[MAP] Correction (Re: Hamiltonian-gauge potentials
Robert D Ryne
rdryne at lbl.gov
Fri Mar 18 00:38:59 EDT 2011
What I wrote below is not correct. As Kirk just pointed out to me, and
Alex wrote earlier, it is true only in the linear approximation.
As Alex wrote earlier,
> But the eigen emittances are invariant under linear symplectic
> transformations, and therefore also under gauge transformations in
> the linear approximation.
Rob
On Mar 17, 2011, at 4:29 PM, Robert D Ryne wrote:
> Kirk,
>
>> On Mar 17, 2011, at 3:24 PM, Kirk T McDonald wrote:
>> It remains that rms emittance (and eigen-emittance, I believe) is
>> not gauge invariant. But we have to choose some gauge to proceed.
>
>
> The eigen-emittances are gauge invariant.
>
> More precisely, consider a numerical distribution of particles in
> the presence of electromagnetic fields. These can be defined, e.g.,
> using Cartesian coordinates and velocities at some time, or using
> transverse coordinates and velocities along with energy and arrival
> time at some location z, etc. Next, express the numerical
> distribution using canonical variables. Some elements of the 6-
> vector describing each particle will depend on your choice of gauge
> (e.g. p_{x,canonical} and p_{y,canonical}). Next, compute the beam
> second moment matrix \Sigma. Some of the matrix elements will depend
> on your choice of gauge. Next, compute the moduli of the eigenvalues
> of J \Sigma (these are the eigen-emittances). Though the numerical
> distribution (the collection of 6-vectors) and the \Sigma matrix
> will depend on the gauge, the eigen-emittances will be independent
> of the choice of gauge.
>
> Rob
>
>
> On Mar 17, 2011, at 3:24 PM, Kirk T McDonald wrote:
>
>> Folks
>>
>> I believe that what Alex Dragt has been trying to tell us is that
>> for applications involving Hamiltonian dynamics it is most favored
>> to use the so-called Hamiltonian gauge, in which the scalar
>> potential V is zero everywhere. Further, this ties in nicely with
>> the use of coordinates (x,y,t) rather than (x,y,z).
>>
>> For a general expression for the vector potential A in this gauge,
>> see sec. 8 of
>> http://puhep1.princeton.edu/~mcdonald/examples/EM/jackson_ajp_70_917_02.pdf
>>
>> For fields with time dependence e^{- i omega t), with nonzero wave
>> number k = omega / c, then the vector potential is simply
>> A = – i E / k. (Gaussian units).
>> Note that A = 0 wherever E = 0, in which regions B can only be
>> static.
>>
>> For a static magnetic field, the vector potential is the same as
>> that in the Coulomb gauge (and in the Lorenz gauge). [In some
>> static cases, such a toroidal magnets, the static vector potential
>> will be nonzero in regions where B is zero; but in regions where a
>> Fourier component B_omega is zero for nonzero omega, A_omega will
>> be zero also.]
>>
>> A static electric field has the vector potential
>> A = – c(t – t_0) E.
>> This seems a bit odd, but will not bother us.
>>
>> An unusual feature of the Hamiltonian gauge vector potential is
>> that is is not continuous at a perfectly conducting surface – which
>> did bother me for quite a while.
>>
>> However, in using A to compute B, the (ill-defined) normal
>> derivative at a perfectly conducting surface is not needed to
>> deduce the tangential B.
>>
>> Of course, the Hamiltonian gauge vector potential makes the
>> canonical momentum p = p_mech + q A / c
>> discontinuous at the surface of the rf cavity.
>>
>> This is troublesome if we use coordinates (x,y,z) and have an
>> accelerating cavity with E_z, such that p_z takes a step on
>> entering or leaving the cavity.
>>
>> However, if we switch to coordinates (x,y,t) the t-canonical
>> momentum is
>> p_t = – E_mech – q V = – E_mech
>> in the Hamiltonian gauge, which is continuous at the cavity wall.
>> Also, canonical momenta p_x and p_y are continuous if the particles
>> enter and leave the cavity through faces at constant z (of a good
>> conducting material).
>>
>> All this is serendipitous for the cooling sections of a muon
>> collider, where we are almost certain to use cavities with flat
>> (Be) faces where the particles enter and exit.
>>
>> It remains that rms emittance (and eigen-emittance, I believe) is
>> not gauge invariant. But we have to choose some gauge to proceed.
>>
>> It now looks like the Hamiltonian gauge is the one to use, along
>> with coordinates (x,y,t) rather than (x,y,z).
>>
>> 1. Time-dependent A_omega follows immediately from knowledge of
>> E_omega, and is zero where E_omega and B_omega are zero.
>>
>> 2. Static A is same as in the Coulomb gauge (which is what we
>> almost always use now).
>>
>> 3. No steps in canonical momenta so long as all rf cavities have
>> flat faces where particles enter/exit.
>>
>> 4. No scalar potential to worry about, so p_t = – E_mech, as in
>> our present software. (It doesn’t hurt anything to define p_t = +
>> E_mech, as we actually do.)
>>
>> ---------------------------------------------------------
>> 5. Although phase volume is the same where or not we include the
>> potentials in the momenta, this is not true for rms emittance (or
>> eigen-emittance). So we should stop using ECAL9, and switch to
>> emitcalc (with a better approximation to the vector potential) and/
>> or equivalent programs developed by Tom Roberts, Chris Rogers, et al.
>>
>> --Kirk
>> _______________________________________________
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>> MAP-l at lists.bnl.gov
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>
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