Calculation of electron-impact rotationally elastic total cross sections for NH<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msub><mml:mrow/><mml:mrow><mml:mn>3</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math>, H<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msub><mml:mrow/><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math>S, and PH<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msub><mml:mrow/><mml:mrow><mml:mn>3</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math>over the energy range from 0.01 eV to 2 keV-Reference-Cited by-同舟云学术

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Calculation of electron-impact rotationally elastic total cross sections for NH3, H2S, and PH3over the energy range from 0.01 eV to 2 keV

Published:2011-04-18 Issue:4 Volume:83 Page:
ISSN:1050-2947
Container-title:Physical Review A
language:en
Short-container-title:Phys. Rev. A

Author:

Limbachiya Chetan,Vinodkumar Minaxi,Mason Nigel

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevA.83.042708/fulltext

Reference58 articles.

1. Electron impact calculations of total elastic cross sections over a wide energy range – 0.01 eV to 2 keV for CH4, SiH4 and H2O

2. The Jovian spectrum in the region 0.4–1.1 µm: The C/H ratio

3. Near infrared reflection spectra of ammonia frost: Interpretation of the upper clouds of Saturn

4. Scattering of cold electrons by ammonia, hydrogen sulfide, and carbonyl sulfide

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