We investigate amplification of optical images by means of a traveling-wave
optical parametric amplifier. As shown recently for a cavity-based geometr
y, such a scheme can amplify images without deteriorating their signal-to-n
oise ratio thus working as a noiseless amplifier. Here we consider a config
uration without cavity, which is more realistic for a possible experimental
realization. We study in detail the quantum fluctuations of the amplifier
and formulate criteria for its noiseless performance. We investigate physic
al features of noiseless amplification, which take place for both traveling
-wave and ring-cavity configurations. We demonstrate how the optimum phase
matching of a phase-sensitive wave front of an image (by means of a thin le
ns or a small displacement of the crystal) can improve the noise performanc
e of the amplifier and bring it to the ultimate value achievable under give
n physical conditions. We discuss the possibility of using detectors with t
he area much smaller than the area of the input image elements. We compare
our results with those obtained for the ring-cavity configuration. [S1050-2
947(99)02209-X].