Envelope instability in love-energy proton synchrotrons
نویسندگان
چکیده
In this paper we investigate the limits on beam intensity in low-energy proton synchrotrons due to the instability of the beam envelope . This instability has been previously examined in the context of space charge dominated ion beams, in particular for inertial confinement fusion applications. We generalize the formalism of beam envelope evolution to include effects found in circular accelerators, i .e . curvature focusing and momentum dispersion . Several example lattices are analyzed to determine intensity limits imposed by onset of envelope instability ; it is found that the instability can occur without depressing the phase advance below 90' per cell .
منابع مشابه
Summary of Instabilities and Damping Group
There are a number of new high intensity proton synchrotrons proposed: the SNS[6] at Oakridge and ESS[7] in Europe, as neutron sources; the JHF/NSP[9] in Japan, a multi-disciplinary facility sponsored by KEK and JAERI; the New FNAL Booster[5]; and the Proton Driver[4, 8] as first stage of a μ − μ collider. In addition there are operating machines such as ISIS[1] at RAL, the Brookhaven AGS[3] an...
متن کاملImpedance Considerations for the Design of the Vacuum System of the Cern Ps2 Proton Synchrotron∗
In order for the LHC to reach an ultimate luminosity goal of 10 35 /cm 2 /s, CERN is considering upgrade options for the LHC injector chain, including a new 50 GeV synchrotron of about 1.3 km length for protons and heavy ions, to be called the PS2 [1]. The proton energy will be ramped from 4 GeV to 50 GeV in 1.2 s, and the design proton current for LHC operation is 2.7 A. In the LARP framework ...
متن کاملA Preliminary Comparative Study of the Electron - Cloud Effect
We present preliminary electron-cloud simulation results for the Proton Storage Ring (PSR) at LANL, the ISIS synchrotron at RAL, and the European Spallation Source (ESS). For each machine, we simulate the build-up and dissipation of the electron cloud (EC) in a representative field-free section of the vacuum chamber. For all three cases, we choose the same residual gas temperature, secondary em...
متن کاملMagnetic field generation in relativistic shocks
We present an analytical estimate for the magnetic field strength generated by the Weibel instability in ultra-relativistic shocks in a hydrogen plasma. We find that the Weibel instability is, by itself, not capable of converting the kinetic energy of protons penetrating the shock front into magnetic field energy. Other (nonlinear) processes must determine the magnetic field strength in the wak...
متن کاملAcceleration mechanism in compact objects
We investigate the kinetic theory of a mixing of rela-tivistic pair plasma in a conventional electron-proton plasma and an intense anisotropic Compton radiation field as those found in the vicinity of a compact object, a neutron star or a black hole. In a two-flow configuration we discriminate two regimes: the first one is realized when the mass energy density of the pair plasma is lower than t...
متن کامل