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@INPROCEEDINGS{Hlsenbusch:453471,
author = {Hülsenbusch, T. and Eichner, Timo and Lang, T. and
Winkelmann, L. and Hartl, I. and Maier, Andreas},
title = {{E}xperimental {R}esults on an {OPCPA} {S}eed {S}ystem for
a {L}aser-{P}lasma {A}cceleration {D}rive {L}aser},
reportid = {PUBDB-2020-05272},
year = {2019},
abstract = {Laser-plasma acceleration[1], among others[2,3],promises to
be a powerful technology for driving future compact light
sources. LUX, which is operated by University of Hamburg,is
such a laser-plasma accelerator. It is driven by the 200 TW
Ti:Sapphire double chirped pulse amplification (CPA)laser
system ANGUS, designed for long-term stability.The laser, as
well as the electron beam line,are integrated in a control
system, enabling continuous operation for many hours. This
has been demonstrated with day-long measurement runs where
electron beams with energies above 600 MeV and spontaneous
undulator radiation well below 9 nm were achieved [4]. From
the long runs large data sets can be collected to provide
reliable statistics. To extend the long-term operation
abilities of the laser system, and therefore the runtime of
the measurement campaigns, we are currently developing a new
front end for the ANGUS laser system.With the design
approach of the ANGUS laser system in mind we focus on the
long-term stability in the development of the new front-end.
The target is to reach 35 μJ pulse energy with 20 fs
transform limit at 1 kHz close to 800 nm central wavelength.
For these parameters and application optical parametric
chirped pulse amplification (OPCPA) is a suitable candidate.
It has been demonstrated that such systems can be operated
for more than a week with stable generation of high contrast
ultrafast pulses reaching down to the few cycle regime [5].A
measure to get to long-term stability is to use an
industrial grade Yb:KGW femto second laser as a common
source for white light generation(WLG)and pump for the
subsequent OPCPA stages. As only a fraction of the pulse
energy emitted by the drive laser is needed for WLG in a
bulk YAG crystal to provide the seed, complicated
synchronization schemes between two lasers can be
avoided.The major part of the pulse energy is converted in a
second harmonic generation (SHG)stage to be used as a pump
for the OPCPA stages. With headroom to spare the SHG stages
can be optimized for stable operation instead of maximum
conversion efficiency.Furthermore, without the necessity to
reach the few cycle regime, the OPCPA stages can be designed
for pulse energy stability instead of maximum amplification
bandwidth. Also the fact that no additional laser amplifier
stages are needed in the pump arm allows for a compact setup
that should be less sensitive on environmental influences.
Our approach is unique in the sense, that we focus on
maximum stability in parameters, rather than optimizing the
setup for minimum pulse lengths or efficiency.Currently we
are optimizing the SHG and the OPCPA stages for the
stability goals with a 3D+1 split step code.In parallel we
are setting up the first prototype OPCPA stage.We will
report on simulation as well as experimental results
regarding the SHG pump and the firstOPCPA stage with focus
on the achievable stability in pulse energy and spectral
parameters.[1] W.P. Leemanns et al. “GeV electron beams
from a centimetre-scale accelerator”, in Nature Physics 2,
696–699 (2006)[2] A-L. Calendron et al. “Laser system
design for table-top X-ray light source”,in High Power
Laser Science and Engineering 6: e12 (2018)[3] E. A. Peralta
et al.“Demonstration of Electron Acceleration in a
Laser-Driven Dielectric Micro-Structure”,Nature 503, 7474
(2013)[4] N. Delbos et al."LUX --A Laser-Plasma Driven
Undulator Beamline", Nucl. Instr. Meth. Phys. Res. A 909,
318 (2018)[5]R. Budriūnas et al."53 W average power
CEP-stabilized OPCPA system delivering 5.5 TW few cycle
pulses at 1 kHz repetition rate”, Opt. Express 25,
5797-5806 (2017)},
month = {Sep},
date = {2019-09-29},
organization = {Advanced Solid State Lasers, Vienna
(Austria), 29 Sep 2019 - 3 Oct 2019},
cin = {CFEL-LUX / FS-LA},
cid = {I:(DE-H253)CFEL-LUX-20160909 / I:(DE-H253)FS-LA-20130416},
pnm = {631 - Accelerator R $\&$ D (POF3-631)},
pid = {G:(DE-HGF)POF3-631},
experiment = {EXP:(DE-MLZ)NOSPEC-20140101},
typ = {PUB:(DE-HGF)24},
url = {https://bib-pubdb1.desy.de/record/453471},
}