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George Parzen

Publications and source records attributed to George Parzen.

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Theory of the friction force using electron cooling as an intrabeam scattering process

Using the results found previously for the cooling rates of the emittances, due to collisions between the electrons and the ions, a result is found for the friction force acting on the ions. It is shown that the friction force found here when used to track the ion bunch will give the same emittance cooling rates as those found using the intrabeam scattering theory for electron cooling >.For the case of the uniform in space electron bunch distribution, the friction force found here agrees with the friction force result found with the usual theory of electron cooling.

physics.acc-ph

Theory of electron cooling using electron cooling as an intrabeam scattering process

Electron cooling that results when a bunch of electrons overlaps a bunch of ions , with both bunches moving at the same velocity, may be considered to be an intrabeam scattering process. The process is similar to the usual intrabeam scattering, where the ions scatter from each other and usually results in beam growth. An important difference is that in electron cooling the mass of the ion is different from and much larger than the mass of the electron. This difference considerably complicates the intrabeam scattering theory. It introduces a new term in the emittance growth rate, which vanishes when the particles are identical and their masses are equal, and can give rise to emittance cooling of the heavier particles . The term that gives rise to beam growth for the usual intrabeam scattering is also present but is much smaller than the cooling term when one particle is much heavier than the other. This paper derives the results found for the emittance cooling rates due to the scattering of the ions in the ion bunch by the electons in the electron bunch.

physics.acc-ph

Intrabeam scattering growth rates for a bi-gaussian beam

This note finds results for the intrabeam scattering growth rates for a bi-gaussian distribution. The bi-gaussian distribution is interesting for studying the possibility of using electron cooling in RHIC. Experiments and computer studies indicate that in the presence of electron cooling, the beam distribution changes so that it developes a strong core and a long tail which is not described well by a gaussian, but may be better described by a bi-gaussian. Being able to compute the effects of intrabeam scattering for a bi-gaussian distribution would be useful in computing the effects of electron cooling, which depend critically on the details of the intrabeam scattering. The calculation is done using the reformulation of intrabeam scattering theory given in [1] based on the treatments given by A. Piwinski [2] and J. Bjorken and S.K. Mtingwa [3]. The bi-gaussian distribution is defined below as the sum of two gaussians in the particle coordinates $x,y,s,p_x,p_y,p_s$. The gaussian with the smaller dimensions produces most of the core of the beam, and the gaussian with the larger dimensions largely produces the long tail of the beam. The final result for the growth rates are expressed as the sum of three terms which can be interperted respectively as the contribution to the growth rates due to the scattering of the particles in the first gaussian from themselves, the scattering of the particles in the second gaussian from themselves, and the scattering of the particles in the first gaussian from the particles in the second gaussian.

physics.acc-ph

A reformulation of intrabeam scattering theory

The motivation for the treatment of intrabeam scattering theory given in this paper was to find results which would be convenient for computing the intrabeam scattering growth rates for particle distributions which are more complicated than a simple gaussian. It was shown by A. Piwinski that beam growth rates due to intrabeam scattering can be expressed as a multidimensional integral [1]. It was pointed out by J. Bjorken and S. Mtingwa [2] that the reduction of the multidimensional integral to a 3-dimensional untegral is made easier by writing the integral so that its relativistic transformation properties are more obvious. The starting point in [2] was a result from the treatment of the two body scattering problem in relativistic quantum theory . In this paper the starting point is the relativistic transformation properties of the scattering cross section which may be a more familiar starting point. The resulting expression for the multidimensional integral is simpler to reduce. In addition, the results do not depend on the particular form of the Coulomb cross section that was used in [2] and are valid for any collision cross section.

physics.acc-ph