Specific heat capacity of diatomic gases

Breathe in. Roughly four out of every five molecules that just entered your lungs are nitrogen, N2\text{N}_2, and almost all the rest is oxygen, O2\text{O}_2 — both diatomic molecules, two atoms joined by a bond, tumbling and rushing through the air at hundreds of metres per second. A monatomic gas like helium is a bare point mass: hit it, and all the energy you give it goes into making it move faster in a straight line. A diatomic molecule is a tiny dumbbell. Hit it off-centre — which is almost always — and some of your push makes it move, but some makes it spin. That extra way of storing energy is not a footnote; it is the entire reason nitrogen and oxygen heat up differently from helium and argon, and why the ratio γ=Cp/Cv\gamma = C_p/C_v that governs everything from the pitch of a flute to the compression stroke of an engine takes a different, measurable value for the air we actually breathe. This article picks up exactly where the monatomic derivation left off. We reuse the same tool — the law of equipartition of energy, "a half of kBTk_BT per independent quadratic term" — but now count degrees of freedom for a rigid dumbbell instead of a point mass. The bookkeeping changes by exactly two rotational terms, and that single change cascades through UU, CvC_v, CpC_p and γ\gamma, turning 5/3≈1.675/3 \approx 1.67 into 7/5=1.47/5 = 1.4. We will derive that result carefully from first principles, work two CBSE-style numericals (heating nitrogen gas at constant pressure, and adiabatically compressing a diatomic gas), flag the exact places students lose marks — miscounting the rotational axes, or reaching for the monatomic γ\gamma out of habit — and finish with a look at why vibration, quietly excluded from the ordinary syllabus numbers, would change the picture yet again at very high temperature.

Key takeaways
  • A diatomic molecule (e.g. N2\text{N}_2, O2\text{O}_2, H2\text{H}_2) is modelled as a rigid rotor: two point masses joined by a rigid bond, free to translate in 3 directions and rotate about 2 independent axes.
  • Rotation about the bond axis itself does not count — the moment of inertia there is negligible, so that third rotational term is dropped.
  • This gives f=5f = 5 degrees of freedom, so by equipartition the internal energy of one mole is U=52RTU = \tfrac52RT.
  • Differentiating gives Cv=52R≈20.79 J/mol ⋅ KC_v = \tfrac52R \approx 20.79\ \text{J/mol}\,\cdot\,\text{K}, and Mayer's relation gives Cp=Cv+R=72R≈29.10 J/mol ⋅ KC_p = C_v + R = \tfrac72R \approx 29.10\ \text{J/mol}\,\cdot\,\text{K}.
  • The ratio of specific heats is γ=Cp/Cv=7/5=1.4\gamma = C_p/C_v = 7/5 = 1.4 — smaller than the monatomic value 5/3≈1.675/3 \approx 1.67, because more of any absorbed heat now goes into rotation rather than being available to do external work.
  • At very high temperature the vibrational mode switches on, adding 2 more to ff (making f=7f=7) and pulling γ\gamma down further toward 9/7≈1.299/7 \approx 1.29 — CBSE expects this only as a qualitative idea, not a numeric substitution unless a question says so explicitly.
  • Key idea: a rigid diatomic molecule has 5 degrees of freedom (3 translational, 2 rotational), so equipartition gives Cv=52RC_v = \tfrac52R, Cp=72RC_p = \tfrac72R, and γ=7/5=1.4\gamma = 7/5 = 1.4 — smaller than a monatomic gas because rotation soaks up part of every joule of heat.
The core insight

Counting 3 translational plus 2 rotational degrees of freedom for a rigid diatomic molecule (f=5f=5, rotation about the bond axis excluded) and applying the law of equipartition gives U=52RTU=\tfrac52RT, Cv=52RC_v=\tfrac52R, Cp=72RC_p=\tfrac72R, and γ=7/5=1.4\gamma = 7/5 = 1.4.

Where it fits in the syllabus

This section sits directly inside the CBSE Class 11 Kinetic Theory chapter, right after degrees of freedom and the (statement-only) law of equipartition of energy, and right after the monatomic specific-heat result. The prescribed board scope asks you to apply the same equipartition reasoning to a diatomic molecule modelled as a rigid rotor, and to know — qualitatively only — that vibration can raise ff at high temperature; the syllabus does not ask for a derivation of equipartition itself, nor for the Maxwell–Boltzmann speed distribution, nor for a numeric vibrational correction unless a question states one. Everything below stays inside those limits.

The physical picture

Picture a diatomic molecule as two small spheres (the atoms) joined by a stiff, weightless rod (the bond) — a rigid dumbbell, free to move as a whole. Set up axes through its centre of mass: one along the bond, and two perpendicular to it. The molecule can translate along any of the three ordinary spatial directions, contributing the same 3 translational degrees of freedom every gas has, monatomic or not. But unlike a point particle, this dumbbell can also tumble: it can rotate about either of the two axes perpendicular to the bond, and each such rotation carries its own kinetic energy, 12Iω2\tfrac12 I\omega^2, which is a quadratic term just like 12mv2\tfrac12 mv^2 and so earns its own 12kBT\tfrac12 k_BT under equipartition. What about rotation about the bond axis itself — spinning the dumbbell like a drill bit along its own length? Classically that motion exists, but the two atoms are treated as point masses sitting essentially on that axis, so the moment of inertia about it is vanishingly small compared with the other two axes. A negligible moment of inertia means a negligible contribution to kinetic energy for any ordinary angular speed, so this third rotational term is dropped from the count. That is the one deliberate exclusion that separates a diatomic molecule's f=5f=5 from what a naive "three axes, three rotations" guess would give.

ftranslation=3,frotation=2,ftotal=5f_{\text{translation}} = 3, \qquad f_{\text{rotation}} = 2, \qquad f_{\text{total}} = 5

where: ftranslationf_{\text{translation}} counts motion of the centre of mass along the three ordinary directions of space, frotationf_{\text{rotation}} counts tumbling about the two axes perpendicular to the bond (rotation about the bond itself excluded), and ftotalf_{\text{total}} is the degrees of freedom used in the equipartition sum below. Physically: every one of these five is an independent way the molecule can store kinetic energy, and the law of equipartition treats each one exactly alike, handing it 12kBT\tfrac12 k_BT of average energy regardless of what kind of motion it represents.

Figure
A rigid dumbbell diatomic molecule with two atoms joined by a bond, showing three translation arrows along the x y and z directions and two rotation arrows about axes perpendicular to the bond, with a faded no-entry mark on the third axis along the bond itself
Degrees of freedom of a rigid diatomic molecule: f = 5 A B translation (3) x y z rotation axis 1 (perp. to bond) rotation axis 2 (perp. to bond) bond axis: excluded negligible moment of inertia 3 translational + 2 rotational = 5 quadratic energy terms per molecule

The core idea, derived

Derivation ASpecific heats of a diatomic gas from equipartition

We want to show, starting from the count f=5f=5 and the law of equipartition of energy (each independent quadratic energy term averaging 12kBT\tfrac12 k_BT per molecule), that one mole of a diatomic ideal gas has internal energy U=52RTU = \tfrac52RT, and that this forces Cv=52RC_v = \tfrac52R, Cp=72RC_p = \tfrac72R, and γ=Cp/Cv=7/5=1.4\gamma = C_p/C_v = 7/5 = 1.4 — the central numerical result the CBSE syllabus expects for nitrogen, oxygen, hydrogen and similar gases near room temperature, treated throughout as rigid rotors with no vibration active.

Step 1. Total energy per molecule. Each of the f=5f=5 degrees of freedom identified above — 3 translational, 2 rotational — contributes an average kinetic energy of 12kBT\tfrac12 k_BT under the law of equipartition, since each is an independent quadratic term in the molecule's total energy. Summing all five, the average total energy of one diatomic molecule is εˉ=5×12kBT=52kBT\bar\varepsilon = 5 \times \tfrac12 k_BT = \tfrac52 k_BT.

Step 2. Scale up to one mole. A mole contains NAN_A molecules, so the total internal energy of one mole of diatomic gas is U=NAεˉ=NA(52kBT)=52(NAkB)TU = N_A\bar\varepsilon = N_A\left(\tfrac52 k_BT\right) = \tfrac52\left(N_Ak_B\right)T. Since NAkB=RN_Ak_B = R, the universal gas constant, this simplifies to U=52RTU = \tfrac52RT — the internal energy grows linearly with absolute temperature, exactly as the equipartition idea promises, with the coefficient fixed entirely by the degrees-of-freedom count f=5f=5.

Step 3. Differentiate to get CvC_v. Molar specific heat at constant volume is defined as the rate of change of internal energy with temperature, Cv=dUdTC_v = \dfrac{dU}{dT}, because at constant volume no work is done and every joule supplied goes into raising UU. Differentiating U=52RTU=\tfrac52RT with respect to TT gives Cv=52RC_v = \tfrac52R. Substituting R=8.314 J/mol ⋅ KR = 8.314\ \text{J/mol}\,\cdot\,\text{K} gives the numerical value Cv=2.5×8.314=20.79 J/mol ⋅ KC_v = 2.5\times 8.314 = 20.79\ \text{J/mol}\,\cdot\,\text{K}.

Step 4. Apply Mayer's relation for CpC_p. For an ideal gas, heating at constant pressure must supply both the same rise in internal energy and the extra work P dVP\,dV done as the gas expands, which for one mole works out to the fixed relation Cp=Cv+RC_p = C_v + R. Substituting the Step 3 result, Cp=52R+R=72RC_p = \tfrac52R + R = \tfrac72R, numerically Cp=3.5×8.314=29.10 J/mol ⋅ KC_p = 3.5\times8.314 = 29.10\ \text{J/mol}\,\cdot\,\text{K}.

Step 5. Form the ratio γ\gamma. Dividing, γ=CpCv=7/2 R5/2 R=75=1.4\gamma = \dfrac{C_p}{C_v} = \dfrac{7/2\,R}{5/2\,R} = \dfrac{7}{5} = 1.4. Notice the RR and the factor of 22 both cancel, leaving γ\gamma as a pure number fixed only by the degrees-of-freedom count ff, through the general pattern γ=1+2/f\gamma = 1 + 2/f. Checking: with f=5f=5, γ=1+2/5=7/5\gamma = 1 + 2/5 = 7/5, matching. This is smaller than the monatomic value 1+2/3=5/3≈1.671+2/3 = 5/3 \approx 1.67, because the extra rotational degrees of freedom in a diatomic molecule soak up part of any heat supplied, leaving relatively less available to expand the gas and do external work at constant pressure — which is precisely what a smaller γ\gamma means.

Worked examples

Board level - heating nitrogen gas at constant pressure

Find the heat required to raise the temperature of 3 mol of nitrogen gas (diatomic, treated as a rigid rotor) from 280 K to 320 K at constant pressure.

Step 1. Identify the process and the right specific heat. Heating at constant pressure means the heat supplied equals ΔQ=nCpΔT\Delta Q = nC_p\Delta T, using CpC_p rather than CvC_v because the gas is also doing work as it expands against constant pressure, and that extra work must be paid for out of the same heat input.

Step 2. Use the diatomic value derived above, Cp=72R=29.10 J/mol ⋅ KC_p = \tfrac72R = 29.10\ \text{J/mol}\,\cdot\,\text{K}, since nitrogen is diatomic and well described as a rigid rotor at these ordinary temperatures (no vibration active).

Step 3. Substitute the numbers: n=3 moln=3\ \text{mol}, ΔT=320−280=40 K\Delta T = 320-280 = 40\ \text{K}.

ΔQ=3×29.10×40=3492 J\Delta Q = 3 \times 29.10 \times 40 = 3492\ \text{J}

The heat required is 3492 J, or about 3.49 kJ, for this constant-pressure heating of nitrogen.

Competitive level - adiabatic compression of a diatomic gas

An ideal diatomic gas (rigid rotor, γ=7/5\gamma = 7/5) occupies volume VV at pressure PP. It undergoes an adiabatic process in which its volume is halved. Find the ratio of the final pressure to the initial pressure, and compare with what an isothermal compression to the same volume would give.

Step 1. Write the adiabatic condition. For a quasi-static adiabatic process on an ideal gas, PVγ=constantPV^\gamma = \text{constant}, so between the initial and final states, P1V1γ=P2V2γP_1V_1^\gamma = P_2V_2^\gamma, which rearranges to P2P1=(V1V2)γ\dfrac{P_2}{P_1} = \left(\dfrac{V_1}{V_2}\right)^\gamma.

Step 2. Substitute the given compression. Halving the volume means V2=V1/2V_2 = V_1/2, so V1/V2=2V_1/V_2 = 2, giving P2P1=2γ=27/5\dfrac{P_2}{P_1} = 2^{\gamma} = 2^{7/5}.

Step 3. Evaluate 27/52^{7/5} using logarithms. Since log⁡102=0.301\log_{10}2 = 0.301, 1.4×0.301=0.42141.4 \times 0.301 = 0.4214, so 21.4=100.4214≈2.642^{1.4} = 10^{0.4214} \approx 2.64.

Step 4. Compare with isothermal compression to the same final volume. For an isothermal process, P1V1=P2V2P_1V_1 = P_2V_2 (γ\gamma effectively replaced by 1), so halving the volume would only double the pressure, P2/P1=2P_2/P_1 = 2. The adiabatic case gives a final pressure about 2.64 times the initial pressure — noticeably more than the isothermal factor of 2, because in the adiabatic process no heat escapes, so the compression work itself raises the temperature and pushes the pressure up further than an isothermal squeeze would. Timing note: in an exam, don't re-derive PVγ=constantPV^\gamma=\text{constant} from scratch — quote it directly, plug in the given volume ratio, and evaluate the power using logarithms (or recognise standard values like 21.4≈2.642^{1.4}\approx 2.64 from practice) in well under two minutes; this whole problem should take about 90 seconds once γ=7/5\gamma=7/5 is recalled.

Common traps

  • Miscounting rotational axes. Students often assume a diatomic molecule has 3 rotational degrees of freedom, one about each axis, forgetting that rotation about the bond axis has negligible moment of inertia and is excluded — the correct count is f=5f=5, not f=6f=6.
  • Reusing the monatomic γ\gamma. Writing γ=5/3\gamma = 5/3 out of habit for any ideal gas, instead of switching to the diatomic value γ=7/5=1.4\gamma = 7/5 = 1.4 once the problem says nitrogen, oxygen, hydrogen, or any other diatomic gas.
  • Applying f=5f=5 at temperatures where vibration matters. The rigid-rotor result γ=7/5\gamma = 7/5 assumes vibration is frozen out, which is true near room temperature for most diatomic gases but not at very high temperature; CBSE expects only a qualitative awareness of this, never a numeric switch mid-problem unless the question explicitly asks for it.
  • Confusing the isothermal and adiabatic gas laws. Using PV=constantPV = \text{constant} (isothermal) when the process described is adiabatic, or vice versa — the exponent γ\gamma appears only in the adiabatic relation, and it is exactly the diatomic γ=7/5\gamma=7/5 that must be used there.
  • Forgetting Mayer's relation links CpC_p and CvC_v. Some students try to derive CpC_p from equipartition directly instead of using Cp=Cv+RC_p = C_v + R, which is both faster and less error-prone once CvC_v is known.

You should be able to…

  • Count the degrees of freedom of a rigid diatomic molecule (f=5f=5) and explain clearly why rotation about the bond axis is excluded.
  • Derive Cv=52RC_v = \tfrac52R, Cp=72RC_p = \tfrac72R, and γ=7/5\gamma = 7/5 for a diatomic gas starting from the law of equipartition of energy.
  • State, without deriving, how vibrational modes at high temperature would raise ff and lower γ\gamma further.
  • Apply ΔQ=nCvΔT\Delta Q = nC_v\Delta T or ΔQ=nCpΔT\Delta Q = nC_p\Delta T correctly, choosing the right specific heat for the process described.
  • Apply PVγ=constantPV^\gamma = \text{constant} for an adiabatic process on a diatomic gas, and distinguish it from the isothermal relation PV=constantPV=\text{constant}.
  • Compare the diatomic result against the monatomic case and explain, in words, why more degrees of freedom means a smaller γ\gamma.

Ask the tutor: Want a walkthrough of why the bond-axis moment of inertia is treated as zero, or more practice problems mixing constant-volume, constant-pressure, and adiabatic diatomic-gas calculations? Ask the AI tutor.

Why doesn't rotation about the bond axis count as a degree of freedom?

Classically, a diatomic molecule can spin about any axis, including the line joining its two atoms. But in the rigid-rotor model the atoms are treated as point masses sitting essentially on that axis, so the moment of inertia about it is almost zero — and rotational kinetic energy is 12Iω2\tfrac12 I\omega^2, so a near-zero II means near-zero energy for any physically reasonable spin rate. Since that term contributes nothing measurable, it is dropped from the equipartition count, leaving only the 2 rotations about axes perpendicular to the bond.

Why is gamma smaller for diatomic gases than for monatomic gases?

Gamma is the ratio Cp/CvC_p/C_v, and it measures how much of the heat supplied at constant pressure goes into expansion work versus how much goes into raising internal energy. A diatomic molecule has more ways to store energy (rotation, on top of translation), so a bigger share of any heat you add goes into internal energy rather than being "extra" and available to push the piston outward. More degrees of freedom means relatively less heat left over for work, which is exactly what a smaller gamma reflects: monatomic gases have gamma 5/3, diatomic gases 7/5, and polyatomic gases smaller still.

If vibration exists, why does the syllabus ignore it for diatomic gases at room temperature?

Vibration is a real motion — the bond stretching and compressing like a tiny spring — and it does contribute 2 more degrees of freedom (kinetic plus potential energy of vibration) when it is thermally active. But exciting a vibrational mode needs a certain minimum amount of thermal energy, and for most diatomic gases at ordinary room temperature that threshold isn't reached, so the mode stays effectively frozen and doesn't participate. Only at much higher temperatures does it switch on, which is why CBSE keeps the numeric answer at f=5, gamma=7/5 for standard problems and treats vibration as a qualitative, not computational, extension.

How is this different from the monatomic gas case I studied just before this?

The method is identical — count degrees of freedom, apply equipartition to get U, differentiate for Cv, use Mayer's relation for Cp, divide for gamma — only the number f changes. Monatomic gases like helium or argon have no meaningful rotational energy (a bare atom's moment of inertia about any axis through its centre is essentially zero), so f=3 and gamma=5/3. Diatomic gases add 2 rotational terms, giving f=5 and gamma=7/5. The next article on polyatomic gases extends the same logic once more, adding a further rotational term for nonlinear molecules.

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Where this leads