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A Hot-electron Direct Detector for RadioastronomyA hot-electron transition-edge superconducting bolometer with adjustable thermal relaxation speed is proposed. The bolometer contacts are made from a superconductor with high critical temperature which blocks the thermal diffusion of hot carriers into the contacts. Thus electron-phonon interaction is the only mechanism for heat removal. The speed of thermal relaxation for hot electrons in a nanometer-size superconducting bolometer with T(sub c) = 100-300 mK is controlled by the elastic electron mean free path l. The relaxation rate behaves as T(sup 4)l at subkelvin temperatures and can be reduced by a factor of 10-100 by decreasing 1. Then an antenna- or wave guide-coupled bolometer with a time constant approx. = 10(exp -3) to 10(exp -4) s will exhibit photon-noise limited performance at millimeter and submillimeter wavelengths. The bolometer will have a figure-of-merit NEPtau = 10(exp -22) - 10(exp -21) W/Hz at 100 mK which is 10(exp 3) to 10(exp 4) times better (ie: smaller) than that of a state-of-the-art bolometer. A tremendous increase in speed and sensitivity will have a significant impact for observational mapping applications.
Document ID
20000057408
Acquisition Source
Headquarters
Document Type
Preprint (Draft being sent to journal)
Authors
Karasik, Boris S.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
McGrath, William R.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
LeDuc, Henry G.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Gershenson, Michael E.
(Rutgers Univ. Piscataway, NJ United States)
Date Acquired
September 7, 2013
Publication Date
April 30, 1999
Subject Category
Astronomy
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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