IPAC2018 - List of Authors (Ranjan, N.)

Paper	Title	Page
TUPMF005	Simulation of Inverse Compton Scattering and Its Implications on the Scattered Linewidth	1254
SUSPF014	use link to see paper's listing under its alternate paper code
	N. Ranjan, B. Terzić ODU, Norfolk, Virginia, USA I. Drebot, L. Serafini Istituto Nazionale di Fisica Nucleare, Milano, Italy G.A. Krafft JLab, Newport News, Virginia, USA V. Petrillo Universita' degli Studi di Milano & INFN, Milano, Italy
	Funding: This paper is authored by Jefferson Science Associates, LLC under U.S. DOE Contract No. DE-AC05-06OR23177. Compton scattering, though first described some one hundred years ago, has recently experienced a surge of interest due to the search for energy sources that are capable of yielding low emission bandwidths. In particular, the desire for hard x-rays with energies greater than 10 keV has led to increased study of inverse Compton sources. The rise in interest concerning 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 of Monte Carlo-based methods, which may fail to properly model collisions of bunches in low-probability regions of the spectrum. Furthermore, the random sampling of the simulations may lead to inordinately high runtimes. Our methods can properly model behaviors exhibited by the collisions by integrating over the emissions of the electrons in the bunch in a lessened amount of time. Analytical simulations of Gaussian laser beams closely verify the behavior predicted by an analytically derived scaling law describing bandwidth of scattered radiation. Current affiliation of primary author (Nalin Ranjan) is Princess Anne High, Virginia Beach, VA 23452, USA.
DOI •	reference for this paper ※ https://doi.org/10.18429/JACoW-IPAC2018-TUPMF005
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Paper

Title

Page

TUPMF005

Simulation of Inverse Compton Scattering and Its Implications on the Scattered Linewidth

1254

SUSPF014

use link to see paper's listing under its alternate paper code

N. Ranjan, B. Terzić
ODU, Norfolk, Virginia, USA
I. Drebot, L. Serafini
Istituto Nazionale di Fisica Nucleare, Milano, Italy
G.A. Krafft
JLab, Newport News, Virginia, USA
V. Petrillo
Universita' degli Studi di Milano & INFN, Milano, Italy

Funding: This paper is authored by Jefferson Science Associates, LLC under U.S. DOE Contract No. DE-AC05-06OR23177.
Compton scattering, though first described some one hundred years ago, has recently experienced a surge of interest due to the search for energy sources that are capable of yielding low emission bandwidths. In particular, the desire for hard x-rays with energies greater than 10 keV has led to increased study of inverse Compton sources. The rise in interest concerning 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 of Monte Carlo-based methods, which may fail to properly model collisions of bunches in low-probability regions of the spectrum. Furthermore, the random sampling of the simulations may lead to inordinately high runtimes. Our methods can properly model behaviors exhibited by the collisions by integrating over the emissions of the electrons in the bunch in a lessened amount of time. Analytical simulations of Gaussian laser beams closely verify the behavior predicted by an analytically derived scaling law describing bandwidth of scattered radiation.
Current affiliation of primary author (Nalin Ranjan) is Princess Anne High, Virginia Beach, VA 23452, USA.

DOI •

reference for this paper ※ https://doi.org/10.18429/JACoW-IPAC2018-TUPMF005

Export •

reference for this paper using ※ BibTeX, ※ LaTeX, ※ Text/Word, ※ RIS, ※ EndNote (xml)