<?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>2026-10-19T01:10:03Z</responseDate><request verb="GetRecord" identifier="oai:ebyu-rdlopen.rawdatalibrary.net:ebyu/14305" metadataPrefix="oai_dc">https://ebyu-rdlopen.rawdatalibrary.net/oai/request</request><GetRecord><record><header><identifier>oai:ebyu-rdlopen.rawdatalibrary.net:ebyu/14305</identifier><datestamp>2026-10-18T20:39:06Z</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>L X-ray relative intensity ratios of uranium, lead, hafnium and samarium</dc:title><dc:creator>Akkuş, Tuba</dc:creator><dc:creator>Durdaǧl, Sevil</dc:creator><dc:creator>Yllmaz, Demet</dc:creator><dc:creator>Şahin, Yusuf</dc:creator><dc:contributor>Y., Oktem</dc:contributor><dc:contributor>F.C., Ozturk</dc:contributor><dc:contributor>G.S., Dogan</dc:contributor><dc:contributor>F., Guzelcimen</dc:contributor><dc:contributor>B., Akkus</dc:contributor><dc:subject>ELEMENTS</dc:subject><dc:subject>Physics, Applied</dc:subject><dc:subject>Physics, Multidisciplinary</dc:subject><dc:subject>Physics</dc:subject><dc:description>In this study the L shell X-ray relative intensities (ILl/ILγ,ILα/ILγandILβ/ILγ) for uranium, lead, hafnium and samarium have been measured for several scattering angles (85°, 95°, 105°, 115°, 125°and 135°) at 59.54 keV photon energy by using a Si(Li) detector which has a resolution of 160 eV at 5.9 keV. In previous studies, the Lγ X-rays were usually found independ on the scattering angles, therefore we found reasonable to give the ratio to the Lγ X-rays. © 2018 Author(s).</dc:description><dc:publisher>American Institute of Physics Inc.</dc:publisher><dc:date>2018</dc:date><dc:type>Conference Object</dc:type><dc:identifier>https://rdlopen.rawdatalibrary.net/r/ebyu/14305</dc:identifier><dc:identifier>https://doi.org/10.1063/1.5078898</dc:identifier><dc:identifier>978-073541768-7</dc:identifier><dc:identifier>0094-243X</dc:identifier><dc:language>en</dc:language><dc:relation>AIP Conference Proceedings</dc:relation><dc:rights>info:eu-repo/semantics/openAccess</dc:rights><dc:type>info:eu-repo/semantics/conferenceObject</dc:type><dc:identifier>https://ebyu-rdlopen.rawdatalibrary.net/tr/items/ebyu/14305</dc:identifier></oai_dc:dc></metadata></record></GetRecord></OAI-PMH>