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Cryogenic silicon detectors with implanted contacts for the detection of visible photons using the Neganov-Luke Effect

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arxiv 1509.06266 v2 pith:WNHNREV4 submitted 2015-09-21 astro-ph.IM physics.ins-det

Cryogenic silicon detectors with implanted contacts for the detection of visible photons using the Neganov-Luke Effect

classification astro-ph.IM physics.ins-det
keywords effectexperimentsneganov-lukeabsorbercryogenicdetectiondetectorselectric
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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There is a common need in astroparticle experiments such as direct dark matter detection, 0{\nu}\b{eta}\b{eta} (double beta decay without emission of neutrinos) and Coherent Neutrino Nucleus Scattering experiments for light detectors with a very low energy threshold. By employing the Neganov-Luke Effect, the thermal signal of particle interactions in a semiconductor absorber operated at cryogenic temperatures, can be amplified by drifting the photogenerated electrons and holes in an electric field. This technology is not used in current experiments, in particular because of a reduction of the signal amplitude with time which is due to trapping of the charges within the absorber. We present here the first results of a novel type of Neganov-Luke Effect detector with an electric field configuration designed to improve the charge collection within the semiconductor.

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