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Abstracts Brochure - CERN

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THPCH — Poster Session 29-Jun-06 16:00 - 18:00<br />

charge density is approximately constant this increase can be reached by the beam cross section growth. It can not be<br />

done for the most known accelerator structures. The appropriate acceleration schema is proposed and the results of<br />

the beam dynamics analysis and simulation are presented and discussed.<br />

Resonance Trapping, Halo Formation and Incoherent Emittance Growth due to Electron<br />

Cloud<br />

The pinched electron cloud introduces a<br />

tune shift along the bunch, which together<br />

with synchrotron motion, leads to a periodic<br />

crossing of resonances. The resonances are<br />

E. Benedetto, E. Benedetto (Politecnico di Torino) G. Franchetti<br />

(GSI) G. Rumolo, F. Zimmermann (<strong>CERN</strong>)<br />

excited by the longitudinal distribution of the electron cloud around the storage ring. We benchmark the PIC code<br />

HEADTAIL against a simplified weak-strong tracking code based on an analytical field model, obtaining an excellent<br />

agreement. The simplified code is then used for exploring the long term evolution of the beam emittance, and for<br />

studying more realistic lattice models. Results are presented for the <strong>CERN</strong> SPS and the LHC.<br />

Halo and Tail Generation Studies for Linear Colliders<br />

Halo particles in linear colliders can result<br />

in significant losses and serious background L. Neukermans, H. Burkhardt (<strong>CERN</strong>)<br />

which may reduce the overall performances.<br />

We present a study of various halo generation processes with numerical estimates. The aim is to allow to predict and<br />

minimize the halo throughout the accelerator chain including the final focus up to the experimental detectors. We<br />

include estimates for the planned CLIC beam line.<br />

Acceleration of Charged Particles by Field of Intensive Electromagnetic Waves in a Vacuum<br />

The dynamics of charged particles in a field<br />

of intensive electromagnetic waves or im- V.A. Buts, V.V. Kuzmin (NSC/KIPT)<br />

pulses is studied. A wave is called “intensive”<br />

when its strength parameter* approaches or become larger than one. We show that conventional schemes of<br />

acceleration such as IFEL** are not efficient. A stochastic instability suppresses its realization and leads to energy<br />

spread of accelerating particles and to destruction of accelerating bunches. From other side, the energy restrictions,<br />

caused by a radiational friction in a system of laser acceleration can be lifted. Moreover, the frictional forces can<br />

enhance acceleration of particles by a laser radiation. Analytical conditions for this enhancement are determined.<br />

Friction becomes particularly significant for interaction of electromagnetic waves with clusters. All particles in a laser<br />

pulse could move identically because of the friction. Additional benefits for acceleration under these conditions are<br />

provided by circularly polarized laser impulse. In this case energy of particles repeats the shape of the impulse’s<br />

envelope and the acceleration is very efficient. Several new IFEL and FEL*** schemes are discussed.<br />

* Epsion==e E/( m cΩ >=1) ** IFEL – inverse free electron lasers *** FEL – free electron lasers<br />

391<br />

THPCH018<br />

THPCH019<br />

THPCH020

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