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    Characterization of low-energy ionization signals in silicon detectors for the Nab experiment

    R. J. Taylor1,2,*, August Mendelsohn3, Arlee Shelby1,2, William C. McCray1,2, Jin Ha Choi1,2, Nicholas Macsai3, Grant Riley4, Erick Smith4, Stefan Baeßler5,6 et al.

    Leah J. Broussard6, Christopher B. Crawford7, Michael Gericke3, Francisco M. Gonzalez6, David Harrison3, Leendert Hayen1,8, Mark Makela4, Russell Mammei3,9, David G. Mathews6, Dinko Poc̆anić5, Glenn Randall10, Americo Salas-Bacci5, W. Scott Wilburn4, and A. R. Young1,2

    • *Contact author: rjtaylo2@ncsu.edu

    Phys. Rev. C 114, 025501 – Published 10 August, 2026

    DOI: https://doi.org/10.1103/lqlg-b7cx

    Abstract

    The Nab (Neutron a b) experiment is designed to measure the beta-antineutrino angular correlation in free neutron β decay with an ultimate precision goal of 0.1%, providing input for tests of Cabibbo-Kobayashi-Maskawa matrix unitarity. This measurement is performed via detection of electrons and protons in delayed coincidence using custom large-area segmented silicon detectors. We present the characterization of one such detector system to establish the proton energy and timing response, using a dedicated proton accelerator. The detected proton peak was studied for 25, 30, and 35 keV incident protons on a set of detector segments and multiple cooling cycles over a one-year period. Ionization losses were consistent with models of the detector dead layer with thicknesses less than 100 nm. The detected proton peak was stable within the uncertainty from energy calibration (0.25 keV). The rise times of detector pulses from Cd109 and Sn113 conversion electron sources were used to extract the impurity density profile and establish a precise model for the detector timing response. The observed impurity density profile varied from (2±2)×109/cm3 at the center to (26±2)×109/cm3 at the edge. This impurity density profile was then used to characterize systematic effects in proton time-of-flight measurements due to detector pulse-shape effects; the resultant proton timing systematic uncertainties were below 0.3 ns, which is sufficient for the Nab experiment.

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