TY - JOUR
T1 - Two-photon inner-shell transitions in molybdenum
AU - Bannett, Yigal B.
AU - Freund, Isaac
PY - 1984
Y1 - 1984
N2 - The two-photon x-ray emission spectra of inner-shell transitions in metallic Mo have been studied using large-area energy-dispersive Si(Li) detectors and fast, computer-controlled, time-coincidence electronics. The discrete energy-summation spectrum displays a peak at 17.1 keV corresponding to the expected 2s1s transition, as well as a second, more intense peak at 19.7 keV. Based upon very recent analytical H-atom calculations by Florescu, this latter peak is tentatively identified as due primarily to 3d1s transitions. The continuous two-photon spectrum has also been measured on an absolute intensity scale and compared with a frozen-orbital calculation based upon direct summation of the second-order perturbation expansion for the relevant matrix elements. For the 2s1s transition, excellent quantitative agreement is found using the self-consistent-field Hartree-Fock wave functions of Clementi and Roetti. The same calculation predicts that the 3s1s transition is of negligible relative amplitude. Because the calculational method is inapplicable to d states, a simple closure approximation is developed which is found to be reasonably good for both the 2s and 3s two-photon transitions, but apparently fails for the 3d transition since it predicts a result which is relatively much too small. Our data are the first for inner-shell transitions and it is anticipated that further developments in both instrumentation and in theory will yield a new, rich, multiphoton inner-shell spectroscopy.
AB - The two-photon x-ray emission spectra of inner-shell transitions in metallic Mo have been studied using large-area energy-dispersive Si(Li) detectors and fast, computer-controlled, time-coincidence electronics. The discrete energy-summation spectrum displays a peak at 17.1 keV corresponding to the expected 2s1s transition, as well as a second, more intense peak at 19.7 keV. Based upon very recent analytical H-atom calculations by Florescu, this latter peak is tentatively identified as due primarily to 3d1s transitions. The continuous two-photon spectrum has also been measured on an absolute intensity scale and compared with a frozen-orbital calculation based upon direct summation of the second-order perturbation expansion for the relevant matrix elements. For the 2s1s transition, excellent quantitative agreement is found using the self-consistent-field Hartree-Fock wave functions of Clementi and Roetti. The same calculation predicts that the 3s1s transition is of negligible relative amplitude. Because the calculational method is inapplicable to d states, a simple closure approximation is developed which is found to be reasonably good for both the 2s and 3s two-photon transitions, but apparently fails for the 3d transition since it predicts a result which is relatively much too small. Our data are the first for inner-shell transitions and it is anticipated that further developments in both instrumentation and in theory will yield a new, rich, multiphoton inner-shell spectroscopy.
UR - http://www.scopus.com/inward/record.url?scp=0037828612&partnerID=8YFLogxK
U2 - 10.1103/physreva.30.299
DO - 10.1103/physreva.30.299
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AN - SCOPUS:0037828612
SN - 1050-2947
VL - 30
SP - 299
EP - 308
JO - Physical Review A
JF - Physical Review A
IS - 1
ER -