Relativistic calculations of angle-dependent photoemission time delay

Anatoli Kheifets, Ankur Mandal, Pranawa C. Deshmukh, Valeriy K. Dolmatov, David A. Keating, and Steven T. Manson
Phys. Rev. A 94, 013423 – Published 25 July 2016

Abstract

Angular dependence of photoemission time delay for the valence np3/2 and np1/2 subshells of Ar, Kr, and Xe is studied in the dipole relativistic random phase approximation. Strong angular anisotropy of the time delay is reproduced near respective Cooper minima while the spin-orbit splitting affects the time delay near threshold.

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  • Received 20 May 2016

DOI:https://doi.org/10.1103/PhysRevA.94.013423

©2016 American Physical Society

Physics Subject Headings (PhySH)

Atomic, Molecular & Optical

Authors & Affiliations

Anatoli Kheifets*

  • Research School of Physics and Engineering, Australian National University, Canberra ACT 0200, Australia

Ankur Mandal and Pranawa C. Deshmukh

  • Department of Physics, Indian Institute of Technology Madras, Chennai, Tamil Nadu 600036, India

Valeriy K. Dolmatov§

  • Department of Physics and Earth Science, University of North Alabama, Florence, Alabama 35632, USA

David A. Keating and Steven T. Manson

  • Department of Physics and Astronomy, Georgia State University, Atlanta, Georgia 30303, USA

  • *a.kheifets@anu.edu.au
  • amankur@physics.iitm.ac.in
  • pcd@physics.iitm.ac.in
  • §vkdolmatov@una.edu
  • dkeating2@student.gsu.edu
  • smanson@gsu.edu

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Issue

Vol. 94, Iss. 1 — July 2016

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