Publication:
Calculation of angular distribution of 662 keV gamma rays by Monte Carlo method in copper medium

dc.contributor.authorKahraman A., Ozmutlu E., Gurler O., Yalcin S., Kaynak G., Gundogdu O.
dc.contributor.authorKahraman, A, Ozmutlu, EN, Gurler, O, Yalcin, S, Kaynak, G, Gundogdu, O
dc.date.accessioned2023-05-09T15:56:07Z
dc.date.available2023-05-09T15:56:07Z
dc.date.issued2009-12-01
dc.date.issued2009.01.01
dc.description.abstractThis paper presents results on the angular distribution of Compton scattering of 662 keV gamma photons in both forward and backward hemispheres in copper medium. The number of scattered events graph has been determined for scattered gamma photons in both the forward and backward hemispheres and theoretical saturation thicknesses have been obtained using these results. Furthermore, response function of a 51×51 mm NaI(Tl) detector at 60° angle with incoming photons scattered from a 10 mm thick copper layer has been determined using Monte Carlo method. © 2009 Elsevier Ltd. All rights reserved.
dc.identifier.doi10.1016/j.apradiso.2009.04.013
dc.identifier.endpage2087
dc.identifier.issn0969-8043
dc.identifier.scopus2-s2.0-70349805061
dc.identifier.startpage2083
dc.identifier.urihttps://hdl.handle.net/20.500.12597/12754
dc.identifier.volume67
dc.identifier.wosWOS:000271482800005
dc.relation.ispartofApplied Radiation and Isotopes
dc.relation.ispartofAPPLIED RADIATION AND ISOTOPES
dc.rightsfalse
dc.subjectAngular distribution | Compton scattered events | Monte Carlo
dc.titleCalculation of angular distribution of 662 keV gamma rays by Monte Carlo method in copper medium
dc.titleCalculation of angular distribution of 662 keV gamma rays by Monte Carlo method in copper medium
dc.typeArticle
dspace.entity.typePublication
oaire.citation.issue12
oaire.citation.volume67
relation.isScopusOfPublicationc6268e20-5177-44ea-b5e4-db8da37450a0
relation.isScopusOfPublication.latestForDiscoveryc6268e20-5177-44ea-b5e4-db8da37450a0
relation.isWosOfPublication60b03775-90f0-450e-a523-a97cdc1fc5a9
relation.isWosOfPublication.latestForDiscovery60b03775-90f0-450e-a523-a97cdc1fc5a9

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