Acessibilidade / Reportar erro

Production of 1s2s2p4P states by transfer-loss cascades in O5+ collisions with he and H2 targets

Abstract

Single differential cross-sections for transfer-loss (TL) leading to the production of O5+(1s2s³S)nl4L states were computed for 0.2-1.2 MeV/u collisions of O5+(1s²2s) ions with He and H2 targets. At these collision energies, 1s loss is significant and electron transfer to n = 3-4 levels is dominant. Furthermore, due to spin conservation, quartet states can only be populated by TL. Within the independent particle model (IPM), the probability of 1s electron loss from O5+(1s²2s) projectiles was calculated using the semi-classical approach, while the probability for electron transfer to the O5+(1s2s³S)nl4L states (n > 2) was computed using the continuum distorted wave (CDW) approximation. The majority of states with n > 2 can be assumed to have sufficient time to eventually decay with an almost 100% probability to the long-living metastable 1s2s2(4)P level via a much faster sequence of electric dipole transitions, thus establishing an upper limit to such cascade contributions. The inclusion of this cascade feeding is found to lead to a strong enhancement in the production of the 1s2s2p4P states, particularly for collisions with the H2 target, thus reducing dramatically the existing two-order of magnitude discrepancy between older TL calculations (for n = 2 only) and existing zero-degree Auger projectile electron spectroscopy measurements.

Metastable states; Cascade feeding; Ion-atom collisions; Electron capture


Production of 1s2s2p4P states by transfer-loss cascades in O5+ collisions with he and H2 targets

T. J. M. ZourosI; B. SulikII; L. GulyásII; A. OrbánII

IDept. of Physics, University of Crete, P.O. Box 2208, 71003 Heraklion, Crete, Greece and Institute of Electronic Structure and Laser, P.O. Box 1527, 71110 Heraklion, Crete, Greece

IIInstitute of Nuclear Research of the Hungarian Academy of Sciences, Debrecen, Hungary

ABSTRACT

Single differential cross-sections for transfer-loss (TL) leading to the production of O5+(1s2s3S)nl4L states were computed for 0.2-1.2 MeV/u collisions of O5+(1s22s) ions with He and H2 targets. At these collision energies, 1s loss is significant and electron transfer to n = 3-4 levels is dominant. Furthermore, due to spin conservation, quartet states can only be populated by TL. Within the independent particle model (IPM), the probability of 1s electron loss from O5+(1s22s) projectiles was calculated using the semi-classical approach, while the probability for electron transfer to the O5+(1s2s3S)nl4L states (n > 2) was computed using the continuum distorted wave (CDW) approximation. The majority of states with n > 2 can be assumed to have sufficient time to eventually decay with an almost 100% probability to the long-living metastable 1s2s24P level via a much faster sequence of electric dipole transitions, thus establishing an upper limit to such cascade contributions. The inclusion of this cascade feeding is found to lead to a strong enhancement in the production of the 1s2s2p4P states, particularly for collisions with the H2 target, thus reducing dramatically the existing two-order of magnitude discrepancy between older TL calculations (for n = 2 only) and existing zero-degree Auger projectile electron spectroscopy measurements.

Keywords: Metastable states; Cascade feeding; Ion-atom collisions; Electron capture

I. INTRODUCTION - THE 1s2s2p4P TRANSFER-LOSS PUZZLE

In 1989, Zouros et al. [1] showed that the 1s®2p projectile excitation cross section for Li-like F6+ and O5+ ions in collisions with H2 and He (see Figs.1 - 2) was found to increase when the projectile velocity Vp was such that m DE, where DE is the projectile 1s®2p excitation energy and m the mass of the electron. This enhancement of the projectile excitation cross section on passing the electron impact excitation threshold DE was interpreted as being due to the onset of direct projectile-electron-target-electron interactions in a process named electron-electron excitation (eeE) [1]. In reverse kinematics, the quasi-free target electrons as seen by the ion from the projectile frame, forms an "electron beam" that can excite the projectile electrons once its impact kinetic energy is larger than DE. This threshold, however, is partially diffused by the rather broad electron momentum distribution due to its orbital motion around the target. Today, this process is well understood within the electron scattering model [2-5] and the Born approximation [6,7] and is found to be important in excitation [1,7-9] and ionization [10-13] processes in ion-atom collisions [,,]. It is particularly prevalent in ion collisions with low-Z targets, where competition from excitation due to the target-nucleus charge is relatively smaller [16].



The eeE results of Ref. [1] referred to the production of a particular state, the 1s2s2p4P, for which other competing target-nucleus excitation processes are forbidden due to spin selection rules, thus making this state uniquely accessible by the eeE process:

However, below the electron impact excitation threshold DE, an increase in the excitation cross section of the 1s2s2p4P state was also observed [17] in collisions of O5++He (see Fig. 2), having an energy dependence reminiscent of capture. Capture is maximized when the projectile velocity matches the velocity of the electron to be captured and drops rapidly with increasing collision energy. The production of the 1s2s2p4P state, below ~ 16 MeV, showed a similar behavior which Stolterfoht et al. [17] attributed to the two-electron process named transfer-loss (TL). TL requires the transfer of a target electron to the projectile ion with the simultaneous loss of a projectile electron, thus leaving the projectile in a doubly-excited three-electron state. In particular, for the production of 1s2s2p4P by TL we study the process:

Within the IPM it is assumed that TL can be modeled by the following two independent one-electron transitions:

where X represents the target. The energy dependence of 1s2s2p4P is shown in Figs.1 and 2. The data refer to existing high resolution electron spectroscopy measurements of the Auger decay of the 1s2s2p4P state observed at zero degree to the beam direction for O5+ in collisions with H2 [1,9,18] and He targets [1,9,17,18]. Also shown for comparison in Fig.1 (open squares) are the 1989 results of a coupled-channel TL calculation performed by R. Shingal (shown in Fig. 1c of Ref. [1] as a private communication) for O5++H. What was particularly puzzling at that time was that this quite sophisticated TL calculation was almost two orders of magnitude smaller than measurement. This puzzle remained uninvestigated over the next 10 years.

II. RECENT TL CALCULATIONS

Recently, new TL calculations were performed in the IPM by Sulik et al. [19] for both H2 and He targets using exclusive [20] unitarized [21] impact parameter b-dependent probabilities, P(b). Electron transfer probabilities were computed using the continuum distorted wave (CDW) approach [22], while 1s loss (projectile ionization) probabilities were calculated using a semiclassical approximation (SCA) code [23] for the production of an uncoupled determinant state |(1s2s2pm) >:

where X represents the He or H targets. To closer simulate the molecular H2 target used in the experiments, the CDW and SCA calculations were performed for an effective H atom (with = 1.062) [24] including an averaging over all the orientations of the H2 molecular axis. For the capture probability, , the term in large curly brackets represents the exclusive probability [20] that there is no other capture allowed from the other X 1s electron to the oxygen ion. In this work "any shell" represents an additional capture to oxygen. Such a capture would necessarily lead to a different ionic state with different configuration and energy and therefore to a different Auger transition which must be explicitly excluded. For the loss probability, PL, the first term is the single ionization probability of the oxygen 1s shell, while the second and third terms represent the probabilities that the other 1s and 2s electrons of oxygen must remain untouched for the same reason as in the transfer process above. For the "any state" probabilities, the excitation from the ground state of O5+ into a set of excited and continuum states was considered. Finally, the uncoupled TL probabilities were then coupled together to obtain the probabilities for the specific determinant state |(1s2s2pm) 4P > , which upon integrating over the impact parameter gave the state-selected cross section. Auger yields, and anisotropic electron emission due to alignment effects were also taken into account in calculating the theoretical zero-degree Auger emission cross section for the 1s2s2p4P line.

Furthermore, in an attempt to investigate other possible scenarios which might further enhance the production of the 1s2s2p4P states, the process of double-transfer-loss (T2L) involving a double capture to n > 2 levels accompanied with a 1s loss and followed by LXY Auger transitions was also included since it was noticed that the calculated probabilities for electron capture to n > 2 shells were much larger than for those to the n = 2 shell (see Figs.3-4). However, since the various branching ratios between the LXY Auger transitions and other competing processes were not known, and assuming that the LXY Auger transition is the dominant channel, the sum of the TL+T2L components can be used as an upper limit, with the TL alone representing the calculated lower limit for the sum of the two processes. It was clearly demonstrated that the calculated T2L contribution is much less important for the H2 molecule than for the He atom (see Figs. 1 and 2 dashed lines).


In the above calculations of Sulik et al. [19], the projectile-energy dependence of the data was well reproduced for both collision systems. However, the calculated cross-sections were more than a factor of 2 too small for He and still much smaller for H2. For the He target, the difference between the measured and calculated cross-sections was traced to the CDW capture calculations since the calculated electron loss cross-sections alone were in very good agreement with experiments [24]. For H2, the TL calculations also seemed to be consistent with the low cross section results of R. Shingal already mentioned. The main reason for the low TL cross-sections for the hydrogen target lay in the fact that the CDW electron transfer probabilities for hydrogen were more than one order of magnitude smaller than for helium.

III. NEW TL CALCULATIONS: INCLUSION OF CASCADE CONTRIBUTIONS

Here, we present new improved TL calculations, along the previous lines of Ref. [19]. Small improvements include a CDW capture recalculation using the slightly larger effective = 1.195, rather than = 1.062 used previously for H2. The justification for this change is based on the recent findings of Galassi et al. [25] that = 1.195 gives a better account of the initial state momentum distribution (and, in turn, the Compton profile) of the hydrogen molecule. Even double differential cross sections were found to be accurately described by applying such wave functions [24]. Using = 1.195, we obtained on average an increase in the capture probabilities from H by a factor of 1.7, closing the previously observed large capture difference between He and H target. Finally, the angular emission probability was recomputed within the intermediate coupling scheme more appropriate for the case of the metastable 1s2s2p4P state [26]. The newly computed angular distribution for electron emission was found to be rather close to isotropic. Accordingly, the zero-degree electron emission cross sections are smaller than their previously calculated values within the LS-coupling scheme which favored emission from the 2p0 sublevel for zero-degree observation.

Apart from these slight improvements that resulted in rather moderate changes in the new TL calculation, a new and very important point was also considered. As already pointed out above, the CDW calculations brought out the fact that capture to n = 2—4 is dominant at these collision velocities. Thus, nTL to higher lying n > 2 levels is also dominant, as shown in Figs. 3-4, where TL cross sections to uncoupled 1s2snl states of O5+ are computed as a function of n (summed over all possible l-values) for a few collision energies. Such nTL-formed quartet states may now photon-decay in a cascade that will effectively feed the production of the 1s2s2p4P state [28], thus enhancing its production. Furthermore, the 1s2s2p4PJ state, due to its very long lifetime (0.91 ns for J = 1/2, 3.34 ns for J = 3/2 and 27.67 ns for J = 5/2 [27]), would be an excellent collector of such cascade products involving much faster photon decays. In particular, due to spin conservation, only 1s2snl 4L states can decay to the 1s2s2p4P state, further simplifying the cascade sequence [29]. Such cascade schemes are well known in the literature [28]. In particular, such a cascade scenario has already been explored to some extent (only for n = 3) and found to be important in studies of single electron capture in low energy collisions of O6+(1s2s 3S) with He [29]. However, since all the various branching ratios for the photon transitions are not yet known, we have assumed that nTL to all the 1s2snl 4L states end up feeding the 1s2s2p4P state with an almost 100% efficiency. This cascade TL contribution (CTL), should clearly be considered only as an upper limit to such cascade feeding. It is shown in Figs. 1 and 2.

As seen from Figs. 1-2, our computed CTL upper limit increases the production of 1s2s2p4P states by a further factor of 2.5 for He and 4 for H2, clearly establishing cascade feeding as possibly the most important contributor to the production of 1s2s2p4P states by TL for these low-Z collision systems. Detailed calculations of transition rates and branching ratios need to be worked out for n = 3—4 and possibly higher n values to evaluate more precisely the cascade feeding contributions. Even the addition of the cascade feeding mechanism might not be enough to explain the remaining difference of close to a factor of 1.5 for He and 2 for H2. Whether yet another mechanism is required to close the remaining gap between theory and experiment will remain an interesting possibility.

IV. SUMMARY AND CONCLUSION

We have shown that the production of O5+(1s2s2p4P) states due to TL should also consider the contributions of optical cascade (CTL) feeding from higher lying prompt states that may be produced by TL to (1s2snl 4L) states for n > 2, since transfer to n = 3—7 is also very strong. Our rather rough CTL calculations place only an upper limit on the contributions of such a cascade feeding process resulting in much better agreement with existing measurements. Clearly, a more detailed theoretical investigation of the possible cascade feeding of the 1s2s2p4P states is needed before a more definitive quantitative understanding can be established. We are presently pursuing such a detailed cascade feeding model.

Acknowledgments

We acknowledge partial support from the Division of Chemical Sciences, Geosciences and Biosciences, Office of Basic Energy Sciences, Office of Science, U.S. Department of Energy, the Hungarian National Sciences Foundation (OTKA, Project No. T046905) and the Greek-Hungarian Intergovernmental Science and Technology Bilateral cooperation program (KPI and the Greek Ministry of Development, GSRT Project No. GR-11/03). We also thank Nico Stolterfoht for communicating published data in digital form.

[1] T. J. M. Zouros, D. H. Lee, and P. Richard, Phys. Rev. Lett. 62, 2261 (1989).

[2] E. P. Benis, T.J.M. Zouros, T.W. Gorczyca, A.D. González, and P. Richard, Phys. Rev. A 69, 052718 (2004).

[3] C. P. Bhalla, Phys. Rev. Lett. 64, 1103 (1990).

[4] P. Hvelplund, A. D. Gonzalez, P. Dahl, and C. P. Bhalla, Phys. Rev. A 49, 2535 (1994).

[5] P. Richard, C. P. Bhalla, S. Hagmann, and P. A. Závodszky, Phys. Scr. T80, 87 (1999).

[6] S. Ricz, B. Sulik, N. Stolterfoht, and I. Kádár, Phys. Rev. A 47, 1930 (1993).

[7] N. Stolterfoht et al., Phys. Rev. A 48, 2986 (1993).

[8] B. Sulik, S. Ricz, I. Kadar, G. Xiao, G. Schiwietz, K. Sommer, P.L Grande, R. Koehrbrueck, M. Grether, and N. Stolterfoht, Phys. Rev. A 52, 387 (1995).

[9] G. Toth et al., Nucl. Instrum. Methods Phys. Res. B 124, 413 (1997).

[10] H. P. Hülskötter, W. E. Meyerhof, E. Dillard, and N. Guardala, Phys. Rev. Lett. 63, 1938 (1989).

[11] M. B. Shah and H. B. Gilbody, J. Phys. B 24, 977 (1991).

[12] D. H. Lee, T. J. M. Zouros, J. M. Sanders, P. Richard, J. M. Anthony, Y. D. Wang, and J. H. McGuire,, Phys. Rev. A 46, 1374 (1992).

[13] E. C. Montenegro, W. S. Melo, W. E. Meyerhof, and A. G. de Pinho, Phys. Rev. Lett. 69, 3033 (1992).

[14] N. Stolterfoht, Phys. Scr. 42, 192 (1990).

[15] E. C. Montenegro, W. E. Meyerhof, and J. H. McGuire, Adv. At. Mol. & Opt. Phys. 34, 249 (1994).

[16] T. J. M. Zouros, Comm. At. Mol. Phys. 32, 291 (1996).

[17] N. Stolterfoht et al., Nucl. Instrum. Methods Phys. Res. B 24/25, 168 (1987).

[18] D. H. Lee, Ph.D. dissertation, Kansas State University, 1990, (unpublished).

[19] B. Sulik, T. J. M. Zouros, A. Orbán, and L. Gulyás, J. Electron Spectrosc. and Relat. Phenom. 114-116, 191 (2001).

[20] I. Ben–-Itzhak, T. J. Gray, J. C. Legg, and J. H. McGuire, Phys. Rev. A 37, 3685 (1988).

[21] V. A. Sidorovich, V. S. Nikolaev, and J. H. McGuire, Phys. Rev. A 31, 2193 (1985).

[22] J. M. Cheshire, Proc. R. Soc. London A 83, 227 (1964); Dz. Belki\'c, R. Gayet, and A. Salin, Phys. Rep. 56, 279 (1979); P. D. Fainstein, V. H. Ponce, and R. D. Rivarola, J. Phys. B 24, 3091 (1991); G. R. Deco and R. D. Rivarola, J. Phys. B 18, 2283 (1985); ibid. J. Phys. B 19, 1759 (1986).

[23] G. Schiwietz and P.L. Grande, Radiat. Eff. & Defects in Solids 130-131, 137 (1994).

[24] L. C. Tribedi et al., Phys. Rev. A 54, 2154 (1996); ibid., J. Phys. B 31, L369 (1998).

[25] M. E. Galassi, R. D. Rivarola, P. D. Fainstein, and N. Stolterfoht, Phys. Rev. A 66, 052705 (2002).

[26] M. H. Chen, Phys. Rev. A 45, 1684 (1992).

[27] B. F. Davis and K. T. Chung, Phys. Rev. A 36, 1948 (1987); ibid. Phys. Rev. A 39, 3942 (1989); D. Charalambidis, R. Brenn, and K. J. Koulen, Phys. Rev. A 40, 2359 (1989).

[28] N. Stolterfoht, D. Schneider, R. Mann, and F. Folkmann, J. Phys. B 10, L281 (1977); R. Mann, H. F. Beyer, and F. Folkmann, Phys. Rev. Lett. 46, 646 (1981); S. Mannervik, Phy. Scr. 22, 575 (1981).

[29] S. Bliman et al., J. Phys. B 25, 2065 (1992).

Received on 29 July, 2005

  • [1] T. J. M. Zouros, D. H. Lee, and P. Richard, Phys. Rev. Lett. 62, 2261 (1989).
  • [2] E. P. Benis, T.J.M. Zouros, T.W. Gorczyca, A.D. González, and P. Richard, Phys. Rev. A 69, 052718 (2004).
  • [3] C. P. Bhalla, Phys. Rev. Lett. 64, 1103 (1990).
  • [4] P. Hvelplund, A. D. Gonzalez, P. Dahl, and C. P. Bhalla, Phys. Rev. A 49, 2535 (1994).
  • [5] P. Richard, C. P. Bhalla, S. Hagmann, and P. A. Závodszky, Phys. Scr. T80, 87 (1999).
  • [6] S. Ricz, B. Sulik, N. Stolterfoht, and I. Kádár, Phys. Rev. A 47, 1930 (1993).
  • [7] N. Stolterfoht et al., Phys. Rev. A 48, 2986 (1993).
  • [8] B. Sulik, S. Ricz, I. Kadar, G. Xiao, G. Schiwietz, K. Sommer, P.L Grande, R. Koehrbrueck, M. Grether, and N. Stolterfoht, Phys. Rev. A 52, 387 (1995).
  • [9] G. Toth et al., Nucl. Instrum. Methods Phys. Res. B 124, 413 (1997).
  • [10] H. P. Hülskötter, W. E. Meyerhof, E. Dillard, and N. Guardala, Phys. Rev. Lett. 63, 1938 (1989).
  • [11] M. B. Shah and H. B. Gilbody, J. Phys. B 24, 977 (1991).
  • [12] D. H. Lee, T. J. M. Zouros, J. M. Sanders, P. Richard, J. M. Anthony, Y. D. Wang, and J. H. McGuire,, Phys. Rev. A 46, 1374 (1992).
  • [13] E. C. Montenegro, W. S. Melo, W. E. Meyerhof, and A. G. de Pinho, Phys. Rev. Lett. 69, 3033 (1992).
  • [14] N. Stolterfoht, Phys. Scr. 42, 192 (1990).
  • [15] E. C. Montenegro, W. E. Meyerhof, and J. H. McGuire, Adv. At. Mol. & Opt. Phys. 34, 249 (1994).
  • [16] T. J. M. Zouros, Comm. At. Mol. Phys. 32, 291 (1996).
  • [17] N. Stolterfoht et al., Nucl. Instrum. Methods Phys. Res. B 24/25, 168 (1987).
  • [19] B. Sulik, T. J. M. Zouros, A. Orbán, and L. Gulyás, J. Electron Spectrosc. and Relat. Phenom. 114-116, 191 (2001).
  • [20] I. Ben-Itzhak, T. J. Gray, J. C. Legg, and J. H. McGuire, Phys. Rev. A 37, 3685 (1988).
  • [21] V. A. Sidorovich, V. S. Nikolaev, and J. H. McGuire, Phys. Rev. A 31, 2193 (1985).
  • [22] J. M. Cheshire, Proc. R. Soc. London A 83, 227 (1964);
  • Dz. Belki\'c, R. Gayet, and A. Salin, Phys. Rep. 56, 279 (1979);
  • P. D. Fainstein, V. H. Ponce, and R. D. Rivarola, J. Phys. B 24, 3091 (1991);
  • G. R. Deco and R. D. Rivarola, J. Phys. B 18, 2283 (1985);
  • [23] G. Schiwietz and P.L. Grande, Radiat. Eff. & Defects in Solids 130-131, 137 (1994).
  • [24] L. C. Tribedi et al., Phys. Rev. A 54, 2154 (1996);
  • [25] M. E. Galassi, R. D. Rivarola, P. D. Fainstein, and N. Stolterfoht, Phys. Rev. A 66, 052705 (2002).
  • [26] M. H. Chen, Phys. Rev. A 45, 1684 (1992).
  • [27] B. F. Davis and K. T. Chung, Phys. Rev. A 36, 1948 (1987);
  • ibid. Phys. Rev. A 39, 3942 (1989); D. Charalambidis, R. Brenn, and K. J. Koulen, Phys. Rev. A 40, 2359 (1989).
  • [28] N. Stolterfoht, D. Schneider, R. Mann, and F. Folkmann, J. Phys. B 10, L281 (1977);
  • R. Mann, H. F. Beyer, and F. Folkmann, Phys. Rev. Lett. 46, 646 (1981);
  • S. Mannervik, Phy. Scr. 22, 575 (1981).
  • [29] S. Bliman et al., J. Phys. B 25, 2065 (1992).

Publication Dates

  • Publication in this collection
    31 July 2006
  • Date of issue
    June 2006
Sociedade Brasileira de Física Caixa Postal 66328, 05315-970 São Paulo SP - Brazil, Tel.: +55 11 3091-6922, Fax: (55 11) 3816-2063 - São Paulo - SP - Brazil
E-mail: sbfisica@sbfisica.org.br