FEL2013 - List of Authors (Litvinenko, V.)

Paper

Title

Page

The Present Status of the Theory of the FEL-based Hadron Beam Cooling

52

A. Elizarov, V. Litvinenko
BNL, Upton, Long Island, New York, USA

Funding: Work supported by Brookhaven Science Associates, LLC under Contract No. DE-AC02-98CH10886 with the U.S. Department of Energy.
The coherent electron cooling (CeC)* device is one of the new facilities under construction in BNL. The CeC is a realization of the stochastic cooling with an electron beam serving as a pick-up and kicker. Hadrons generate electron density perturbations in the modulator section, then these perturbations are amplified in an FEL, and then, they accelerate (or decelerate) hadrons in the kicker by electric field with respect to their velocities. Here we present the theoretical description of the modulator sector**,***, where the electron density perturbations are formed and our new results on the time evolution of these perturbations in the FEL section, where they are amplified.
* V. N. Litvinenko, Y. S. Derbenev, Phys. Rev. Lett. 102, 114801 (2009).
** A. Elizarov, V. Litvinenko, G. Wang, IPAC'12, weppr099 (2012).
*** A. Elizarov, V. Litvinenko, IPAC'13, mopwo088 (2013).

MOPSO81

Broad-band Amplifier Based on Two-stream Instability

144

G. Wang, Y.C. Jing, V. Litvinenko
BNL, Upton, Long Island, New York, USA

A broadband FEL amplifier is of great interests for short-pulse generation in FEL technology as well as for novel hadron beam cooling technique, such as CeC. We present our founding of a broadband amplification in 1D FEL based on electron beam with two energy peaks and a strong space charge forces. We present the optimization of such amplifier and connect its origin to the two-stream instability in electron plasma. In this work, we study how the two-stream instability affects the FEL process and consider various applications in amplifying short spikes of electron current modulation.

WEOCNO01

Simulation Studies of FEL Green Function and Its Saturation

Y.C. Jing, Y. Hao, V. Litvinenko, G. Wang
BNL, Upton, Long Island, New York, USA

FEL amplifiers can be used for a number of applications ranging from the HGHG [1] , the coherent seed amplifying [2] or amplifier in Coherent electron Cooler [3]. Linear response of an FEL amplifier can be described using its Green function. In this paper we present results of detailed studies of the evolution and saturation of the Green function in FEL as function of its length. We are using time resolved mode of the code Genesis [4] for these studies, which include delta-function like seed and shot noise in electron beam. We simulate a statistically representative set of initial shot noise with and without the seed, and extract the Green function amplitude and phase evolution, as well as their fluctuation. We present results for three spectral ranges: the IR, the visible and the soft X-rays. We summarize our finding and compare them with a simple theoretical formula.
[1] L.H. Yu et al., science, 289 (2000)
[2] J. Feldhaus et al., NIMA, 1997
[3] V. N. Litvinenko et al., Phys. Rev. Lett. 102, 114801 (2009)
[4] S.Reiche, Genesis 2.0

Slides WEOCNO01 [0.479 MB]

Paper	Title	Page
MOPSO17	The Present Status of the Theory of the FEL-based Hadron Beam Cooling	52
	A. Elizarov, V. Litvinenko BNL, Upton, Long Island, New York, USA
	Funding: Work supported by Brookhaven Science Associates, LLC under Contract No. DE-AC02-98CH10886 with the U.S. Department of Energy. The coherent electron cooling (CeC)* device is one of the new facilities under construction in BNL. The CeC is a realization of the stochastic cooling with an electron beam serving as a pick-up and kicker. Hadrons generate electron density perturbations in the modulator section, then these perturbations are amplified in an FEL, and then, they accelerate (or decelerate) hadrons in the kicker by electric field with respect to their velocities. Here we present the theoretical description of the modulator sector,, where the electron density perturbations are formed and our new results on the time evolution of these perturbations in the FEL section, where they are amplified. V. N. Litvinenko, Y. S. Derbenev, Phys. Rev. Lett. 102, 114801 (2009). A. Elizarov, V. Litvinenko, G. Wang, IPAC'12, weppr099 (2012). * A. Elizarov, V. Litvinenko, IPAC'13, mopwo088 (2013).

MOPSO81	Broad-band Amplifier Based on Two-stream Instability	144
	G. Wang, Y.C. Jing, V. Litvinenko BNL, Upton, Long Island, New York, USA
	A broadband FEL amplifier is of great interests for short-pulse generation in FEL technology as well as for novel hadron beam cooling technique, such as CeC. We present our founding of a broadband amplification in 1D FEL based on electron beam with two energy peaks and a strong space charge forces. We present the optimization of such amplifier and connect its origin to the two-stream instability in electron plasma. In this work, we study how the two-stream instability affects the FEL process and consider various applications in amplifying short spikes of electron current modulation.

WEOCNO01	Simulation Studies of FEL Green Function and Its Saturation
	Y.C. Jing, Y. Hao, V. Litvinenko, G. Wang BNL, Upton, Long Island, New York, USA
	FEL amplifiers can be used for a number of applications ranging from the HGHG [1] , the coherent seed amplifying [2] or amplifier in Coherent electron Cooler [3]. Linear response of an FEL amplifier can be described using its Green function. In this paper we present results of detailed studies of the evolution and saturation of the Green function in FEL as function of its length. We are using time resolved mode of the code Genesis [4] for these studies, which include delta-function like seed and shot noise in electron beam. We simulate a statistically representative set of initial shot noise with and without the seed, and extract the Green function amplitude and phase evolution, as well as their fluctuation. We present results for three spectral ranges: the IR, the visible and the soft X-rays. We summarize our finding and compare them with a simple theoretical formula. [1] L.H. Yu et al., science, 289 (2000) [2] J. Feldhaus et al., NIMA, 1997 [3] V. N. Litvinenko et al., Phys. Rev. Lett. 102, 114801 (2009) [4] S.Reiche, Genesis 2.0
	Slides WEOCNO01 [0.479 MB]