Deriving Cp - Cv = R for an Ideal Gas (Mayer's Relation)

Chemistry · Thermodynamics · NEET

For one mole of an ideal gas, Cp - Cv = R. This is called Mayer's relation. It works because at constant pressure the gas must also do extra work by pushing back the surroundings, so it needs R joules more heat per degree than at constant volume. Memory hook: "P needs more Push, so Cp is bigger by exactly R."
Cp − Cv = R : the same heating, two waysConstant Volume (Cv)heat → ΔU onlyqV = Cv ΔT = ΔUConstant Pressure (Cp)heat → ΔU + workgas expands (push)qp = Cp ΔT = ΔH+ R ΔTExtra work = R ΔT ⇒ Cp = Cv + R ⇒ Cp − Cv = R
Heating one mole of ideal gas by ΔT: at constant volume the heat only raises U, but at constant pressure the gas also does R ΔT of push-work, so Cp exceeds Cv by exactly R.

Your doubts, answered

Why is Cp always greater than Cv?

At constant volume (Cv), all the heat you add goes only to raising the temperature (increasing internal energy U). At constant pressure (Cp), the gas expands, so part of the heat also does work pushing the surroundings back. So you must supply extra heat to get the same temperature rise. That extra amount is exactly R per mole. This is why Cp is always bigger than Cv.

Where does the R come from in Cp - Cv = R?

Start from H = U + pV. For one mole of an ideal gas, pV = RT. So H = U + RT. When temperature changes by ΔT, ΔH = ΔU + R ΔT. Now use qV = Cv ΔT = ΔU and qp = Cp ΔT = ΔH. Putting these in: Cp ΔT = Cv ΔT + R ΔT. Cancel ΔT and you get Cp - Cv = R. The R is simply the gas constant that appears because pV = RT.

Is Cp - Cv = R true for any amount of gas?

The clean form Cp - Cv = R is for ONE mole (molar heat capacities). For n moles, the total heat capacities give Cp - Cv = nR, because pV = nRT. In NEET, if it says 'molar' or 'one mole', use R. If it gives n moles of total heat capacity, use nR. Always check the wording.

Does Cp - Cv = R work for real gases and liquids too?

No. This exact result is only for an IDEAL gas, because we used pV = RT. For real gases the difference is not exactly R. For solids and liquids, volume barely changes on heating, so Cp and Cv are almost equal (their difference is very small). NEET questions on this relation always assume an ideal gas.

What is the difference between qV and qp used in the proof?

qV is the heat at constant volume; here no work is done, so all heat becomes ΔU. So qV = Cv ΔT = ΔU. qp is the heat at constant pressure; here the gas expands and the heat becomes ΔH. So qp = Cp ΔT = ΔH. The whole derivation just plugs these two facts into ΔH = ΔU + R ΔT.

⚠️ The NEET trap
Cv - Cp = R, or writing Cp - Cv = R for n moles without the n.
For one mole: Cp - Cv = R (Cp is the larger one). For n moles: Cp - Cv = nR.
🧠 Cp is bigger because constant pressure needs extra push-work, so the bigger minus the smaller = +R. If you get a negative, you flipped the order.

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Frequently asked

State Mayer's relation for an ideal gas.

Mayer's relation says that for one mole of an ideal gas, the molar heat capacity at constant pressure minus the molar heat capacity at constant volume equals the gas constant: Cp - Cv = R.

What is the value of R used in Cp - Cv = R?

R is the universal gas constant, equal to 8.314 J K⁻¹ mol⁻¹ (or about 2 cal K⁻¹ mol⁻¹). So for an ideal gas, Cp is about 8.314 J K⁻¹ mol⁻¹ larger than Cv.

Why do we take one mole in this derivation?

We take one mole so that pV = RT (instead of pV = nRT). This makes Δ(pV) = R ΔT, which directly gives the clean result Cp - Cv = R. For n moles the same steps give Cp - Cv = nR.

Does Cp - Cv = R help find the ratio γ (gamma)?

Yes. The ratio γ = Cp/Cv is used in adiabatic processes. Since Cp = Cv + R, once you know Cv (for example (3/2)R for a monatomic gas), you can find Cp and then γ. This links the relation to adiabatic NEET problems.

Is Cp - Cv = R part of the NEET syllabus?

Yes. It is from Class 11 Chemistry Thermodynamics (and also appears in Physics kinetic theory). NEET can ask the derivation, the meaning of R here, or use it inside numerical problems on heat capacity and adiabatic processes.