Add to ORKGThe effect of choice of the statistical exchange parameter a on the x-ray emission rate has been studied by the use of the relativistic Hartree-Fock-Slater method. The finite nuclear size effect and the retardation effect are taken into account. It is found that the K x-ray emission rate increases with increasing a. The difference between the emission rates with a=2/3 and a=1 is less than 3.2 % for transitions studied here. KEY WORDS: Statistical exchange parameter / K x-ray emission rate/ Relativistic Hartree-Fock-Slater method/ 1
Background: The neutron emission rates in thermal excited nuclei are conventionally described by sta...
A simple statistical model in terms of light-front kinematic variables is used to explain the nuclea...
The relativistic Hartree-Fock-Slater transition-state method is used to calculate the energies of th...
K x-ray emission rates in superheavy elements have been calculated by the use of the Dirac-Fock-Slat...
The energies and rates of Kα X-ray satellites due to 1s − 2p transitions in iodine and gold with one...
International audienceThe simulation of atomic relaxation relies on data libraries with tabulated pa...
M x-ray production cross sections from 1 to 1500 keV were obtained for elements with 70 less than or...
The theory of X-ray transition radiation is generalised to the case of absorbing media. The energy-a...
A systematic and quantitative validation of the K and L shell X-ray transition probability calculati...
This paper considers the impact of Lyman α coupling and X-ray heating on the 21-cm brightness-temper...
The original Kompaneets equation fails to describe down-Comptonization, which is the most important ...
The influence of nuclear data input on r-process calculations can best be studied within the “waitin...
M x-ray production cross sections from 1 to 1500 keV were obtained for elements with 70 ≤ Z ≤ 92. Ob...
Transition rates for radiative decays to the L-shell were obtained for Yb, Hf and Ta by means of a m...
Relative L-shell radiative transition rates were obtained for a number of decays in Gd, Dy, Er, Yb, ...
Background: The neutron emission rates in thermal excited nuclei are conventionally described by sta...
A simple statistical model in terms of light-front kinematic variables is used to explain the nuclea...
The relativistic Hartree-Fock-Slater transition-state method is used to calculate the energies of th...
K x-ray emission rates in superheavy elements have been calculated by the use of the Dirac-Fock-Slat...
The energies and rates of Kα X-ray satellites due to 1s − 2p transitions in iodine and gold with one...
International audienceThe simulation of atomic relaxation relies on data libraries with tabulated pa...
M x-ray production cross sections from 1 to 1500 keV were obtained for elements with 70 less than or...
The theory of X-ray transition radiation is generalised to the case of absorbing media. The energy-a...
A systematic and quantitative validation of the K and L shell X-ray transition probability calculati...
This paper considers the impact of Lyman α coupling and X-ray heating on the 21-cm brightness-temper...
The original Kompaneets equation fails to describe down-Comptonization, which is the most important ...
The influence of nuclear data input on r-process calculations can best be studied within the “waitin...
M x-ray production cross sections from 1 to 1500 keV were obtained for elements with 70 ≤ Z ≤ 92. Ob...
Transition rates for radiative decays to the L-shell were obtained for Yb, Hf and Ta by means of a m...
Relative L-shell radiative transition rates were obtained for a number of decays in Gd, Dy, Er, Yb, ...
Background: The neutron emission rates in thermal excited nuclei are conventionally described by sta...
A simple statistical model in terms of light-front kinematic variables is used to explain the nuclea...
The relativistic Hartree-Fock-Slater transition-state method is used to calculate the energies of th...