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Dive into the research topics where Anil K. Pradhan is active.

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Featured researches published by Anil K. Pradhan.


Physical Review A | 2007

Breakdown of the quasistatic approximation at high densities and its effect on the heliumlike Kα complex of nickel, iron, and calcium

Justin Oelgoetz; Christopher J. Fontes; Hong Lin Zhang; Anil K. Pradhan

The General Spectral Modeling (GSM) code employs the quasi-static approximation, a standard, low-density methodology that assumes the ionization balance is separable from a determination of the excited-state populations that give rise to the spectra. GSM also allows for some states to be treated only as contributions to effective rates. While these two approximations are known to be valid at low densities, this work investigates using such methods to model high-density, non-LTE emission spectra and determines at what point the approximations break down by comparing to spectra produced by the LANL code ATOMIC which makes no such approximations. As both approximations are used by other astrophysical and low-density modeling codes, the results should be of broad interest. He-like K


Archive | 2011

Re-examination of Stellar Interior Opacities and the Solar Abundances Problem

Anil K. Pradhan; Sultana N. Nahar; Marc H. Pinsonneault; James Bailey

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Archive | 2011

Anomalous Abundances in Gaseous Nebulae From Recombination and Collisional Lines: Improved Photoionization and Recombination Studies

Anil K. Pradhan; Sultana N. Nahar; Werner Eissner; Maximiliano Montenegro

emission spectra are presented for Ni, Fe, and Ca, in order to gauge the effect of both approximations employed in GSM. This work confirms that at and above the temperature of maximum abundance of the He-like ionization stage, the range of validity for both approximations is sufficient for modeling the low- and moderate-density regimes one typically finds in astrophysical and magnetically confined fusion plasmas. However, a breakdown does occur for high densities; we obtain quantitative limits that are significantly higher than previous works. This work demonstrates that, while the range of validity for both approximations is sufficient to predict the density-dependent quenching of the z line, the approximations break down at higher densities. Thus these approximations should be used with greater care when modeling high-density plasmas such as those found in inertial confinement fusion and electromagnetic pinch devices.


Archive | 2011

Effective collision strengths and A-values

Anil K. Pradhan; Sultana N. Nahar


Archive | 2011

Angular algebra and generalized radiative transitions

Anil K. Pradhan; Sultana N. Nahar


Archive | 2011

Coefficients of the fine structure components of an LS multiplet

Anil K. Pradhan; Sultana N. Nahar


Archive | 2011

Atomic Astrophysics and Spectroscopy: Atomic processes

Anil K. Pradhan; Sultana N. Nahar


Archive | 2011

Atomic Astrophysics and Spectroscopy: Radiative transitions

Anil K. Pradhan; Sultana N. Nahar


Archive | 2011

Atomic Astrophysics and Spectroscopy: Gaseous nebulae and H II regions

Anil K. Pradhan; Sultana N. Nahar


Archive | 2011

K α transition probabilities for platinum and uranium ions for possible X-ray biomedical

Sultana N. Nahar; Anil K. Pradhan; Sara Lim

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Justin Oelgoetz

Los Alamos National Laboratory

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Christopher J. Fontes

Los Alamos National Laboratory

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Hong Lin Zhang

Los Alamos National Laboratory

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Alberto Rodriguez-Ardila

National Council for Scientific and Technological Development

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T. A. A. Sigut

University of Western Ontario

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