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A reaction microscope ia a powerfull tool which
allows the complete kinematical analysis of all charged particles
(ions and electrons) from a molecular reaction induced for example
by laser radiation. Coupling a reaction microscope to a high order
harmonic source driven by intense fsec laser pulses opens the doorway
to the analysis of extremely fast electronic processes in molecules
on a sub-fsec time scale in great detail. In order to exploit the
enormous possibilities of such a setup it is essential to be able
to stabilize delay lines used in typical pump-probe experiments
for long time intervals (many hours) to better than about 20 attosec.
In terms of the wavelength l of the laser pulses driving the high
order harmonic source this means long term interferometric stability
to better than l/100. We implemented a setup capable of reaching
the required stability and demonstrated the delay stability by analysing
an attosecond pulse train in the extreme ultraviolet (XUV) spectral
range using the RABITT
(resolution of attosecond beating by interference of two-photon
transitions) method [M.
Böttcher et al.].
Our experimental setup which combines
a high order harmonic source with a reaction microscope. A delay
line which allows to delay the XUV harmonic pulses with respect
to infrared laser pulses is made up by the split mirror. The center
part reflects the XUV harmonic radiation and the annular part the
infrared radiation which generates the harmonics. The split mirror
pair is part of an external interferometer which actively fixes
the relative position of the two mirror parts (for the details see
[M.
Böttcher et al.]).

High Harmonics - How are they generated?
The experimental setup shows
the generation schematically. A millimeter size cell filled with
the nonlinear medium, typically a noble gas, inside a vacuum chamber
is irradiated by an ultrashort near infrared focused laser pulse.
Harmonics are generated in the focal spot at light intensities of
~1014 W/cm2. Harmonics at odd multiples of
the driving laser frequency are generated. They exit the cell together
with the transmitted infrared (IR) beam. The IR light is then either
removed from the harmonics by a thin aluminium foil or single harmonics
are selected by a grating monochromater as shown in the experimental
setup and the figure below (from A.
L'Huillier and Ph. Balcou).

High harmonics - What are their characteristics?
A characteristic feature of the high harmonics
is that they are generated over a broad range of orders with nearly
constant intensity. This part of the spectrum forms the so-called
plateau. It is followed by a short cut-off region where the intensity
of the harmonics drops to a negligible value over only a few harmonic
orders. This behaviour can well be identified in the spectrum
above. The harmonic orders are coupled by a specific phase relation.
Under particular generation conditions this relation allows to superimpose
harmonic orders coherently. In this way it is possible to generate
a beam of XUV radiation which consists of a train of pulses separated
by half the period of the carrier wave of the driving laser radiation.
The width of the individual XUV pulses has been shown by several
research groups to reach down to ~0.1 fsec, i.e. significantly less
than the oscillation period of the driving radiation. A typical
train pulse we generated and reconstructed from a RABITT
scan with our setup is shown below (full line,
for details see [M.
Böttcher et al.]). The harmonic orders 11 - 17 contribute
to the pulse train shown. The individual pulses have a width of
~330 attosec.

Starting with an driving pulse which consists of
only few optical cycles it is even possible to generate single XUV
pulses through harmonic generation.
High harmonics - What is the generation mechanism?
The semiclassical model on the atomic scale:
In each optical half cycle of the driving laser radiation the electric
field of the light wave rises to a strength that allows an electron
bound to an atom in the generating medium to become electric field
ionized. This happens close to the maxima of the electric field
strength. Completely analogous to nonsequential double ionization
the free electron is first accelerated by the light electric field
away from the ion. Then the field changes sign, stops the electron
and accelerates it back to the ion core. When it returns back to
the ion it may have a substantial kinetic energy (depending on the
driving laser intensity up to several hundred eV). In the collision
with the ion core the electron recombines and emits a short wavelength
photon.

Emitted spectrum:
The emitted photon has an energy of the atomic ionization potential
plus the energy the recombining electron has gathered in the course
of its acceleration by the driving laser field. The periodicity
of the driving light wave demands that harmonic photons can be emitted
only at multiples of the fundamental driving frequency. Parity conservation
further restricts the harmonics to odd multiples of this frequency.
The harmonic radiation emitted by the individual atoms in the gaseous
nonlinear medium adds up coherently. The cutoff of the harmonic
spectrum is determined either by the intensity of the driving NIR
laser pulses or by the medium specific light intensity, where ionization
becomes saturated, whichever is higher.
Application of high harmonics in photo double
ionization studies
We have started to use single high order harmonics
of Ti:Sapphire laser radiation to study 1-photon and few-photon
two-color photo double ionization (PDI) of Xenon atoms near the
PDI threshold. This is done in an ideal way with our reaction
microscope. The harmonics we used have been generated in Argon
gas as nonlinear medium. A single harmonic with order in the range
between 17 (l = 47.65 nm) and 25 (l
= 32.4 nm) was selected from the beam of harmonic radiation by a
monochromator and directed into the reaction microscope. In the
reaction microscope a split off part of the NIR Ti:Sapphire laser
radiation was superimposed on the XUV harmonic beam to study the
two-color excitation processes. Synchronization in time of the XUV
and NIR pulses is achieved by a delay line.
1.) 1-Photon Photo Double Ionization of Xenon

In order to demonstrate the capabilities of the
setup we only show a few exemplary results. The graph above shows
the kinetic energy distribution for photoelectrons from 1-photon
PDI of Xenon. Only electrons detected together with doubly charged
xenon ions are included (experimental data: black curve). Here the
25th harmonic of the 810 nm radiation of the Ti:Sapphire
laser has been used to photo double ionize Xe. The colored lines
represent a decomposition of the measured spectrum according to
the different PDI mechanisms of Xe. Two mechanisms are present,
a direct and an indirect one. The direct PDI pathway yields two
photoelectrons which are emitted simultaneously in a highly correlated
way. They share the excess energy arbitrarily, leaving the the doubly
charged ion in one of several accessible final states (green curves).
On the indirect pathway Xe first looses one electron leaving Xe+
in a highly excited autoionizing Rydberg state beyond the PDI threshold.
Autoionization of this state results in PDI of Xe. The yellow curve
represents the kinetic energy distribution of the photoelectron
and the orange one that of the electron from the autoionization
step (the detailes of this experiment can be found in our publication).

The figure above shows the momentum correlation
of the two photoelectrons for the momentum components parallel to
the direction of polarization of the high harmonic radiation. As
is typical for a reaction microscope the momenta are determined
from the measured momentum of one of the photoelectrons and the
recoil momentum of the doubly charged Xe ion. The contours are given
for constant event counts per bin. The structure of the momentum
distribution (its deviation from rotational symmetry) points to
a correlated emission of the two photoelectrons. A back-to-back
emission is preferred.
2.) Few-Photon 2-Colour Photo Double Ionization
of Xenon
Pulse width of a selected harmonic (21st
harmonic)

The pulse width of the 21st harmonic
has been determined by 2-color PDI of Xenon using the XUV and the
NIR laser beams (see the experimental setup).
The energy of the XUV photons of this harmonic is not sufficient
for 1-photon PDI of Xe, further photons from the superimposed NIR
laser beam (at least one) have to be absorbed for PDI. This allows
a cross-correlation measurement of the pulse width of the high harmonic
pulses by determining the Xe++ ion yield as a function
of the delay of the NIR pulses with respect to the harmonic pulses
(see the figure above). When the harmonic pulse arrives after the
NIR pulse no Xe++ ions are formed. The Xe++
yield increases when the pulses start to overlap. When the NIR pulse
follows the harmonic pulse the Xe++ ion yield becomes
constant. The rising part of the curve can be used to determine
the XUV pulse width to be approximately 2.8 psec. This pulse width
is completely determined by the monochromator used to select one
harmonic. The Xe++ ion yield stays at a constant level
different from zero when the NIR pulse follows the harmonic pulse
because the main PDI pathway is stepwise via excited states of the
Xe+ ion which are populated by the XUV pulse. They live
for a time long compared to the delay times used for the NIR laser
pulse.
Electron kinetic energy distributions

As an example the figure above shows the photoelectron
kinetic energy distribution for 2-color PDI of Xenon using the 17th
harmonic and the NIR Ti:Sapphire laser pulses focused to a light
intensity of ~1 x 1013 W/cm2 within the XUV
beam. The spectrum for single ionization of Xe by absorption of
one XUX photon is shown (SI) and the PDI spectrum (DI). PDI at this
XUV wavelength needs the absorption of at least 5 photons of the
NIR radiation in adition to the XUV photon.
PDI is mainly sequential at this XUV wavelength.
First, one XUV photon is absorbed leaving Xe+ in an excited
state. As can be seen in the (SI) spectrum a state with a 5s-shell
hole [5s(5p)6] or the accompanying satellites [(5s)2(5p)5]
may become populated in this first step. Subsequently, the NIR pulse
photoionizes these excited Xe+ states by multiphoton
absorption leaving Xe++ in one of the [(5s)2(5p)4]
open shell fine structure states. A qualitative analysis of the
PDI spectrum shows that mainly the minimum number of NIR photons
is absorbed for PDI. If at all only a small above threshold ionization
contribution is found. One of the two low energy peaks in the PDI
spectrum stems from XUV single ionization of Xe the other one can
be attributed to NIR multiphoton ionization of Xe+ excited
states. They show completely different angular distributions. An
important fact is, that the [5s(5p)6] 5s-shell hole state
does not contribute to PDI. This means, a filling of the 5s-hole
during multiphoton ionization is not possible. The full details
of this experiment can be found in our publication.
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