Energy and coincidence-time resolution of the LaBr3:Ce-MPPC™ detectors under magnetic fields

dc.contributor.authorYAP, IAN C. J.
dc.contributor.authorHEINIGER-SCHELL, JULIANA
dc.contributor.authorDANG, THIEN T.
dc.contributor.authorLIMA, NICOLE P. de
dc.contributor.authorDORSCHEL, BJORN
dc.contributor.authorSTEGENBORG, MAGNUS H.
dc.contributor.authorSOUZA, ALEXANDRE P. dos S.
dc.contributor.authorCORREA, BRUNO S.
dc.contributor.authorMIRANDA FILHO, ARNALDO A.
dc.contributor.authorGERAMI, ADELEH M.
dc.contributor.authorLUPASCU, DORU C.
dc.coverageInternacional
dc.date.accessioned2026-10-02T17:02:28Z
dc.date.available2026-10-02T17:02:28Z
dc.date.issued2026
dc.description.abstractTime-differential perturbed angular correlation (TDPAC) spectroscopy is a nuclear solid-state technique that requires high energy and coincidence-time resolutions from scintillation crystals and photodetectors. Traditionally, photomultiplier tubes (PMTs) have been coupled to LaBr3:Ce crystals; however, they have been replaced by Multi Pixel Photon Counters (MPPCs) for TDPAC experiments conducted under external magnetic fields. In this report, we show that, for TDPAC spectroscopy, the performance of the LaBr3:Ce-MPPC detector remains stable under magnetic fields up to 8.5 T (in 1 T steps), as evidenced by the unchanged energy and coincidence-time resolutions of the 511 keV peaks from positron–electron (e+-e-) annihilation in a sealed 22Na calibration source.
dc.description.sponsorshipGerman Federal Ministry of Research, Technology and Space (BMFTR)
dc.description.sponsorshipIDBMFTR: 05K22PGA; 05K25PGA; 05K22PGB
dc.format.extent1-11
dc.identifier.citationYAP, IAN C. J.; HEINIGER-SCHELL, JULIANA; DANG, THIEN T.; LIMA, NICOLE P. de; DORSCHEL, BJORN; STEGENBORG, MAGNUS H.; SOUZA, ALEXANDRE P. dos S.; CORREA, BRUNO S.; MIRANDA FILHO, ARNALDO A.; GERAMI, ADELEH M.; LUPASCU, DORU C. Energy and coincidence-time resolution of the LaBr3:Ce-MPPC™ detectors under magnetic fields. <b>Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment</b>, v. 1088, p. 1-11, 2026. DOI: <a href="https://dx.doi.org/10.1016/j.nima.2026.171480">10.1016/j.nima.2026.171480</a>. Disponível em: https://repositorio.ipen.br/handle/123456789/50191.
dc.identifier.doi10.1016/j.nima.2026.171480
dc.identifier.issn0168-9002
dc.identifier.percentilfi33.2
dc.identifier.percentilfiCiteScore56.5
dc.identifier.urihttps://repositorio.ipen.br/handle/123456789/50191
dc.identifier.vol1088
dc.language.isoeng
dc.relation.ispartofNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
dc.rightsopenAccess
dc.titleEnergy and coincidence-time resolution of the LaBr3:Ce-MPPC™ detectors under magnetic fields
dc.typeArtigo de periódico
dspace.entity.typePublication
ipen.autorNICOLE PEREIRA DE LIMA
ipen.autorALEXANDRE PINHO DOS SANTOS SOUZA
ipen.autorBRUNO SANTOS CORREA
ipen.autorARNALDO ALVES MIRANDA FILHO
ipen.codigoautor14277
ipen.codigoautor15442
ipen.codigoautor15164
ipen.codigoautor15159
ipen.contributor.ipenauthorNICOLE PEREIRA DE LIMA
ipen.contributor.ipenauthorALEXANDRE PINHO DOS SANTOS SOUZA
ipen.contributor.ipenauthorBRUNO SANTOS CORREA
ipen.contributor.ipenauthorARNALDO ALVES MIRANDA FILHO
ipen.identifier.fi1.5
ipen.identifier.fiCiteScore2.9
ipen.identifier.ipendoc32125
ipen.identifier.iwosWoS
ipen.range.fi1.500 - 2.999
ipen.range.percentilfi25.00 - 49.99
ipen.type.genreArtigo
relation.isAuthorOfPublication588a3118-cce3-4c6c-8dcc-a1cee1a4a117
relation.isAuthorOfPublication164c9934-6d0f-430d-a47a-d7b9fdcfbe08
relation.isAuthorOfPublication0cfcf140-1709-41ab-ab72-877c86f94225
relation.isAuthorOfPublication02361e77-4a61-450d-b0be-b5fc3966a7e9
relation.isAuthorOfPublication.latestForDiscovery588a3118-cce3-4c6c-8dcc-a1cee1a4a117
sigepi.autor.atividadeNICOLE PEREIRA DE LIMA:14277:310:N
sigepi.autor.atividadeALEXANDRE PINHO DOS SANTOS SOUZA:15442:450:N
sigepi.autor.atividadeBRUNO SANTOS CORREA:15164:310:N
sigepi.autor.atividadeARNALDO ALVES MIRANDA FILHO:15159:310:N

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