Start Learning Free

Before You Begin

Question #43486

Difficulty: 8/10 | 🟢 Free

The Question

Consider a crystalline solid where the interatomic potential energy U(r)U(r) between two adjacent atoms separated by a distance rr is modeled as: U(r)=U0+12c(r−r0)2−g(r−r0)3U(r) = U_0 + \frac{1}{2}c(r-r_0)^2 - g(r-r_0)^3 where r0r_0 is the equilibrium separation at absolute zero temperature. The constants cc (in J⋅m−2\text{J}\cdot\text{m}^{-2}) and gg (in J⋅m−3\text{J}\cdot\text{m}^{-3}) are positive. The term −g(r−r0)3-g(r-r_0)^3 represents the anharmonicity of the potential. Assume the anharmonic term is small compared to the thermal energy kTkT, where kk is the Boltzmann constant (in J⋅K−1\text{J}\cdot\text{K}^{-1}) and TT is the absolute temperature (in K\text{K}). Using classical statistical mechanics, determine the coefficient of linear thermal expansion α\alpha of the solid. (Hint: The average displacement ⟨x⟩=⟨r−r0⟩\langle x \rangle = \langle r - r_0 \rangle can be evaluated using the Boltzmann factor e−U(x)/kTe^{-U(x)/kT} and the approximation egx3/kT≈1+gx3kTe^{gx^3/kT} \approx 1 + \frac{gx^3}{kT}. Standard integral: ∫−∞∞x4e−ax2dx=34a2πa\int_{-\infty}^{\infty} x^4 e^{-ax^2} dx = \frac{3}{4a^2}\sqrt{\frac{\pi}{a}})

Options

  • A.

    3gkr0c2\frac{3gk}{r_0 c^2}

  • B.

    gkr0c2\frac{gk}{r_0 c^2}

  • C.

    3gk2r0c2\frac{3gk}{2 r_0 c^2}

  • D.

    0

Check Your Answer

Correct Answer

Step-by-Step Solution

Explanation

How the Examiner Thinks

Variable_Constraint

Develop pure symbolic logic skills by mastering algebraic constraints without relying on numerical data.

Concepts Behind This Question

Graphical Concavity Significance|Interatomic Force Curve|Thermal Expansion of Area and Volume

Why This Question Is Tricky

Common Mistakes

This question tests the fundamental microscopic origin of macroscopic thermal expansion.

A common misconception among students is that thermal expansion arises simply because atoms have more kinetic energy and vibrate with larger amplitudes.

However, if the interatomic potential were purely parabolic (a simple harmonic oscillator), the average position ⟨r⟩\langle r \rangle would remain exactly at r0r_0 regardless of temperature, yielding zero thermal expansion.

Option D traps students who assume symmetric oscillations.

By forcing the evaluation of the anharmonic cubic term −g(r−r0)3-g(r-r_0)^3 using the Boltzmann distribution, the problem highlights that the asymmetry (concavity change) of the potential well is the strict physical requirement for thermal expansion.

Quick Facts About This Question

Question Information

SubjectPhysics
ChapterMotion in a Straight Line - Class 11 Part 1
ConceptGraphical Concavity Significance
Difficulty8
Cognitive Load7
Target Solve Time160 sec
AccessFree