Germanium doped with gallium (Ge:Ga) far-infrared photoconductors with
a Ga concentration of 1 x 10(14) cm(-3) are fabricated or use in sens
ors for detecting extremely weak radiation, such as for astronomical o
bservations by a space-borne cooled telescope, The performance of the
photoconductor at low temperatures and under low background photon inf
luxes to simulate operation in a space environment was evaluated, The
responsivity of the new Ge:Ga photoconductor is approximately double t
hat of the previous Ge:Ga photoconductors with a Ga concentration of 2
x 10(14) cm(-3) which was developed for astronomical observations usi
ng the Infrared Telescope in Space (IRTS) satellite. This increase in
responsivity: which is proportional to the product of hole mobility, h
ole lifetime, and quantum efficiency, is interpreted as being due to t
he enlargement of both hole mobility and hole lifetime and also becaus
e or almost equal quantum efficiency due to the utilization of a metal
cavity in which the photoconductor is mounted, The new photoconductor
has a slow transient response to a step change in photon influx simil
ar to that in the previous photoconductors, but its magnitude is large
r than that: of the previous ones. We found good agreement between the
time constants estimated from curve-fitting lu the response to a step
change in photon influx and the transient time constants derived by a
nalytical considerations based on the two-region, model of the Ge:Ga p
hotoconductor with ion-implanted ohmic contacts.