P. Piot, ASTA users’ and PAC meeting 1 ASTA Linac Beamline configurations & capabilities presented by P. Piot 1,2 based on work by C. Prokop 1 , D. Mihalcea 1 , F. Lemery 1 , M. Church 2 , and collaborations with B. E. Carlsten 3 , and P. Stoltz 4 1 Northern Illinois University, 2 Fermilab, 3 Los Alamos National Laboratory, 4 Tech-X corp. Credits: extensive use of beam-dynamics simulation codes provided by M. Borland (ANL), K. Flottmann, M Dohlus (DESY), J. Qiang and R. Ryne (LBNL)
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P. Piot, ASTA users’ and PAC meeting
1
ASTA Linac Beamline configurations & capabilities
presented by P. Piot1,2 based on work by C. Prokop1, D. Mihalcea1,
F. Lemery1, M. Church2, and collaborations with B. E. Carlsten3, and P. Stoltz4
1 Northern Illinois University, 2 Fermilab, 3 Los Alamos National Laboratory, 4 Tech-X corp.
Credits: extensive use of beam-dynamics simulation codes provided by M. Borland (ANL), K. Flottmann,
M Dohlus (DESY), J. Qiang and R. Ryne (LBNL)
Introduction
P. Piot, ASTA users’ and PAC meeting 2
• Ultimately variable energy from ~50 (possibly lower) to ~800 MeV,
CAV39 leads to long tail (good for sampling wakes – see Lemery’s talk)
• possibility to combine with disper- sive scarping (see Thangaraj’s talk)
• use of CAV39 to impart controlled nonlinearities (later stage)
P. Piot, ASTA users’ and PAC meeting 10
Q= 3.2 1.0 0.2 0.02 nC
afte
r BC
1 b
efor
e B
C1
C. P
rokop, IPAC
11
P. Piot, P
RL 2012
CAV39 OFF
CAV39 ON varied phase/amplitude
P. Piot, FLASH Accelerator workshop, Oct 4th, 2011 11
Generation of a witness population • Witness bunch produced
with a birefringent crystal • Drive/witness hierarchy
preserve downstream of BC1 • Preliminary experiments plan-
ned at A0/HBESL
to cathode
α-BBO
θ incoming uv laser pulse
L
δτ
drive
witness
GUN EXIT
drive
witness
AFTER BC1
CAV39 ON
EEX-based bunch temporal shaping
• emittance exchanger (EEX) could be used to shape the bunch current profile (bunch train, ramped bunches, …)
• 1st experiment planned w. Los Alamos to explore performance of pulse shaper
• need SC cavities to exploit multi-bunch capabilities
P. Piot, ASTA users’ and PAC meeting 12
P. Piot, A
AC
08, P. Piot, P
RS
TAB
2011, Y.-E S
un PR
L2010, C. P
rokop, IPAC
13]
(εx, εz) = (10, 1) µm (εx, εz) = (1, 10) µm
See
als
o pr
opos
al/ta
lk fr
om E
. Sim
akov
Ultra-low-emittance low-charge beams
• small laser spot on photocathode or field- emitter cathodes lead to extremely small emit- tances (sub-10-nm)
• produced beam are chal- lenging to diagnose with ASTA nominal diagnostics
• Field-emission with gated cathodes could enable the production of low-charge bunches repeated at 1.3 GHz with 1 ms!
P. Piot, ASTA users’ and PAC meeting 13
C. B
rau, SR
N (2012), W
. Gabella N
IMB
(2013), D. M
ihalcea, Phys. S
cript. (2013) S
ee re
cent
exp
erim
ent
P. M
usum
ecci
, PR
STA
B 2
012)
100% 95%
85%
90%
200 fC from field emitter
C. B
rau,
B. C
hoi V
ande
rbilt
Summary
• ASTA will provide beams within a vast parameter space, • Some of the advanced phase-space manipulations
pioneered at Fermilab’s A0 photoinjector are integral part of the design (flat beam) or will be installed early (EEX),
• Low-energy chicane-based bunch compression is not optimal but viable, at a later stage (after ACC1 installed), a second stage compressor will be added,
• Beam-dynamics performances of ASTA should be able to support most of the proposed experiments,
• We will be glad to collaborate and/or provide detailed calculations in support of your experiment [eventually all simulations files will be posted on ASTA web page so user can freely carry these calculations]