FEL2017 - List of Authors (Jacobson, B.T.)

Paper	Title	Page
MOP053	High Spectral Density Compton Back-Scattered Gamma-Ray Sources at Fermilab	174
	D. Mihalcea, A. Khizhanok, P. Piot Northern Illinois University, DeKalb, Illinois, USA B.T. Jacobson, A.Y. Murokh RadiaBeam, Santa Monica, California, USA P. Piot, J. Ruan Fermilab, Batavia, Illinois, USA
	A ~1 MeV gamma-ray source is planned to be built at Fermilab following the completion of the ~300 MeV superconducting linac. The high-energy photons are back-scattered from the interactions between electrons and high-intensity IR laser pulses. In this contribution, we discuss some of the experiment design challenges and evaluate the performances of the gamma-ray source. We expect the peak brilliance to be of the order of 10²² photons/s-(mm-mrad)²-0.1\% BW and the spectral density of the radiation in excess of 3x10⁵ photons/s/eV.
DOI •	reference for this paper ※ https://doi.org/10.18429/JACoW-FEL2017-MOP053
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Paper

Title

Page

High Spectral Density Compton Back-Scattered Gamma-Ray Sources at Fermilab

174

D. Mihalcea, A. Khizhanok, P. Piot
Northern Illinois University, DeKalb, Illinois, USA
B.T. Jacobson, A.Y. Murokh
RadiaBeam, Santa Monica, California, USA
P. Piot, J. Ruan
Fermilab, Batavia, Illinois, USA

A ~1 MeV gamma-ray source is planned to be built at Fermilab following the completion of the ~300 MeV superconducting linac. The high-energy photons are back-scattered from the interactions between electrons and high-intensity IR laser pulses. In this contribution, we discuss some of the experiment design challenges and evaluate the performances of the gamma-ray source. We expect the peak brilliance to be of the order of 10²² photons/s-(mm-mrad)²-0.1\% BW and the spectral density of the radiation in excess of 3x10⁵ photons/s/eV.

DOI •

reference for this paper ※ https://doi.org/10.18429/JACoW-FEL2017-MOP053

Export •

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