Start Learning Free

Before You Begin

Question #42125

Difficulty: 8/10 | 🟢 Free

The Question

A conducting incompressible fluid of density ρ\rho, dynamic viscosity η\eta, and electrical conductivity σ\sigma flows with an average velocity vv through a non-conducting cylindrical pipe of diameter dd. A uniform transverse magnetic field BB is applied. The induced eddy currents generate a local Lorentz body force. A student incorrectly models the eddy currents as closed magnetic dipoles and concludes that since the field is uniform, the net magnetic force is zero. In reality, the local Lorentz force acts as an additional velocity-dependent drag. Assuming the inertial force per unit volume is fi=ρv2df_i = \rho \frac{v^2}{d}, the standard viscous force per unit volume is fv=ηvd2f_v = \eta \frac{v}{d^2}, and the magnetic drag force per unit volume is fm=σvB2f_m = \sigma v B^2, the flow transitions to turbulence when the effective Reynolds number (ratio of inertial force to total drag force) reaches a critical value Re0Re_0. What is the correct critical velocity vcv_c for the onset of turbulence?

Options

  • A.

    Re0ρd(η+σB2d2)\frac{Re_0}{\rho d} (\eta + \sigma B^2 d^2)

  • B.

    Re0ηρd\frac{Re_0 \eta}{\rho d}

  • C.

    Re0ρdη2+σ2B4d4\frac{Re_0}{\rho d} \sqrt{\eta^2 + \sigma^2 B^4 d^4}

  • D.

    Re0ηρd−σB2dρ\frac{Re_0 \eta}{\rho d} - \frac{\sigma B^2 d}{\rho}

Check Your Answer

Correct Answer

Step-by-Step Solution

Explanation

How the Examiner Thinks

Multi-Concept_Bridge

Master problems that require linking physics and math concepts to solve complex competitive questions.

Concepts Behind This Question

Reynolds Number Transition|Lenz’s Law Energy Conservation (652)|Vector Cross-Product

Why This Question Is Tricky

Common Mistakes

This question tests the understanding of Magnetohydrodynamics (MHD) and the Hartmann effect.

A common trap is treating the induced eddy currents purely as macroscopic magnetic dipoles.

Students incorrectly assume that because the external magnetic field is uniform, the net force on these 'dipoles' is zero (∇(m⃗⋅B⃗)=0\nabla(\vec{m} \cdot \vec{B}) = 0), leading them to ignore the magnetic damping entirely.

In reality, the local Lorentz force (J⃗×B⃗\vec{J} \times \vec{B}) acts as a distributed body force that opposes the flow, effectively increasing the apparent viscosity of the fluid.

This electromagnetic dissipation must be added to the mechanical viscous shear stress when calculating the effective Reynolds number for turbulence transition.

Quick Facts About This Question

Question Information

SubjectPhysics
ChapterMechanical Properties of Fluids - Class 11 Part 2
ConceptReynolds Number Transition
Difficulty8
Cognitive Load7
Target Solve Time160 sec
AccessFree