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eISSN: 2576-4543

Physics & Astronomy International Journal

Short Communication Volume 3 Issue 6

Electron impact ionization of helium, neon and argon at intermediate energies

RI Campeanu

Department of Physics and Astronomy, York University, Canada

Correspondence: RI Campeanu, Professor, Department of Physics and Astronomy, 3059 DB, York University, 4700 Keele Street, Toronto, Canada, Tel 1-905-882-1173, Fax 1-416- 7365287

Received: October 13, 2019 | Published: November 7, 2019

Citation: Campeanu RI. Electron impact ionization of helium, neon and argon at intermediate energies. Phys Astron Int J. 2019;3(6):230-233. DOI: 10.15406/paij.2019.03.00188

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Abstract

With a relatively simple distorted-wave model, in which the ejected and the scattered electrons see different residual systems depending on their energies, in this paper we show the calculation of the CPE cross sections for electron impact ionization of He, Ne and Ar. Combined with the ‘maximum interference’ exchange approximation, this model gives results which for Ne and Ar are in better agreement with the experiment than the other existing theoretical models.

Keywords: electron impact ionization, noble gases, quantum models for atomic collisions

Abbreviations

CCC, convergent close coupling; BED, binary encounter dipole; CCO, coupled-channel-optical

Introduction

Ionization of noble gases by electron impact is a process for which accurate experimental integrated cross sections are available. We shall refer in this paper to the most recent data of Rejoub et al.1 On the theory side work is still needed for atoms heavier than helium. For helium the convergent close coupling (CCC) method2 can produce an excellent agreement with the experiment. In the CCC method the convergence of the results is tested by including an ever increasing set of target states. These target states are obtained by diagonalizing the target Hamiltonian in an orthogonal Laguerre basis. Excellent agreement with the experiment is also obtained with the binary encounter dipole (BED) model.3 In this approximation the continuum dipole oscillator strength is calculated from the relativistic random-phase approximation. The CCC and the BED methods were not applied to heavier targets than helium.

The distorted wave Born approximation is another method to obtain electron impact ionization cross sections for helium.4 This is a first-order perturbation theory, which can be easily applied to other heavier targets. An elaborate calculation with this model, using distorted waves calculated for static, exchange and polarization potentials, was able to reproduce the helium experimental ionization cross sections, except in the peak range where the theoretical cross sections are slightly higher than the measurements.

For neon and argon theoretical cross sections produced by various methods are in general significantly higher than the experimental data. These methods include time-dependent close coupling calculations of Pindzola et al.5 This paper presents cross sections for the ionization of one of the outer shell electrons of neon. The inner shell electrons are treated with pseudopotentials, while the remaining core electrons of the outer shell are handled in a configuration-average approximation. Another paper in this group is the coupled-channel-optical (CCO) model of McCarthy and Zhou.6 CCO is a close coupling approximation which, in addition to the discrete channels, has a coupling potential that includes an ab initio polarization part describing the excitation of the continuum. This paper presents CCO ionization cross sections for all noble gases. The distorted-wave-R-matrix hybrid model of Bartschat and Burke7 uses a two-state R-matrix approach in combination with a distorted-wave Born approximation. Their paper presents electron impact ionization cross sections for argon. The distorted wave Born approximation was applied by Younger8 to the calculation of the electron impact ionization of argon. In this paper the distorted waves were obtained for potentials which accounted for the interaction between the free particles and the target nucleus and bound electrons.

A different situation exists in the case of positron impact ionization, where for all the noble gases simple distorted-wave models can produce cross sections which are in good agreement with some experiments.9 One such model is CPE, a model which considers the full energy range of the ionization system and represents the leptons with either Coulomb or plane waves. Model CPE was introduced by Campeanu et al.10 for positron impact ionization of helium. CPE will be discussed in detail in the next section. This paper presents CPE cross sections for electron impact ionization of He, Ne and Ar.

The electron impact ionization

The electron impact ionization total cross section can be written as:

Q( E i )  = 16 π E i 0 E/2  dEe l i l e l f    ( 2L+1 )   l( l i l e l f   ) MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcLbsacaWGrb qcfa4aaeWaaOqaaKqzGeGaamyraKqbaoaaBaaaleaajugWaiaadMga aSqabaaakiaawIcacaGLPaaaqaaaaaaaaaWdbiaacckacaGGGcqcLb sapaGaeyypa0tcfa4aaSaaaeaacaaIXaGaaGOnaaqaaiabec8aWjaa dwealmaaBaaajuaGbaqcLbmacaWGPbaajuaGbeaaaaGaey4kIi=aa0 baaeaajugWaiaaicdaaKqbagaajugWaiaadweacaGGVaGaaGOmaaaa k8qacaGGGcqcfa4daiaadsgacaWGfbGaamyzamaaqababaWdbiaacc kapaWaaeWaaeaacaaIYaGaamitaiabgUcaRiaaigdaaiaawIcacaGL PaaapeGaaiiOaiaacckacaGGGcWdaiaadYgadaqadaqaa8qacaWGSb WdamaaBaaabaWdbmaaBaaabaqcLbmacaWGPbaajuaGbeaaa8aabeaa peGaamiBa8aadaWgaaqaa8qadaWgaaqaaKqzadGaamyzaaqcfayaba aapaqabaWdbiaadYgapaWaaSbaaeaapeWaaSbaaeaajugWaiaadAga aKqbagqaaiaacckaa8aabeaaaiaawIcacaGLPaaaaeaapeGaamiBaS WdamaaBaaajuaGbaqcLbmapeGaamyAaaqcfa4daeqaa8qacaWGSbWa aSbaaeaal8aadaWgaaqcfayaaKqzadWdbiaadwgaaKqba+aabeaaa8 qabeaacaWGSbWdamaaBaaabaWdbmaaBaaabaqcLbmacaWGMbaajuaG beaacaGGGcaapaqabaaabeGaeyyeIuoaaaa@7FC5@   (1)

where li le lf represent the orbital angular momentum quantum numbers of the incident, ejected and scattered electrons respectively, Ei is the energy of the incident electron, Ee the energy of the ejected electron, E=Ei–I Ee+Ef is the total energy of the scattered electrons, with I the ionization energy. I (li le lf) can be approximated in the ‘maximum interference’ model 11 as:

I ( l i l e l f ) = | F | 2 +  | G 0 | 2 | F || G 0 | MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcLbsaqaaaaa aaaaWdbiaadMeacaqGGaqcfa4damaabmaakeaajugib8qacaWGSbqc fa4damaaBaaaleaajugWa8qacaWGPbaal8aabeaajugib8qacaWGSb qcfa4damaaBaaaleaajugWa8qacaWGLbaal8aabeaajugib8qacaWG Sbqcfa4damaaBaaaleaajugWa8qacaWGMbaal8aabeaaaOGaayjkai aawMcaaKqzGeWdbiaabccacqGH9aqpjuaGpaWaaqWaaOqaaKqzGeWd biaadAeaaOWdaiaawEa7caGLiWoajuaGdaahaaWcbeqaaKqzadWdbi aaikdaaaqcLbsacqGHRaWkcaqGGaqcfa4damaaemaakeaajugib8qa caWGhbqcfa4damaaCaaaleqabaqcLbsapeGaaGimaaaaaOWdaiaawE a7caGLiWoajuaGdaahaaWcbeqaaKqzadWdbiaaikdaaaqcLbsacqGH sisljuaGpaWaaqWaaOqaaKqzGeWdbiaadAeaaOWdaiaawEa7caGLiW oajugibiaacYhapeGaam4raKqba+aadaahaaWcbeqaaKqzadWdbiaa icdaaaqcLbsapaGaaiiFaaaa@6C3B@   (2)

where F is the direct scattering amplitude and G0 the singlet exchange amplitude, defined by the same expression as F, but with the energies of the ejected and scattered electrons interchanged.

The scattering amplitudes are obtained by first calculating the wave functions of the leptons in different channels of the ionization system. In the model CPE these wave functions of the ejected and scattered electron were calculated numerically for an electrostatic potential which depends on their energies. In model CPE the incident electron sees a neutral atom and therefore  V i = 0. MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcLbsaqaaaaa aaaaWdbiaadAfajuaGpaWaaSbaaSqaaKqzadWdbiaadMgaaSWdaeqa aKqzGeWdbiabg2da9iaabccacaaIWaGaaiOlaaaa@3E43@

When the ejected electron is faster than the scattered electron (i.e. Ee>Ef ) it sees the residual atomic ion plus the scattered electron, which we approximate to be the neutral atom. Consequently for these energies we use Ve = 0. We assume that the scattered electron sees only the atomic ion and therefore  V f = 1 r . MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcLbsaqaaaaa aaaaWdbiaadAfajuaGpaWaaSbaaSqaaiaadAgaaeqaaKqzGeGaeyyp a0JaeyOeI0scfa4aaSaaaeaacaaIXaaabaGaamOCaaaacaGGUaaaaa@3EB8@

When the ejected electron is slower than the scattered electron (i.e. Ee<Ef ) it sees only the residual He+ and we use   V e = 1 r . MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcLbsaqaaaaa aaaaWdbiaadAfajuaGpaWaaSbaaSqaaiaadwgaaeqaaKqzGeGaeyyp a0JaeyOeI0scfa4aaSaaaeaacaaIXaaabaGaamOCaaaacaGGUaaaaa@3EB7@   For these energies it is the scattered electron which sees both the residual atomic ion and the ejected electron, which we approximate to be a neutral atom  ( i.e. V i = 0 ). MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaaeaaaaaaaaa8 qadaqadaqaaiaadMgacaGGUaGaamyzaiaac6cajugibiaadAfajuaG paWaaSbaaSqaaKqzadWdbiaadMgaaSWdaeqaaKqzGeWdbiabg2da9i aabccacaaIWaaakiaawIcacaGLPaaajugibiaac6caaaa@43A1@

We also introduce model DCPE which is different from CPE only in the representation of the channels which use plane waves (i.e. with the potential V=0). In DCPE we replace V=0 with the sum the static and polarization potentials:  V =  V st + V pol . MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcLbsaqaaaaa aaaaWdbiaadAfacaqGGaGaeyypa0JaaeiiaiaadAfajuaGpaWaaSba aSqaaKqzadWdbiaadohacaWG0baal8aabeaajugib8qacqGHRaWkca WGwbqcfa4damaaBaaaleaajugWa8qacaWGWbGaam4BaiaadYgaaSWd aeqaaKqzGeGaaiOlaaaa@4751@

Electron impact ionization cross sections for He, Ne and Ar

Table 1 presents our total ionization cross-sections for helium. This table shows that the DCPE data are only slightly higher than the CPE data. As the same situation was found to be true for neon and argon we shall not present the DCPE results in the graphs.

Energy (eV)             

He(total)

CPE

CPE

50

0.233

0.240

60

0.307

0.314

80

0.386

0.391

100

0.409

0.412

120

0.41

0.414

200

0.350

0.354

300

0.270

0.274

400

0.230

0.233

500

0.198

0.201

Table 1 Electron-helium ionization cross sections (in 10-16 cm2) in the CPE and DCPE models

Figure 1 presents the comparison of our CPE results and the experimental data of Rejoub et al.1 In addition to the CPE data Figure 1 also contains the DWE data from the paper by Campeanu et al.4 and the coupled-channel-optical (CCO) results of McCarthy and Zhou.6 We do not present the results of references2 and,3 which are in perfect agreement with the experiment.

Figure 1 Total cross-sections for electron impact ionization of He as a function of the electron impact energy.
The experimental points are from Rejoub et al.1 The short dashed line corresponds to reference,6 the long dashed curve to reference4  and the solid line to model CPE.

This figure shows that the distorted wave method provides a better agreement with the experiment than the CCO method. We also found that the agreement with the experiment is quite similar for both distorted wave models in spite of the differences in their complexity. The DWE calculation of reference4 employed in all scattering channels elaborate distortion potentials containing the static potential, polarization, and exchange. The CPE model contains by comparison very simple descriptions of the various scattering channels. In spite of these theoretical differences both models produce cross sections in good agreement with the experiment except in the peak range where they are higher than the experiment by maximum 13.8%.

Table 2 and Table 3 present total cross sections for the ionization of the two most external shells of neon and argon. For argon we also added the contribution from the 2p and 2s shells, which have an impact on the total cross sections for the 500 eV case.

Energy (eV)         

Energy (eV)         

Ne(2s)                

Ne(total)

60

0.403

0.139

80

0.559

0.559

100

0.596

0.077

0.673

120

0.601

0.108

0.708

200

0.543

0.165

0.728

350

0.409

0.164

0.728

500

0.323

0.139

0.462

Table 2 Electron-neon ionization cross sections (in 10-16 cm2) in the CPE model

Energy (eV)       

Ar(3p)              

Ar(3s)          

Ar(2s+2p)           

Ar(total)

30

Ar(total)

1.364

40

1.957

1.957

60

2.409

0.251

2.660

80

2.464

0.442

2.906

100

2.385

0.542

2.927

120

2.262

0.581

2.843

200

1.748

0.546

2.294

350

1.075

0.368

1.443

500

0.711

0.249

0.15

1.110

Table 3 Electron-argon ionization cross sections (in 10-16 cm2) in the CPE model

Figure 2 and Figure 3 compare the sum of the shell ionization cross sections with the experimental data. Figure 2 shows that the time-dependent close coupling calculations of Pindzola et al.5 are well above the experiment, while the CCO model of McCarthy and Zhou6 agrees with the experiment for impact energies higher than 200 eV. For lower energies the CCO curve is significantly above the experiment. Our CPE model is the best agreement with the experiment. A small disagreement of maximum 8% is seen in the peak area, where CPE data are above the experiment.

Figure 2 Total cross-sections for electron impact ionization of Ne as a function of the electron impact energy. The experimental points are from Rejoub et al.,1 the short dashed curve corresponds to reference,5 the long dashed line to reference6 and the solid line to model CPE.

Figure 3 shows that the distorted-wave-R-matrix hybrid models7 and the distorted wave model of Younger8 produce cross sections well above the experiment. The agreement with the experiment is better in the case of the COO method.6 Our CPE cross sections are in the best agreement with the experiment. The disagreement in the peak area between our data and the experiment is at the level of the He agreement (i.e. CPE data are higher than the experiment by maximum 13.8%).

Figure 3 Total cross-sections for electron impact ionization of Ar as a function of the electron impact energy. The experimental points are from Rejoub et al.1 the shortest dashed curve corresponds to reference,7 the intermediate dashed line to reference,6 the longest dashed line to reference8 and the solid line to model CPE.

Conclusion

This work demonstrates that the distorted-wave model CPE can produce good agreement with experiments for electron impact ionization of He, Ne and Ar. We found that for helium CPE model produces results which have a very similar agreement with the experiment as the elaborate distorted-wave model DWE of reference.4 For neon and argon our CPE results are in better agreement with the experiment than the other existing theoretical data. For argon the agreement with the experiment is at the level of the helium case, with the theory being above the experiment in the peak range, while for neon the agreement of CPE with the experiment is better that in the helium and argon cases. We conclude that relatively simple distorted-wave models of electron impact ionization of He, Ne and Ar can achieve the same level of success as in the positron impact case if the post-collision interactions are correctly represented.

Acknowledgments

None.

Funding details

None.

Conflicts of interest

The author declares that there is no conflict of interest.

References

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