Abstract:
The ground-state ground-state mechanical and radiative electron-capture processes are studied at very high, but not relativistic, projectile velocities. Three-body calculations were carried out with use of the continuum distorted-wave theoretical method for both processes. Total cross sections and final-atom angular distributions were computed, and the importance of each mechanism examined. For total cross sections, the numerical results reaffirm that the radiative process is the predominant mechanism at very high projectile energies. For a given incident charge, the range of projectile energies in which the nonrelativistic radiative mechanism is the most important decreases as the target charge increases. It is found that the radiative mechanism produces a very sharp final-atom angular distribution in the forward direction. When both processes, the radiative and mechanical, give the same total cross section, the calculations show that the radiative differential cross section in the forward direction is almost 2 orders of magnitude larger than the mechanical one. © 1984 The American Physical Society.
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Citas:
---------- APA ----------
Gonzalez, A.D. & Miraglia, J.E.
(1984)
. Comparison between the mechanical and radiative electron-capture processes at high energies. Physical Review A, 30(5), 2292-2296.
http://dx.doi.org/10.1103/PhysRevA.30.2292---------- CHICAGO ----------
Gonzalez, A.D., Miraglia, J.E.
"Comparison between the mechanical and radiative electron-capture processes at high energies"
. Physical Review A 30, no. 5
(1984) : 2292-2296.
http://dx.doi.org/10.1103/PhysRevA.30.2292---------- MLA ----------
Gonzalez, A.D., Miraglia, J.E.
"Comparison between the mechanical and radiative electron-capture processes at high energies"
. Physical Review A, vol. 30, no. 5, 1984, pp. 2292-2296.
http://dx.doi.org/10.1103/PhysRevA.30.2292---------- VANCOUVER ----------
Gonzalez, A.D., Miraglia, J.E. Comparison between the mechanical and radiative electron-capture processes at high energies. 1984;30(5):2292-2296.
http://dx.doi.org/10.1103/PhysRevA.30.2292