Problem 1:
A sphere of radius R is uniformly magnetized with magnetization M and
has a magnetic dipole moment m = 4πR3M/3.
The magnetic field due to this sphere is a pure dipole field outside the sphere
and it is uniform inside the sphere.
(a) Find Binside and Hinside in terms
of M.
(b) If the sphere is made of lih material
with magnetic susceptibility Χm > 0 and it is magnetized because
it is located in a uniform external field B0, find M
in terms B0 or H0
Solution:
- Concepts:
Magnetostatics, magnetic materials
- Reasoning:
Orient your coordinate system so that M points in
the z-direction and place the center of the sphere at the origin
B is continuous on the z-axis at at z = R.
- Details of the calculation:
(a) B(r) = (μ0/4π)(3(m·r)r/r5
- m/r3) = (μ0m/(4πr3))[2 cosθ (r/r)
+ sinθ (θ/θ)] outside the sphere.
On the z-axis at z = R we have B = 2μ0m/(4πR3)
= 2μ0M/3.
Bin = 2μ0M/3,
Hinside
= Bin/μ0 -
M = -M/3.
(b) The total field inside the sphere is the superposition of the
field of a uniform magnetized sphere and the constant external field B0.
We need to find M.
Bin = B0 + 2Mμ0/3,
μHin =
Bin,
M = χmHin
= (χm/μ)Bin.
(1 - 2μ0χm/(3μ))Bin
= B0.
μ = μ0(1 + Χm). Therefore
Bin
= B0(3 + 3χm)/(3 + χm).
μ0M = B0([(3 + 3χm)/(3 + χm)][ χm/(1 + Χm)]
= 3χmB0/(3 + χm).
M = 3χmH0/(3 + χm).
Problem 2:
An electric dipole p0 makes an angle of 30 degrees
with respect to the z-axis as it rotates about the z-axis with angular speed ω.
Find its initial rate of energy loss.
Solution:
- Concepts:
Electric dipole radiation
- Reasoning:
The x and y components of the
dipole moment are oscillating with angular frequency ω. The rotating
electric dipole will radiate energy at a rate Prad = <(d2p/dt2)2>/(6πε0c3).
- Details of the calculation:
p(t) = p0 cosθ
k + p0 sinθ (cos(ωt)
i +
sin(ωt) j), where θ is the tilt angle.
d2p/dt2 = -ω2p0 sinθ [cos(ωt)
i + sin(ωt) j].
<(d2p/dt2)2> = ω4p02sin2θ
= ω4p02/4, Prad = ω4p02/(24πε0c3).
Problem 3:
The Larmor formula gives the power radiated by a particle of charge q with an
acceleration a. Use this formula and the Bohr model of the hydrogen
atom to estimate the time for an electron in the lowest Bohr orbit to spiral
into the nucleus. It is a valid approximation to assume that the orbits
remain almost circular as the electron spirals. Show your work!
Solution:
- Concepts:
The radiation field of a point charge moving
non-relativistically, the Larmor formula
- Reasoning:
The electron orbits the "infinitely heavy" proton. Its
acceleration is a = v2/r, and it therefore radiates away energy,
P = -dE/dt = [q2/(6πε0c3)]a2.
(SI units)
- Details of the calculation:
To solve for the total time it takes the
electron to spiral into the nucleus, we can express the acceleration a in
terms of E. We then have
-dE/dt = f(E), ∫dt = Δt = ∫E0-∞dE/f(E).
Alternatively, we can express E as a function of the radius r and derive an
expression -dr/dt = f(r). We then have
∫dt = ΔT = ∫r00dr/f(r).
To find the relationship between E and a we can use
F = q2/(4πε0r2)
= mv2/r. mv2 = q2/(4πε0r),
E
= ½mv2 - q2/(4πε0r) = - q2/(8πε0r)
= -½mv2.
Now we can express a in terms of E.
a = v2/r
= q2/(4πε0r2m) = 2E28πε0/(q2m).
-dE/dt = E4162πε0/(6c3q2m2).
dt = -(dE/E4) (6c3q2m2)/(162πε0).
Δt = (6c3q2m2)/(162πε0)∫E0-∞(dE/E4)
= -(6c3q2m2)/(162πε0)(E0-3/3)
where E0 = -13.6 eV, Δt = 1.5*10-11s.
Or we can
also express both E and a in terms of r.
a = F/m = q2/(4πε0r2m),
E = - q2/(8πε0r),
dE = [q2/(8πε0r2)]dr
= -Pdt.
dt = -[q2/(8πε0r2)]dr/P
= -[q2/(8πε0r2)]dr/[q2a2/(6πε0c3)].
dt = -dr[3c3/(4r2a2)] = -r2dr[12c3π2ε02m2/q4].
Δt = -[12c3π2ε02m2/q4]∫r00r2dr
= [12c3π2ε02m2/q4](r03/3)
where r0 = Bohr radius = 5.29*10-11m, Δt = 1.5*10-11s.