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QUANTUM NOISE CONTRIBUTION TO THE RECEIVER NOISE TEMPERATURE OF HEB THZ HETERODYNE RECEIVERS

E. Kollberg, Sigfrid Yngvesson

Open publisher page 5 citations

Abstract

In this paper we discuss the quantum limit of bolometric mixer receivers. The importance of the optics attenuation is emphasized. Based on a simple bolometer model we predict that the system and receiver quantum noise limits referred to the input of a double-sideband hotelectron bolometer mixer receiver are, respectively, 2(h113) and 1 (hf/3). The quantum limit to the DSB receiver noise temperature is hf/2k, in agreement with what has previously often been assumed. We suggest that an image-rejection single-sideband version of the HEB mixer would have a system quantum noise limit of WO). We also suggest that at a frequency of several THz the quantum noise may indeed be responsible for about half the total receiver noise temperature in a typical HEB receiver system.

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In this paper we discuss the quantum limit of bolometric mixer receivers. The importance of the optics attenuation is emphasized. Based on a simple bolometer model we predict that the system and receiver quantum noise limits referred to the input of a double-sideband hotelectron bolometer mixer receiver are, respectively, 2(h113) and 1 (hf/3). The quantum limit to the DSB receiver noise temperature is hf/2k, in agreement with what has previously often been assumed. We suggest that an image-rejection single-sideband version of the HEB mixer would have a system quantum noise limit of WO). We also suggest that at a frequency of several THz the quantum noise may indeed be responsible for about half the total receiver noise temperature in a typical HEB receiver system.

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Available abstract

In this paper we discuss the quantum limit of bolometric mixer receivers. The importance of the optics attenuation is emphasized. Based on a simple bolometer model we predict that the system and receiver quantum noise limits referred to the input of a double-sideband hotelectron bolometer mixer receiver are, respectively, 2(h113) and 1 (hf/3). The quantum limit to the DSB receiver noise temperature is hf/2k, in agreement with what has previously often been assumed. We suggest that an image-rejection single-sideband version of the HEB mixer would have a system quantum noise limit of WO). We also suggest that at a frequency of several THz the quantum noise may indeed be responsible for about half the total receiver noise temperature in a typical HEB receiver system.

Key concepts: Sideband, Physics, Bolometer, Quantum limit, Quantum noise, Superheterodyne receiver, Noise temperature, Noise (video)

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