ANIL K. PRADHAN

Professor, Department of Astronomy, Adjunct Professor, Chemical Physics, The Ohio State University

E-mail: pradhan@astronomy.ohio-state.edu OR pradhan.1@osu.edu, Ph: 614-292-5850, Fax: 614-292-2928



MAIN RESEARCH AREAS

PHOTOIONIZATION
RECOMBINATION
COLLISION STRENGTHS
TRANSITION PROBABILITIES
ASTROPHYSICAL SPECTROSCOPY
OPACITIES

DATABASE (Updates: Nahar)

ENERGY LEVELS
ELECTRON IMPACT EXCITATION
ELECTRON-ION RECOMBINATION
TRANSITION PROBABILITIES
PHOTOIONIZATION CROSS SECTIONS

COURSES TAUGHT

Astronomy 161 - Solar System
Astronomy 162 - Stars and Galaxies
Astronomy 823 - Astrophysical Spectroscopy (Graduate)
Astronomy 641 - Stellar Astrophysics
Scattering Theory (Graduate), Univ. of Colorado
Atomic Physics (Graduate), Univ. of Windsor

ATOMIC ASTROPHYSICS AND SPECTROSCOPY

AND

COMPUTATIONAL NANOSPECTROSCOPY

Greetings! This homepage reports the research by the OSU Atomic Astrophysics Group, with senior Research Scientist Sultana Nahar, Postdoctoral Fellow Chiranjib Sur, Graduate student Maximiliano Montenegro and collaborators.

Research interests are theoretical studies of radiative and collisional atomic processes, and spectral formation in astrophysical plasmas - an integrated program of atomic physics and astronomy.

New directions in theoretical atomic physics research include a combination of Relativistic Coupled Cluster Method (RCCM) and the R-matrix method.

This website will also report on the activties of a new INTERDISCIPLINARY COMPUTATIONAL NANOSCIENCE initiative devoted to nanospectroscopy of material and biological nanostrcutures. The group comprises of Russell Pitzer (Chemistry), Sultana Nahar (Astronomy), Yan Yu (Thomas Jefferson University Medical School), postdoctoral fellow Chiranjib Sur, and graduate students Mike Mrozik, and Maximiliano Montenegro. The program was supported by a Large Interdisciplinary Grant Award from the OSU Office of Research, College of Mathematical and Physical Sciences, and the Department of Astronomy.


The OSU group represents the U.S. participants in the international Opacity Project (OP) , and the Iron Project (IP/RmaX) Network aimed at large-scale atomic calculations using the relativistic R-matrix method for iron-peak elements and X-ray astrophysics. The databases TIPTOPBASE and OPSERVER offer OP and IP atomic data, and on-line calculation of "customized" astrophysical opacities, at the Ohio Supercomputer Center in Columbus Ohio.

This homepage is also intended as a guide to recommended ATOMIC DATA for astrophysical and laboratory applications. In addition, the database Nahar OSU Radiative Data (NORAD) contains a large number of datafiles for energy levels, transition probabilities, photoionization cross sections, and total and partial (electron+ion) recombination rate coefficients (including radiative and dielectronic recombination processes in a unified and ab initio manner using the R-matrix method).

The radiative data supercede earlier TOPbase data.


HIGH ACCURACY ATOMIC PHYSICS IN ASTRONOMY

Workshop organized by Anil Pradhan and Sultana Nahar, sponsored by the Institute of Theoretical Atomic and Molecular Astrophysics (ITAMP) at the Harvard-Smithsonian Center for Astrophysics, Cambridge (MA), jointly with the Iron Project, in honor of Michael J. Seaton, Professor Emeritus, University College London, London, UK, for monumental contributions to atomic physics and astrophysics and as founder of the Opacity Project, the forerunner of the Iron Project. Mike passed away in May 2007; his last paper "Updated Opacity Project radiative accelerations" appeared after his death in August 2007 (Mon. Not. R. Astron. Soc., 382, 245). Obituary: "Michael J. Seaton", by Anil Pradhan and Sultana Nahar, Bulletin of American Astronomical Society, Vol. 39, No. 4, 1081, 2007.


PUBLICATIONS: 1995 -