242
B. J. Holzer et al.
ultra-relativistic case, when the particle speed is very close to the speed of light,
β ≈ c, most of the radiation is emitted in the forward direction [48] into a cone
centred on the tangent to the trajectory and with an opening angle of 1/γ , where γ
is the Lorentz factor (since for a few GeV electron or a few TeV proton, γ ≈ 1000,
the photon emission angles are within a milliradian of the tangent to the trajectory).
The power emitted by a particle is proportional to the square of its energy E and
to the square of the deflecting magnetic field B:
P SR ∝ E
2 B
2 ,
(6.47)
and in terms of Lorentz factor γ and the local bending radius ρ can be written as
follows:
P SR =
2
3
α
2 γ 4
ρ 2 ,
(6.48)
where α is the fine-structure constant and the Plank’s constant is given in a
convenient conversion constant:
α =
1
137
and = 197 MeV fm.
(6.49)
The emitted power is a very steep function of both the particle energy and particle
mass, being proportional to the fourth power of γ .
Integrating the above expression around the machine we obtain the amount of
energy lost per turn:
U 0 =
4π
3
α
γ 4
ρ
.
(6.50)
The emitted radiation spectrum consists of harmonics of the revolution frequency
and peaks near the so-called critical frequency or critical photon energy. It is defined
such that exactly half of the radiated power is emitted below it:
ε c =
2
3
γ 3
ρ
.
(6.51)
On the average a particle then emits n c ≈ 2παγ photons per turn.
6.5.2 Radiation Damping
In a storage ring the steady loss of energy to synchrotron radiation is compensated in
the RF cavities, where the particle receives each turn the average amount of energy
Précédent

- 250/867

Suivant