Abstract

i-TED is an innovative detection system which exploits Compton imaging techniques to achieve a superior signal-to-background ratio in ( $$n,\gamma $$ ) cross-section measurements using time-of-flight technique. This work presents the first experimental validation of the i-TED apparatus for high-resolution time-of-flight experiments and demonstrates for the first time the concept proposed for background rejection. To this aim, the $$^{197}$$ Au( $$n,\gamma $$ ) and $$^{56}$$ Fe( $$n, \gamma $$ ) reactions were studied at CERN n_TOF using an i-TED demonstrator based on three position-sensitive detectors. Two C $$_6$$ D $$_6$$ detectors were also used to benchmark the performance of i-TED. The i-TED prototype built for this study shows a factor of $$\sim $$ 3 higher detection sensitivity than state-of-the-art C $$_6$$ D $$_6$$ detectors in the 10 keV neutron-energy region of astrophysical interest. This paper explores also the perspectives of further enhancement in performance attainable with the final i-TED array consisting of twenty position-sensitive detectors and new analysis methodologies based on Machine-Learning techniques.

Highlights

  • Neutron capture cross-section measurements are fundamental in the study of astrophysical phenomena, such as the slow neutron capture (s-) process of nucleosynthesis operating in red-giant stars [1]

  • This paper explores the perspectives of further enhancement in performance attainable with the final i-Total Energy Detector (TED) array consisting of twenty position-sensitive detectors and new analysis methodologies based on Machine-Learning techniques

  • The first experimental validation of the background reduction in a 56Fe(n,γ) measurement at CERN n TOF using a previous prototype has been presented. This result is based on a comparison with state-of-the-art C6D6 detectors to benchmark the performance of this novel methodology and apparatus

Read more

Summary

Introduction

Neutron capture cross-section measurements are fundamental in the study of astrophysical phenomena, such as the slow neutron capture (s-) process of nucleosynthesis operating in red-giant stars [1]. I-TED exploits Compton imaging techniques with the aim of obtaining information about the incoming direction of the detected γ-rays This additional information can help to reject events which do not arise directly from the capture sample under study, thereby enhancing the signal-to-background ratio (SBR). Two different neutron capture experiments were carried out at the CERN n TOF facility [18] The objective here was to demonstrate the background rejection capability of i-TED and to quantify the attainable enhancement in terms of signal-to-background ratio (SBR) This reaction was chosen because it shows an isolated resonance at E◦ = 1.15 keV, which is well suited to evaluate SBRs in the several ∼10 keV of neutron energy, which is the range of interest for astrophysics

The n TOF facility and experimental set-up
The i-TED demonstrator
Energy calibration and γ-ray imaging validation
Perspectives on background suppression with 4π i-TED
MC simulations of i-TED
Machine Learning: algorithms and methodology
ML-based background suppression with i-TED
ML-based background suppression on i-TED prototype data
Findings
Babiano-Suarez
Full Text
Published version (Free)

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call