_version_ 1866908579576938496
author Skowronski, Jakub
Gesuè, Riccardo Maria
Boeltzig, Axel
Ciani, Giovanni Francesco
Piatti, Denise
Rapagnani, David
Aliotta, Marialuisa
Ananna, Chemsedinne
Barile, Francesco
Bemmerer, Daniel
Best, Andreas
Broggini, Carlo
Bruno, Carlo Giovanni
Caciolli, Antonio
Campostrini, Matteo
Cavanna, Francesca
Colombetti, Paolo
Compagnucci, Alessandro
Corvisiero, Piero
Csedreki, Laszlo
Davinson, Tom
Depalo, Rosanna
Di Leva, Antonino
Elekes, Zoltan
Ferraro, Federico
Formicola, Alba
Fülöp, Zsolt
Gervino, Gianpiero
Guglielmetti, Alessandra
Gustavino, Carlo
Gyürky, György
Imbriani, Gianluca
Junker, Matthias
Lugaro, Maria
Marigo, Paola
Masha, Eliana
Menegazzo, Roberto
Paticchio, Vincenzo
Perrino, Roberto
Prati, Paolo
Rigato, Valentino
Schiavulli, Luigi
Sidhu, Ragandeep Singh
Straniero, Oscar
Szűcs, Tamás
Zavatarelli, Sandra
author_facet Skowronski, Jakub
Gesuè, Riccardo Maria
Boeltzig, Axel
Ciani, Giovanni Francesco
Piatti, Denise
Rapagnani, David
Aliotta, Marialuisa
Ananna, Chemsedinne
Barile, Francesco
Bemmerer, Daniel
Best, Andreas
Broggini, Carlo
Bruno, Carlo Giovanni
Caciolli, Antonio
Campostrini, Matteo
Cavanna, Francesca
Colombetti, Paolo
Compagnucci, Alessandro
Corvisiero, Piero
Csedreki, Laszlo
Davinson, Tom
Depalo, Rosanna
Di Leva, Antonino
Elekes, Zoltan
Ferraro, Federico
Formicola, Alba
Fülöp, Zsolt
Gervino, Gianpiero
Guglielmetti, Alessandra
Gustavino, Carlo
Gyürky, György
Imbriani, Gianluca
Junker, Matthias
Lugaro, Maria
Marigo, Paola
Masha, Eliana
Menegazzo, Roberto
Paticchio, Vincenzo
Perrino, Roberto
Prati, Paolo
Rigato, Valentino
Schiavulli, Luigi
Sidhu, Ragandeep Singh
Straniero, Oscar
Szűcs, Tamás
Zavatarelli, Sandra
contents Studies of charged-particle reactions for low-energy nuclear astrophysics require high sensitivity, which can be achieved by means of detection setups with high efficiency and low backgrounds, to obtain precise measurements in the energy region of interest for stellar scenarios. High-efficiency total absorption spectroscopy is an established and powerful tool for studying radiative capture reactions, particularly if combined with the cosmic background reduction by several orders of magnitude obtained at the Laboratory for Underground Nuclear Astrophysics (LUNA). We present recent improvements in the detection setup with the Bismuth Germanium Oxide (BGO) detector at LUNA, aiming to reduce high-energy backgrounds and to increase the summing detection efficiency. The new design results in enhanced sensitivity of the BGO setup, as we demonstrate and discuss in the context of the first direct measurement of the 65 keV resonance ($E_{x} = 5672$ keV) of the $^{17}$O($p,γ$)$^{18}$F reaction. Moreover, we show two applications of the BGO detector, which exploit its segmentation. In case of complex $γ$-ray cascades, e.g. the de-excitation of $E_{x} = 5672$ keV in $^{18}$F, the BGO segmentation allows to identify and suppress the beam-induced background signals that mimic the sum peak of interest. We demonstrate another new application for such a detector in form of in-situ activation measurements of a reaction with $β^{+}$ unstable product nuclei, e.g., the $^{14}$N($p,γ$)$^{15}$O reaction.
format Preprint
id arxiv_https___arxiv_org_abs_2510_05939
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Advances in Radiative Capture Studies at LUNA with a Segmented BGO Detector
Skowronski, Jakub
Gesuè, Riccardo Maria
Boeltzig, Axel
Ciani, Giovanni Francesco
Piatti, Denise
Rapagnani, David
Aliotta, Marialuisa
Ananna, Chemsedinne
Barile, Francesco
Bemmerer, Daniel
Best, Andreas
Broggini, Carlo
Bruno, Carlo Giovanni
Caciolli, Antonio
Campostrini, Matteo
Cavanna, Francesca
Colombetti, Paolo
Compagnucci, Alessandro
Corvisiero, Piero
Csedreki, Laszlo
Davinson, Tom
Depalo, Rosanna
Di Leva, Antonino
Elekes, Zoltan
Ferraro, Federico
Formicola, Alba
Fülöp, Zsolt
Gervino, Gianpiero
Guglielmetti, Alessandra
Gustavino, Carlo
Gyürky, György
Imbriani, Gianluca
Junker, Matthias
Lugaro, Maria
Marigo, Paola
Masha, Eliana
Menegazzo, Roberto
Paticchio, Vincenzo
Perrino, Roberto
Prati, Paolo
Rigato, Valentino
Schiavulli, Luigi
Sidhu, Ragandeep Singh
Straniero, Oscar
Szűcs, Tamás
Zavatarelli, Sandra
Nuclear Experiment
Instrumentation and Detectors
Studies of charged-particle reactions for low-energy nuclear astrophysics require high sensitivity, which can be achieved by means of detection setups with high efficiency and low backgrounds, to obtain precise measurements in the energy region of interest for stellar scenarios. High-efficiency total absorption spectroscopy is an established and powerful tool for studying radiative capture reactions, particularly if combined with the cosmic background reduction by several orders of magnitude obtained at the Laboratory for Underground Nuclear Astrophysics (LUNA). We present recent improvements in the detection setup with the Bismuth Germanium Oxide (BGO) detector at LUNA, aiming to reduce high-energy backgrounds and to increase the summing detection efficiency. The new design results in enhanced sensitivity of the BGO setup, as we demonstrate and discuss in the context of the first direct measurement of the 65 keV resonance ($E_{x} = 5672$ keV) of the $^{17}$O($p,γ$)$^{18}$F reaction. Moreover, we show two applications of the BGO detector, which exploit its segmentation. In case of complex $γ$-ray cascades, e.g. the de-excitation of $E_{x} = 5672$ keV in $^{18}$F, the BGO segmentation allows to identify and suppress the beam-induced background signals that mimic the sum peak of interest. We demonstrate another new application for such a detector in form of in-situ activation measurements of a reaction with $β^{+}$ unstable product nuclei, e.g., the $^{14}$N($p,γ$)$^{15}$O reaction.
title Advances in Radiative Capture Studies at LUNA with a Segmented BGO Detector
topic Nuclear Experiment
Instrumentation and Detectors
url https://arxiv.org/abs/2510.05939