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Accelerator Physics Statistical and Collective Effects II
A. S. Bogacz, G. A. Krafft, S. DeSilva, R. Gamage Jefferson Lab Old Dominion University Lecture 17 G. A. Krafft Jefferson Lab
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Beam Temperature K-V has single value for the transverse Hamiltonian
No Temperature! Temperature in beam introduces thermal spreads Transverse Temperature Debye length Longitudinal Temperature Landau Damping
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Waterbag Distribution
Lemons and Thode were first to point out SC field is solved as Bessel Functions for a certain equation of state. Later, others, including my advisor and I showed the equation of state was exact for the waterbag distribution.
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Equation for Beam Radius
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Debye Length Picture* *Davidson and Qin
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Collisionless (Landau) Damping
Other important effect of thermal spreads in accelerator physics Longitudinal Plasma Oscillations (1 D)
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Linearized In fluid limit plasma oscillations are undamped
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Vlasov Analysis of Problem
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Initial Value Problem Laplace in t and Fourier in z
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Dielectric function Landau (self-consistent) dielectric function
Solution for normal modes are
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Collisionless Damping
For Lorentzian distribution Landau damping rate
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Negative Mass Instability
Simplified argument: assume longitudinal clump on otherwise uniform beam Particles pushed away from clump centroid If above transition, come back LATER if ahead of clump center and EARLIER if behind it The clump is therefore enhanced! INSTABILITY; particles act as if they have negative mass (they accelerate backward compared to force!) θ
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Longitudinal Impedance
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Frequency Domain
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NMI Simple Analysis
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Linearized Continuity Equation
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Oscillation Frequency
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NMI Growth time rc rb Δz
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Stabilization by Beam Temperature?
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Dispersion Relation
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Landau Damping
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LD from another view
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Resonance Effect
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Inhomogeneous Solution
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Oscillators Similtaneously Excited
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Oscillation Frequency
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NMI Growth time rc rb Δz
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Multipass BBU Instability
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BBU Theory
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Perturbation Theory Works
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CEBAF (Design) Simulations
Stable Bunch Number
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Close to threshold Bunch Number
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Unstable Bunch Number
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Chromatic (Landau) Damping
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