5 p
2
P
j
\5 d
2
D
3Õ2
transition matrix elements in atomic
87
Rb
S. B. Bayram,* M. Havey,
²
M. Rosu, and A. Sieradzan
Department of Physics, Central Michigan University, Mt. Pleasant, Michigan 48859
A. Derevianko
‡
and W. R. Johnson
Department of Physics, University of Notre Dame, Notre Dame, Indiana 46556
Received 1 February 2000; published 7 April 2000
A combined precision experimental and theoretical study of 5 p
2
P
j
→5 d
2
D
3/2
electric-dipole transition
matrix elements in atomic
87
Rb has shown that they are dominated by electron correlation. The relative size
and sign of the measured matrix element ratio is found to be 1.0688, in very good agreement with the value
of 1.135 obtained from relativistic third-order many-body perturbation theory.
PACS numbers: 32.70.Cs, 31.30.Jv, 31.15.Md, 32.80.-t
Determination of multipole matrix elements, quantities
that define a scale of interaction between electromagnetic
radiation and atomic matter 1, remains a fundamental prob-
lem of considerable theoretical and experimental interest.
Such quantities are important to a wide range of basic and
applied problems, including determination of astrophysical
abundances of atoms in stellar atmospheres 2 and analysis
of atomic parity-violation experiments 3. As opposed to
observables related to energy intervals in atoms or mol-
ecules, which may be determined to a precision of 10
-11
4,5, the best measurements of atomic dipole matrix ele-
ments have only recently achieved a precision of 5
10
-4
6. And despite remarkable advances in the devel-
opment of relativistic many-body techniques in atomic phys-
ics, calculations of electric-dipole matrix elements for
heavier atoms such as cesium have been limited to an accu-
racy of about 0.5% 7,9,10. Nevertheless, at this level in-
sight into important physical effects determining the matrix
elements may be given. For example, a recent report of cal-
culation of magnetic dipole matrix elements associated with
ns
2
S
1/2
→n ' s
2
S
1/2
transitions in the alkali-metal atoms has
revealed that negative-energy states can produce significant
anomalies in the magnetic transition strength 11.
A number of novel techniques have recently been applied
to precise absolute and relative measurements of the strength
of resonance transitions in the heavier alkali-metal atoms.
These have included refined lifetime measurements in
atomic-beam experiments 12, photoassociative spectros-
copy of cold atoms confined to atomic traps 13–15, and
direct measurements of the natural width of the 3 s
2
S
1/2
→3 p
2
P
3/2
transition in Na 16. Meticulous light-absorption
measurements have determined the relative strength of the
Cs resonance transitions 17 to 5 10
-4
. It has also been
shown 18 that the frequency dependence of polarized Ray-
leigh and Raman scattering of light from atoms depends sen-
sitively on the relative strengths of radiative transitions be-
tween manifolds of atomic levels. Further, recent experi-
ments 19 on the 5 s
2
S
1/2
→5 p
2
P
j
→8 s
2
S
1/2
transition in
atomic Rb demonstrated that precision measurements of the
polarization dependence of the two-photon transition rate in
atoms can yield sum rules for combinations of atomic
electric-dipole matrix elements.
We have made a combined experimental and theoretical
study of the 5 s
2
S
1/2
→5 p
2
P
j
→5 d
2
D
3/2
transition in atomic
87
Rb. In this case, precision measurements of the nonreso-
nant two-photon, two-color linear depolarization spectrum
show remarkable polarization-dependent interference struc-
ture which is partly due to the near degeneracy of the two
photons driving the process. From the measurements it was
possible to extract the ratio of the reduced excited-state tran-
sition matrix elements for two contributing pathways:
5 p
2
P
3/2
→5 d
2
D
3/2
and 5 p
2
P
1/2
→5 d
2
D
3/2
. The ratio of re-
duced matrix elements for the multiplet transition shows a
significant departure from the nonrelativistic limit of unity.
To understand the results, we have performed third-order
many-body perturbation theory 7 calculations of the matrix
elements, including spin-orbit and relativistic effects in an ab
initio fashion. The calculations reveal that, although the main
departure appears in the Dirac-Hartree-Fock values, excep-
tionally large correlation contributions dominate the excited-
state transition matrix elements.
The experimental scheme is illustrated in the inset to Fig.
1, which shows low-lying energy levels for atomic Rb. Two
independently tunable lasers having frequencies
1
and
2
are adjusted to satisfy the two-photon resonance condition
1
+
2
=
0
, where
0
is the resonance frequency of the
5 s
2
S
1/2
→5 d
2
D
3/2
transition. Averaged over hyperfine
structure,
0
=25 700.56 cm
-1
. In the weak laser fields of
the present experiment, there are two contributing virtual
levels; these are indicated by the horizontal broken lines in
Fig. 1. In the present case, these merge when one laser fre-
quency is offset from the 5 s
2
S
1/2
→5 p
2
P
3/2
transition by
about 33.7 cm
-1
. In this paper detuning is defined as
1
=
1
-
3/2
, where
3/2
=12 816.58 cm
-1
is the resonance
frequency of the 5 s
2
S
1/2
→5 p
2
P
3/2
transition. For the
5 s
2
S
1/2
→5 p
2
P
1/2
transition,
1/2
=12 578.96 cm
-1
. De-
tection of atoms promoted to the 5 d
2
D
3/2
levels is achieved
by monitoring the 6 p
2
P
j
→5 s
2
S
1/2
fluorescence around 420
nm.
*Present address: University of Michigan, Ann Arbor, MI.
²
Permanent address: Old Dominion University, Norfolk, VA.
‡
Present address: Harvard Smithsonian Center for Astrophysics,
Cambridge, MA.
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