Ionization of He, Ne, Ar, Kr, and Xe by proton impact: Single differential distributions in energy and angles

In this paper we report energy and angular distributions of electrons emitted in collisions of protons with neon- (F-, Ne0, Na+), argon- (Cl-, Ar0, K+), krypton- (Br-, Kr0, Rb+), and xenon- (I-, Xe0) isoelectronic series for high and intermediate impact energies. Calculations were performed within t...

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Autor principal: Miraglia, Jorge Esteban
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Lenguaje:Inglés
Publicado: 2009
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100 1 |a Miraglia, Jorge Esteban 
245 1 0 |a Ionization of He, Ne, Ar, Kr, and Xe by proton impact: Single differential distributions in energy and angles 
260 |c 2009 
270 1 0 |m Miraglia, J. E.; Instituto de Astronomía y Física Del Espacio, Consejo Nacional de Investigaciones Científicas y Técnicas, Universidad de Buenos Aires, Casilla de Correo 67, Sucursal 28, C1428EGA, Buenos Aires, Argentina 
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504 |a Ederer, D.L., (1964) Phys. Rev. Lett., 13, p. 760. , It is interesting to recall the photoionization of 4dXe presents a maximum at 100 eV [10.1103/PhysRevLett.13.760 
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504 |a The experimental recommended value in Ref. is 5.07±0.50 a.u. Other experiments of proton on Ar at 1 MeV give similar values, for example, Ref. reports 4.39±0.85, Ref. reports 5.57±0.32, and Ref. reports 4.57±0.46; Manson, S.T., Toburen, L.H., Madison, D.H., Stotelfoht, N., (1975) Phys. Rev. A, 12, p. 60. , 10.1103/PhysRevA.12.60 
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506 |2 openaire  |e Política editorial 
520 3 |a In this paper we report energy and angular distributions of electrons emitted in collisions of protons with neon- (F-, Ne0, Na+), argon- (Cl-, Ar0, K+), krypton- (Br-, Kr0, Rb+), and xenon- (I-, Xe0) isoelectronic series for high and intermediate impact energies. Calculations were performed within the continuum distorted wave-eikonal initial-state method using an angular expansion in spherical harmonics and a numerical evaluation of the radial functions corresponding to both: the initial (bound) and the final (continuum) states in the same central potential. The first Born approximation was calculated on equal footing. The shellwise local plasma approximation was also calculated when possible. A complete and exhaustive comparison with the available experimental data is carried out. We have spanned almost all the published experiments in our range of interest. Successes and failures of the different theoretical methods are pointed out. Possible signatures of many-electron effects are noticed. © 2009 The American Physical Society.  |l eng 
593 |a Instituto de Astronomía y Física Del Espacio, Consejo Nacional de Investigaciones Científicas y Técnicas, Universidad de Buenos Aires, Casilla de Correo 67, Sucursal 28, C1428EGA, Buenos Aires, Argentina 
650 1 7 |2 spines  |a ARGON 
650 1 7 |2 spines  |a NEON 
650 1 7 |2 spines  |a XENON 
690 1 0 |a ANGULAR DISTRIBUTION 
690 1 0 |a APPROXIMATION THEORY 
690 1 0 |a ATOMS 
690 1 0 |a BORN APPROXIMATION 
690 1 0 |a DISTORTION (WAVES) 
690 1 0 |a HARMONIC ANALYSIS 
690 1 0 |a HELIUM 
690 1 0 |a IMPACT IONIZATION 
690 1 0 |a KRYPTON 
690 1 0 |a PROTONS 
690 1 0 |a RUBIDIUM 
690 1 0 |a SODIUM 
690 1 0 |a ANGULAR EXPANSIONS 
690 1 0 |a CENTRAL POTENTIALS 
690 1 0 |a CONTINUUM DISTORTED WAVES 
690 1 0 |a EIKONAL 
690 1 0 |a ELECTRON EFFECTS 
690 1 0 |a EXPERIMENTAL DATUM 
690 1 0 |a FIRST BORN APPROXIMATIONS 
690 1 0 |a IMPACT ENERGIES 
690 1 0 |a ISO-ELECTRONIC SERIES 
690 1 0 |a NUMERICAL EVALUATIONS 
690 1 0 |a PROTON IMPACTS 
690 1 0 |a RADIAL FUNCTIONS 
690 1 0 |a SINGLE DIFFERENTIALS 
690 1 0 |a SPHERICAL HARMONICS 
773 0 |d 2009  |g v. 79  |k n. 2  |p Phys Rev A  |x 10502947  |t Physical Review A - Atomic, Molecular, and Optical Physics 
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