Download - Feasibility of X-ray Cherenkov Diffraction radiation for beam diagnostics of linear accelerators
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Feasibility of X-ray Cherenkov Diffraction radiation for beam
diagnostics of linear acceleratorsA.S. Konkov, A.P. Potylitsyn, A.S. Gogolev, Tomsk Polytechnic
University
P.V. Karataev, JAI at Royal Holloway, University of London
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Introduction
R(t)
O z(t) ( ) 1cosθ
( ) βc n tR t
z t vt n
Cherenkov Radiation is generated whenever the charged particle velocity is larger than the phase velocity of light
Is there Cherenkov radiation in X-ray region?
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Carbon Dielectric Permittivity
−δ
η K-edge
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Geometry
X-Ray ChTR
X-Ray ChDR
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Theoretical ApproachThe theoretical approach is based on the method of polarization currents. For a non-magnetic medium the density of the polarization currents in a right hand side of the Maxwell’s equations
where conductivity is
The field of the Polarization Radiation (PR) emitted by medium atoms excited (polarized) by the external field of the passing particle moving rectilinearly and with constant velocity in a substance (or in its vicinity) can be represented as a solution of Maxwell equations
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X-Ray Cherenkov Transition Radiation
http://ibic2013.org/prepress/html/sessi0n.htm
WEPF36
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Intensity vs observation angle θ and thickness d
γ = 240ћω = 284 eVα = 0φ = π
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Intensity vs observation angle θ and thickness d
γ = 10ћω = 284 eVα = 0φ = π
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Oblique Incidence
γ = 24, ћω = 284 eV, d = 5 μm, α = 5°, φ = π
ChR
TR
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X-Ray Cherenkov Diffraction Radiation
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Intensity vs observation angle θ and thickness dγ = 240ћω = 284 eVα = 0h = 1 μmφ = π
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Intensity vs observation angle θ and thickness dγ = 10ћω = 284 eVα = 0h = 0.1 μmφ = π
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Intensity vs observation angle θ for different photon energies
γ = 240d = 5 μmα = 0h = 1 μmφ = π
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Intensity vs observation angle θ for different electron energies
d = 5 μmα = 0h = 0.1 μmφ = π
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Oblique Incidence
γ = 240, ћω = 284 eV, d = 5 μm, α = 3°, h = 1 μm, φ = π
ChRDR
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Intensity vs observation angle θ for different incidence angles
γ = 240 ћω = 284 eV d = 5 μm h = 1 μmφ = π
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Conclusion
The model based on Polarization Current method agrees with other models for given beam parameters and approximations;
The Cherenkov Radiation is highly monochromatic in X-ray wavelength range;
The Angular distribution can be used to measure the beam energy with 10% accuracy;
In the energy range of γ > 100 the Polarization Radiation can be used to determine the beam angular divergence;
A real application for beam diagnostics is yet to be estimated!
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Thank you for your attention!