30
Analytical calculation of the spectral-angular characteristics of coherent Smith-Purcell radiation generated by the short bunches with THz repetition rate Leonid Sukhikh

Leonid Sukhikh

  • Upload
    rangle

  • View
    65

  • Download
    0

Embed Size (px)

DESCRIPTION

Analytical calculation of the spectral-angular characteristics of coherent Smith-Purcell radiation generated by the short bunches with THz repetition rate. Leonid Sukhikh. Contents. Introduction Polarization radiation theory Super-radiant Smith-Purcell radiation model Calculation results - PowerPoint PPT Presentation

Citation preview

Page 1: Leonid Sukhikh

Analytical calculation of the spectral-angular characteristics of coherent Smith-Purcell radiation generated by the short bunches with THz repetition rateLeonid Sukhikh

Page 2: Leonid Sukhikh

ContentsIntroductionPolarization radiation theorySuper-radiant Smith-Purcell

radiation modelCalculation resultsConclusion

Page 3: Leonid Sukhikh

INTRODUCTION

Page 4: Leonid Sukhikh

Coherent Radiation from a single bunchCoherent radiation from a single

bunch:

Bunch form-factor:

Page 5: Leonid Sukhikh

Gaussian form-factors

Page 6: Leonid Sukhikh

~0.2ps ~1ps

Coherent Radiation from a train of bunches

Page 7: Leonid Sukhikh

CR spectrum

Radiation line width is proportional to Nb-1

Page 8: Leonid Sukhikh

Gaussian form-factors for several bunches

Page 9: Leonid Sukhikh

Frequency-locked CTR

Page 10: Leonid Sukhikh

Smith-Purcell Radiation

Page 11: Leonid Sukhikh

Frequency-locked CSPR

Page 12: Leonid Sukhikh

Bunched CSPR power measurement

Page 13: Leonid Sukhikh

Bunched CSPR power measurement

Bunch charge 4.67 pC

Page 14: Leonid Sukhikh

Smith-Purcell radiation models

Numerical solution of integral equation

Van den Berg model

(based on grating theory)

Kesar model

Induced currents

Surface currents model

Resonant diffraction radiation

model

Polarization radiation

modelIncludes

It is a big challenge to compare all models with known experimental data

and to find/create the best one

Page 15: Leonid Sukhikh

POLARIZATION RADIATION THEORY

Page 16: Leonid Sukhikh

Polarization radiation

Polarization

radiation

Transition radiation

Diffraction radiationSmith-Purcell

radiationCherenkov radiation

Page 17: Leonid Sukhikh

Theory 1Polarization radiation theory

was developed by D. V. Karlovets and A.P. Potylitsyn:

1. D.V. Karlovets and A.P. Potylitsyn, JETP Lett. 2009, Volume 90, Number 5, Pages 326-331

2. D. V. Karlovets, JETP, 2011, Volume 113, Number 1, Pages 27-45

Page 18: Leonid Sukhikh

For non magnetic media a polarization current is a linear function of the full field

where:

Maxwell equations may be written as:

Unwanted term

Theory 2

Page 19: Leonid Sukhikh

For the simplest case of the flat vacuum-medium boundary:

where - Surface normal

Due to boundary conditions:

The unwanted term disappears.

And

Theory 3

Page 20: Leonid Sukhikh

Theory 3The exact solution of the Maxwell equations may be

written as following:

where

This is exact field of polarization radiation inside the target with arbitrary permittivity. Additional manipulations are required to find the field outside the target. One should use the reciprocity theorem and Fresnel coefficients.

Page 21: Leonid Sukhikh

SUPER-RADIANT SMITH-PURCELL RADIATION MODEL

Page 22: Leonid Sukhikh

Smith-Purcell radiation modelIn the case of ideal-conducting thin grating the

radiation field in far field assumption may be written as:

Page 23: Leonid Sukhikh

Smith-Purcell radiation spectrum

Parameter ValueElectron energy, Ee

10 MeV

Grating period, d 300 umNumber of strips, N 101

Impact-parameter, h 1 mm

Observation angle,

On the figure

Microbunch length, 0

# of microbunches, Nb

1

Distance between microbunches, rf

-

Smith-Purcell radiation spectrum

Page 24: Leonid Sukhikh

Smith-Purcell radiation gain due to several microbunches

Parameter ValueElectron energy, Ee

10 MeV

Grating period, d 300 umNumber of strips, N 101

Impact-parameter, h 1 mm

Observation angle,

90 degree

Microbunch length, 0

# of microbunches, Nb

On the figure

Distance between microbunches, rf

300 um

Smith-Purcell radiation spectrum

Page 25: Leonid Sukhikh

Radiation gain strongly depends on bunching frequency…

Parameter ValueElectron energy, Ee

10 MeV

Grating period, d 300 umNumber of strips, N

101

Impact-parameter, h

1 mm

Observation angle,

90 deg

Microbunch length,

0

# of microbunches, Nb

10

Distance between microbunches, rf

On the figure

Smith-Purcell radiation spectrum

Page 26: Leonid Sukhikh

Tilted grating For the first time was calculated by P. Karataev et

al.

The developed model allows calculation of spectral-angular parameters of super-radiant Smith-Purcell radiation generated by a tilted grating

Page 27: Leonid Sukhikh

Line shiftParameter ValueElectron energy, Ee

10 MeV

Grating period, d 300 umNumber of strips, N 101

Impact-parameter, h 1 mm

Observation angle, 90 degMicrobunch length, 0

# of microbunches, Nb

1

Distance between microbunches, rf

-

Page 28: Leonid Sukhikh

CONCLUSION

Page 29: Leonid Sukhikh

ConclusionSmith-Purcell radiation intensity

significantly increases due to beam microbunching at the frequencies that correspond to the microbunching frequency.

Microbunching frequency control and diagnostics is really important.

One may try to use the grating tilt for such control.

Page 30: Leonid Sukhikh

THANK YOU FOR YOUR ATTENTION