Add to ORKGK x-ray emission rates in superheavy elements have been calculated by the use of the Dirac-Fock-Slater wave functions with finite-size nuclei. Calculations have been made relativistically and all possible multipoles as well as the retardation effect are taken into account. The x-ray energies are obtained as the difference bet-ween the initial and final binding energies of the atomic shells concerned. The importance of contributions from magnetic multipoles and the behavior of emission rates as a function of atomic number are discussed. KEY WORDS: Superheavy elements / Inner-shell binding energy/ K x-ray emission rates
M x-ray production cross sections from 1 to 1500 keV were obtained for elements with 70 less than or...
M x-ray production cross sections from 1 to 1500 keV were obtained for elements with 70 ≤ Z ≤ 92. Ob...
The results of extensive microscopic Relativistic Mean Field (RMF) calculations for the nuclei appea...
The effect of choice of the statistical exchange parameter a on the x-ray emission rate has been stu...
In this paper, we report on internal conversion coefficients for Z=111 to Z=126 superheavy elements ...
The energies and rates of Kα X-ray satellites due to 1s − 2p transitions in iodine and gold with one...
The 1s bound state of superheavy atoms and molecules reaches a binding energy of -2mc2 at Z≈16...
The K -shell and L -shell ionizations potentials for 268 109Mt were calculated at the Dirac-Hartree-...
There is strong interest in atomic and nuclear physics to the study of superheavy elements by the se...
The results of extensive microscopic relativistic mean field (RMF) calculations for the nuclei appea...
The structure of superheavy elements claimed to have been discovered in the recent Pb-208(Kr-86,n) r...
Hollow atoms in which the K shell is empty while the outer shells are populated allow studying a var...
This study focus on the weak lines that appear on high energy side of the diagram lines which is cal...
A non-relativistic correction to the radiative transition rate in nuclei due to the presence of extr...
Energies and radiative transition rates of electronic K x-rays in light muonic atoms have been calcu...
M x-ray production cross sections from 1 to 1500 keV were obtained for elements with 70 less than or...
M x-ray production cross sections from 1 to 1500 keV were obtained for elements with 70 ≤ Z ≤ 92. Ob...
The results of extensive microscopic Relativistic Mean Field (RMF) calculations for the nuclei appea...
The effect of choice of the statistical exchange parameter a on the x-ray emission rate has been stu...
In this paper, we report on internal conversion coefficients for Z=111 to Z=126 superheavy elements ...
The energies and rates of Kα X-ray satellites due to 1s − 2p transitions in iodine and gold with one...
The 1s bound state of superheavy atoms and molecules reaches a binding energy of -2mc2 at Z≈16...
The K -shell and L -shell ionizations potentials for 268 109Mt were calculated at the Dirac-Hartree-...
There is strong interest in atomic and nuclear physics to the study of superheavy elements by the se...
The results of extensive microscopic relativistic mean field (RMF) calculations for the nuclei appea...
The structure of superheavy elements claimed to have been discovered in the recent Pb-208(Kr-86,n) r...
Hollow atoms in which the K shell is empty while the outer shells are populated allow studying a var...
This study focus on the weak lines that appear on high energy side of the diagram lines which is cal...
A non-relativistic correction to the radiative transition rate in nuclei due to the presence of extr...
Energies and radiative transition rates of electronic K x-rays in light muonic atoms have been calcu...
M x-ray production cross sections from 1 to 1500 keV were obtained for elements with 70 less than or...
M x-ray production cross sections from 1 to 1500 keV were obtained for elements with 70 ≤ Z ≤ 92. Ob...
The results of extensive microscopic Relativistic Mean Field (RMF) calculations for the nuclei appea...