PUC program: The pulse pile up correction for x-ray and gamma ray spectrometry

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Özet

Pile up and dead time are two important corrections in the analysis of X-ray and gamma ray spectra. The most important of these is pile up correction because these peaks do not really exist in the spectra; they only seem to exist. For this reason, these peaks affect both the qualitative and quantitative accuracy of the analysis. In addition, the pile up pulses forming the pile up peaks increase the background count in the spectrum. Companies that produce X-ray or gamma ray detector systems design pile up reject circuits and integrate them into detector systems to prevent these pulses. These circuits have time limitations because they are made up of electronic devices. For this reason, the pile up problem cannot be solved completely in these circuits. Therefore, mathematical models based on a statistical approach are needed. Such a model was developed in this study. A computer program based on this model was developed. This developed program has been applied to X-ray and gamma ray spectra. It has been shown that this model provides about 2% correction in the main peak regions and significantly reduces background counts.

Anahtar Kelimeler

RDL Kalıcı Bağlantı (PID)
https://rdlopen.rawdatalibrary.net/r/gumushane/12892Resmi atıflarda kullanılan kalıcı adres
DOI
https://doi.org/10.1139/cjp-2019-0431Yayıncı resmi DOI adresi
Tam Kayıt
AlanDeğerDil
dc.contributor.authorKarabıdak, S.M.
dc.contributor.authorKaya, S.
dc.date.accessioned2026-10-22T10:20:40.473879229Z
dc.date.available2026-10-22T10:20:40.473879229Z
dc.date.issued2020
dc.description.abstractPile up and dead time are two important corrections in the analysis of X-ray and gamma ray spectra. The most important of these is pile up correction because these peaks do not really exist in the spectra; they only seem to exist. For this reason, these peaks affect both the qualitative and quantitative accuracy of the analysis. In addition, the pile up pulses forming the pile up peaks increase the background count in the spectrum. Companies that produce X-ray or gamma ray detector systems design pile up reject circuits and integrate them into detector systems to prevent these pulses. These circuits have time limitations because they are made up of electronic devices. For this reason, the pile up problem cannot be solved completely in these circuits. Therefore, mathematical models based on a statistical approach are needed. Such a model was developed in this study. A computer program based on this model was developed. This developed program has been applied to X-ray and gamma ray spectra. It has been shown that this model provides about 2% correction in the main peak regions and significantly reduces background counts.
dc.identifier.doi10.1139/cjp-2019-0431
dc.identifier.eissn1208-6045
dc.identifier.endpage882
dc.identifier.issn0008-4204
dc.identifier.issue9
dc.identifier.scopus2-s2.0-85090357399
dc.identifier.startpage877
dc.identifier.urihttps://rdlopen.rawdatalibrary.net/r/gumushane/12892
dc.identifier.volume98
dc.identifier.wosWOS:000569363900009
dc.language.isoen
dc.publisherCanadian Science Publishing
dc.relation.ispartofCanadian Journal of Physics
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.subjectComputer program
dc.subjectMinimum resolving time
dc.subjectPeaking time
dc.subjectPile up correct
dc.subjectPile up pulse
dc.subject.classificationPhysics, Multidisciplinary
dc.subject.classificationPhysics
dc.subject.otherGamma ray spectrometers
dc.subject.otherPiles
dc.subject.otherSpectrometry
dc.subject.otherUltraviolet spectroscopy
dc.subject.otherX ray detectors
dc.subject.otherX rays
dc.subject.otherDetector systems
dc.subject.otherElectronic device
dc.subject.otherGamma ray detector
dc.subject.otherGamma ray spectra
dc.subject.otherGamma ray spectrometry
dc.subject.otherPulse pile-up
dc.subject.otherQuantitative accuracy
dc.subject.otherStatistical approach
dc.subject.otherGamma rays
dc.titlePUC program: The pulse pile up correction for x-ray and gamma ray spectrometry
dc.typeArticle
dspace.entity.typePublication
rdl.citation.openalex3
rdl.citation.scopus3
rdl.citation.wos2
rdl.oa.statusclosed
rdl.source.indexSCOPUS
rdl.source.indexWOS
rdl.wos.indexScience Citation Index Expanded (SCI-EXPANDED)