M. M.
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Penning traps

ItsaTrap

Charged particles can be trapped in two main ways: Paul traps and Penning traps. This post dives into Penning traps, their physics and how they keep ions in place. Want to learn about Paul traps? See my earlier posts on Paul traps and ion crystallization.

Charged particles in a magnetic field

A charged particle of charge qq and mass mm moving in a magnetic field BB experiences the Lorentz force,

(1)

Since the force is always perpendicular to the velocity, it does no work: the kinetic energy is conserved and the speed stays constant. The motion is a uniform circular orbit in the plane orthogonal to BB, with radius rcr_c and frequency ωc\omega_c given by,

(2)

This is the cyclotron motion. If the particle has a velocity component vv_{\parallel} along BB, its path is helical: circular motion in the plane perpendicular to BB plus free propagation along the field lines.

Below is an interactive simulation of NN interacting particles in a magnetic field BB. Each particle starts with a random velocity in xx, yy, and zz. The magnetic field affects motion in the xyx–y plane but leaves motion along zz unchanged. Particles with smaller zz-momentum move more slowly in that direction and can appear confined within the region.

Use the slider below the animation to adjust the number of particles and the field strength BB. As expected from Eq.2, larger BB produces tighter, faster radial orbits.

Loading charged particle in B field simulation…

The animation shows that the magnetic field provides confinement only in the radial plane. A particle with vz=0v_z = 0 may appear stationary along zz, but in a real trap tiny electric-field imperfections give it a small axial kick. With no restoring force along that axis, the particle simply keeps going and eventually escapes the trap. To achieve full 3D confinement, we need a restoring force along z. As for the case of Paul traps, this can be done by adding a static DC electric field in the form of a quadrupole potential,

(3)

we can make sure that the particle is trapped in the zz-direction. Let's now look at the Lagrangian of the whole system,

(4)

For a uniform magnetic field B=Bz^\mathbf{B} = B\,\hat{z}, is convenient to use a symmetric gauge,

(5)

Plugging these into the minimal-coupling Lagrangian gives,

(6)

Along z, the magnetic term does nothing, so the the equation of motion is the same as for a harmonic oscillator,

(7)

with ωz=q2V0md2\omega_z = \sqrt{q\frac{2 V_0}{m d^2}}.

On the xyx-y plane, the equation of motion are slightly more complicated and the two coordinates mix,

(8)

These can be solved by introducing the complex coordinate u(t)=x(t)+iy(t)u(t) = x(t) + i\,y(t) so that u˙=x˙+iy˙\dot{u} = \dot{x} + i\dot{y} and u¨=x¨+iy¨\ddot{u} = \ddot{x} + i\ddot{y}. In this coordinate system the radial dynamics reduce to a single complex equation,

(9)

which, by assuming u(t)=u0eiωtu(t) = u_0 e^{-i\omega t}, can be reduced to a quadratic equation ω2ωcω+ωz22=0\omega^2 - \omega_c\omega + \frac{\omega_z^2}{2} = 0 with solutions,

(10)

The larger root, ω+\omega_+, is known as the modified cyclotron frequency. It corresponds to a rapid circular motion with a relatively small radius. The smaller root, ω\omega_-, is the magnetron frequency, which corresponds to a much slower circular drift with a larger radius. These two motions together describe the full trajectory of a charged particle in a Penning trap. For both frequencies to be real, the condition ωc2>2ωz2\omega_c^2 > 2\omega_z^2 must be satisfied. The plot below illustrates the motional frequencies as function of the axial frequency for a given magnetic field.

To solve Eq. 8 let's introduce the complex coordinate

(1.a)

so that u˙=x˙+iy˙\dot{u} = \dot{x} + i\dot{y} and u¨=x¨+iy¨\ddot{u} = \ddot{x} + i\ddot{y}. After substituting this into Eq. 8, we obtain Eq. 9. We look for normal-mode solutions of the form u(t)=u0eiωtu(t) = u_0 e^{-i\omega t} such that u˙=iωu\dot{u} = -i\omega u and u¨=ω2u\ddot{u} = -\omega^2 u obtaining,

(2.a)

This quadratic equation has two solutions

(3.a)

with ω+\omega_+ the modified cyclotron frequency and ω\omega_- the magnetron frequency. Note that for both solutions to be real, ωc2>2ωz2\omega_c^2 > 2\omega_z^2 must be satisfied.

Loading sketch…

Perhaps more interactive, the animation below show the motion of a charged particle in a Penning trap with variable magnetic and electric fields. In the inset you can see the various cyclotron, magnetron and axial frequencies and how they vary with magnetic and electric field strength.

Loading Penning trap simulation…

Cooling and quantum

In order to quantize the motion of a charged particle in a Penning trap we have to move to an Hamiltonian description after a Legendre transformation of Eq.6.

(11)

Defining ωc=qBm\omega_c = \frac{qB}{m}, ωz2=2qV0md2\omega_z^2 = \frac{2 q V_0}{m d^2} and Ω2=ωz22\Omega^2 = \frac{\omega_z^2}{2} the Hamiltonian can be written as,

(12)

Introducing a new set of complex coordinates u=x+iyu = x + i y and v=xiyv = x - i y with corresponding momenta pu=12(pxipy)p_u = \frac{1} {2}(p_x - i p_y) and pv=12(px+ipy)p_v = \frac{1} {2}(p_x + i p_y) the Hamiltonian Eq. 12 becomes diagonal in terms of u, v and their conjugate momenta.

(13)

And where we defined

(14)

and,

(14)

The frequency ω+\omega_+ is also called the modified cyclotron frequency, this is larger than the usual cyclotron frequency and largely positive. In contrast, ω\omega_-, known as the magnetron frequency, corresponds to a negative-energy mode in the Hamiltonian. This negative-energy character arises when we define the complex coordinates which allow the Hamiltonian to separate into two independent modes. The “negative” does not imply a negative angular velocity; it reflects the structure of the Hamiltonian in this complex (rotating) basis. Finally, to ensure stable trapping (i.e., real frequencies), we have to satisfy ωc2>2ωz2\omega_c^2 > 2\,\omega_z^2.

Perhaps one of the most confusing dynamics of the motion of a charged particle in a penning trap is that, in order to be trapped the particle should always be in motion (as the Lorentz force is needed to provide confinement). But in the quantum ground state, there’s no motion at all! To get a feel for this, we can imagine the quantum motion as the average behavior of many classical particles, each starting in slightly different positions. The animation below shows exactly that, alongside the classical motion of a single particle, with and without cooling.

Loading Penning trap simulation…
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