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electric dipole in a sphere
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Working notes by Phil dated 3.29.17, part of a rigid body appendix. Uses Euler's equations with the sphere's isotropic inertia (2/5)Mr^2 and torque N = p x E to get equations for the angular velocity components. He tries a dumbbell analogy and spherical-unit-vector and Euler-angle relations, gets stuck, and concludes it is the heavy top problem with a simpler inertia tensor.
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Electric dipole in a sphere PhL 3.29.17
Step 1. If the dipole is embedded in a uniform density sphere, I know at once that all three inertia components are the same no matter how you choose the principal axes, so the Frame S' equations of motion are :
(N)'1 = I'1 ()'1 - (ω)'2(ω)'3 (I'2 - I'3)
(N)'2 = I'2 ()'2 - (ω)'3(ω)'1 (I'3 - I'1)
(N)'3 = I'3 ()'3 - (ω)'1(ω)'2 (I'1 - I'2) . (I.4.3)
and then
(N)'1 = I'1 ()'1
(N)'2 = I'1 ()'2
(N)'3 = I'1 ()'3 I'1 = (2/5)Mr2 looking it up on the web (could calc it here)
Let I'1 = (2/5)Mr2 ≡ J. then the above three equations say
(N)'i = J ()'i
Since this is true for all Frame S' components, it must be true as a vector equation, so
N = J
and therefore in Frame S we could write
Ni = J ()i
Step 2. We know that the torque on the dipole is this
N = p x E
based on our I.10 problem work. Thus, in Frame S we have
εijkpjEk = J ()i
But only E3 = E exists in Frame S, so set k = 3 to get
εij3pjE = J ()i
Write out these equations
i=1 ε123p2E = J ()1 p2E = J ()1
i=2 ε213p1E = J ()2 -p1E = J ()2
i = 3 ε3j3pjE = J ()3 0 = J ()3
We then end up with :
ω3 = constant
()1 = [p2E/J]
()2 = - [p1E/J]
Now since p = p by fiat (I declare the embedded p to be in the direction) , we have
p = p [ sinθcosφ, sinθsinφ,cosθ] = [p1,p2,p3]
This our equations can be written
ω3 = constant
()1 = [pE/J] sinθsinφ
()2 = - [pE/J] sinθcosφ
At this point I know nothing about θ(t) and φ(t) so cannot simply integrate. So what do I do next??
What is L ?
L = Iω = Jω J = scalar = (2/5)MR2
= J
What does Newton say in Frame S?
N =
Thus we know that
p x E = J
εijkpjEδk3 = J ()i
but I already know this, so nothing new here!
Maybe look for some conserved quantities! Maybe I should be starting by writing force and torque as I did in the electric dipole dumbbell problem.
Plan A: Imagine that the dumbbell is embedded in the sphere so that there are charges q and -q as before, and the stick length is 2r where r is the radius of the mass sphere. . Then p = 2rq. So this is just the dumbbell problem with a different inertia tensor. In this case I have
F = 0
N = N1+ N2 = 2N1 = -2rqEsinθ
Thus the equation of motion can be written
p x E = J
N = J =
-2rqEsinθ = J
= - (2rqE/J)sinθ
or
= - (pE/J) sinθ
So here then is the equations of motion in terms of spherical unit vectors. I have to be careful now not to make my previous mistake in trying to solve this equation! I think I can still claim that
()r = 0 ()r = 0 Nr = 0
()θ = 0 ()θ = 0 Nθ = 0
()φ = -pEsinθ . ()φ = -(pE/J) sinθ Nφ = -2rqEsinθ (I.10.9)
But now I no longer have (F.2.2) for L, maybe I have to complete L somehow!! Go back to
ω3 = constant
()1 = [pE/J] sinθsinφ
()2 = - [pE/J] sinθcosφ
I have four unknowns ω1(t), ω2(t), θ(t) and φ(t), but only two equations! I need more equations!
How about these equations,
ω1 = sinθcosφ - sinφ
ω2 = sinθsinφ + cosφ
ω3 = cosθ + . // Frame S (H.6.18)
Can I use them somehow? Can I assume ψ = constant? Is there torque about the axis? Well above I have written Nr = 0 so do I know somehow that = Nr ?
Look at ()r = 0 = 0
(dL/dt)S = 0 [(dL/dt)S]r = 0
I used this kind of fact in (H.4.1).
ωφ =
ωθ = '
ωψ = ' . (H.4.1)
How did I get these three equations? How do I know that does not contribute to ωφ ? // OK, I pondered this and added a new paragraph to frames doc below (H.4.1), I think this was worth pondering and getting stated.
So OK, what does the information ()r = 0 tell me?
Here is what I want to say
Nr = 0 ψ = constant
How do I justify this?
N =
Nr = ()r = 0
Can I say this
(dL/dt)r = dLr/dt ?
If I could say this, then I would have
Nr = dLr/dt = 0 Lr = constant
Then I have to argue that Lr = Jωr and then ωr = 0 and so then ψ = constant
But this is a commutation theorem issue. I really have
L = Lr + Lθ + Lφ
Then
= r + Lr ∂t + θ + Lθ ∂t + φ + Lφ ∂t
= r + Lr [ + sinθ ]
+ θ + Lθ [ – + cosθ ] + φ + Lφ [ – sinθ – cosθ ]
= {r - Lθ - sinθLφ } + {Lr + θ - cosθ Lφ} + { Lr sinθ + Lθ cosθ + φ }
This tells me that
()r = r - Lθ - sinθLφ
()θ = Lr + θ - cosθ Lφ
()φ = Lr sinθ + Lθ cosθ + φ
I then combine these with results from above
()r = 0 ()r = 0 Nr = 0
()θ = 0 ()θ = 0 Nθ = 0
()φ = -pEsinθ . ()φ = -(pE/J) sinθ Nφ = -2rqEsinθ (I.10.9)
and I end up with these equations of motion
r - Lθ - sinθLφ = 0
Lr + θ - cosθ Lφ = 0
Lr sinθ + Lθ cosθ + φ = -pEsinθ
This is very ugly stuff. I suppose I can say
= J
and rewrite this mess in terms of ω components. I hate it! But recall my conjecture from above
(dL/dt)r = dLr/dt ?
Well in fact
(dL/dt)r = r - Lθ - sinθLφ
so forget that pathway!
I really need to solve things within Frame S'!
Status: Today 3.29.17 I have spent perhaps 4 hours on this problem, and I have made zero progress. Typical for the course!
Is this perhaps the same as the top problem? There the torque is N = r x [-mg ] about the center of mass of the top, whereas here the torque is N = p x E = 2q r x E , sure looks the same. Both torques are about the CMS. Then connection ought then to be 2qE = -mg or 2qE = -mg.
So I think it really is the top problem, but with a simpler inertia tensor.