The decay times of D-1 emission lines of Rb and Cs atoms in superfluid
helium were measured at 1.6 K as functions of helium pressure in a ra
nge from the saturated vapor pressure to about 25 atm. In the case of
Cs, the measured decay time is almost independent of the helium pressu
re and is given by the lifetime of the 6P(1/2) state of the free atom.
However, we have found that the decay time of the Rb D-1 line decreas
es with increasing pressure. This suggests the coexistence of two proc
esses leading from the excited P state to the ground state, one an ord
inary D-1 emission transition and the other a process decaying via a l
ower energy state before reaching the ground state. The pressure-depen
dent quenching observed only for the Rb atom can be explained by the c
ompetition of the above two processes. A possible mechanism for quench
ing of the Rb 5P states is discussed in terms of the interaction poten
tials of the alkali-metal-atom-He-N system, where two or six helium at
oms are localized near the alkali core in a particular anisotropic con
figuration. The dynamics of processes leading from the excited P state
s of Na and Cs atoms are also discussed.