Welcome, future physicists! In this detailed session, we're going to dive deep into two fundamental concepts in the Kinetic Theory of Gases: the
Law of Equipartition of Energy and its profound implications for the
Specific Heats of Gases. These topics are not just theoretical constructs; they are essential for understanding how gases behave under different conditions and are frequently tested in JEE Mains & Advanced.
Let's begin our journey from the very basics.
### 1. The Concept of Degrees of Freedom (DOF)
Imagine a gas molecule moving around. How many independent ways can it store energy? This question leads us to the concept of
Degrees of Freedom (DOF).
A degree of freedom of a dynamical system is defined as the total number of independent ways in which the system can possess energy.
For a gas molecule, this energy can typically be stored in three forms:
1.
Translational Kinetic Energy: Energy due to the motion of the entire molecule's center of mass.
2.
Rotational Kinetic Energy: Energy due to the rotation of the molecule about its center of mass.
3.
Vibrational Energy: Energy due to the oscillation of atoms within the molecule relative to each other. This includes both kinetic and potential energy of vibration.
Let's break down the degrees of freedom for different types of molecules:
#### a. Translational Degrees of Freedom (f
t)
Any molecule, regardless of its shape or size, can move independently along the three perpendicular axes (x, y, z) in space. Each of these independent motions contributes a translational degree of freedom.
* Therefore,
every molecule has 3 translational degrees of freedom.
#### b. Rotational Degrees of Freedom (f
r)
Rotation occurs around the molecule's center of mass.
*
Monoatomic Gas (e.g., He, Ne, Ar): These are single atoms, essentially point masses. They have negligible moment of inertia about any axis passing through them. So, they have
0 rotational degrees of freedom. (Technically, they can rotate, but the energy associated with such rotation is typically quantized at very high levels and negligible for classical calculations).
*
Diatomic Gas (e.g., H₂, O₂, N₂, CO): These molecules consist of two atoms. We can imagine them as two masses connected by a rigid rod. They can rotate about two mutually perpendicular axes, both perpendicular to the axis connecting the two atoms. Rotation about the interatomic axis itself has negligible moment of inertia. So, they have
2 rotational degrees of freedom.
*
Non-linear Polyatomic Gas (e.g., H₂O, NH₃, CH₄): These molecules have three or more atoms arranged in a non-linear fashion. They can rotate about three mutually perpendicular axes. So, they have
3 rotational degrees of freedom.
*
Linear Polyatomic Gas (e.g., CO₂, C₂H₂): Similar to diatomic, but with more atoms in a line. They also have
2 rotational degrees of freedom.
#### c. Vibrational Degrees of Freedom (f
v)
Vibrational motion involves atoms within a molecule oscillating relative to each other. Each vibrational mode corresponds to two degrees of freedom: one for kinetic energy and one for potential energy associated with the oscillation.
*
Monoatomic Gas: No internal bonds, so
0 vibrational degrees of freedom.
*
Diatomic Gas: A single bond between two atoms can vibrate along the interatomic axis. This gives
1 vibrational mode, contributing 2 degrees of freedom (one for kinetic energy, one for potential energy). So, f
v = 2.
*
Polyatomic Gas: The number of vibrational modes is more complex. For N atoms, the total degrees of freedom is 3N.
* For a linear molecule, f
v = 3N - 5 (translational + rotational).
* For a non-linear molecule, f
v = 3N - 6 (translational + rotational).
So, a diatomic molecule (N=2) is linear, f
v = 3(2) - 5 = 1 mode, or 2 degrees of freedom.
JEE Advanced Note: Vibrational degrees of freedom are often 'inactive' at room temperature. This is because vibrational energy levels are quantized and spaced relatively far apart. It requires a significant amount of energy (higher temperatures) to excite these modes. Unless specified, for typical room temperature problems, we usually consider only translational and rotational DOFs.
Let's summarize the total degrees of freedom (f = f
t + f
r + f
v) for common gas types, assuming vibrational modes are inactive at room temperature:
| Gas Type | Translational (f
t) | Rotational (f
r) | Vibrational (f
v, room temp) | Total DOF (f) |
| :------------------- | :--------------------------: | :-----------------------: | :-------------------------------------: | :------------: |
|
Monoatomic (He, Ne) | 3 | 0 | 0 |
3 |
|
Diatomic (O₂, N₂) | 3 | 2 | 0 |
5 |
|
Non-linear Polyatomic (H₂O, CH₄) | 3 | 3 | 0 |
6 |
|
Linear Polyatomic (CO₂, C₂H₂) | 3 | 2 | 0 |
5 |
Important: If vibrational modes are active (usually specified for higher temperatures), each vibrational mode contributes 2 degrees of freedom. For example, a diatomic gas with one active vibrational mode would have f = 3 (translational) + 2 (rotational) + 2 (vibrational) = 7.
### 2. The Law of Equipartition of Energy
This is a cornerstone principle in kinetic theory, connecting the microscopic world of molecular motion to macroscopic properties like temperature.
The Law of Equipartition of Energy states that for a system in thermal equilibrium, the total energy is equally distributed among all its degrees of freedom, and the average energy associated with each degree of freedom per molecule is ½ kBT.
Here:
*
kB is the Boltzmann constant (k
B = 1.38 × 10⁻²³ J/K).
*
T is the absolute temperature of the gas in Kelvin.
What does this mean?
Imagine you have a certain amount of energy in your gas system. This law tells you that this energy doesn't just concentrate in one type of motion (say, only translational). Instead, it's fairly distributed. If a molecule has 3 translational degrees of freedom, each of these (motion along x, y, or z) will, on average, have an energy of ½ k
BT. If it also has 2 rotational degrees of freedom, those two will also each have ½ k
BT of energy, and so on.
Derivation Intuition (Statistical Mechanics Perspective):
While a full derivation requires advanced statistical mechanics, the essence comes from the fact that at thermal equilibrium, the system explores all possible microstates with equal probability. Any quadratic term in the energy expression of a molecule (like ½mv² for kinetic energy, or ½Iω² for rotational energy, or ½kx² for potential energy in vibration) is found to contribute ½ k
BT to the average energy. All translational and rotational energy terms are quadratic. Vibrational energy has both kinetic (½mv²) and potential (½kx²) components, hence it contributes two quadratic terms (i.e., 2 * ½ k
BT = k
BT) per vibrational mode.
### 3. Internal Energy of an Ideal Gas (U)
The internal energy of an ideal gas is the sum of the kinetic and potential energies of its constituent molecules. For an ideal gas, we assume no intermolecular forces, so the potential energy due to interaction between molecules is zero. Thus, the internal energy is purely the sum of the kinetic energies (translational, rotational, vibrational) of its molecules.
Using the law of equipartition of energy:
* The average energy per molecule = f * (½ k
BT), where 'f' is the total number of active degrees of freedom.
* For
1 mole of gas, the total number of molecules is Avogadro's number (N
A).
* So, the
internal energy of 1 mole of gas (U) = N
A * f * (½ k
BT)
Since R = N
A * k
B (Universal Gas Constant), we can write:
U = ½ f R T
Let's calculate the internal energy per mole for different types of gases at room temperature (assuming vibrational modes are inactive):
1.
Monoatomic Gas (f = 3):
U = ½ * 3 * R * T =
(3/2) R T
2.
Diatomic Gas (f = 5):
U = ½ * 5 * R * T =
(5/2) R T
3.
Non-linear Polyatomic Gas (f = 6):
U = ½ * 6 * R * T =
3 R T
This formula for internal energy is crucial for solving problems involving the First Law of Thermodynamics and specific heats.
### 4. Specific Heats of Gases (C
v and C
p)
The specific heat of a gas tells us how much heat energy is required to raise the temperature of a unit mass (or 1 mole) of the gas by 1 degree Celsius (or Kelvin). We define two principal specific heats:
*
Molar Specific Heat at Constant Volume (Cv): The amount of heat required to raise the temperature of 1 mole of gas by 1 K when its volume is kept constant.
*
Molar Specific Heat at Constant Pressure (Cp): The amount of heat required to raise the temperature of 1 mole of gas by 1 K when its pressure is kept constant.
#### a. Molar Specific Heat at Constant Volume (C
v)
From the First Law of Thermodynamics (ΔQ = ΔU + ΔW), if the volume is constant, ΔW = PΔV = 0.
So, ΔQ
v = ΔU.
For 1 mole of gas, C
v = (dQ/dT)
v = (dU/dT)
v.
Since U = ½ f R T (for 1 mole), we can differentiate U with respect to T:
Cv = d(½ f R T)/dT = ½ f R
Let's calculate C
v for different types of gases at room temperature:
1.
Monoatomic Gas (f = 3):
C
v = ½ * 3 * R =
(3/2) R
2.
Diatomic Gas (f = 5):
C
v = ½ * 5 * R =
(5/2) R
3.
Non-linear Polyatomic Gas (f = 6):
C
v = ½ * 6 * R =
3 R
#### b. Molar Specific Heat at Constant Pressure (C
p)
We use
Mayer's Relation, which links C
p and C
v for an ideal gas:
Cp - Cv = R
Therefore,
Cp = Cv + R
Let's calculate C
p for different types of gases at room temperature:
1.
Monoatomic Gas (Cv = 3/2 R):
C
p = (3/2)R + R =
(5/2) R
2.
Diatomic Gas (Cv = 5/2 R):
C
p = (5/2)R + R =
(7/2) R
3.
Non-linear Polyatomic Gas (Cv = 3 R):
C
p = 3R + R =
4 R
#### c. Ratio of Specific Heats (γ)
The ratio of specific heats,
γ (gamma), is an important parameter in thermodynamics, particularly for adiabatic processes.
γ = Cp / Cv
Let's calculate γ for different types of gases at room temperature:
1.
Monoatomic Gas (Cp = 5/2 R, Cv = 3/2 R):
γ = (5/2 R) / (3/2 R) =
5/3 ≈ 1.67
2.
Diatomic Gas (Cp = 7/2 R, Cv = 5/2 R):
γ = (7/2 R) / (5/2 R) =
7/5 = 1.4
3.
Non-linear Polyatomic Gas (Cp = 4 R, Cv = 3 R):
γ = (4 R) / (3 R) =
4/3 ≈ 1.33
In general, for any ideal gas with 'f' degrees of freedom:
* C
v = fR/2
* C
p = (f/2 + 1)R
*
γ = (f/2 + 1)R / (fR/2) = (f+2)/f = 1 + 2/f
### 5. Temperature Dependence of Specific Heats (JEE Advanced Perspective)
This is a critical concept for advanced problems. The assumption that vibrational degrees of freedom are 'inactive' is valid only at moderate (room) temperatures.
Advanced Insight: The equipartition theorem is a classical result. However, molecular energy levels (especially vibrational and rotational) are quantized. At low temperatures, only the translational modes are active because the energy spacing between rotational and vibrational levels is too large to be excited by the average thermal energy (kBT).
Let's consider the specific heat of
Hydrogen (H₂) gas as a classic example:
*
Very Low Temperatures (T < ~70 K): Only translational modes are active.
* f = 3
* C
v = (3/2)R
*
Moderate Temperatures (~70 K to ~2000 K): Translational and rotational modes are active. Vibrational modes are still 'frozen out'.
* f = 3 (translational) + 2 (rotational) = 5
* C
v = (5/2)R
*
High Temperatures (T > ~2000 K): Translational, rotational, and vibrational modes are all active. For a diatomic molecule like H₂, there's 1 vibrational mode, contributing 2 degrees of freedom.
* f = 3 (translational) + 2 (rotational) + 2 (vibrational) = 7
* C
v = (7/2)R
This stepwise increase in C
v with temperature is direct experimental evidence for the existence of degrees of freedom and the quantization of energy levels.
This variation of specific heat with temperature is a classic JEE Advanced question. Always be mindful of the temperature range provided in the problem statement. If not specified, assume room temperature conditions where vibrational modes are inactive.
### Example Calculation:
Let's compare Molar Internal Energy, C
v, C
p, and γ for Argon (monoatomic) and Oxygen (diatomic) at room temperature.
1. Argon (Ar) - Monoatomic Gas:
* Degrees of Freedom (f): 3 (3 translational, 0 rotational, 0 vibrational)
* Molar Internal Energy (U): U = (f/2)RT = (3/2)RT
* Molar Specific Heat at Constant Volume (C
v): C
v = (f/2)R = (3/2)R
* Molar Specific Heat at Constant Pressure (C
p): C
p = C
v + R = (3/2)R + R = (5/2)R
* Ratio of Specific Heats (γ): γ = C
p/C
v = (5/2 R) / (3/2 R) = 5/3 ≈ 1.67
2. Oxygen (O₂) - Diatomic Gas:
* Degrees of Freedom (f): 5 (3 translational, 2 rotational, 0 vibrational at room temp)
* Molar Internal Energy (U): U = (f/2)RT = (5/2)RT
* Molar Specific Heat at Constant Volume (C
v): C
v = (f/2)R = (5/2)R
* Molar Specific Heat at Constant Pressure (C
p): C
p = C
v + R = (5/2)R + R = (7/2)R
* Ratio of Specific Heats (γ): γ = C
p/C
v = (7/2 R) / (5/2 R) = 7/5 = 1.4
### Summary Table for Quick Reference
| Property | General (f DOF) | Monoatomic (f=3) | Diatomic (f=5) | Non-linear Polyatomic (f=6) |
| :----------------------- | :--------------: | :--------------: | :------------: | :--------------------------: |
|
Internal Energy (U) | ½ f RT | (3/2)RT | (5/2)RT | 3RT |
|
Cv | ½ f R | (3/2)R | (5/2)R | 3R |
|
Cp | (½ f + 1)R | (5/2)R | (7/2)R | 4R |
|
γ = Cp/Cv | (f+2)/f | 5/3 | 7/5 | 4/3 |
*(Note: Values for diatomic and polyatomic gases are for room temperature, assuming vibrational modes are inactive.)*
### CBSE vs. JEE Focus
*
CBSE/Boards: Primarily focuses on understanding the definitions of degrees of freedom, the statement of the Law of Equipartition, and calculating U, C
v, C
p, and γ for monoatomic and diatomic gases at room temperature. The concept of vibrational degrees of freedom being inactive is usually given or implicitly assumed.
*
JEE Mains & Advanced: Requires a much deeper understanding.
* Ability to determine DOF for various complex polyatomic molecules.
* Crucially, understanding the
temperature dependence of specific heats and when vibrational modes become active.
* Application of these concepts in complex thermodynamic cycles (adiabatic, isothermal, isobaric, isochoric processes).
* Questions might involve a mixture of gases or phase changes where these concepts are applied.
By mastering the concepts of degrees of freedom and the Law of Equipartition of Energy, you gain powerful tools to analyze and predict the thermal behavior of ideal gases, a skill indispensable for success in physics. Keep practicing with diverse problems to solidify your understanding!