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J. Phys. B: At. Mol. Opt. Phys. 36 No 16 (28 August 2003) L241-L247
PII: S0953-4075(03)63257-8

LETTER TO THE EDITOR

A procedure to extract the complex amplitudes of He photodouble ionization from experimental data

P Bolognesi1, A S Kheifets2, I Bray3, L Malegat4, P Selles4, A K Kazansky5 and L Avaldi1,6

1CNR-IMIP, Area della Ricerca di Roma, CP10, 00016 Monterotondo Scalo, Italy
2Research School of Physical Sciences and Engineering, Australian National University, Canberra, ACT 2000, Australia
3CAMSP, School of Mathematical and Physical Sciences, Murdoch University, Murdoch, Perth 6150, Australia
4LIXAM, UMR 8624 du CNRS, Bâtiment 350, Université Paris-Sud, 91405 Orsay-Cedex, France
5Fock Institute of Physics, The University of St Petersburg, St Petersburg 198504, Russia
6INFM-TASC, Gas Phase Beamline at Elettra, Area Science Park, I-34012 Trieste, Italy

Received 5 May 2003
Published 5 August 2003

Abstract. A procedure to extract the two complex amplitudes that govern the He photodouble ionization process from the experimental data is proposed. The results are compared with the predictions of the convergent close coupling and hyperspherical R-matrix with semiclassical outgoing wave theories.

Photodouble ionization (PDI) of He is the archetypal three-body Coulomb problem (two interacting particles in the field of a positive structureless residual ion) and as such it has attracted a lot of experimental and theoretical interest. The complete experimental characterization of this process implies experiments in which either the two photoelectrons [1, 2] or one of the photoelectrons and the residual ion [3] are detected in coincidence. In such experiments the triply differential cross section (TDCS) Inline equation, i.e. a cross section differential in the angles of emission of the two photoelectrons Inline equation and Inline equation and in one kinetic energy E1, is measured. The kinetic energy E2 of the other electron is determined by energy conservation. Since the first experimental determination of the TDCS in 1993 [1] a large set of data from the near-threshold [2] region up to a photon energy of about 500 eV [4] has been published. At pace with the experimental work extensive theoretical effort has been applied [5, 6, 7, 8, 9, 10]. Experimentally, at a fixed incident energy the TDCS can be measured under a variety of kinematic conditions (changing the energy sharing between the electrons and/or their angles of emission). This results in a large body of data and hampers direct comparison between different sets of data and between experiment and theory. In this paper we propose a procedure to overcome this difficulty by extracting from the experimental data the underlying basic quantities which allow one to reconstruct any particular TDCS, namely the moduli and the relative phase of the gerade and ungerade complex amplitudes of the process.

By considering the 1Po symmetry of the electron pair continuum wavefunction, the TDCS can indeed be written in a way that allows the full separation of the geometrical factors and the dynamic parameters [11, 12]. In the case of incident radiation that propagates along the z axis and is fully linearly polarized along the x axis the TDCS measured in the (x,y) plane can be written

Equation (1)

where Inline equation and Inline equation are the angles of emission of the two photoelectrons in the (x,y) plane, measured from 0 to Inline equation with respect to the polarization axis x, and Inline equation is the relative angle between the directions of emission of the two photoelectrons. The complex amplitudes Ag and Au are respectively symmetric (gerade) and antisymmetric (ungerade) with respect to the exchange of the two electrons - which amounts to the exchange of E1 and E2 since Inline equation. The Inline equation, E1 and E2 dependence of the amplitudes includes all the physical information on the dynamics of the process, i.e. the effects of the electron-electron and electron-residual ion interactions. It is clear from (1) that the TDCS is invariant upon multiplication of the two amplitudes by the same phase factor. Hence the only quantities of physical significance are the moduli of Ag and Au and their relative phase Inline equation. Since the theoretical models directly calculate these quantities it is of considerable interest to look for a procedure which extracts them from the experimental measurements.

Recently such a procedure, based on internormalized data sets at four specific experimental geometries, was proposed by Krässig [13]. Here we propose a different procedure that allows one to extract |Ag|, |Au| and Inline equation from any set of three absolute experimental determinations of the TDCS at the same E1,E2 and Inline equation values but at different Inline equation. The same procedure allows one to extract the scaled complex amplitudes |ag|  = C|Ag|, |au|  = C|Au| and Inline equation from any set of three relative internormalized experimental determinations of the TDCS, where C is a real positive constant independent of E1,E2 and Inline equation.

Thus, for each experimental determination i =  1,2,3, let us denote by Inline equation the measured quantity, be it the absolute TDCS or the coincidence yield that is proportional to the latter, and by

Equation (2a)

Equation (2b)

the geometric factors. The measured quantities can then be expressed by expanding (1) as

Equation (3)

or in matrix notation Inline equation. The solution to this equation reads Inline equation. The elements of the covariance matrix associated with the calculated quantities are then given by

Equation (4)

Assuming that the uncertainties in the quantities Inline equation are statistically independent, i.e. Inline equation, we get

Equation (5a)

Equation (5b)

The uncertainty in Inline equation is then easily obtained from the elements of the covariance matrix as

Equation (6)

The technique outlined above can be used only if certain dynamic and geometric conditions are fulfilled, so that the A matrix can be inverted to yield non-zero values of the components of Inline equation.

Figure 1

Figure 1. |ag|2 obtained from the two experimental TDCS at E =  40 eV, E1 =  35 eV and E2 =  5 eV (open circles), and E1 =  5 eV and E2 =  35 eV (black circles) (a) and from the weighted average of the two experiments (b) versus the relative angle Inline equation. The experimental results are compared with the predictions of the CCC (full curve) and HRM-SOW (dotted line) theories.

Figure 2

Figure 2. |au|2 versus the relative angle Inline equation. The same symbols as in figure 1(b) are used.

It is worthwhile mentioning that the procedure outlined above only enables one to determine the cosine of the relative phase between the two complex amplitudes. Thus the experiment cannot be considered a complete one, because the sign of the phase remains undetermined. Therefore, not all the observables of the double photoionization process can be determined from (3). For example, the sign of the circular dichroism in experiments with radiation including a circularly polarized component [14] cannot be obtained. However, this procedure can easily be turned into a complete one. For instance, one could consider absolute measurements of the TDCS obtained using elliptically polarized light: the absolute magnitudes and relative phase (i.e. the cosine and sine of this phase) of the two amplitudes would be obtained from a quadruplet of such measurements performed for the same energies and relative angle of the two electrons. The extraction procedure would then imply solving a linear system of four equations in the four variables |ag|2, |au|2, Inline equation and Inline equation.

The procedure also assumes that the experimental uncertainty in Inline equation is negligible compared to the uncertainties Inline equation of the measured coincidence yield. This means that the application of the method to experimental TDCS resulting from an integration over large Inline equation and Inline equation intervals is not straightforward.

In this respect, our procedure is complementary to the one previously proposed by Krässig [13]. That procedure has the advantage of making use of the full set of coincidence events that can be obtained by a COLTRIMS complete set of data. However, the four specific experimental geometries needed are not easily achieved by most of the experimental apparatuses used in PDI experiments. In contrast, the simpler procedure used here can be applied with no restrictions to any set of experimental data.

The procedure has been applied to the TDCS of He measured on a relative scale at an excess energy E = E1 + E2 =  40 eV above threshold in unequal energy sharing (E1 =  5 eV and E2 =  35 eV) by Bolognesi et al [15]. This data set is particularly suited for the proposed procedure because three angular distributions have been measured simultaneously. In the experiment one electron was detected at Inline equation, 30° and 60° for i =  1,2 and 3, respectively, while the second one was collected at Inline equation. Moreover, complementary TDCS patterns, obtained in two experiments by the interchange of the electron kinetic energies, Inline equation, have been measured. Due to the symmetry properties of ag and au the only difference between the solutions of (3) based on the two complementary sets should be a difference of Inline equation in the respective relative phases of the gerade and ungerade amplitudes. Comparison of these two sets of solutions will therefore illustrate the reliability of the method. To conclude, a final advantage of this set of measurements is that the ± 3° [15] angular acceptance in the dispersion plane of the spectrometers makes plausible the assumption of a negligible uncertainty in the determination of the angles.

The |ag|2 and |au|2 squared amplitudes, their ratio and the cosine of their relative phase obtained applying the procedure to the experimental data are shown in figures 1-4, respectively. In figure 1(a) |ag|2 obtained using both sets of measurements in the complementary kinematics are shown. At the Inline equation values, where multiple experimental determinations exist, a weighted average has been calculated and reported in the figure. The two sets of results are in agreement within the respective uncertainties, thus in figure 1(b) as well as in all the other figures only the weighted average of the two sets is reported. In the same figures the results are compared with the predictions of the convergent close coupling (CCC) [7] and the hyperspherical R-matrix with semiclassical outgoing (HRM-SOW) [8] methods. For a better comparison of the experimental and theoretical shape of the |ag|2 and |au|2 squared amplitudes, the experimental |ag|2 has been rescaled to the mean value of the two theories at Inline equation in figure 1. The same scaling factor has been used in figure 2 for the |au|2 squared amplitude. The absolute values of the complex amplitudes and Inline equation predicted by the theories at Inline equation, together with the maximum values of |ag|2/|au|2 are presented in table 1.

Table 1. Absolute values of |ag|2, |au|2, Inline equation at Inline equation and the maximum values of |ag|2/|au|2 predicted by the CCC [7] and HRM-SOW [8] methods.
  CCC HRM-SOW
Inline equation
(barn eV - 1sr - 2)
47.748 46.972
Inline equation
(barn eV - 1sr - 2)
2.341 2.644
|ag|2/|au|2max 78.00 77.98
Inline equation 99 92
Inline equation  - 0.5236  - 0.5056

Despite the good statistical quality of the experimental data (see figures 1, 2 in [15]) the results for the |ag|2/|au|2 ratio and Inline equation display some scattering. Moreover, the error propagation results in large error bars, especially in the region near Inline equation for |ag|2 and Inline equation for |au|2.

Figure 3

Figure 3. The |ag|2/|au|2 ratio versus the relative angle Inline equation. The same symbols are used as presented in figure 1(b).

Figure 4

Figure 4Inline equation versus the relative angle Inline equation. The same symbols as in figure 1(b) are used. The stripe shows the value obtained by Bolognesi et al [15] in the framework of the practical parametrization proposed by Cvejanovic and Reddish [16].

As for |ag|2 the two theories predict the same shape in good agreement with experiment. The values of |au|2 near Inline equation predicted by both theories overestimate the experimental results, with the CCC value being closer to experiment than the HRM-SOW one. From figures 1 and 2, the half widths at half maximum of |ag|2 and |au|2 can be estimated roughly as 87° and 66°, respectively. This indicates a steeper decrease of the ungerade squared amplitude from its maximum, compared to the gerade one, resulting in a maximum of the |ag|2/|au|2 ratio located away from 180° as one can see from figure 3. A small difference in the shape and the position of the maximum of the ratio is observed in the predictions of the two theories. Unfortunately the quality of the data in the region Inline equation and the absence of experimental determinations in the region below Inline equation does not allow one to distinguish between the two predictions. Figure 4 shows that the relative phase is varying with Inline equation, although the variation in the experiments seems to be less pronounced than in the theoretical predictions. Thus the constant phase proposed within the framework of the practical parametrization by Cvejanovic and Reddish [16] might be too crude an approximation. The dashed stripe in figure 4 shows the band of uncertainty of the constant value obtained in a previous representation of the same data by Bolognesi et al [15] using the practical parametrization [16]. This value is quite close to the average ( - 0.68 ± 0.27) of the values obtained in the present analysis. The agreement between the theoretical values and experimental ones is reasonable for Inline equation. Theories then predict a phase difference close to 180° at Inline equation. A smaller value is determined by experiment at Inline equation, while no experimental data are available in the region below 100° to prove or disprove the predicted trend.

In summary we have proposed a procedure to extract from the experimental data the two complex amplitudes of PDI. This direct procedure does not rely upon any assumption regarding the functional dependence of these amplitudes in E1, E2, or Inline equation. The use of the amplitudes makes the comparison among the various experiments as well as between experiment and theory more compact and direct, and allows one to outline differences that may be hidden in the comparison of the TDCS because of the modulation imposed by the kinematic factors. The results for an experiment performed in complementary kinematics at E =  40 eV prove that the method is feasible provided the measured TDCS are characterized by a high statistical accuracy. Moreover, this first application shows that direct comparison of the amplitudes predicted by the different theories may be valuable by itself. For example, some differences have been observed between the predictions of the two theories used for Inline equation for the |ag|2/|au|2 ratio and cos Inline equation, thus suggesting that future measurements should not neglect this region.

LA and PB gratefully acknowledge stimulating discussions with Norberto Tomassini. PS and LM acknowledge support from the CNRS computer centre IDRIS through project 31485. ASK and IB are indebted to the Australian Partnership for Advanced Computing and the Australian Research Council.

References

[1]
Schwarzkopft O, Krässig B, Elminger J and Schmidt V 1993 Phys. Rev. Lett. 70 3008 
CrossRefPubMed
[2]
Huetz A and Mazeau J 2000 Phys. Rev. Lett. 85 530 
CrossRefPubMed
[3]
Ullrich J, Moshammer R, Dörner R, Jagutzki O, Mergel V, Schmidt-Böcking H and Spielberg L 1997 J. Phys. B: At. Mol. Opt. Phys. 30 2917 
IOPscience
[4]
Knapp A et al 2002 Phys. Rev. Lett. 89 033004 
CrossRefPubMed
[5]
Maulbetsch F and Briggs J S 1994 J. Phys. B: At. Mol. Opt. Phys. 27 4095 
IOPscience
[6]
Pont M and Shakeshaft R 1995 J. Phys. B: At. Mol. Opt. Phys. 28 L571 
IOPscience
[7]
Kheifets A S and Bray I 1998 J. Phys. B: At. Mol. Opt. Phys. 31 L447 
IOPscience
Kheifets A S and Bray I 1998 Phys. Rev. Lett. 81 4588 
CrossRef
[8]
Malegat L, Selles P and Kazansky A K 2000 Phys. Rev. Lett. 85 4450 
CrossRefPubMed
Selles P, Malegat L and Kazansky A K 2002 Phys. Rev. A 65 032711 
CrossRef
[9]
Pindzola M S and Robicheaux F 1998 Phys. Rev. A 57 318 
CrossRef
[10]
Rescigno T N, Baertschy M, Isaacs W A and McCurdy C W 1999 Science 286 2474 
CrossRefPubMed
[11]
Briggs J S and Schmidt V 2000 J. Phys. B: At. Mol. Opt. Phys. 33 R1 
IOPscience
[12]
Huetz A, Selles P, Waymel D and Mazeau J 1991 J. Phys. B: At. Mol. Opt. Phys. 24 1917 
IOPscience
[13]
Krässig B 2001 Correlations, Polarization and Ionization in Atomic Systems ed D H Madison and M Schulz (AIP Conf. Proc. vol 604) (Rolla, MO: American Institute of Physics) p 12 
[14]
Soejima K, Danjo A, Okumo K and Yagishita A 1999 Phys. Rev. Lett. 83 1546 
CrossRef
[15]
Bolognesi P, Camilloni R, Coreno M, Turri G, Berakdar J, Kheifets A S and Avaldi L 2001 J. Phys. B: At. Mol. Opt. Phys. 34 3193 
IOPscience
[16]
Cvejanovic S and Reddish T J 2000 J. Phys. B: At. Mol. Opt. Phys. 33 4691 
IOPscience




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