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Large-mass ultralow noise germanium detectors: performance and applications in neutrino and astroparticle physics

2007/01/07 by P. S. Barbeau, J. I. Collar, O. Tench
Physics and Astronomy · #Dark Matter and Cosmic Phenomena #Neutrino Physics Research #Particle Detector Development and Performance #astro-ph #hep-ex #nucl-ex #physics.ins-det

paper · pdf · doi:10.1088/1475-7516/2007/09/009

published as JCAP 0709:009,2007 · submitted to Phys. Rev. C

arxiv created 2007/01/07 · openalex publication_date 2007/09/11 · arxiv updated 2011/05/12 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/30

Abstract

A new type of radiation detector, a p-type modified electrode germanium diode, is presented. It is shown that the prototype displays, for the first time, a combination of features (mass, energy threshold and background expectation) required for a measurement of coherent neutrino–nucleus scattering in a nuclear reactor experiment. First results are presented from its calibration using sub-kiloelectronvolt nuclear recoils similar to those expected from reactor antineutrinos or light WIMPs (weakly interacting massive particles) beyond the reach of present detectors. The device hybridizes the mass and energy resolution of a conventional HPGe coaxial gamma spectrometer with the low electronic noise and threshold of a small x-ray semiconductor detector, also displaying an intrinsic ability to distinguish multiple-site from single-site particle interactions. The present performance of the prototype and possible further improvements are discussed, as well as other applications for this new type of device in neutrino and astroparticle physics (double-beta decay, neutrino magnetic moment and novel WIMP searches).

Citations