3\gamma - 1 = 2/3. The path is a reversible adiabatic one for an ideal gas, so TVγ1TV^{\gamma-1} is constant.

T2=T1(V1V2)γ1=300×(12)2/3T_2 = T_1\left(\frac{V_1}{V_2}\right)^{\gamma-1} = 300 \times \left(\frac{1}{2}\right)^{2/3}

(12)2/3=20.667=0.630\left(\frac{1}{2}\right)^{2/3} = 2^{-0.667} = 0.630

T2=300×0.630=189 KT_2 = 300 \times 0.630 = 189\ \mathrm{K}

The gas cooled by 111 K, which is what an adiabatic expansion must do. With q=0q = 0 the work equals the internal energy change.

w=ΔU=nCv,m(T2T1)=1.0×12.47×(111)=1384 Jw = \Delta U = nC_{v,m}(T_2 - T_1) = 1.0 \times 12.47 \times (-111) = -1384\ \mathrm{J}

The same number from the other form, as a check:

w=nR(T2T1)γ1=1.0×8.314×(111)2/3=1384 Jw = \frac{nR(T_2-T_1)}{\gamma-1} = \frac{1.0 \times 8.314 \times (-111)}{2/3} = -1384\ \mathrm{J}

ΔH=nCp,mΔT=1.0×20.79×(111)=2308 J\Delta H = nC_{p,m}\Delta T = 1.0 \times 20.79 \times (-111) = -2308\ \mathrm{J}

Ans: T2=189 KT_2 = 189\ \mathrm{K}, q=0q = 0, w=ΔU=1.38 kJw = \Delta U = -1.38\ \mathrm{kJ}, ΔH=2.31 kJ\Delta H = -2.31\ \mathrm{kJ} Watch out: The exponent in TVγ1TV^{\gamma-1} is γ1\gamma - 1, not γ\gamma. Using γ\gamma by mistake gives 300×(0.5)5/3=94.5 K300 \times (0.5)^{5/3} = 94.5\ \mathrm{K}, which looks like a perfectly reasonable answer and is not one.

Question 5: Adiabatic compression using pressures and volumes

1.0 mol of an ideal diatomic gas at 1.00 bar occupying 20.0 L is compressed reversibly and adiabatically to 5.0 L. Find the final pressure and the work done. Take 1 barL=100 J1\ \mathrm{bar\,L} = 100\ \mathrm{J}.

Answer:

For a diatomic gas γ=1.4\gamma = 1.4. The path is reversible and adiabatic, so p1V1γ=p2V2γp_1V_1^{\gamma} = p_2V_2^{\gamma}.

p2=p1(V1V2)γ=1.00×(20.05.0)1.4=41.4p_2 = p_1\left(\frac{V_1}{V_2}\right)^{\gamma} = 1.00 \times \left(\frac{20.0}{5.0}\right)^{1.4} = 4^{1.4}

log(41.4)=1.4×0.602=0.84341.4=6.96\log(4^{1.4}) = 1.4 \times 0.602 = 0.843 \qquad 4^{1.4} = 6.96

p2=6.96 barp_2 = 6.96\ \mathrm{bar}

For the work I use the form built from pressures and volumes.

w=p2V2p1V1γ1=(6.96)(5.0)(1.00)(20.0)0.4 barLw = \frac{p_2V_2 - p_1V_1}{\gamma - 1} = \frac{(6.96)(5.0) - (1.00)(20.0)}{0.4}\ \mathrm{bar\,L}

=34.820.00.4=14.80.4=37.0 barL=+3.70 kJ= \frac{34.8 - 20.0}{0.4} = \frac{14.8}{0.4} = 37.0\ \mathrm{bar\,L} = +3.70\ \mathrm{kJ}

The positive sign is correct: this is a compression, so work is done on the gas.

The temperatures come from the gas equation at each end, with R=0.08314 LbarK1mol1R = 0.08314\ \mathrm{L\,bar\,K^{-1}\,mol^{-1}}.

T1=p1V1nR=20.01.0×0.08314=241 KT2=p2V2nR=34.80.08314=419 KT_1 = \frac{p_1V_1}{nR} = \frac{20.0}{1.0 \times 0.08314} = 241\ \mathrm{K} \qquad T_2 = \frac{p_2V_2}{nR} = \frac{34.8}{0.08314} = 419\ \mathrm{K}

Checking the work by the temperature form, with Cv,m=52R=20.79 JK1mol1C_{v,m} = \tfrac{5}{2}R = 20.79\ \mathrm{J\,K^{-1}\,mol^{-1}} for a diatomic gas:

w=nCv,m(T2T1)=1.0×20.79×(419241)=+3700 Jw = nC_{v,m}(T_2-T_1) = 1.0 \times 20.79 \times (419-241) = +3700\ \mathrm{J}

which agrees with the pressure-volume form to the precision of the rounding.

Ans: p2=6.96 barp_2 = 6.96\ \mathrm{bar}, T2=419 KT_2 = 419\ \mathrm{K}, w=ΔU=+3.70 kJw = \Delta U = +3.70\ \mathrm{kJ}, q=0q = 0 Watch out: γ1\gamma - 1 in the denominator is 0.4, not 1.4. Dividing by 1.4 gives 1.06 kJ, and the answer is out by a factor of three and a half.

Question 6: Adiabatic expansion against a constant external pressure

1.0 mol of an ideal monatomic gas at 300 K and 5.0 bar expands adiabatically against a constant external pressure of 1.0 bar until mechanical equilibrium is reached. Find the final temperature and the work done.

Answer:

The path is adiabatic but irreversible, because the gas pressure is 5.0 bar while the opposing pressure is 1.0 bar. The relation pVγ=pV^{\gamma} = constant was derived for a reversible path and cannot be used here. What survives is q=0q = 0, so ΔU=w\Delta U = w, together with w=pex(V2V1)w = -p_{ex}(V_2 - V_1).

The gas stops expanding when its pressure equals the external pressure, so p2=1.0 barp_2 = 1.0\ \mathrm{bar}.

nCv,m(T2T1)=pex(nRT2p2nRT1p1)nC_{v,m}(T_2 - T_1) = -p_{ex}\left(\frac{nRT_2}{p_2} - \frac{nRT_1}{p_1}\right)

Putting in n=1n = 1, Cv,m=32RC_{v,m} = \tfrac{3}{2}R, pex=p2=1.0 barp_{ex} = p_2 = 1.0\ \mathrm{bar}, p1=5.0 barp_1 = 5.0\ \mathrm{bar} and dividing both sides by RR:

32(T2300)=(T23005)=(T260)\frac{3}{2}(T_2 - 300) = -\left(T_2 - \frac{300}{5}\right) = -(T_2 - 60)

1.5T2450=T2+601.5T_2 - 450 = -T_2 + 60

2.5T2=510T2=204 K2.5T_2 = 510 \qquad T_2 = 204\ \mathrm{K}

w=ΔU=nCv,m(T2T1)=1.0×12.47×(204300)=1197 Jw = \Delta U = nC_{v,m}(T_2-T_1) = 1.0 \times 12.47 \times (204 - 300) = -1197\ \mathrm{J}

The entropy change is worth adding, because it shows what "irreversible" costs. Using the pressure form for an ideal gas,

ΔS=nCp,mlnT2T1nRlnp2p1=20.79ln2043008.314ln1.05.0\Delta S = nC_{p,m}\ln\frac{T_2}{T_1} - nR\ln\frac{p_2}{p_1} = 20.79\ln\frac{204}{300} - 8.314\ln\frac{1.0}{5.0}

=20.79×(0.386)8.314×(1.609)=8.02+13.38=+5.36 JK1= 20.79 \times (-0.386) - 8.314 \times (-1.609) = -8.02 + 13.38 = +5.36\ \mathrm{J\,K^{-1}}

No heat crossed the boundary, so ΔSsurr=0\Delta S_{surr} = 0 and ΔStotal=+5.36 JK1\Delta S_{total} = +5.36\ \mathrm{J\,K^{-1}}, which is positive as the second law requires for a change that happens on its own. A reversible adiabatic expansion between a different pair of end states would have given exactly zero.

Ans: T2=204 KT_2 = 204\ \mathrm{K}, w=ΔU=1.20 kJw = \Delta U = -1.20\ \mathrm{kJ}, q=0q = 0, ΔH=20.79×(96)=2.00 kJ\Delta H = 20.79 \times (-96) = -2.00\ \mathrm{kJ}, ΔS=+5.36 JK1\Delta S = +5.36\ \mathrm{J\,K^{-1}} Watch out: The reversible formula T2=T1(p2/p1)(γ1)/γT_2 = T_1(p_2/p_1)^{(\gamma-1)/\gamma} would give 158 K here. That number is wrong for this problem, and it is the single most common error in adiabatic questions: the word "adiabatic" alone does not license pVγpV^{\gamma}.

Question 7: Isothermal against adiabatic, same expansion

1.0 mol of an ideal monatomic gas at 300 K expands from 10.0 L to 20.0 L, once reversibly and isothermally, and once reversibly and adiabatically. Compare the work delivered to the surroundings.

Answer:

For the isothermal path the temperature stays at 300 K throughout.

wiso=2.303nRTlogV2V1=2.303×1.0×8.314×300×log2w_{iso} = -2.303\,nRT\log\frac{V_2}{V_1} = -2.303 \times 1.0 \times 8.314 \times 300 \times \log 2

=5744×0.301=1729 J= -5744 \times 0.301 = -1729\ \mathrm{J}

The adiabatic path is the one worked in Question 4: the same gas, the same starting state, the same doubling of volume. There T2=189 KT_2 = 189\ \mathrm{K} and

wad=1384 Jw_{ad} = -1384\ \mathrm{J}

Work delivered to the surroundings is w\lvert w \rvert, so the isothermal expansion delivers 1729 J and the adiabatic one 1384 J. The ratio is 0.80.

wiso>wad\lvert w_{iso} \rvert > \lvert w_{ad} \rvert

The reason is visible in the two final temperatures. The isothermal gas is held at 300 K by heat flowing in, so its pressure stays high all the way and it pushes hard right to the end. The adiabatic gas cools to 189 K, its pressure sags faster, and the area under its curve is smaller.

The final pressures make the same point from the other side. The initial pressure is p1=nRT/V1=(0.08314)(300)/10.0=2.49 barp_1 = nRT/V_1 = (0.08314)(300)/10.0 = 2.49\ \mathrm{bar}. The isothermal path ends at p1/2=1.25 barp_1/2 = 1.25\ \mathrm{bar}, while the adiabatic path ends at p1(1/2)5/3=2.49×0.315=0.79 barp_1(1/2)^{5/3} = 2.49 \times 0.315 = 0.79\ \mathrm{bar}. The adiabatic gas finishes both colder and at a lower pressure, having spent its own internal energy on the work.

Ans: Isothermal 1729 J, adiabatic 1384 J; the isothermal expansion does more work Watch out: This ordering holds when both paths start from the same state and end at the same volume. If instead they end at the same pressure, the volumes differ and the comparison has to be redone.

Question 8: A rectangular cycle

An ideal gas is taken round the cycle A(1.0 bar, 10.0 L)B(3.0 bar, 10.0 L)C(3.0 bar, 30.0 L)D(1.0 bar, 30.0 L)A\mathrm{A}(1.0\ \mathrm{bar},\ 10.0\ \mathrm{L}) \rightarrow \mathrm{B}(3.0\ \mathrm{bar},\ 10.0\ \mathrm{L}) \rightarrow \mathrm{C}(3.0\ \mathrm{bar},\ 30.0\ \mathrm{L}) \rightarrow \mathrm{D}(1.0\ \mathrm{bar},\ 30.0\ \mathrm{L}) \rightarrow \mathrm{A}. Find the net work and the net heat for one cycle.

Answer:

I take the steps one at a time, in bar L, and convert at the end.

AB\mathrm{A} \rightarrow \mathrm{B}: volume fixed at 10.0 L, so w1=0w_1 = 0.

BC\mathrm{B} \rightarrow \mathrm{C}: expansion at a constant 3.0 bar, ΔV=+20.0 L\Delta V = +20.0\ \mathrm{L}.

w2=pΔV=(3.0)(20.0)=60.0 barLw_2 = -p\Delta V = -(3.0)(20.0) = -60.0\ \mathrm{bar\,L}

CD\mathrm{C} \rightarrow \mathrm{D}: volume fixed at 30.0 L, so w3=0w_3 = 0.

DA\mathrm{D} \rightarrow \mathrm{A}: compression at a constant 1.0 bar, ΔV=20.0 L\Delta V = -20.0\ \mathrm{L}.

w4=(1.0)(20.0)=+20.0 barLw_4 = -(1.0)(-20.0) = +20.0\ \mathrm{bar\,L}

wnet=60.0+20.0=40.0 barL=4.0 kJw_{net} = -60.0 + 20.0 = -40.0\ \mathrm{bar\,L} = -4.0\ \mathrm{kJ}

As a check, the loop is a rectangle of height Δp=2.0 bar\Delta p = 2.0\ \mathrm{bar} and width ΔV=20.0 L\Delta V = 20.0\ \mathrm{L}, giving an enclosed area of 40.0 bar L. The sequence goes up the left side, right along the top, down the right side and back left along the bottom, which is clockwise, so the net work is done by the gas and ww is negative.

The cycle returns the gas to state A, so ΔU=0\Delta U = 0 and

qnet=wnet=+4.0 kJq_{net} = -w_{net} = +4.0\ \mathrm{kJ}

The step-by-step heats follow if the gas is specified. Taking it as monatomic and using pV=nRTpV = nRT to compare temperatures, the ratio T/TAT/T_{\mathrm{A}} at A, B, C, D is 1:3:9:31 : 3 : 9 : 3, so the gas is heated on AB\mathrm{A}\rightarrow\mathrm{B} and BC\mathrm{B}\rightarrow\mathrm{C} and cooled on the return steps.

Step ww / bar L ΔU\Delta U / bar L qq / bar L
AB\mathrm{A}\rightarrow\mathrm{B} 00 +30+30 +30+30
BC\mathrm{B}\rightarrow\mathrm{C} 60-60 +90+90 +150+150
CD\mathrm{C}\rightarrow\mathrm{D} 00 90-90 90-90
DA\mathrm{D}\rightarrow\mathrm{A} +20+20 30-30 50-50
Cycle 40-40 00 +40+40

The internal energy entries use ΔU=32nRΔT=32Δ(pV)\Delta U = \tfrac{3}{2}nR\Delta T = \tfrac{3}{2}\Delta(pV) for a monatomic gas, which needs no value of nn at all. The ΔU\Delta U column sums to zero and qnet=wnetq_{net} = -w_{net}, so the table is consistent.

Heat is absorbed on the first two steps, 30+150=180 barL30 + 150 = 180\ \mathrm{bar\,L}, so

η=40180=0.22\eta = \frac{40}{180} = 0.22

Ans: wnet=4.0 kJw_{net} = -4.0\ \mathrm{kJ} (4.0 kJ of work done by the gas), qnet=+4.0 kJq_{net} = +4.0\ \mathrm{kJ}, ΔU=ΔH=0\Delta U = \Delta H = 0, η=22%\eta = 22\% Watch out: The area gives only the magnitude. The direction of travel gives the sign, and reversing the cycle to ADCBA\mathrm{A} \rightarrow \mathrm{D} \rightarrow \mathrm{C} \rightarrow \mathrm{B} \rightarrow \mathrm{A} would give wnet=+4.0 kJw_{net} = +4.0\ \mathrm{kJ} instead.

Question 9: A cycle containing isothermal steps

1.0 mol of an ideal monatomic gas is taken round this cycle: (i) reversible isothermal expansion at 300 K from 10.0 L to 20.0 L; (ii) cooling at constant volume to 150 K; (iii) reversible isothermal compression at 150 K from 20.0 L to 10.0 L; (iv) heating at constant volume back to 300 K. Find ww and qq for each step and for the cycle.

Answer:

Step (i), isothermal at 300 K, ΔU1=0\Delta U_1 = 0:

w1=2.303nRTlog2=2.303×8.314×300×0.301=1729 Jw_1 = -2.303\,nRT\log 2 = -2.303 \times 8.314 \times 300 \times 0.301 = -1729\ \mathrm{J}

q1=w1=+1729 Jq_1 = -w_1 = +1729\ \mathrm{J}

Step (ii), constant volume, w2=0w_2 = 0:

q2=ΔU2=nCv,mΔT=12.47×(150300)=1871 Jq_2 = \Delta U_2 = nC_{v,m}\Delta T = 12.47 \times (150 - 300) = -1871\ \mathrm{J}

Step (iii), isothermal at 150 K, ΔU3=0\Delta U_3 = 0, and the volume ratio is now 1/21/2:

w3=2.303×8.314×150×log12=2872×(0.301)=+864 Jw_3 = -2.303 \times 8.314 \times 150 \times \log\frac{1}{2} = -2872 \times (-0.301) = +864\ \mathrm{J}

q3=864 Jq_3 = -864\ \mathrm{J}

Step (iv), constant volume, w4=0w_4 = 0:

q4=ΔU4=12.47×(300150)=+1871 Jq_4 = \Delta U_4 = 12.47 \times (300 - 150) = +1871\ \mathrm{J}

Cycle totals:

wnet=1729+0+864+0=865 Jw_{net} = -1729 + 0 + 864 + 0 = -865\ \mathrm{J}

qnet=17291871864+1871=+865 Jq_{net} = 1729 - 1871 - 864 + 1871 = +865\ \mathrm{J}

The internal energy column sums to 01871+0+1871=00 - 1871 + 0 + 1871 = 0, as it must for a closed cycle, and qnet=wnetq_{net} = -w_{net}.

Heat is absorbed in steps (i) and (iv), a total of 1729+1871=3600 J1729 + 1871 = 3600\ \mathrm{J}, so the efficiency is

η=8653600=0.24\eta = \frac{865}{3600} = 0.24

Ans: wnet=865 Jw_{net} = -865\ \mathrm{J} (865 J done by the gas), qnet=+865 Jq_{net} = +865\ \mathrm{J}, η=24%\eta = 24\% Watch out: The denominator of the efficiency is the heat absorbed, 3600 J, not the net heat, 865 J. Using the net heat gives 100% efficiency for every cycle, which is impossible.

Question 10: Kirchhoff's equation for ammonia synthesis

For N2(g)+3H2(g)2NH3(g)\mathrm{N_2(g) + 3H_2(g) \rightarrow 2NH_3(g)}, ΔrH=92.4 kJmol1\Delta_r H^{\circ} = -92.4\ \mathrm{kJ\,mol^{-1}} at 298 K. The molar heat capacities at constant pressure are N2\mathrm{N_2} 29.1, H2\mathrm{H_2} 28.8 and NH3\mathrm{NH_3} 35.1, all in JK1mol1\mathrm{J\,K^{-1}\,mol^{-1}} and taken as constant. Find ΔrH\Delta_r H at 500 K.

Answer:

First I build ΔCp\Delta C_p as products minus reactants, each weighted by its coefficient.

ΔCp=2(35.1)[1(29.1)+3(28.8)]\Delta C_p = 2(35.1) - \left[1(29.1) + 3(28.8)\right]

=70.2[29.1+86.4]=70.2115.5=45.3 JK1mol1= 70.2 - \left[29.1 + 86.4\right] = 70.2 - 115.5 = -45.3\ \mathrm{J\,K^{-1}\,mol^{-1}}

The temperature interval is T2T1=500298=202 KT_2 - T_1 = 500 - 298 = 202\ \mathrm{K}.

ΔrH(500)=ΔrH(298)+ΔCp(T2T1)\Delta_r H(500) = \Delta_r H(298) + \Delta C_p(T_2 - T_1)

ΔCp(T2T1)=(45.3)(202)=9151 Jmol1=9.15 kJmol1\Delta C_p(T_2-T_1) = (-45.3)(202) = -9151\ \mathrm{J\,mol^{-1}} = -9.15\ \mathrm{kJ\,mol^{-1}}

ΔrH(500)=92.49.15=101.6 kJmol1\Delta_r H(500) = -92.4 - 9.15 = -101.6\ \mathrm{kJ\,mol^{-1}}

ΔCp\Delta C_p is negative, so the reaction becomes more exothermic as the temperature rises, which is the direction the sign predicted.

The matching internal energy change at 500 K follows from ΔrH=ΔrU+ΔngRT\Delta_r H = \Delta_r U + \Delta n_g RT. Counting gaseous moles, Δng=2(1+3)=2\Delta n_g = 2 - (1+3) = -2.

ΔngRT=(2)(8.314×103)(500)=8.31 kJmol1\Delta n_g RT = (-2)(8.314 \times 10^{-3})(500) = -8.31\ \mathrm{kJ\,mol^{-1}}

ΔrU(500)=ΔrH(500)ΔngRT=101.6(8.31)=93.3 kJmol1\Delta_r U(500) = \Delta_r H(500) - \Delta n_g RT = -101.6 - (-8.31) = -93.3\ \mathrm{kJ\,mol^{-1}}

Ans: ΔrH(500 K)=101.6 kJmol1\Delta_r H(500\ \mathrm{K}) = -101.6\ \mathrm{kJ\,mol^{-1}}, ΔrU(500 K)=93.3 kJmol1\Delta_r U(500\ \mathrm{K}) = -93.3\ \mathrm{kJ\,mol^{-1}} Watch out: The correction comes out in joules while the reaction enthalpy is in kilojoules. Adding 9151-9151 to 92.4-92.4 without converting gives nonsense. The answer also rests on ΔCp\Delta C_p being constant from 298 K to 500 K, which is only an approximation.

Question 11: Entropy change of an ideal gas, three ways

(a) 2.0 mol of an ideal monatomic gas goes from 300 K and 10.0 L to 400 K and 40.0 L. Find ΔS\Delta S. (b) Find ΔS\Delta S if the same gas goes from 300 K and 10.0 L to 300 K and 40.0 L. (c) 1.0 mol of N2\mathrm{N_2} and 1.0 mol of O2\mathrm{O_2}, both at the same temperature and pressure, are allowed to mix. Find ΔSmix\Delta S_{mix}, treating both as ideal.

Answer:

(a) Entropy is a state function, so I use the general ideal-gas expression with Cv,m=12.47 JK1mol1C_{v,m} = 12.47\ \mathrm{J\,K^{-1}\,mol^{-1}}.

ΔS=nCv,mlnT2T1+nRlnV2V1\Delta S = nC_{v,m}\ln\frac{T_2}{T_1} + nR\ln\frac{V_2}{V_1}

nCv,mln400300=2.0×12.47×ln1.333=24.94×0.288=7.18 JK1nC_{v,m}\ln\frac{400}{300} = 2.0 \times 12.47 \times \ln 1.333 = 24.94 \times 0.288 = 7.18\ \mathrm{J\,K^{-1}}

nRln40.010.0=2.0×8.314×ln4=16.63×1.386=23.05 JK1nR\ln\frac{40.0}{10.0} = 2.0 \times 8.314 \times \ln 4 = 16.63 \times 1.386 = 23.05\ \mathrm{J\,K^{-1}}

ΔS=7.18+23.05=+30.2 JK1\Delta S = 7.18 + 23.05 = +30.2\ \mathrm{J\,K^{-1}}

(b) The temperature term vanishes, leaving only the volume term, which is the number already computed.

ΔS=2.303nRlogV2V1=2.303×16.63×log4=38.29×0.602=+23.1 JK1\Delta S = 2.303\,nR\log\frac{V_2}{V_1} = 2.303 \times 16.63 \times \log 4 = 38.29 \times 0.602 = +23.1\ \mathrm{J\,K^{-1}}

(c) Each gas ends up with a mole fraction of 0.50.5.

ΔSmix=Rinilnxi=8.314[(1.0)ln0.5+(1.0)ln0.5]\Delta S_{mix} = -R\sum_i n_i\ln x_i = -8.314\left[(1.0)\ln 0.5 + (1.0)\ln 0.5\right]

=8.314×(1.386)=+11.5 JK1= -8.314 \times (-1.386) = +11.5\ \mathrm{J\,K^{-1}}

Ans: (a) +30.2 JK1+30.2\ \mathrm{J\,K^{-1}} (b) +23.1 JK1+23.1\ \mathrm{J\,K^{-1}} (c) +11.5 JK1+11.5\ \mathrm{J\,K^{-1}} Watch out: Part (a) never asked whether the path was reversible, and it did not need to. The formula was derived along a reversible path, but the answer depends only on the two end states.

Question 12: Direction of a reaction from ΔG\Delta G and QQ

For N2(g)+3H2(g)2NH3(g)\mathrm{N_2(g) + 3H_2(g) \rightleftharpoons 2NH_3(g)} at 298 K, ΔrG=33.2 kJmol1\Delta_r G^{\circ} = -33.2\ \mathrm{kJ\,mol^{-1}}. A vessel holds N2\mathrm{N_2} at 1.0 bar, H2\mathrm{H_2} at 3.0 bar and NH3\mathrm{NH_3} at 0.020 bar. Find ΔrG\Delta_r G and say which way the reaction runs.

Answer:

First the reaction quotient, with all pressures in bar so that QQ is a pure number.

Qp=pNH32pN2pH23=(0.020)2(1.0)(3.0)3=4.0×10427=1.48×105Q_p = \frac{p_{\mathrm{NH_3}}^{2}}{p_{\mathrm{N_2}}\,p_{\mathrm{H_2}}^{3}} = \frac{(0.020)^{2}}{(1.0)(3.0)^{3}} = \frac{4.0 \times 10^{-4}}{27} = 1.48 \times 10^{-5}

lnQ=2.303log(1.48×105)=2.303×(4.830)=11.12\ln Q = 2.303\log(1.48 \times 10^{-5}) = 2.303 \times (-4.830) = -11.12

RT=8.314×298=2478 Jmol1=2.478 kJmol1RT = 8.314 \times 298 = 2478\ \mathrm{J\,mol^{-1}} = 2.478\ \mathrm{kJ\,mol^{-1}}

ΔrG=ΔrG+RTlnQ=33.2+(2.478)(11.12)\Delta_r G = \Delta_r G^{\circ} + RT\ln Q = -33.2 + (2.478)(-11.12)

=33.227.6=60.8 kJmol1= -33.2 - 27.6 = -60.8\ \mathrm{kJ\,mol^{-1}}

ΔrG\Delta_r G is negative, so the mixture runs forward and makes more ammonia.

The same conclusion follows from comparing QQ with KK. From ΔrG=2.303RTlogK\Delta_r G^{\circ} = -2.303\,RT\log K,

logK=332002.303RT=332005705.8=5.818K=6.6×105\log K = \frac{33200}{2.303\,RT} = \frac{33200}{5705.8} = 5.818 \qquad K = 6.6 \times 10^{5}

Q=1.48×105Q = 1.48 \times 10^{-5} is far below KK, so the reaction must move forward, and ΔrG=RTln(Q/K)\Delta_r G = RT\ln(Q/K) is strongly negative.

Ans: ΔrG=60.8 kJmol1\Delta_r G = -60.8\ \mathrm{kJ\,mol^{-1}}; the reaction runs forward Watch out: ΔrG\Delta_r G^{\circ} and ΔrG\Delta_r G are different quantities. The standard value 33.2 kJmol1-33.2\ \mathrm{kJ\,mol^{-1}} belongs to the reaction with every gas at 1 bar; the actual driving force in this particular vessel is nearly twice as large because the ammonia is so dilute.