Fast neutron scattering and multiple-neutrion detection in MoNA
ORAL
Abstract
With the new FRIB facility coming online soon, studies of neutron-unbound systems near the neutron dripline will have
access to heavier systems, including many new unbound states decaying via multiple-neutron (MN) emission. The MoNA/LISA
neutron detector array measures the energy and momentum of fast neutrons resulting from in-flight decays, and the
challenge for studying MN decays has been to filter out contributions from 1N scattering two or more times in the array.
We have traditionally employed a simple ``causality cut'' to filter out 1N events by requiring a minimum distance
between hits (typically ~30-50 cm) and a minimum effective velocity between hits (neutron beam velocity). This method
provides a clean removal of 1N events, but reduces the number of MN events that survive the filter and reduces the
efficiency for detecting lower decay energies. We have developed a new sorting algorithm that increases the MN/1N signal
for MN datasets. All hits in an event above a pre-determined light threshold are sorted according to cluster type with
the neutron scatter site assigned to the earliest hit in the cluster. Events are then sorted by pair according to their
causal relationship to determine the number of independent neutrons involved in the event, and their first-scatter
sites. This sorting is performed in a two-dimensional parameter space consisting of scattering angle and neutron
spacetime interval for the pair ($NSI =(v_{beam}^2-v_{12}^2)t_{12}^2$). Successful tests of the MN filter using previous
MoNA 1N and 2N datasets and Monte Carlo simulations will be presented, as well as additional diagnostics for tracking
scattering behavior.
access to heavier systems, including many new unbound states decaying via multiple-neutron (MN) emission. The MoNA/LISA
neutron detector array measures the energy and momentum of fast neutrons resulting from in-flight decays, and the
challenge for studying MN decays has been to filter out contributions from 1N scattering two or more times in the array.
We have traditionally employed a simple ``causality cut'' to filter out 1N events by requiring a minimum distance
between hits (typically ~30-50 cm) and a minimum effective velocity between hits (neutron beam velocity). This method
provides a clean removal of 1N events, but reduces the number of MN events that survive the filter and reduces the
efficiency for detecting lower decay energies. We have developed a new sorting algorithm that increases the MN/1N signal
for MN datasets. All hits in an event above a pre-determined light threshold are sorted according to cluster type with
the neutron scatter site assigned to the earliest hit in the cluster. Events are then sorted by pair according to their
causal relationship to determine the number of independent neutrons involved in the event, and their first-scatter
sites. This sorting is performed in a two-dimensional parameter space consisting of scattering angle and neutron
spacetime interval for the pair ($NSI =(v_{beam}^2-v_{12}^2)t_{12}^2$). Successful tests of the MN filter using previous
MoNA 1N and 2N datasets and Monte Carlo simulations will be presented, as well as additional diagnostics for tracking
scattering behavior.
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Presenters
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Warren F Rogers
Indiana Wesleyan University
Authors
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Warren F Rogers
Indiana Wesleyan University
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Andrea Munroe
Indiana Wesleyan Univ, Indiana Wesleyan University
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Jeremy E Hallett
Indiana Wesleyan Univ, Indiana Wesleyan University