<?xml version="1.0" encoding="UTF-8"?><OAI-PMH xmlns="http://www.openarchives.org/OAI/2.0/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd"><responseDate>2026-10-19T04:52:52Z</responseDate><request verb="GetRecord" identifier="oai:ebyu-rdlopen.rawdatalibrary.net:ebyu/13881" metadataPrefix="oai_dc">https://ebyu-rdlopen.rawdatalibrary.net/oai/request</request><GetRecord><record><header><identifier>oai:ebyu-rdlopen.rawdatalibrary.net:ebyu/13881</identifier><datestamp>2026-10-18T21:13:30Z</datestamp><setSpec>openaire</setSpec><setSpec>driver</setSpec><setSpec>com_ebyu_10000</setSpec><setSpec>col_ebyu_10001</setSpec></header><metadata><oai_dc:dc xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd"><dc:title>Dependence of albedo factors on mean atomic number for 662 keV gamma photons</dc:title><dc:creator>Akkuş, Tuba</dc:creator><dc:creator>Yılmaz, Demet</dc:creator><dc:subject>Albedo factors</dc:subject><dc:subject>Backscattering</dc:subject><dc:subject>Dilution</dc:subject><dc:subject>Gamma rays</dc:subject><dc:subject>Mean atomic number</dc:subject><dc:subject>Germanium Compounds</dc:subject><dc:subject>Phosphorus Compounds</dc:subject><dc:subject>Radioactivity</dc:subject><dc:subject>Sun Light</dc:subject><dc:subject>Solar radiation</dc:subject><dc:subject>bismuth</dc:subject><dc:subject>cellulose</dc:subject><dc:subject>cesium 137</dc:subject><dc:subject>Atomic numbers</dc:subject><dc:subject>Cellulose powder</dc:subject><dc:subject>Dilution technique</dc:subject><dc:subject>Gamma photons</dc:subject><dc:subject>HPGe detectors</dc:subject><dc:subject>Radioactive sources</dc:subject><dc:subject>Scattering angles</dc:subject><dc:subject>albedo</dc:subject><dc:subject>Article</dc:subject><dc:subject>dosimetry</dc:subject><dc:subject>electromagnetic radiation</dc:subject><dc:subject>gamma radiation</dc:subject><dc:subject>photon</dc:subject><dc:subject>priority journal</dc:subject><dc:subject>radiation dose</dc:subject><dc:subject>radiation energy</dc:subject><dc:subject>radiation scattering</dc:subject><dc:description>The albedo factors (number, energy and dose) of the samples with various mean atomic number have been investigated at a scattering angle of 180°. Fourteen different samples in the mean atomic number range 9.743 ≤ Z‾ ≤ 83.00 were obtained with bismuth and cellulose powders by using dilution technique. Thus, albedo factors have been investigated in a wide atomic number range. The samples were irritated by 662 keV gamma rays emitted from a137Cs radioactive source. The scattered γ -rays were counted by an HPGe detector with active area of 200 mm2. It has been observed that albedo factors decrease with increasing mean atomic number. Also, there is a high correlation between albedo factors and mean atomic numbers. © 2019 Elsevier Ltd</dc:description><dc:publisher>Elsevier Ltd</dc:publisher><dc:date>2019</dc:date><dc:type>Article</dc:type><dc:identifier>https://rdlopen.rawdatalibrary.net/r/ebyu/13881</dc:identifier><dc:identifier>https://doi.org/10.1016/j.apradiso.2019.108870</dc:identifier><dc:identifier>0969-8043</dc:identifier><dc:language>en</dc:language><dc:relation>Applied Radiation and Isotopes</dc:relation><dc:rights>info:eu-repo/semantics/openAccess</dc:rights><dc:type>info:eu-repo/semantics/article</dc:type><dc:identifier>https://ebyu-rdlopen.rawdatalibrary.net/tr/items/ebyu/13881</dc:identifier></oai_dc:dc></metadata></record></GetRecord></OAI-PMH>