Intrabeam Scattering

Intrabeam Scattering

Intrabeam scattering (IBS) is an effect in accelerator physics where collisions between particles couple the beam emittance in all three dimensions. This generally causes the beam size to grow. In proton accelerators, intrabeam scattering causes the beam to grow slowly over a period of several hours. This limits the luminosity lifetime. In circular lepton accelerators, intrabeam scattering is counteracted by radiation damping, resulting in a new equilibrium beam emittance with a relaxation time on the order of milliseconds. Intrabeam scattering creates an inverse relationship between the smallness of the beam and the number of particles it contains, therefore limiting luminosity.

The two principal methods for calculating the effects of intrabeam scattering were done by Anton Piwinski in 1974 and James Bjorken and Sekazi Mtingwa in 1983. The Bjorken-Mtingwa formulation is regarded as being the most general solution. Both of these methods are computationally intensive. Several approximations of these methods have been done that are easier to evaluate, but less general. These approximations are summarized in "Intrabeam scattering formulas for high energy beams" by K. Kubo "et al".

Intrabeam scattering rates have a 1/gamma^{4} dependence. This means that its effects diminish with increasing beam energy. Other ways of mitigating IBS effects are the use of wigglers, and reducing beam intensity. Transverse intrabeam scattering rates are sensitive to dispersion.

Intrabeam scattering is closely related to the Touschek effect. The Touschek effect is a lifetime based on intrabeam collisions that result in both particles being ejected from the beam. Intrabeam scattering is a risetime based on intrabeam collisions that result in momentum coupling.

Bjorken-Mtingwa formulation

The betatron growth rates for intrabeam scattering are defined as,: frac{1}{T_{p stackrel{mathrm{def{=} frac{1}{sigma_{p frac{dsigma_{p{dt},: frac{1}{T_{h stackrel{mathrm{def{=} frac{1}{epsilon_{h}^{1/2 frac{depsilon_{h}^{1/2{dt},: frac{1}{T_{v stackrel{mathrm{def{=} frac{1}{epsilon_{v}^{1/2 frac{depsilon_{v}^{1/2{dt}.The following is general to all bunched beams,: frac{1}{T_{i = 4pi A (log) leftlangle int_{0}^{infty} ,dlambda frac{lambda^{1/2{ [det(L+lambda I)] ^{1/2 left{TrL^{i}Trleft(frac{1}{L+lambda I} ight) - 3 Trleft [L^{i}left(frac{1}{L+lambda I} ight) ight] ight} ight angle,where T_{p}, T_{h}, and T_{v} are the momentum spread, horizontal, and vertical are the betatron growth times.The angle brackets <...> indicate that the integral is averaged around the ring.: (log) = ln frac{b_{min{b_{max = ln frac{2}{ heta_{min: A = frac{r_0^2 c N}{64 pi^2 eta^3 gamma^4 epsilon_h epsilon_v sigma_s sigma_p}: L = L^{(p)} + L^{(h)} + L^{(v)},: L^{(p)} = frac{gamma^2}{sigma^2_p}egin{pmatrix}0 & 0 & 0\0 & 1 & 0\0 & 0 & 0end{pmatrix}: L^{(h)} = frac{eta_h}{epsilon_h}egin{pmatrix}1 & -gammaphi_h & 0\-gammaphi_h & frac{gamma^2 {mathcal H}_h}{eta_h} & 0\0 & 0 & 0end{pmatrix}: L^{(v)} = frac{eta_v}{epsilon_v}egin{pmatrix}0 & 0 & 0\0 & frac{gamma^2 {mathcal H}_v}{eta_v} & -gammaphi_v\0 & -gammaphi_v & 1end{pmatrix}:{mathcal H}_{h,v} = [eta^2_{h,v} + (eta_{h,v}eta'_{h,v} - frac{1}{2}eta'_{h,v}eta_h)^2] /eta_{h,v}:phi_{h,v} = eta'_{h,v} - frac{1}{2}eta'_{h,v}eta_{h,v}/eta_{h,v}Definitions::r_0^2 is the classical radius of the particle:c is the speed of light:N is the number of particles per bunch:eta is velocity divided by the speed of light:gamma is energy divided by mass:eta_{h,v} and eta'_{h,v} is the betatron function and its derivative, respectively:eta_{h,v} and eta'_{h,v} is the dispersion function and its derivative, respectively:epsilon_{h,v} is the emittance:sigma_s is the bunch length:sigma_p is the momentum spread:b_{min} and b_{max} are the minimum and maximum impact parameters. The minimum impact parameter is the closest distance of approach between two particles in a collision. The maximum impact parameter is the largest distance between two particles such that their trajectories are unaltered by the collision.: heta_{min} is the minimum scattering angle.

References

* A. Piwinski, in "Proceesings of the 9th International Conference on High Energy Accelerators, Stanford, CA, 1974" (SLAC, Stanford, 1974), p.405
* J. Bjorken and S. Mtingwa, Part. Accel. 13, 115 (1983).
* K. Kubo "et al"., Phys. Rev. ST Accel. Beams 8, 081001 (2005).


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