A hot-electron direct detector for radioastronomy

A hot-electron transition-edge superconducting bolometer with adjustable th ermal relaxation speed is proposed. The bolometer contacts are made from a superconductor with high critical temperature which blocks the thermal diff usion of hot carriers into the contacts. Thus electron-phonon interaction i s the only mechanism for heat removal. The speed of thermal relaxation for hot electrons in a nanometre-size superconducting bolometer with T-c = 100- 300 mK is controlled by the elastic electron mean free path l. The relaxati on rate behaves as T(4)l at subkelvin temperatures and can be reduced by a factor of 10-100 by decreasing l. Then an antenna- or waveguide-coupled bol ometer with a time constant similar to 10(-3)-10(-4) s will exhibit photon- noise-limited performance at millimetre and submillimetre wavelengths. The bolometer will have a figure of merit NEP tau(1/2) = 10(-23)-10(-22) J(-1) at 100 mK which is 10(3)-10(4) times better (i.e. smaller) than that of a s tate-of-the-art bolometer. A tremendous increase in speed and sensitivity w ill have a significant impact for observational mapping applications.