Simulation of inverse Compton scattering and its implications on the scattered linewidth
Abstract
Rising interest in inverse Compton sources has increased the need for efficient models that properly quantify the behavior of scattered radiation given a set of interaction parameters. The current state-of-the-art simulations rely on Monte Carlo-based methods, which, while properly expressing scattering behavior in high-probability regions of the produced spectra, may not correctly simulate such behavior in low-probability regions (e.g. tails of spectra). Moreover, sampling may take an inordinate amount of time for the desired accuracy to be achieved. Here in this article, we present an analytic derivation of the expression describing the scattered radiation linewidth and propose a model to describe the effects of horizontal and vertical emittance on the properties of the scattered radiation. We also present an improved version of the code initially reported in Krafft et al. [Phys. Rev. Accel. Beams 19, 121302 (2016)], that can perform the same simulations as those present in cain and give accurate results in low-probability regions by integrating over the emissions of the electrons. Finally, we use these codes to carry out simulations that closely verify the behavior predicted by the analytically derived scaling law.
- Authors:
- Publication Date:
- Research Org.:
- Thomas Jefferson National Accelerator Facility (TJNAF), Newport News, VA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), Nuclear Physics (NP)
- OSTI Identifier:
- 1423922
- Alternate Identifier(s):
- OSTI ID: 1427019
- Report Number(s):
- JLAB-ACP-18-2669; DOE/OR/23177-4379
Journal ID: ISSN 2469-9888; PRABCJ; 030701
- Grant/Contract Number:
- AC05-06OR23177
- Resource Type:
- Published Article
- Journal Name:
- Physical Review Accelerators and Beams
- Additional Journal Information:
- Journal Name: Physical Review Accelerators and Beams Journal Volume: 21 Journal Issue: 3; Journal ID: ISSN 2469-9888
- Publisher:
- American Physical Society
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 43 PARTICLE ACCELERATORS
Citation Formats
Ranjan, N., Terzić, B., Krafft, G. A., Petrillo, V., Drebot, I., and Serafini, L. Simulation of inverse Compton scattering and its implications on the scattered linewidth. United States: N. p., 2018.
Web. doi:10.1103/PhysRevAccelBeams.21.030701.
Ranjan, N., Terzić, B., Krafft, G. A., Petrillo, V., Drebot, I., & Serafini, L. Simulation of inverse Compton scattering and its implications on the scattered linewidth. United States. https://doi.org/10.1103/PhysRevAccelBeams.21.030701
Ranjan, N., Terzić, B., Krafft, G. A., Petrillo, V., Drebot, I., and Serafini, L. Tue .
"Simulation of inverse Compton scattering and its implications on the scattered linewidth". United States. https://doi.org/10.1103/PhysRevAccelBeams.21.030701.
@article{osti_1423922,
title = {Simulation of inverse Compton scattering and its implications on the scattered linewidth},
author = {Ranjan, N. and Terzić, B. and Krafft, G. A. and Petrillo, V. and Drebot, I. and Serafini, L.},
abstractNote = {Rising interest in inverse Compton sources has increased the need for efficient models that properly quantify the behavior of scattered radiation given a set of interaction parameters. The current state-of-the-art simulations rely on Monte Carlo-based methods, which, while properly expressing scattering behavior in high-probability regions of the produced spectra, may not correctly simulate such behavior in low-probability regions (e.g. tails of spectra). Moreover, sampling may take an inordinate amount of time for the desired accuracy to be achieved. Here in this article, we present an analytic derivation of the expression describing the scattered radiation linewidth and propose a model to describe the effects of horizontal and vertical emittance on the properties of the scattered radiation. We also present an improved version of the code initially reported in Krafft et al. [Phys. Rev. Accel. Beams 19, 121302 (2016)], that can perform the same simulations as those present in cain and give accurate results in low-probability regions by integrating over the emissions of the electrons. Finally, we use these codes to carry out simulations that closely verify the behavior predicted by the analytically derived scaling law.},
doi = {10.1103/PhysRevAccelBeams.21.030701},
journal = {Physical Review Accelerators and Beams},
number = 3,
volume = 21,
place = {United States},
year = {Tue Mar 06 00:00:00 EST 2018},
month = {Tue Mar 06 00:00:00 EST 2018}
}
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https://doi.org/10.1103/PhysRevAccelBeams.21.030701
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Cited by: 23 works
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Works referencing / citing this record:
Compensation of non-linear bandwidth broadening by laser chirping in Thomson sources
journal, August 2018
- Maroli, C.; Petrillo, V.; Drebot, I.
- Journal of Applied Physics, Vol. 124, Issue 6
Inverse Compton radiation: a novel x-ray source for K-edge subtraction angiography?
journal, September 2019
- Paternò, G.; Cardarelli, P.; Gambaccini, M.
- Physics in Medicine & Biology, Vol. 64, Issue 18
High-brilliance, high-flux compact inverse Compton light source
journal, August 2018
- Deitrick, K. E.; Krafft, G. A.; Terzić, B.
- Physical Review Accelerators and Beams, Vol. 21, Issue 8