Shallow donor impurities in silicon at low temperatures are able to bind two electrons, forming negative donor ions, analogous to atomic H− ions. The second electron has a binding energy of only a few meV. Far-infrared radiation can be used to excite these electrons into the conduction band, giving a photoconductive signal. This mechanism is the basis of a new type of far-infrared detector, with promising applications for heterodyne detection at wavelengths on the order of 300 μm. The nature of the negative donor ion is discussed, in part from the effective mass analogy with H− atomic ions, and also with H−2 molecular ions. The theory of how this detector will perform as a function of such variables as bias voltage, background intensity, signal level, and signal speed has been examined. Response speeds on the order of 1 nsec are expected, for operation at temperatures ?2 K, with bias voltage as high as 100 V/cm. With unfiltered 300-K background radiation, the NEP is estimated to be on the order of 10−11 W/(Hz)1/2 at the response peak. In the heterodyne mode of operation, the theoretical noise level will be only fractionally larger than the noise level of a conventional impurity photoconductor. Unlike GaAs far-infrared detector material which is only available in relatively thin epitaxial layers, silicon detectors can be made thick enough to absorb the radiation effectively, and should have much higher quantum efficiency. The wavelength dependence of the photosignal as a function of temperature indicates that for samples doped on the order of 1016 cm−3, a distribution of binding energies exists for an electron bound to a group of randomly spaced donors. Such a distribution of binding energies may be related to excitonic spectra seen at similar doping densities.