A crystal of Sr
F2:
Sm2+ was operated as a pulsed optical maser at temperatures close to 4.2\ifmmode^\circ\else\textdegree\fi{}K. The 6969 \AA{} output corresponds to the wavelength of an exceedingly sharp line ($\ensuremath{\Delta}\ensuremath{\nu}<0.6$ ${\mathrm{cm}}^{\ensuremath{-}1}$) in which almost all of the low-temperature fluorescence is concentrated. In contrast to what prevails in Ca
F2:
Sm+2 masers, the output is characterized by strong relaxation oscillations. This may be explained by the large difference in the fluorescent lifetimes in the two systems. While in Ca
F2:
Sm2+ the value of $\ensuremath{\tau}$ is approximately 1.5\ifmmode\times\else\texttimes\fi{}${10}^{\ensuremath{-}6}$ sec, in Sr
F2:
Sm2+ it has a value of 15 msec. The reason for the large difference in $\ensuremath{\tau}$ values, in turn, depends upon the relative proximity of the long-wavelength edge of the red band to the position of the metastable
5D0 level from which fluorescence occurs. Absorption measurements taken at helium temperatures on Sr
F2:
Sm2+ show that the lowest vibrational level of the lowest lying $4f\ensuremath{-}5d$ band lies \ensuremath{\sim}600 ${\mathrm{cm}}^{\ensuremath{-}1}$ above the position of the
5D0 level while in Ca
F2:
Sm2+ there is near coincidence of the corresponding levels and consequently strong configurational mixing. Crystals of Sr
Cl2:
Sm2+ were also studied in this regard and display an expected close similarity in spectral characteristics to Sr
F2:
Sm2+. The vibrational structure on the $4f\ensuremath{-}5d$ bands is much more pronounced, however, than in Ca
F2:
Sm2+ and Sr
F2:
Sm2+, indicating weaker coupling to the lattice in the excited
5d state. A tentative interpretation for the splitting of the red band seen in the absorption spectra of
Sm2+ ions is given.
The two-photon transitions between the Stark levels of the
7F0 and
5D2 multiplets of the
Sm2+ ion in BaClF are investigated both from an experimental and theoretical viewpoint. Direct two-photon excitation spectra of the
5D2 fluorescence resulting from an optical excitation with an infrared laser beam are presented and the polarization dependence of the observed transitions is analyzed. These new data are interpreted along the lines of a simple model which originates in the second-order theory developed by Axe [Phys. Rev. 136, A42 (1964)] for two-photon processes in complex atoms. The extension of this theory to the case of rare-earth ions embedded in crystalline fields is carried out by use of symmetry-adaptation techniques based on the use of an SU(2)\ensuremath{\supset}
G∗ chain of groups. It is shown that the resulting model (limited up to second-order terms) describes correctly the relative intensities of the two-photon transitions between the Stark levels of the
7F0 and
5D2 multiplets of
Sm2+ in BaClF.
One-color two-photon excitation spectra of the
7F0${\ensuremath{\rightarrow}}^{5}$
D0 and
7F0${\ensuremath{\rightarrow}}^{5}$
D2 transitions of
Sm2+ in
SrF2 have been measured at low temperature and their dependences upon photon polarization analyzed. Linewidths on the order of 0.2, 0.6, and 1.0 ${\mathrm{cm}}^{\mathrm{\ensuremath{-}}1}$ are obtained for the
7F0${\ensuremath{\rightarrow}}^{5}$
D0(
A1g),
7F0${\ensuremath{\rightarrow}}^{5}$
D2(
Eg), and
7F0${\ensuremath{\rightarrow}}^{5}$
D2(
T2g) Stark components observed at 15 K, respectively. The
7F0${\ensuremath{\rightarrow}}^{5}$
D0(
A1g) transition is observed to be isotropic within experimental error, while the
Eg and
T2g components of the
7F0${\ensuremath{\rightarrow}}^{5}$
D2 transition exhibit the anisotropic patterns expected in
Oh symmetry. Calculations of two-photon transition intensities are conducted within the framework of the phenomenological model previously used for
Sm2+ in MClF (M=Ba,Sr) and
Eu3+ in
LuPO4, where the rare-earth ion occupies sites of
C4v and
D2d symmetries, respectively. The present results are compared and contrasted with those obtained in these previous cases.
The natural radiative lifetimes of the 5${\mathit{d}}^{9}
6{\mathit{s}}^{2}$
(2D5/2 and
2D3/2) metastable states of
Hg+ as well as of the 5${\mathit{d}}^{9}
6s{(}^{3}$${\mathit{D}}_{2}$) metastable state of ${\mathrm{Hg}}^{2+}$ have been measured by counting for equal time intervals either the 282-, 198-, or 217-nm photons emitted when the respective metastable ions decay to the ground state. The metastable Hg ions are produced inside a cylindrical electrostatic ion trap by electron bombardment of background Hg vapor maintained at pressures ranging from 4 to 50\ifmmode\times\else\texttimes\fi{}${10}^{\mathrm{\ensuremath{-}}8}$ Torr. The trap consists of a 5.0-cm-diam, 7.5-cm-long cylinder with end caps plus a concentric 0.003-cm-diam central cylinder maintained at a negative potential of 140 V. Following electron impact of the Hg vapor, some of the photons emitted by the decaying metastable ion population are focused onto a narrow-bandwidth interference filter. The photons transmitted by the filter are detected by a photomultiplier tube as a function of time and generate a decay curve. However, the signal detected with the interference filter used to monitor the $^{2}$${\mathit{D}}_{3/2}$ metastable-state population consists of two exponentially decaying components, indicating the presence of another metastable state decaying through the emission of a photon within the bandpass of the filter. The second component is assumed to arise from a cascade originating with the 5${\mathit{d}}^{9}$6s6p (J=9/2) metastable state of
Hg+. Therefore, as dictated by the composition of the photon decay curve, the pressure-dependent decay rates of the metastable states are obtained from a least-squares fit of either a single- or double-component exponential decay to the natural logarithm of the decay curve.Mean decay rates extrapolated to zero pressure of the background Hg vapor using a straight-line least-squares fit, and the inverse of the zero-pressure intercept yields the natural radiative lifetime of the relevant metastable state. Our results for the lifetimes of the
2D5/2,
2D3/2, and J=9/2 metastable states of
Hg+ are 87\ifmmode\pm\else\textpm\fi{}4, 8.8\ifmmode\pm\else\textpm\fi{}0.4, and 60\ifmmode\pm\else\textpm\fi{}6 msec, respectively, while the lifetime of the
Hg2+ (3D2) metastable state is 34\ifmmode\pm\else\textpm\fi{}3 msec.
It was first shown by Axe and Sorokin that nonradiative decay of the terminal optical maser level (
7F1) Ca
F2:
Sm2+ is forbidden to first order even though many phonon states are available with the proper energy for the transition. At first sight this would indicate the
7F1 level to be metastable. It is shown that a second-order two-phonon emission transition can alleviate this bottleneck, and the decay process rate is computed. This process, involving virtual transitions to a higher level (
7F2), is shown to be very effective and to lead to a nonradiative lifetime of \ensuremath{\sim}${10}^{\ensuremath{-}6}$ sec, in accord with the necessary conditions for the existence of optical maser action in Ca
F2:
Sm2+.
The recently demonstrated process of photon-gated spectral hole burning has been used to measure the small frequency shifts necessary for the determination of linear Stark and nonlinear Zeeman coefficients of the 4
f6 7F0A1\ensuremath{\rightarrow}
5D0A1,
5D1A2, and
5D1E transitions of
Sm2+ in BaClF. The nonlinear Zeeman coefficients obtained in this way agree, to better than 12%, with those calculated assuming free-ion 4
f6 wave functions for
Sm2+. The Stark splitting coefficients (0.068--0.074 MHz/V ${\mathrm{cm}}^{\mathrm{\ensuremath{-}}1}$) are smaller than the few previously reported for
fn\ensuremath{\rightarrow}
fn transitions of rare-earth ions.