Abstract

This work was supported by the Austrian Science Fund FWF (J3503), the Adolf Messer Foundation (Germany), the UK Science and Facilities Council (ST/M006085/1), and the European Research Council ERC-2015-StG No. 677497. We also acknowledge support of Narodowe Centrum Nauki (NCN) under the grant (UMO-2016/22/M/ST2/00183) and University of Lodz under the grant (9/IDUB/MLOD/2021), MEYS of the Czech Republic, the Charles University project UNCE/SCI/013, and the Croatian Science Foundation under the project IP-2018-01-8570.

Highlights

  • Background subtractionSeveral sources of background affect our measured data

  • The environmental background caused by ambient radioactivity

  • cosmic rays is measured in runs without the neutron beam

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Summary

MOTIVATION

High-precision neutron capture data on 76Ge are of interest for fundamental research in nuclear astrophysics and for lowbackground experiments in the search of neutrinoless double β decay. This work presents neutron capture resonance data obtained at the n_TOF facility, providing for the first time information on individual resonance parameters relevant for radiative neutron capture on 76Ge up to 52 keV. These resonance data were used to constrain average resonance parameters and Maxwellian averaged cross sections. Capture events were detected by measuring the prompt capture γ rays with four deuterated benzene (C6D6) liquid scintillators These detectors have been optimized for an extremely low sensitivity to scattered neutrons [24,25].

Time to neutron energy conversion
Experimental capture yield
Detection efficiency
Background subtraction
Neutron fluence and normalisation
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