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HAL Id: jpa-00210263

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Submitted on 1 Jan 1986

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Electron spectroscopy study of single and double multiphoton ionization of strontium by visible

picosecond laser light

G. Petite, P. Agostini

To cite this version:

G. Petite, P. Agostini. Electron spectroscopy study of single and double multiphoton ionization of strontium by visible picosecond laser light. Journal de Physique, 1986, 47 (5), pp.795-808.

�10.1051/jphys:01986004705079500�. �jpa-00210263�

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Electron spectroscopy study of single and double multiphoton ionization

of strontium by visible picosecond laser light

G. Petite and P. Agostini

C.E.N. Saclay, Service de Physique, Atomes et Surfaces, 91191 Gif sur Yvette Cedex, France

(Reçu le 31 octobre 1985, accepti sous forme définitive le 24 janvier 1986)

Résumé.

2014

Les techniques de spectroscopie d’électrons ont été appliquées à l’étude de l’ionisation multiphotonique simple et double du strontium par des impulsions picosecondes de 1011 à quelque 1012 W cm-2, foumies soit par un laser Nd : Yag doublé en fréquence, soit par un laser accordable (à rhodamine 6G). Les spectres d’énergie

d’électrons montrent que l’ionisation multiphotonique simple laisse l’ion soit dans son état fondamental, par un processus à trois photons, soit après absorption d’un quatrième photon, dans un des premiers états excités. Des résonances à deux et trois photons sur des états à un ou deux électrons excités peuvent intervenir dans ces processus et créer une excitation importante du coeur. L’ionisation double apparaît essentiellement comme un processus

en deux étapes, dont la seconde peut avoir pour état initial un état excité de l’ion.

Abstract.

2014

Multiphoton single and double ionization of strontium was studied using electron spectroscopy techniques. Both a picosecond, frequency doubled Nd : Yag Laser and a picosecond rhodamine 6G Dye Laser

were used, with intensities ranging from 1011 W . cm- 2 to a few 1012 W . cm-2. Single MPI was shown to produce

ions in both the ground state (3 photon) and several low lying excited states, through a four photon process. Two and three photon resonances were observed, on singly and doubly excited states of the atom, resulting in an impor-

tant degree of core excitation. Double ionization was shown to be essentially a « stepwise » process which can involve excited states of the ion as the initial state of the second part of the process.

Classification

Physics Abstracts

32.80D - 32.80F - 32.80K

1. Introduction.

Multiphoton Ionization (MPI-[1] and references

therein) has long been studied, because it is the process which dominates the laser-atom interaction when high laser intensities are used. Most of the

emphasis has been put, in the past few years on the

study of MPI under very high laser intensities

(1011 W.cm-2 and above) for which new processes

can occur.

It was shown [2] that under such intensities an atom can absorb more than the number of photon

necessary for ionization, in a process known as

«Above Threshold Ionization » (ATI) leading to

the production of hot electrons. ATI was studied in the case of rare gases [2, 6] and caesium [7]. Both perturbative [8, 9] and non perturbative [10, 11]

approaches were considered in theoretical work.

In [7] a good agreement between experimental

results and a perturbative calculation was obtained.

In the case of rare gases, which deals with both

higher intensities and more complex atoms, such

comparisons are still out of hand.

The study of MPI processes under very high laser

intensities also led to the observation of multiple

ionization of atoms. It was observed in the case of

rare gases [12-15], alkaline earths [16-20] alkalis [21]

and rare earths [13, 22]. In several cases, double

ionization was observed at the same intensity where simple ionization occurs though being of a much higher order.

Here again different situations are encountered

depending on the type of atom considered. Rare gases, with a complete outer shell require very high

laser intensities. They were at the origin of the most impressive results concerning both the number of electrons ejected (up to the complete outer shell),

and the number of photon absorptions involved (a hundred and more). Clearly, for such high order

processes, the perturbative approach is not adequate

and new types of formalisms have to be developed.

A statistical approach of this problem [23] has been recently proposed and is one of the possible paths

towards a better understanding of these processes.

Alkaline earths on the other hand present a quite

different picture. They are easily ionized, involving

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01986004705079500

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processes of a lower order. Though the calculation of ionization probabilities is not easy, one can still

consider the perturbative approach as reasonably fit to

this problem. Moreover, in the case of strontium,

some specific ionization paths leading to double

ionization have been proposed [17, 20] and some observations seem to indicate that ATI can play an important role in double ionization. Resonances in the double ionization signal were observed which

were assigned to transitions in the ion spectrum whose initial state is an excited ion state which can

only be reached by absorption of extra photons.

However the electron spectra presented in proof

did not show the components implied by this inter-

pretation.

In this paper, we present electron energy spectra, and their variations with the laser wavelength, intensity and in some cases, polarization for single

and double ionization of strontium atoms by a

rhodamine 6G picosecond dye laser and a frequency

doubled Nd : Yag Laser. In addition we present

new observations of MPI in situations were multi-

photon excitation of either the atom or the ion

yields an excitation energy close to an ionization threshold. Last, we present new observations con-

cerning electrons which can be unambiguously assigned to a double ionization process. Besides

providing a decisive proof of the interpretations given in references [17, 20], we discuss the following

issues.

(i) ATI in a complex atom : how does it differ from ATI in a single electron atom; are the definitions and concepts used in a single electron atom still valid in the case of alkaline earths ? Can ATI lead to the

production of excited ion states ?

(ii) ATI and double ionization : what are the

relationships between these two « high order » pro- cesses ?

(iii) What are the most probable mechanisms leading to double ionization.

Section 2 is devoted to a theoretical discussion of the points mentioned above. Our aim is to give

clear definitions of the concepts to be used in this

paper rather than to present calculations correspond- ing to the results presented later

-

those are still

out of reach for the moment.

Section 3 will describe our experimental set up.

Our experimental results will be presented and

discussed in section 4 : electron energy spectra, and their variations with the laser wavelength, intensity and in some cases, polarization.

2. Theory.

In this part, our goals are the following :

(i) using the simplest possible model, we obtain predictions concerning some aspects of our experi-

ment which have not been so far considered in the literature.

(ii) clarify the terminology concerning the diffe- rent ionization processes involved in our experiment.

(iii) briefly discuss the issue of double ionization of strontium (direct or stepwise process).

The first two points of this discussion strictly deal

with single ionization of strontium.

2.1 SINGLE IONIZATION OF STRONTIUM.

-

Multipho-

ton ionization of alkaline earth has been the subject

of several theoretical publications these last years, the emphasis being put on the central question of

autoionization under strong laser field [24-26]. These

models all predict strong modifications of the Fano auto-ionization profile under high laser intensity.

Both single photon ionization [24] and MPI [25, 26]

were considered and a quite complete calculation in the case of strontium can be found in [26] in an attempt

to analyse experimental results reported in [27, 28].

However some of the features of our experiment are

not considered in these papers, and will be the subject

of this theoretical part. We use the resolvent operator formalism, as presented in [24], and later developed

in [25, 26].

The different couplings relevant to our experiment

are shown on figure 1. States of interest are : the

ground state I g) of energy E8, two continual I c1 ) and I c2 > (energies E1 and E2) and one auto-ionizing state I a > of energy E. lying between the ionization limits corresponding to continua I c, > and c2 >. We

use the dressed atom model and these states will be dressed respectively by n photons of the laser field

for I g), n - 3 photons for a ) and I c1), and

n - 4 photons for c2 ), etc.

Note that continual I cl > and I C2 > correspond to

different states of the core. For instance, in strontium,

Fig. 1. - Schematic representation of the couplings

involved in 3 and 4 photon ionization with a three photon

resonance on an auto-ionizing state.

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I ci ) is the continuum Ss, E1 ) and I C2 > could be

the continuum 4d, 82 > -

Energies of the dressed states thus are :

If Ha is the atomic Hamiltonian and Hf the field

Hamiltonian, these states are eigenstates of :

If we use the dipole approximation for the atom

field interaction, the total Hamiltonian of our system will be :

Where D is the dipole operator :

in which 8 is the electric field amplitude and E the polarization vector. V is the Coulomb interaction

responsible for the auto-ionization of) [ a ) and even- tually for configuration mixing of other states too.

We can then proceed as in references [24, 26] and compute the evolution operator U(t) of our system from the resolvent operator.

through the inversion integral

with

Couplings between I g) and I a >, I cl > or I c2 >

involve several photons so that it would be necessary to complete the atomic spectrum of figure 1 with a

set of non resonant intermediate states, as it was made in references [25, 26].

Instead we choose to represent the coupling between

the different states by effective interaction Hamilto- nian such as :

so that our interaction Hamiltonian writes :

Note that DC2g represents the coupling between I g ) and c2 ) through a set of non resonant auto-

ionizing states such as I a ), but does not include the

I c1 ) continuum. The coupling between the continua

I c1 > and c2 ) will be neglected as it was done in [24].

With the above definitions, the equations deter- mining the resolvent operator matrix elements are :

At time t

=

0, all the atoms are in the ground state I g >, so that the ionization rates in continual I cl >

and I c2 ) will be determined by I Ug,,(t) 12 aid I Ug-2(t) 12.

We are thus interested in GClg and G129’ which can be expressed, from equations (9. c) and (9. d) by :

Using these expressions in equations (9. a) and (9. b) we get :

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we then define :

which represent the shifts of statues I g > and I a > due to their interaction with the continua :

which are the widths of states I g > and [ a ) due to the same interactions, and :

which is a modified effective interaction between states I g > and I a >, as defined in [24] but with an additional

term due to continuum I c2 > which should be small compared to the others because of its higher order in the laser intensity.

System (II) then writes :

which yields :

Expressions which are strikingly similar to those obtained in the case of resonant multiphoton ionization

of hydrogenic atoms. We then obtain for GCIS and G,,,,, :

From this point on, the calculations have to be carried out numerically, but the physics of our system

is already apparent in these expressions.

Expression (17. a), which describes ionization in

continuum I c, > is made of two terms. The first one

describes direct ionization of I g > in I cl >, when the

second one describes the excitation of I a) followed by auto-ionization of I a) in I c, >. The interference between these two terms leads to the well known Fano profile. This result is identical to the one obtained in [24]. Because of the use of effective Hamiltonians it differs from the results of references [25, 261 : Stark

shift of the ground and auto-ionizing states due to one photon coupling with intermediate bound states are not apparent, and also the modification brought to VaC1 by a two photon coupling via the bound states

is missing. The latter could probably be taken into account by using a modified VaC1 instead of VaC1’ like

it was done in reference [26].

If we now consider expression (17. b) it is strikingly

identical to (17. a) apart from the fact that ionization

of a > is due to a dipole interaction instead of a

Coulomb interaction. The same result was obtained

in the case of resonant multiphoton ionization

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with a formalism sometimes referred to as « pseudo

auto-ionization » : : ionization in continuum I C2 > is

the result of interference between a resonant amplitude (Dc2a Dag) and a non resonant one (DC2g) in the same

way as ionization in I cl > results of an interference between a direct channel and the auto-ionizing one.

Considering expressions (17. a) and (17 . b) a few

remarks can be made.

(i) Expression (17. a), describing ionization to the first continuum is identical to the one obtained in [24]

when only one continuum is considered.

The only differences are in the position of the poles

which are slightly modified by the presence of c2 ),

and in one additional term in Dag which should be small if not negligible.

(ii) Considering ionization in upper continua, as

described by equation (17.b) it appears to be an

usual MPI process, involving a number of bound transitions and one bound-free transition. Since no

free-free transition is involved, and though absorption

of one photon above the lowest ionization threshold is necessary to reach continuum I c2), ATI is not involved, as it has sometimes been stated before [ 17, 20].

In this respect the acronym ATI can be somewhat

confusing in the case of two-electron atoms. It must be applied only to ionizing processes involving c - c

transitions inside the same continuum (I c1) or possibly I c2 >), that is without change of the excitation state of the « core » electron.

As a conclusion to this paragraph, we note that, apart from the high intensity effects already predicted

in auto-ionization, production of excited ion states can exhibit resonances on auto-ionizing states lying

between the two ionization limits in a way analoguous

to resonant multiphoton ionization. The same width should be measured on these resonances and in the usual auto-ionization in the lower continuum; because this width is determined by the poles imaginary parts, which are the same in (17. a) and (17. b) so that the intensity effects predicted in [25, 26] should be seen

in the production of excited ion states.

Note that because the dipole operator is mono- electronic, only resonances on states with the same core can appear in excited ion states production.

This is true of course only when configuration inter-

actions are neglected. In the opposite case, interesting

indications can be obtained in this way, on the impor-

tance of these interactions.

2.2 DOUBLE IONIZATION.

-

Multiple ionization has been repeatedly observed for about ten years now

[12-22, 27-29] and not much is known about the mechanisms leading to multiply charged ion produc-

tion. In the framework of perturbation theory, two apparently different mechanisms can lead to double ionization which will be discussed here :

(i) direct ionization : two electrons are simulta-

neously excited and ejected yielding a doubly charged

ion obtained directly from the neutral atom.

(ii) stepwise ionization : a singly charged ion is

obtained first, and a doubly charged ion results from

multiphoton ionization of this ion.

Thus far, the question of the competition between

these two processes has been considered as a central

one. It was recently considered in a paper [30] which thoroughly discusses this question in view of an application to two-photon ionization of helium.

The following discussion directly stems from the

conclusions of this paper, and only that part of the calculations which are necessary to the understanding

of the discussion will be reproduced.

We consider here, as in [30] and for the sake of

simplicity of the expressions, a two-photon double

ionization process, but the discussion can easily be generalized to a higher order process. We are thus interested in the case where an atom in its ground state g) of energy Eg can be doubly ionized by absorption of two photons of energy Ep, giving a doubly charged ion in its ground state 192 > and two

electrons with energies 81’ and 82 such that :

In the framework of lowest order perturbation theory, the probability of such a process can be expressed, by :

where I is the laser intensity, d the atomic dipole

operator and Ii) an intermediate state with energy E;.

In doing this, we of course neglect correlation for the continuum states.

We then note that d, being a monoelectronic opera- tor, can only couple g2, E1, G2 ) to states pertaining

to the continuum of simple ionization, that is of the

type I el, G1 >, our Ie1, G2 ) where I el > is one of the singly charged ion states (ground or excited), so that (19) yields.

This expression clearly describes the interferences between two series of time ordered two photon inter-

action diagrams representing the following process :

absorption of one photon by the atom in its ground

state yielding a singly charged ion and an electron of

energy s, (or P2), followed by an absorption of a

second photon resulting in ionization of the singly

(7)

charged ion, yielding another electron of energy 82

(resp. Ei). This shows that, in this framework, double

ionization is a sequential process, even if there is no

way to decide which electron has been emitted first.

With this in mind, two different cases have to be considered. Equation (12) reflects the fact that a limited range of electron energies can be obtained in such

processes, and different situations will occur depending

whether in the intermediate state, real ionic states can be reached with emission of an electron in this energy range, as schematised on figure 2.

If not (case A of Fig. 2), the intermediate states of

expression (20) can only be virtual ionic state, and no

particular problem arises in expression (20). But such

states are very short lived (a few optical cycles) and

double ionization can be considered as a direct process.

If a real atomic state (ground or excited) can be reached (case B of Fig. 2), the situation is quite different : one

of the denominators of equation (20) will vanish, in a

way similar to what happens in resonant multiphoton

ionization (while the first case considered above was

typically a non resonant process). Also, real ionic states

have much longer lifetimes than virtual states so that it is reasonable to think of double ionization as a two

step process. We should however remember that this

approach has failed giving a satisfying description of

resonant multiphoton ionization. Therefore, though

the terms of « direct » and « stepwise » will still be

used throughout this paper it should be remembered that these two processes are not fundamentally diffe-

rent : stepwise double ionization is only a double

ionization process presenting a resonance in electron energy which should however be distinguished from

resonances in photon energy which may occur in

Fig. 2.

-

Difl’erent double ionization processes : (A) lowest order non resonant (direct) process; (B) lowest order resonant (stepwise) process; (C) higher order resonant (stepwise) process. I g > : neutral atom ground state;

I g1 > : singly charged ion ground state; ! I e1 > : singly charged ion excited state ; g2 > : doubly charged ion ground state.

higher order processes. The use of o stepwise » should

not conceal the fact that the ionization process takes

place in a time much shorter that the radiative lifetime of the real states involved in these resonances. Such

resonances will of course produce peaks in the electron energy distribution but cannot be detected in experi-

ments based on ion detection only.

So far we have limited ourselves to the case of lowest order processes. Considering processes of higher order

increases the energy range in which electrons can be

ejected, and thus the number or resonances which can

be reached, as shown on figure 2, case C. Though of a higher order, such processes, because they are reso-

nant, may not be negligible if no resonance occurs in the

lowest order process. This is thoroughly discussed in the case of helium in reference [30], and the conclusion in this case is that the non resonant process is negli- gible when compared to resonant processes of the

same order, which was expected, and cannot be neglected when compared to resonant processes of a

higher order. However generalization to high order multiphoton processes is not trivial and only a precise

calculation in the experimental situation, when possi- ble, will give an unambiguous answer to this question.

Concerning now the question of ATI and double ionization, the same remarks can be made than for

production of excited ion states : ATI does produce

excited electrons whose energy would, in the case of

two photon double ionization discussed above, lio above the second ionization limit, but it does not

produce core excitation and thus cannot yield multiple ionization, and therefore states reached by ATI are not privileged intermediate states of the multiple ionization

process.

3. Experimental set up.

Our experimental set up is schematized in figure 3.

Most of its elements have been described in previous publications so that we will limit ourselves to a brief

description of its main characteristics.

3.1 LASER SYSTEM.

-

Two different lasers have been used in this experiment. The first one is a commercial

Fig. 3.

-

Schematic of the experimental set-up.

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Nd : Yag laser system (Quantel) delivering 20 ps Fou- rier limited pulses at a 10 Hertz repetition rate. After frequency doubling, this system can deliver at 0.53 gm up to 20 mJ per pulse. The Nd : Yag oscillator is both

passively and actively mode locked, keeping the pulse- to-pulse energy fluctuations at a low level (± 5 %).

This system can be used directly in the experiment,

or it can alternatively be used to synchronously pump

a dye oscillator-amplifier system as described in [31].

This system can deliver up to 2 mJ in a single 20 ps Fourier limited pulse whose wavelength can be tuned throughout the rhodamine 6G emission band (557 to

575 nm).

Because of the long duration of such a wavelength

scan (up to 15 h when one electron spectrum is taken every angstrom) it is necessary to lock the energy per

pulse mean value. This is achieved through a servo

controlled Fresnel rhomb-Glan prism attenuator placed in front of the experiment chamber with this system, the long term intensity drifts can be compen-

sated for, and the mean laser intensity kept stable

within ± 5 % throughout one wavelength scan.

Different focusing lenses have been used in this

experiment. At low intensity a 140 mm focal length plano-convex lens is used. When high intensities are

necessary, a 70 mm focal length sphero-parabolic

lens can be used. It allows to reach intensities of a few Tw . cm - 2 in the interaction region without having to

face overwhelming space charge problems.

3.2 ELECTRON SPECTROMETER. - The laser beam is focused in a vacuum chamber (residual pressure of 10- 8 torr), crossed at a right angle with an effusive Sr beam similar to the one used in [7], with Sr densities

of a few 109 cm- 3. The electron spe’ctrometer is also identical to the one described in [7]. It is an electrosta- tic time of flight spectrometer with a 23 cm length. As

shown in figure 3, a grid system allows to apply an

acceleration field in the interaction region while keeping the analysis energy at any desired value. This system is very useful in the case of very low energy electrons which are very sensitive to both space charge

and stray magnetic fields.

At the exit of the flight tube, the electrons are

detected by a separated dynodes electron multiplier

and fed into a multichannel analyser : counts are temporarily stored into shifts registers, before being

accumulated into the analyser memory.

Up to 1024 channels of 10 ns to 1 gs time width are

available. After accumulation, the content of the

analyser memory can be transferred to a LSI 11 micro- computer system which is in charge of data processing

and storage. This computer is also used to tune the dye

laser and if necessary control the laser intensity and

the spectrometer settings.

The spectrometer can also be used in ion detection.

In this case, an analog signal is obtained which is processed by a boxcar averager after being, if necessary, amplified.

Because throughout this paper, peaks of different

electron energy will be compared, the question of the spectrometer transmission has to be considered.

Figure 4 shows an experimental measurement of this transmission in the energy range of interest here, which

was obtained as follows : a well known and well isolated peak of our electron spectrum (three photon

ionization of Sr, leaving the ion in its ground state and

an electron of energy 0.89 eV, obtained at low laser intensities) was shifted by scanning the flight tube voltage between - 0.2 and 2 eV, resulting in the varia- tion of the peak amplitude shown in figure 4. This

variation has two different origins :

(i) variations of the collection angle due to the

acceleration of the electrons between the interaction volume and the flight tube;

(ii) variations of the flight tube transmission due

probably to stray magnetic fields whose action on low energy electrons is strong and energy dependent.

The first of these two effects can easily be computed

and subtracted from the measurement of figure 4, allowing a measurement of the second effect only (broken line in Fig. 4).

It shows that for electron energies less than 1.5 eV, losses in the flight tube cannot be neglected. However, contrary to the variations of the collection angle due to acceleration, they do not depend on the electron initial energy but on the electron energy inside the flight

tube only, and can be taken into account using the

curve of figure 4.

Two typical voltage settings have been used in this

experiment. Some spectra were taken with all elec- trodes grounded but this does not allow detection of low energy electrons both because of space charge,

contact potentials and losses in the flight tube. There- fore, when such electrons were studied, a small d.c. electric field (between 5 and 10 V/cm) was applied

in the interaction volume to help charge separation

Fig. 4.

-

Variations of the spectrometer transmission with the electron energy : 0-0 : variations of the electron

peak amplitude with the accelerating voltage; . : :

variation of the t.o.f. tube transmission with the analysis

energy.

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and the flight tube potential was set to a positive value (1 V generally), to prevent important losses in the flight

tube.

4. Experimental results.

Multiphoton ionization of Sr was studied at 532 nm

(Nd : Yag second harmonic) and between 558 nm and 575 nm (tuning range of our rhodamine 6G dye laser).

Both the ions and the electrons were studied, but the

results on ions obtained with the dye laser have already

been published [20] and will not be discussed here.

Some preliminary results on the electrons have also been reported in [32] and will be presented in more

details here.

Before presenting the experimental results, a brief

summary of the Sr spectroscopy relevant to our experi-

ment is necessary, particulary to precise a few ioniza-

tion channels which play an important role in this

experiment, and which are outlined on figure 5.

Fig. 5.

-

Different ionization paths involved in Sr simple

and double ionization.

The simplest ionization process for Sr is the three photon ionization of the ground state neutral

Absorption of a fourth photon can leave the Sr II ion in either the ground state, or two excited states :

« Stepwise » (resonant) double ionization using the above transitions as a first step can also occur :

Note that the non resonant ionization process (# 8)

is of order 8. Resonant processes can be of order 8

or 9 depending on the laser wavelength. The electron

energies also depend on the laser wavelength. Within

the tuning range of the dye laser two thresholds are

crossed in channels # 4 and # 5. Channel # 6 is of order 4 with the frequency doubled Nd : Yag laser

and of order 5 with the dye laser.

4 .1 IONIZATION oF Sr AT 532 nm.

-

Single ionization

of Sr was detected for intensities of the order of 1012 W . cm- 2 and above, using a 75 mm focal length

lens. Double ionization was detected for intensities of the order of 5 x 1012 W.cm-2 and above. Varia- tions of the ion signal with the laser intensity are

shown in figure 6 using the usual log-log representa- tion. They show that doubly ionized Sr is detected for intensities just above the onset of saturation for

single ionization. This behaviour has usually been

considered as the signature of a stepwise double

ionization process. Slopes measured in the linear

region are respectively 3.3 for single ionization and 5.4 for double ionization, in agreement with the number of photons necessary to ionize the neutral atom (3 photons) or the ground state singly charged

ion (5 photons).

In many respects these results are analogous to

those obtained in Ca [19] at the same wavelength, except that the intensity gap between single and second

ionization is larger in the case of Ca.

Figure 7 shows different electron spectra obtained

at this wavelength in different conditions.

The spectrum of figure 7a was obtained for a laser

intensity of 2.8 x 1012 W . cm- 2 and without electron acceleration. The energies of the three peaks displayed

on this spectrum are found to be 1.2, 1.8 and 3.1 eV.

Two processes can be responsible for the peak at

1.2 eV, which are the three photon ionization of neutral Sr (# 1 or Fig. 5) which yield an electron

of 1.29 eV, and four photon ionization of the 5p

(10)

Fig. 6.

-

Variation of the number of singly (o---o) and doubly (.-.) charged Sr ions with the laser energy.

state of Sr II (# 7) which yield an electron of 1.23

or 1.32 eV (depending of the J value of the 5p state).

These energies are too close to be separated in our spectrometer, but comparing the ion signals at this intensity shows that this peak is certainly mainly due

to single ionization of channel # 1. The peak at

1.8 eV can unambiguously be assigned to the process of channel # 3 (single ionization leaving the ion

in one of the 4d states). The last peak at 3.1 eV is certainly due to ATI, but here the resolution of our

spectrometer is too low to ascertain whether it is due to ATI following single ionization of channel # 2

(yielding 3.5 eV electrons) or ATI following double

ionization of channel # 5 (yielding 2.9 eV electrons) which, as we will see, is already important at such

an intensity.

The two following spectra (Figs. 7b and c) have

been obtained using a 6.7 V/cm separation field

and a 1 V acceleration voltage on the flight tube.

The increase of the collection efficiency allows to

work at both a lower neutral density and laser inten-

sity. The spectrum of figure 7b is taken at an intensity

of 0.3 x 1012 W. Crn - 2.

It shows only one peak at 2.2 eV, which is the remnant of the 1.2 eV peak of figure 7a. The 1.8 eV

peak either has disappeared or is not separated from

the main peak. On the trailing edge of the main peak,

there is a weak feature whose position would cor-

respond to 0.6 eV electrons. This peak is clearly

visible in figure 7c, taken at an intensity of 1.2 x 1012 W.CM-2 . Electrons with such an energy can be created in both processes # 4 ( four photon

ionization in the 5p ion state) and # 5 (five photon

ionization of the ground state ion). A third peak

is clearly visible on figure 7c, corresponding to

electrons with an energy of 0.1 eV, such as the ones created in process # 6 (four photon ionization of the 4d ions). The electrons created in process # 7 would appear at the same energy as those of pro-

cess # 1 (1.3 eV). The intensity behaviour of these

different peaks, shown in figure 8 indicates that the electrons of the 0.6 eV peak are mostly created in the double ionization process, as those of the 0.1 eV

peak, since they do not saturate as the 1.3 eV peak

does. Even the 1.3 eV peak does not saturate as

strongly as the singly charged ion signal does (Fig. 6),

(11)

Fig. 7. - Different electron energy spectra taken at A

=

532 nm and for different experimental conditions (see text).

and this may be due to the contribution of electrons of channel # 7, which may not be negligible at high

intensities.

The main conclusion arising from these data is that double ionization of Sr at 530 nm is essentially

a « stepwise » (resonant) process involving principally

the ground state and the first two excited states of the

Sr ion. It can also be deduced from the comparison

of the two higher energy peaks of figure 7a that

excited ion state production is more probable than

ATI of the same order. This suggests than multi-

photon ionization of alkaline earths goes along with

a noticeable degree of core excitation.

4.2 IONIZATION OF Sr FROM 558 nm TO 574 nm.

-

This experiment was repeated using our dye laser,

in the wavelength range between 558 and 574 nm.

Spectra corresponding to those of figure 7 were

obtained and are presented in figure 9. The spectrum of figure 9a was taken without collection field and at an intensity of 3 x 1012 W.em-2. The spectrum of figure 9b was obtained with a few V. cm-1 collec- tion field and a 1 V net acceleration between the focal volume and the flight tube. The intensity in this case

was about 1011 W . cm - 2. On these spectra, peaks corresponding to all the processes discussed in the

previous chapter can be observed. Processes # 2, 5 and 6 do not appear on the spectrum of figure 9b

because it is taken at a much lower intensity, and they disappear of the spectrum of figure 9a when the intensity is decreased.

Some aspects of these results have already been presented in [32] and will be further discussed here.

We first note that the differences in the peak positions

Fig. 8.

-

Variations of selected peaks amplitude (from Fig. 7) with the laser energy. Labels correspond to different

processes of figure 5.

between figures 7 and 9 are due to the change in the

laser wavelength and are all consistent with the inter-

pretations given here for each peak.

The peak labelled 5 in figure 9a corresponds to

six photon ionization of the ground state ion. Depend- ing whether the wavelength is shorter or longer than

520 nm (five photon ionization threshold for the

ground state ion) this is either a normal MPI peak

or a first order ATI peak. As reported in [32], no rapid variation of this peak amplitude is observed

when the laser wavelength is scanned through the

threshold wavelength. This was interpreted on the ground of the continuity between the wavefunctions of the discrete spectrum when n - oo and of the continuum when E - 0. However it is impossible

to identify a five photon ionization peak which should appear at short wavelength, because it is superim- posed to the peak # 4, and the dye laser intensity is

too small to allow an identification through the intensity dependence. As shown in the previous paragraph, this is possible at 532 nm and gives us

full confidence in the above interpretation.

The peak labelled 4 (in Fig. 9b) is essentially due (totally at low intensities) to 4 photon ionization of Sr, leaving the ion in the 5p excited states. The one

labelled (1) + (3) by following peaks (1) and (3)

of figure 9 a when increasing the accellerating field.

Peak (4) is identified, as discussed below, by its wave-

length dependence. The slight energy mismatch visible

in figure 9b is probably due to the use of a separation

(12)

Fig. 9.

-

Two different electron energy spectra taken with the Dye laser for different conditions (see text). Labels

on the peaks correspond to different ionization processes of figure 5.

field which makes the electron energies (inside the flight tube) critically dependent on the position of

the laser focus.

Here again, the two thresholds corresponding to

excitations of the 5P3/2 and 5P 1/2 states of Sr+ are

crossed within the dye laser wavelength range, for 567,8 nm and 574,4 nm respectively. In [32], in order to emphasize the threshold effect, the variations of the

peak # 4 with the laser wavelength in the threshold

region were recorded with the laser polarization at a right angle from the collection axis. (In this configura- tion, our electron spectrometer works as a « threshold spectrometer » because the weak accelerating field is

too low to collect electrons with energies above

0.1 eV - typically

-

when they are emitted preferen- tially along the laser polarization direction). This

detection scheme was usefull in identifying peak # 4

but causes strong variations of the collection efficiency

with the energy.

Figure 10 represents the variations of the peak # 4 amplitude, for a laser intensity of 1011 W.cm-’, and

for laser wavelengths between 565 nm and 574 nm.

The laser polarization is along the detection direction

so that this peak amplitude is a good representation

of the excitation probability for the 5p ion states. The

two thresholds are still clearly visible, the ionization probability presenting in both cases a maximum about 45 cm-1 above the ionization threshold. In addition,

for wavelengths between 590 nm and 572 nm, a broad

maximum can be seen, which was completely cut-off by the transmission drop in [32]. It corresponds to

two photon intermediate resonances on the 5p2 3p 0

and 5s 5d 3Di states of Sr which were observed on the

ion signal in [20, 28]. As will be shown in a forthcoming

paper at the intensity used in this experiment, these

resonances are strongly shifted and broadened and thus are not clearly resolved on the spectrum of figure

10. We finally note that in this wavelength range, the

peak labelled 3 on figure 8a, corresponding to four photon ionization in the 4d states is negligible.

Many two and three photon resonances in the ion

signal were also observed in the wavelength range between 558 nm and 564 nm [20, 28]. These resonances

can also be seen on the electron signals, as shown in figures 11 and 12. These two figures show the wave- length dependences of different peaks. Figures 11 and

12 correspond respectively to a laser linearly polarized along the direction of detection and circularly pola-

rized. Figures 11 (12) a, b and c correspond respectively

to three photon ionization into the Sr+ ground state (channel # 1), four photon ionization into the 4d

(channel # 3) and 5p (channel # 4) states. Figure 11c,

was taken at a laser intensity of 1011 W . cm- 2, figures

11a and b at an intensity of 1.6 x 1011 W .cm-2, and figures 12a, b, c at 2 x 1011 W .em-2. As usual with

tightly focused picosecond pulses, absolute intensities

are not determined to a better precision than a factor 2.

However comparison between the different figures quoted above is exact within 20 %. Intensity changes

between the different spectra of figures 11 and 12

were made necessary by experimental constraints

owing to the limited range of satisfying operating

conditions for the spectrometer and of course to the accumulation time. The wavelengths plotted in

abscissa are in the vacuum and are taken directly from

the computer scanning program, so that the small differences between the positions of the peaks in

different spectra only reflect the limited precision of

our wavelength scanning/measurement system, which is about 1 angstrom.

Some general remarks can be made concerning

these spectra. All the resonances of figures 11 and 12

have already been seen with ion detection [20, 28].

(13)

Figure 10.

-

Wavelength dependence of peak 4, of figure 9b (Sr (5s2) + 4 hv

-+

Sr+ (5p) + e-) in the 5P 1/2,3/2 ionization

threshold region. Vertical bars indicate the position of the thresholds.

Fig. 11. - Wavelength dependence of selected peaks of figure 9 in the 558-nm-564 nm region, for a linear polariza-

tion of the laser, along the detection direction.

Changing the laser polarization from linear to

circular lead to a decrease of the ionization probabi- lity which made necessary and increase of the laser

intensity by a factor of 1.5 to 2 to restore the signal

level. It also results in a sharpening of the resonances,

labelled (I) to (V) in figure l la which can be seen, to a

different degree, on all the spectra of figures 11 and 12.

Resonance (I) at 559.4 nm, with a small satellite at

559.6 nm (which in some cases appears merely as a shoulder) appears, as in [20, 28] at the wavelength corresponding to a three photon resonance on the

5p 6s 1P’ state as deduced from the results of reference

[33]. The fact that this resonance is clearly seen with a circularly polarized laser is a first indication that

Fig. 12. - Same as figure 11, with a circularly polarized

laser.

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