Probability that a magnetic dipole is oriented with theta

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SUMMARY

The discussion focuses on the probability distribution of a magnetic dipole in a magnetic field, specifically using spherical coordinates to derive the probability density function p(θ, φ). The energy interaction is defined by E = −μ·B, leading to the expression p(θ, φ)dθdφ = (e^(μB cos θ) sin(θ) dθ dφ)/z, where z is the normalization constant calculated through the integral z = ∫∫ e^(μB cos θ) sin(θ) dθ dφ. The user expresses uncertainty about integrating in spherical coordinates and seeks clarification on the validity of their approach to the problem.

PREREQUISITES
  • Understanding of classical mechanics and magnetic dipoles
  • Familiarity with spherical coordinate systems
  • Knowledge of the Boltzmann distribution in statistical mechanics
  • Basic integration techniques in multiple dimensions
NEXT STEPS
  • Study the derivation of the Boltzmann distribution in detail
  • Learn about integration in spherical coordinates, focusing on solid angles
  • Explore examples of probability distributions in statistical mechanics
  • Investigate the physical implications of magnetic dipole interactions in various fields
USEFUL FOR

Students and researchers in physics, particularly those studying statistical mechanics, magnetic properties, and thermodynamics, will benefit from this discussion.

potatowhisperer
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1.
the problem goes like this :
The energy of interaction of a classical magnetic dipole with the magnetic field B is given by
E = −μ·B.
The sum over microstates becomes an integral over all directions of μ. The direction of μ
in three dimensions is given by the angles θ and φ of a spherical coordinate system
The integral is over the solid angle element
= sin θdθdφ. In this coordinate system
the energy of the dipole is given by E = −μB cos θ.
Choose spherical coordinates and show that the probability p(θ, φ)dθdφ that the dipole is
between the angles θ and + dθ and φ and φ + dφ is given by

p(θ, φ)dθdφ = (e^(μB cos θ) sin(θ) dθ dφ)/z
2. Homework Equations


z = ∫∫ e^(μB cos θ) sin(θ) dθ dφ .

The Attempt at a Solution


i have no idea what to do , and i tried all i know
i know that the Boltzmann distribution gives you the probability that a particle has an energy is :
e^([/B]μB cos θ)/∫e^(μB cos θ) , but how do i integrate the spherical coordinates i don t know . please help me and thank you .
 
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this is the best that i could do
the probability that the dipole between x and dx is
dp(x) = (1 / Z ) e^(μ(x)B cos θ) dx = dx because we assume that B is parallel to z so μ(x) . B = 0
dp(y) =
(1 / Z ) e^(μ(y)B cos θ) dy = dy
dp(z) = (1 / Z )e^(μ(z)B cos θ) dz
d^3 p( x,y,z)= (1 / Z )e^(μ(z)B cos ) dz dy dx = (1 / Z )e^(μ(z)B cos θ) dv
d^3 p( r,
θ,)
= (1 / Z )e^(μ(z)B cos θ) rd²r dθ dφ

is this true ? or am i making horrible mistakes ?
 

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