LINAC2016 - List of Authors (Ruan, J.)

Paper	Title	Page
MO2A02	Commissioning and Plans at IOTA/FAST
	D.R. Broemmelsiek, C.M. Baffes, C.I. Briegel, K. Carlson, B.E. Chase, D.J. Crawford, E. Cullerton, J.S. Diamond, N. Eddy, D.R. Edstrom, E.R. Harms, J.R. Leibfritz, A.H. Lumpkin, E. Prebys, J. Reid, J. Ruan, T. Sen, V.D. Shiltsev, G. Stancari, J.C.T. Thangaraj, R.M. Thurman-Keup, A. Valishev, A. Warner Fermilab, Batavia, Illinois, USA A. Halavanau, D. Mihalcea, P. Piot Northern Illinois University, DeKalb, Illinois, USA J. Hyun Sokendai, Ibaraki, Japan P. Kobak BYU-I, Rexburg, USA W.D. Rush KU, Lawrence, Kansas, USA
	The electron injector at IOTA/FAST is based on a 50MeV RF photoinjector and SRF 1.3 GHz cryomodule to accelerate beam up to 300 MeV. Photoinjector and Cryomodule (CM2) were commissioned separately. CM2 demonstrated world record accelerating gradient > 30MV/m in all cavities. Commissioning of the 50MeV RF photoinjector was successfully done recently. Results of commissioning, status and plans for IOTA/FAST are presented.
	Slides MO2A02 [6.248 MB]
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MOP106018	Measurement of the Transverse Beam Dynamics in a TESLA-type Superconducting Cavity	323
SPWR025	use link to see paper's listing under its alternate paper code
	A. Halavanau, P. Piot Northern Illinois University, DeKalb, Illinois, USA N. Eddy, D.R. Edstrom, A. Lunin, P. Piot, J. Ruan, N. Solyak Fermilab, Batavia, Illinois, USA
	Funding: US Department of Energy (DOE) under contract DE-SC0011831 with Northern Illinois University. Fermilab is operated by the Fermi Research Alliance LLC under US DOE contract DE-AC02-07CH11359. Superconducting linacs are capable of producing intense, ultra-stable, high-quality electron beams that have widespread applications in Science and Industry. Many project are based on the 1.3-GHz TESLA-type superconducting cavity. In this paper we provide an update on a recent experiment aimed at measuring the transfer matrix of a TESLA cavity at the Fermilab Accelerator Science and Technology (FAST) facility. The results are discussed and compared with analytical and numerical simulations.
DOI •	reference for this paper ※ https://doi.org/10.18429/JACoW-LINAC2016-MOP106018
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TUPLR015	Design of a Gamma-Ray Source Based on Inverse Compton Scattering at the Fast Superconducting Linac	503
	D. Mihalcea Northern Illinois University, DeKalb, Illinois, USA B.T. Jacobson, A.Y. Murokh RadiaBeam, Los Angeles, California, USA P. Piot, J. Ruan Fermilab, Batavia, Illinois, USA
	Funding: This work is sponsored by the DNDO via contract with NIU. A Watt-level average-power gamma-ray source is currently under development at the FermiLab Accelerator Science & Technology (FAST) facility. The source is based on the inverse Compton scattering of a high-brightness 300-MeV beam against a high-power laser beam circulating in an optical cavity. The back scattered gamma rays are expected to have photon energies up to 1.5 MeV. This paper discusses the optimization of the source, its performance and the main challenges ahead.
DOI •	reference for this paper ※ https://doi.org/10.18429/JACoW-LINAC2016-TUPLR015
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Paper

Title

Page

MO2A02

Commissioning and Plans at IOTA/FAST

D.R. Broemmelsiek, C.M. Baffes, C.I. Briegel, K. Carlson, B.E. Chase, D.J. Crawford, E. Cullerton, J.S. Diamond, N. Eddy, D.R. Edstrom, E.R. Harms, J.R. Leibfritz, A.H. Lumpkin, E. Prebys, J. Reid, J. Ruan, T. Sen, V.D. Shiltsev, G. Stancari, J.C.T. Thangaraj, R.M. Thurman-Keup, A. Valishev, A. Warner
Fermilab, Batavia, Illinois, USA
A. Halavanau, D. Mihalcea, P. Piot
Northern Illinois University, DeKalb, Illinois, USA
J. Hyun
Sokendai, Ibaraki, Japan
P. Kobak
BYU-I, Rexburg, USA
W.D. Rush
KU, Lawrence, Kansas, USA

The electron injector at IOTA/FAST is based on a 50MeV RF photoinjector and SRF 1.3 GHz cryomodule to accelerate beam up to 300 MeV. Photoinjector and Cryomodule (CM2) were commissioned separately. CM2 demonstrated world record accelerating gradient > 30MV/m in all cavities. Commissioning of the 50MeV RF photoinjector was successfully done recently. Results of commissioning, status and plans for IOTA/FAST are presented.

Slides MO2A02 [6.248 MB]

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

MOP106018

Measurement of the Transverse Beam Dynamics in a TESLA-type Superconducting Cavity

323

SPWR025

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

A. Halavanau, P. Piot
Northern Illinois University, DeKalb, Illinois, USA
N. Eddy, D.R. Edstrom, A. Lunin, P. Piot, J. Ruan, N. Solyak
Fermilab, Batavia, Illinois, USA

Funding: US Department of Energy (DOE) under contract DE-SC0011831 with Northern Illinois University. Fermilab is operated by the Fermi Research Alliance LLC under US DOE contract DE-AC02-07CH11359.
Superconducting linacs are capable of producing intense, ultra-stable, high-quality electron beams that have widespread applications in Science and Industry. Many project are based on the 1.3-GHz TESLA-type superconducting cavity. In this paper we provide an update on a recent experiment aimed at measuring the transfer matrix of a TESLA cavity at the Fermilab Accelerator Science and Technology (FAST) facility. The results are discussed and compared with analytical and numerical simulations.

DOI •

reference for this paper ※ https://doi.org/10.18429/JACoW-LINAC2016-MOP106018

Export •

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

TUPLR015

Design of a Gamma-Ray Source Based on Inverse Compton Scattering at the Fast Superconducting Linac

503

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

Funding: This work is sponsored by the DNDO via contract with NIU.
A Watt-level average-power gamma-ray source is currently under development at the FermiLab Accelerator Science & Technology (FAST) facility. The source is based on the inverse Compton scattering of a high-brightness 300-MeV beam against a high-power laser beam circulating in an optical cavity. The back scattered gamma rays are expected to have photon energies up to 1.5 MeV. This paper discusses the optimization of the source, its performance and the main challenges ahead.

DOI •

reference for this paper ※ https://doi.org/10.18429/JACoW-LINAC2016-TUPLR015

Export •

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