Author: Sergeeva, D.Yu.
Paper Title Page
TUPSB28 X-ray Thomson Inverse Scattering from Periodically Modulated Laser Pulses 283
 
  • D.Yu. Sergeeva, A.A. Tishchenko
    MEPhI, Moscow, Russia
  • D.Yu. Sergeeva
    BelSU/LRP, Belgorod, Russia
  • D.Yu. Sergeeva, A.A. Tishchenko
    NRC, Moscow, Russia
  • A.A. Tishchenko
    BNRU, Belgorod, Russia
 
  Funding: This work is performed within the project supported by the Russian Foundation for Basic Research (RFBR), grant # 19-29-12036
Being a compact source of x-rays based on the Thomson backscattering Thomson source has potential to be used in medicine and biology and in other area where narrow band x-ray beams are essential. We suggest and investigate theoretically the idea to use laser pulses modulated with a short period in Thomson backscattering. The coherent radiation is obtained with intensity proportional to the squared number of micro-pulses in the whole laser pulse.
 
DOI • reference for this paper ※ doi:10.18429/JACoW-RuPAC2021-TUPSB28  
About • Received ※ 23 September 2021 — Accepted ※ 29 September 2021 — Issued ※ 21 October 2021  
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TUPSB29 Geant4 for Inverse Compton Radiation Source Simulations 286
 
  • A.A. Savchenko, D.Yu. Sergeeva, A.A. Tishchenko
    MEPhI, Moscow, Russia
  • A.A. Savchenko, D.Yu. Sergeeva, A.A. Tishchenko
    NRC, Moscow, Russia
  • A.A. Savchenko, A.A. Tishchenko
    BNRU, Belgorod, Russia
  • D.Yu. Sergeeva
    BelSU/LRP, Belgorod, Russia
 
  Funding: This work was supported by the RFBR grant 19-29-12036.
Compton backscattering* is a promising mechanism for engineering of a bright, compact and versatile X-ray source: with dimensions being significantly smaller, the brightness of this source is comparable with that of synchrotron radiation. Nowadays, active researches are underway on various aspects of this phenomenon** aiming at increasing of radiation intensity and quality. In modern science, such kind of research is necessarily accompanied by the computer simulations. In this report, we are talking about creation and implementation of the Compton backscattering module into the Geant4 package***, which is the leading simulation toolkit in high-energy physics, accelerator physics, medical physics, and space studies. Created module of Compton backscattering has been implemented as a discrete physical process and operates with a fixed light target (a virtual volume with the properties of a laser beam), with which a beam of charged particles interacts. Such a description allows user to flexibly change necessary parameters depending on the problem being solved, which opens up new possibilities for using Geant4 in the studied area.
* K.T. Phuoc et al., Nat. Photonics 6, 308 (2012).
** A. Ovodenko et al., Appl. Phys. Lett. 109, 253504 (2016).
*** S. Agostinelli et al., Nucl. Instrum. Meth. A 506, 250 (2003).
 
DOI • reference for this paper ※ doi:10.18429/JACoW-RuPAC2021-TUPSB29  
About • Received ※ 17 September 2021 — Revised ※ 22 September 2021 — Accepted ※ 23 September 2021 — Issued ※ 02 October 2021
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WED07
Smith-Purcell Radiation in Prewave Zone for Diagnostics of Relativistic Electron Beams  
 
  • D.I. Garaev, D.Yu. Sergeeva, A.A. Tishchenko
    MEPhI, Moscow, Russia
  • D.I. Garaev, D.Yu. Sergeeva, A.A. Tishchenko
    NRC, Moscow, Russia
  • D.Yu. Sergeeva, A.A. Tishchenko
    BNRU, Belgorod, Russia
 
  Funding: The research was supported by Russian Ministry of Science and Higher Education (projects 0723-2020-0037 and FZWG-2020-0032) and by the Horizon 2020 grant No.871072 under CREM-LINplus Project.
Smith-Purcell radiation (SPR) is generated when an electron beam passes near a diffraction grating. Contrary to other methods (scintillator and transition radiation screens, wire scanners, etc.) SPR is not accompanied by the scattering of the beam¿s electrons on the target. This unique feature lets SPR provide non-destructive diagnostics of relativistic electron beams in linacs, including single shot measurements. Beam diagnostics is carried out by comparing experimental data with theoretical ones* and the following extraction of the beam parameters. Existing theoretical models are valid in the wave zone (but for the only exception of qualitative estimates in **), i.e. the detector must be placed at the distances much more than the wavelength of radiation multiplied by gamma2, where gamma is the Lorentz factor of the electrons. For ultrarelativistic beams (e.g., gamma = 100) the wave zone starts from 10 meters or more for the wavelength in mm and sub-mm ranges, which is completely out of realistic experimental conditions. Therefore, theory in prewave zone is needed. In this paper we solve this problem, developing the results published recently in ***. We analyze the radiation characteristics and also discuss how to use the results for the relativistic beam diagnostics.
*H.L. Andrews, et al., Phys. Rev. STAB 17, 052802 (2014).
**D.V. Karlovets, A.P. Potylitsyn, JETP Letters 84, 579 (2006).
***D.I. Garaev, et al., Phys. Rev. B 103, 075403 (2021).
 
slides icon Slides WED07 [4.698 MB]  
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