69 Synchrotron Radiation
Cyclotrons and Synchrotrons
Apart from high voltage electrostatic machines, the first machines to accelerate electrons and protons beyond kilovolt energies were cyclotrons (patented by Lawrence in 1934, this is his patent application, in Wikipedia) in which the particle moves in a planar spiral in a perpendicular magnetic field, given an electric kick every half turn, the increase in speed increases orbit size, but (nonrelativistically) the orbit time is constant, so an AC field can be used to provide the acceleration. The particles can be fed in continuously near the center of the machine, and spiral out to the maximum radius. However, to increase speed into the relativistic range, the increase in mass means that the orbital time is no longer independent of energy. Some lagging can be tolerated, but obviously not much.
Therefore, the particles must be fed into the machine one bunch at a time (rather than continuously) and the timing of electrical impulses then synchronized with the orbital time for the one bunch present, increasing with energy. This is the synchrotron. The limiting factor for increasing energy in a synchrotron is that the particles circling are of course accelerating towards the center and therefore radiating energy.
Perhaps the most important synchrotron radiation facility is the Advanced Photon Source (APS) at Argonne National Lab. There electrons are accelerated to 7 Gev ( ) and then sent into storage rings (1 km diameter) where rf fields are used to maintain their energy. X-rays from this machine have recently made major contributions to finding the structure of important proteins, for example.
Summarizing Radiation Formulas
To analyze synchrotron radiation, we'll first summarize here the radiation formulas found so far.
First, the radiated power:
The nonrelativistic Larmor formula:
and the relativistic generalization: In linear motion, the second term of course disappears.
In circular motion at radius
To find the pattern of radiation needs significantly more work. We need the Lienard-Weichert formula for the electric field, the magnetic field radiated has essentially the same form, so we can find the Poynting vector in any direction.
The electric field is: The first term is just the relativistic static field from the moving charge, the same as for a nonaccelerating (but moving) charge. The second term is the radiation.
Circular Acceleration: Angular Distribution
Following Jackson, we take in to find with lots of algebra Recall now is very close to one, so this beam is well focused in the direction. Huge power per unit solid angle, but over a very small solid angle.
The Heaviside-Feynman Formula
The expression for the electric field of a moving point charge given above can be written in a quite different way (the derivation is nontrivial) first found by Heaviside, discovered independently by Feynman: and the magnetic field is given by
(The formula is given without derivation in Volume 1 of Feynman's Lectures, 28-2. It's derived in Zangwill, and given, naturally, as a long problem in Jackson.)
The first term is the ordinary Coulomb field from the retarded time. The second term more or less updates the field to the one we are now familiar with, the "squashed" Coulomb field for a charge moving at constant velocity, centered at the actual position of the charge. The third term includes the radiative field from the charge's acceleration, notice it's the acceleration in the observer's time of the unit vector pointing to the retarded particle position. But there's more: it is a unit vector, so it's accelerating even if moving uniformly round a circle, and it will in general be accelerating along the circle for a charge in steady linear motion. Since the whole formula is exact, these contributions must be cancelled by the second term, to ensure no radiation from a steadily moving charge.
In fact, though, these contributions are negligible if the accelerating charge is in a localized region smaller than the distance to the observer. Note also that in the third term we are observing an oscillating unit vector at a distance , so amplitude dependence.
The circle represents the synchrotron, radius and a charge at angle The observer is taken to be very far away in the direction. The unit vector points to the observer from the apparent position of the charge, that is, where it was at the retarded timein other words, where the observer sees it to be.
Now the vector where and to a good approximation so
Notice now the component is time-independent, and in the component we can just keep the in the denominator, so Feynman's formula for the radiating electric field becomes
Rearranging, and using and incorporating the constant into the observer's clock setting,
Again use to write
These two equations describe a curve parameterized by We need to plot against and find its second derivative to find as a function of observer time
In fact, this is a generalized cycloid: imagine rolling a wheel of unit radius along a horizontal line, and track a point on the wheel a distance from the center. Now is how long the wheel has been rolling, with angular velocity Its center will have moved through horizontally, the point is horizontally from the center, and vertically displaced by
If the spot is at the center of the wheel, the radiated field is zero. If the electric field oscillates sinusoidally with frequency But as the curve approaches an actual cycloid, tending to a cusp, the second derivative goes to infinity. The radiation becomes a series of pulses.
To get a clear picture of just how the curve goes from a sinusoidal oscillation in the low speed limit to approaching a cycloid in the extreme relativistic limit, click here. The high energy limit corresponds to unit radius (the default setting, easily adjusted). By the way, the cycloid picture in Zangwill (page 895) is incorrect: the intermediate curve should of course be smooth, the cusp only comes in the relativistic limit.
Note on this cycloid curve: the standard notation would be with almost cusp at for Near the origin, so
This tells us the curvature at the cusp compared with the curvature of the rest of the curve (of order unity) is up by a factor of
The Advanced Photon Source has radius one kilometer, so the circling frequency is of order 100 kHz. At that frequency, the wavelength radiated would be of order a kilometer. But near the cusp this is shortened by a factor of order and and the radiation is X-rays.
Cosmic Synchrotron Radiation
Synchrotron radiation is common in astronomy. Of course, it signals the presence of magnetic fields, so gives extra insight into the systems being studied. It has helped understand Jupiter's magnetosphere. It is present in the remnants of supernovae, electrons in a magnetic field give fairly well polarized bright radiation, but also are transparent. Synchrotron radiation from neutron stars suggests magnetic fields of order 108 tesla.