CDW-EIS calculations for multiple ionization of Ne, Ar, Kr and Xe by the impact of H+ and He+, including post-collisional electron emission

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We present theoretical single to quintuple ionization cross sections for Ne, Ar, Kr and Xe bombarded by H+ and He+. Post-collisional contributions due to Auger-like processes are taken into account using recent photoionization data. The present continuum distorted wave-eikonal initial state (CDW-EIS...

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Autor principal: Montanari, C.C
Otros Autores: Montenegro, E.C, Miraglia, Jorge Esteban
Formato: Capítulo de libro
Lenguaje:Inglés
Publicado: 2010
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XENON
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100 1 |a Montanari, C.C. 
245 1 0 |a CDW-EIS calculations for multiple ionization of Ne, Ar, Kr and Xe by the impact of H+ and He+, including post-collisional electron emission 
260 |c 2010 
270 1 0 |m Montanari, C. C.; Instituto de Astronomìa y Fìsica del Espacio, casilla de correo 67 ,Asucursal 28, C1428EGA, Buenos Aires, Argentina; email: mclaudia@iafe.uba.ar 
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506 |2 openaire  |e Política editorial 
520 3 |a We present theoretical single to quintuple ionization cross sections for Ne, Ar, Kr and Xe bombarded by H+ and He+. Post-collisional contributions due to Auger-like processes are taken into account using recent photoionization data. The present continuum distorted wave-eikonal initial state (CDW-EIS) and first Born approximation results are compared with the experimental data available in the energy range of 50-10 000 keV amu-1 for H+ on Ne and Ar, and 50-1000 keV amu -1 for the other cases. In general, the combination of the CDW-EIS with the post-collisional branching ratios describes well the multiple ionization data above 300 keV amu-1, showing a clear tendency to coalesce with the first Born approximation at high energies. The surprising result of this work is the good performance of the first Born approximation which describes rather well the experimental data of double and triple ionization, even in the intermediate energy range (50-300 keV amu-1), where direct ionization is the dominant contribution. © 2010 IOP Publishing Ltd.  |l eng 
593 |a Instituto de Astronomìa y Fìsica del Espacio, casilla de correo 67 ,Asucursal 28, C1428EGA, Buenos Aires, Argentina 
593 |a Departamento de Fìsica, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Buenos Aires, Argentina 
593 |a Instituto de Fìsica, Universidade Federal de Rio de Janeiro, Caixa Postal 68528, Rio de Janeiro 21945-970, RJ, Brazil 
650 1 7 |2 spines  |a NEON 
650 1 7 |2 spines  |a XENON 
690 1 0 |a BRANCHING RATIO 
690 1 0 |a COLLISIONAL CONTRIBUTIONS 
690 1 0 |a CONTINUUM DISTORTED WAVE-EIKONAL INITIAL STATE 
690 1 0 |a DOMINANT CONTRIBUTIONS 
690 1 0 |a ENERGY RANGES 
690 1 0 |a EXPERIMENTAL DATA 
690 1 0 |a FIRST BORN APPROXIMATION 
690 1 0 |a HIGH ENERGY 
690 1 0 |a INTERMEDIATE ENERGY RANGE 
690 1 0 |a IONIZATION CROSS SECTION 
690 1 0 |a MULTIPLE IONIZATION 
690 1 0 |a BORN APPROXIMATION 
690 1 0 |a CHARGE DENSITY WAVES 
690 1 0 |a ELECTROCHEMICAL CORROSION 
690 1 0 |a HIGH ENERGY PHYSICS 
690 1 0 |a KRYPTON 
690 1 0 |a PARTICLE DETECTORS 
690 1 0 |a QUANTUM THEORY 
690 1 0 |a IONIZATION 
700 1 |a Montenegro, E.C. 
700 1 |a Miraglia, Jorge Esteban 
773 0 |d 2010  |g v. 43  |k n. 16  |p J Phys B At Mol Opt Phys  |x 09534075  |w (AR-BaUEN)CENRE-332  |t Journal of Physics B: Atomic, Molecular and Optical Physics 
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