The antinucleus annihilation reconstruction algorithm of the GAPS experiment

The General AntiParticle Spectrometer (GAPS) is an Antarctic balloon-borne detector designed to measure low-energy cosmic antinuclei (<0.25GeV/n), with a specific focus on antideuterons, as a distinctive signal from dark matter annihilation or decay in the Galactic halo. The instrument consists o...

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Published in:Astroparticle Physics
Main Authors: Munini R., Vannuccini E., Boezio M., von Doetinchem P., Gerrity C., Lenni A., Marcelli N., Quinn S., Rogers F., Ryan J. L., Stoessl A., Xiao M., Saffold N., Tiberio A., Yamatani M.
Other Authors: Munini, R., Vannuccini, E., Boezio, M., von Doetinchem, P., Gerrity, C., Lenni, A., Marcelli, N., Quinn, S., Rogers, F., Ryan, J. L., Stoessl, A., Xiao, M., Saffold, N., Tiberio, A., Yamatani, M.
Format: Article in Journal/Newspaper
Language:English
Published: 2021
Subjects:
Online Access:http://hdl.handle.net/11368/2995933
https://doi.org/10.1016/j.astropartphys.2021.102640
https://arxiv.org/abs/2109.00753
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author Munini R.
Vannuccini E.
Boezio M.
von Doetinchem P.
Gerrity C.
Lenni A.
Marcelli N.
Quinn S.
Rogers F.
Ryan J. L.
Stoessl A.
Xiao M.
Saffold N.
Tiberio A.
Yamatani M.
author2 Munini, R.
Vannuccini, E.
Boezio, M.
von Doetinchem, P.
Gerrity, C.
Lenni, A.
Marcelli, N.
Quinn, S.
Rogers, F.
Ryan, J. L.
Stoessl, A.
Xiao, M.
Saffold, N.
Tiberio, A.
Yamatani, M.
author_facet Munini R.
Vannuccini E.
Boezio M.
von Doetinchem P.
Gerrity C.
Lenni A.
Marcelli N.
Quinn S.
Rogers F.
Ryan J. L.
Stoessl A.
Xiao M.
Saffold N.
Tiberio A.
Yamatani M.
author_sort Munini R.
collection Università degli studi di Trieste: ArTS (Archivio della ricerca di Trieste)
container_start_page 102640
container_title Astroparticle Physics
container_volume 133
description The General AntiParticle Spectrometer (GAPS) is an Antarctic balloon-borne detector designed to measure low-energy cosmic antinuclei (<0.25GeV/n), with a specific focus on antideuterons, as a distinctive signal from dark matter annihilation or decay in the Galactic halo. The instrument consists of a tracker, made up of ten planes of lithium-drifted Silicon Si(Li) detectors, surrounded by a plastic scintillator Time-of-Flight system. GAPS uses a novel particle identification method based on exotic atom capture and decay with the emission of pions, protons, and atomic X-rays from a common annihilation vertex. An important ingredient for the antinuclei identification is the reconstruction of the “annihilation star” topology. A custom antinucleus annihilation reconstruction algorithm, called the “star-finding” algorithm, was developed to reconstruct the annihilation star fully, determining the annihilation vertex position and reconstructing the tracks of the primary and secondary charged particles. The reconstruction algorithm and its performances were studied on simulated data obtained with the Geant4-based GAPS simulation software, which fully reproduced the detector geometry. This custom algorithm was found to have better performance in the vertex resolution and reconstruction efficiency compared with a standard Hough-3D algorithm.
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genre_facet Antarc*
Antarctic
geographic Antarctic
geographic_facet Antarctic
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op_collection_id ftunitriestiris
op_doi https://doi.org/10.1016/j.astropartphys.2021.102640
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volume:133
firstpage:1
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journal:ASTROPARTICLE PHYSICS
http://hdl.handle.net/11368/2995933
doi:10.1016/j.astropartphys.2021.102640
info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-85112245746
https://doi.org/10.1016/j.astropartphys.2021.102640
https://arxiv.org/abs/2109.00753
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spelling ftunitriestiris:oai:arts.units.it:11368/2995933 2025-01-16T19:24:28+00:00 The antinucleus annihilation reconstruction algorithm of the GAPS experiment Munini R. Vannuccini E. Boezio M. von Doetinchem P. Gerrity C. Lenni A. Marcelli N. Quinn S. Rogers F. Ryan J. L. Stoessl A. Xiao M. Saffold N. Tiberio A. Yamatani M. Munini, R. Vannuccini, E. Boezio, M. von Doetinchem, P. Gerrity, C. Lenni, A. Marcelli, N. Quinn, S. Rogers, F. Ryan, J. L. Stoessl, A. Xiao, M. Saffold, N. Tiberio, A. Yamatani, M. 2021 http://hdl.handle.net/11368/2995933 https://doi.org/10.1016/j.astropartphys.2021.102640 https://arxiv.org/abs/2109.00753 eng eng info:eu-repo/semantics/altIdentifier/wos/WOS:000692135400001 volume:133 firstpage:1 lastpage:32 numberofpages:32 journal:ASTROPARTICLE PHYSICS http://hdl.handle.net/11368/2995933 doi:10.1016/j.astropartphys.2021.102640 info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-85112245746 https://doi.org/10.1016/j.astropartphys.2021.102640 https://arxiv.org/abs/2109.00753 info:eu-repo/semantics/openAccess Annihilation Cosmic-ray Dark matter info:eu-repo/semantics/article 2021 ftunitriestiris https://doi.org/10.1016/j.astropartphys.2021.102640 2023-04-09T06:20:27Z The General AntiParticle Spectrometer (GAPS) is an Antarctic balloon-borne detector designed to measure low-energy cosmic antinuclei (<0.25GeV/n), with a specific focus on antideuterons, as a distinctive signal from dark matter annihilation or decay in the Galactic halo. The instrument consists of a tracker, made up of ten planes of lithium-drifted Silicon Si(Li) detectors, surrounded by a plastic scintillator Time-of-Flight system. GAPS uses a novel particle identification method based on exotic atom capture and decay with the emission of pions, protons, and atomic X-rays from a common annihilation vertex. An important ingredient for the antinuclei identification is the reconstruction of the “annihilation star” topology. A custom antinucleus annihilation reconstruction algorithm, called the “star-finding” algorithm, was developed to reconstruct the annihilation star fully, determining the annihilation vertex position and reconstructing the tracks of the primary and secondary charged particles. The reconstruction algorithm and its performances were studied on simulated data obtained with the Geant4-based GAPS simulation software, which fully reproduced the detector geometry. This custom algorithm was found to have better performance in the vertex resolution and reconstruction efficiency compared with a standard Hough-3D algorithm. Article in Journal/Newspaper Antarc* Antarctic Università degli studi di Trieste: ArTS (Archivio della ricerca di Trieste) Antarctic Astroparticle Physics 133 102640
spellingShingle Annihilation
Cosmic-ray
Dark matter
Munini R.
Vannuccini E.
Boezio M.
von Doetinchem P.
Gerrity C.
Lenni A.
Marcelli N.
Quinn S.
Rogers F.
Ryan J. L.
Stoessl A.
Xiao M.
Saffold N.
Tiberio A.
Yamatani M.
The antinucleus annihilation reconstruction algorithm of the GAPS experiment
title The antinucleus annihilation reconstruction algorithm of the GAPS experiment
title_full The antinucleus annihilation reconstruction algorithm of the GAPS experiment
title_fullStr The antinucleus annihilation reconstruction algorithm of the GAPS experiment
title_full_unstemmed The antinucleus annihilation reconstruction algorithm of the GAPS experiment
title_short The antinucleus annihilation reconstruction algorithm of the GAPS experiment
title_sort antinucleus annihilation reconstruction algorithm of the gaps experiment
topic Annihilation
Cosmic-ray
Dark matter
topic_facet Annihilation
Cosmic-ray
Dark matter
url http://hdl.handle.net/11368/2995933
https://doi.org/10.1016/j.astropartphys.2021.102640
https://arxiv.org/abs/2109.00753