2003
DOI: 10.1016/s0168-9002(03)00763-0
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VUV detection in large-area avalanche photodiodes as a function of temperature

Abstract: The response of a Peltier-cooled large-area avalanche photodiode to VUV-light is investigated as a function of the operation temperature. The reduction of the temperature down to 5 C will improve both photodiode light-level detection limit and statistical fluctuations; further temperature reduction will not result in improved performance. Optimum operation characteristics are already achieved for gains around 100 and do not depend significantly on the operation temperature. The relative variation of the gain w… Show more

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Cited by 6 publications
(17 citation statements)
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“…In fact, it is the number of primary charge carriers produced by the light pulse that will define The results obtained with this LAAPD for MDP at 172 nm are lower than those obtained with the Peltier-cooled LAAPD in Ref. [22] (∼ 1100 photons). The difference may be attributed to the differences in the LAAPD's dark currents, which limit the electronic noise and, thus, the MDP.…”
mentioning
confidence: 63%
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“…In fact, it is the number of primary charge carriers produced by the light pulse that will define The results obtained with this LAAPD for MDP at 172 nm are lower than those obtained with the Peltier-cooled LAAPD in Ref. [22] (∼ 1100 photons). The difference may be attributed to the differences in the LAAPD's dark currents, which limit the electronic noise and, thus, the MDP.…”
mentioning
confidence: 63%
“…Different studies have proved that the LAAPD response characteristics for VUV are different from those for visible light, used to determine most of the characteristics of the photodiodes [20][21][22]. The X-ray-to-photon detection nonlinearity, the sensitivity to magnetic fields and the relative variation of gain with temperature have been measured for VUV, presenting higher values when compared to visiblelight detection.…”
Section: Introductionmentioning
confidence: 99%
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“…The surface dark current is generated in the p-n junction edges due to high voltage gradients in its vicinity. Since dark current is a noise source and increases considerably with temperature, the electronic noise level can be reduced by cooling the APD, reducing the statistical fluctuations and the minimum detection limit of VUV photons [21,22].…”
Section: Apd Operation Principlementioning
confidence: 99%
“…For the 128 and 172 nm VUV light from argon and xenon scintillation, the effective quantum efficiency, here defined as the average number of free electrons produced in the APD per incident VUV photon is 0.5 and 1.1, respectively, corresponding to a spectral sensitivity of about 50 and 150 mA/W [4,19]. In this chapter, we review and summarize the results of our investigation, namely the gain non-linearity between the detection of X-rays and VUV light [20], the gain dependence on temperature [21,22], the behaviour under intense magnetic fields [23], the minimum detection limit, i.e. the minimum number of photons detectable above the noise level, and the statistical fluctuations in VUV photon detection [24].…”
Section: Introductionmentioning
confidence: 99%