The ASACUSA collaboration has developed a detector consisting of a large size BGO crystal to detect an atomic antihydrogen beam, and performed the direct detection of antihydrogen atoms. Energy spectra from antihydrogen annihilation on the BGO crystal are discussed in comparison to simulation results from the GEANT4 toolkit. Background mainly originating from cosmic rays were strongly suppressed by analyzing the energy deposited in the BGO and requiring a multiplicity of charged pions. Thus antihydrogen events were identified.

Direct detection of antihydrogen atoms using a BGO crystal

Mascagna, V.;
2016-01-01

Abstract

The ASACUSA collaboration has developed a detector consisting of a large size BGO crystal to detect an atomic antihydrogen beam, and performed the direct detection of antihydrogen atoms. Energy spectra from antihydrogen annihilation on the BGO crystal are discussed in comparison to simulation results from the GEANT4 toolkit. Background mainly originating from cosmic rays were strongly suppressed by analyzing the energy deposited in the BGO and requiring a multiplicity of charged pions. Thus antihydrogen events were identified.
2016
840
153
159
7
http://www.sciencedirect.com/science/journal/01689002
Inglese
Antihydrogen; Antimatter; Cosmic ray background suppression; Detector; Inorganic scintillator; Nuclear and High Energy Physics; Instrumentation
262
Nagata, Y.; Kuroda, N.; Ohtsuka, M.; Leali, M.; Lodi-Rizzini, E.; Mascagna, V.; Tajima, M.; Torii, H. A.; Zurlo, N.; Matsuda, Y.; Venturelli, L.; Yama...espandi
none
Articoli su Riviste::Articolo su Rivista
12
info:eu-repo/semantics/article
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11383/2077916
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