Photoionization of neutral iron from the ground and excited states

Autor: Swaraj Tayal, Klaus Bartschat, L. Fernández-Menchero, Oleg Zatsarinny

Publikováno v: Zatsarinny, O, Bartschat, K, Fernandez Menchero, L & Tayal, S S 2019, ' Photoionization of neutral iron from the ground and excited states ', Physical Review A, vol. 99, no. 2, pp. 023430 . https://doi.org/10.1103/PhysRevA.99.023430

The B-spline R-matrix method is used to investigate the photoionization of neutral iron from the ground and excited states in the energy region from the ionization thresholds to 2 Ry. The multiconfiguration Hartree-Fock method in connection with adju

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https://doi.org/10.1103/physreva.99.023430

Collision and Radiative Parameters for Cr ii Lines Observed in Stellar and Nebular Spectra

Autor: Swaraj Tayal, Oleg Zatsarinny

Publikováno v: The Astrophysical Journal. 888:10

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::9f4bf6a25ec0082b0d608196e07063af
https://doi.org/10.3847/1538-4357/ab557b

Breit‐PauliR‐Matrix Calculation for Electron Impact Collision Strengths and Rates of Ovi

Autor: Swaraj Tayal

Publikováno v: The Astrophysical Journal. 582:550-557

The Breit-Pauli R-matrix with pseudostates approach has been used to calculate electron collisional excitation strengths for transitions between the 24 lowest fine-structure levels belonging to 14 LS terms (ns 2S, np 2P0 [n = 2-5], nd 2D [n = 3-5], n

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https://doi.org/10.1086/344569

Electron impact excitation of O III

Autor: Swaraj Tayal, Oleg Zatsarinny

Publikováno v: Journal of Physics: Conference Series. 875:052002

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::579e7e86e041e09c688b5b7520d238bf
https://doi.org/10.1088/1742-6596/875/6/052002

Electron Excitation Cross Sections for the \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $3s^{2}3p^{2}$ \end{document} \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $^{3}Parrow 3s3p^{3}$ \end{document} \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $^{5}S^{o}$ \end{document} Transition in \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $\mathrm{S}\,^{2+}$ \end{document}

Autor: S. J. Smith, A. Chutjian, Swaraj Tayal, Jason B. Greenwood

Publikováno v: The Astrophysical Journal. 541:501-505

Experimental and theoretical collisional excitation cross sections are reported for the 3s23p2 3P → 3s3p3 5So spin-forbidden transition in S2+. The transition energies (wavelengths) are 7.171 eV (1728.9 A, J = 2 → 2) and 7.237 eV (1713.1 A, J = 2

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https://doi.org/10.1086/309405