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An Ultrafast UV Pulse Shaper for Photochemistry

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Title: An Ultrafast UV Pulse Shaper for Photochemistry


1
An Ultrafast UV Pulse Shaper for Photochemistry
Coherent control using the pump probe method
Abigail Nunn Department of Chemistry,
UCL CoCoChem Graduate Student Meeting University
of Birmingham 24th April 2008
2
Dual array liquid crystal spatial light modulator
  • SLMs pulse shaping in the visible and near IR
    gives higher resolution than AOPDF
  • Direct pulse shaping in the UV (AOPDF and MEMS)
    is still in its infancy
  • Shaping in the UV is more difficult, generally
    requires a nonlinearlity after shaping indirect
    shaping
  • After the pulse shaper, the light can be
    converted to the UV by SFG (Nuernberger et al.)
  • OR SHG (Our choice). The pulse is frequency
    doubled in a 100 mm BBO crystal

New phase and amplitude high resolution pulse
shaper, Monmayrant et al., Rev. Sci. Instrum. 75,
2668 (2004).
Generation of shaped ultraviolet pulses at the
third harmonic of titanium-sapphire femtosecond
laser radiation, Nuernberger et al., Appl. Phys.
B. 88, 519 (2007).
3
Pulse shaper set-up
Folded near Littrow Geometry
Traditional 4f Zero Dispersion geometry
4
UV shaped pulse characterisation
  • 640 pixel dual array pulse shaper therefore, we
    can make pulses up to 7 ps long before replicas
    appear, from an input pulse of 35 fs at the
    transform limit
  • Our pulses may be quite weak, 1 mJ, hence
    sensitivity important
  • We want to be able to characterise all possible
    phase and amplitude pulse shapes
  • We need a characterisation method with fast
    feedback to help us understand the doubling
    process
  • SPIDER phase retrieval will fail if the phase
    varies too quickly, and spectral interferometry,
    using a reference pulse, is difficult if we shape
    to very large (ps) durations
  • We cannot make a FROG measurement of a 254 nm UV
    pulse with a frequency doubling crystal

5
Characterisation
  • Our solution characterise an unshaped reference
    pulse using FROG method, and then use this to
    characterise the UV light in an XFROG

E(t)
795 nm
Esignal(w,t)
Eg(tt)
t
398 nm
795 nm
Nonlinear medium
SHG crystal
Commercial instrument (GRENOUILLE)
Strong 795 nm will amplifies weak shaped UV pulse
6
FROG trace inversion
The FROG error is measured as the difference
between this and the experimental trace, and is
iteratively reduced
7
Our shaping and characterisation experiment design
OPA
Amplifier
Chamber
Delay line
Doubling crystal
SLM
XFROG
Grenouille
We use a thin crystal for the XFROG (10 mm), and
we use the chamber to find time zero.
8
Unshaped Pulses
1604085
Time / fs
Wavelength / nm
Temporal FWHM 90 fs Spectral FWHM 1 nm the
minimum FROG error is 0.008
9
Shaped Pulses pulse pairs
?
Frequency doubling
FT
??
?t ??????
t
??
Frequency doubling of phase-modulated, ultrashort
laser pulses, Hacker et al., Appl. Phys. B 73,
273 (2001).
10
Shaped Pulses pulse pairs
Dt 600 fs
Dt 800 fs
Dt 2600 fs
Dt 1800 fs
11
Shaped Pulses sine functions
Phase that is a sine function will double to give
an intensity sine function
12
Further work
  • Characterise the 508 nm shaped light directly
    using an 508 nm 795 nm SFG XFROG

13
Acknowledgements
Dorian Parker
Dr Russell Minns
Prof Helen Fielding
All the rest of the Fielding group
Thank you for listening!
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