<?xml version="1.0" encoding="UTF-8"?><?xml-stylesheet type="text/xsl" href="static/style.xsl"?><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>2026-08-20T02:02:48Z</responseDate><request verb="GetRecord" identifier="oai:docta.ucm.es:20.500.14352/88349" metadataPrefix="mods">https://docta.ucm.es/rest/oai/request</request><GetRecord><record><header><identifier>oai:docta.ucm.es:20.500.14352/88349</identifier><datestamp>2024-09-24T16:06:54Z</datestamp><setSpec>com_20.500.14352_14</setSpec><setSpec>col_20.500.14352_15</setSpec></header><metadata><mods:mods xmlns:mods="http://www.loc.gov/mods/v3" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:doc="http://www.lyncode.com/xoai" xsi:schemaLocation="http://www.loc.gov/mods/v3 http://www.loc.gov/standards/mods/v3/mods-3-1.xsd">
   <mods:name>
      <mods:namePart>Verlinde, M</mods:namePart>
   </mods:name>
   <mods:name>
      <mods:namePart>Kraemer, S.</mods:namePart>
   </mods:name>
   <mods:name>
      <mods:namePart>Moens, J.</mods:namePart>
   </mods:name>
   <mods:name>
      <mods:namePart>Fraile Prieto, Luis Mario</mods:namePart>
   </mods:name>
   <mods:name>
      <mods:namePart>Wilkins, S. G.</mods:namePart>
   </mods:name>
   <mods:extension>
      <mods:dateAvailable encoding="iso8601">2023-10-19T18:23:03Z</mods:dateAvailable>
   </mods:extension>
   <mods:extension>
      <mods:dateAccessioned encoding="iso8601">2023-10-19T18:23:03Z</mods:dateAccessioned>
   </mods:extension>
   <mods:originInfo>
      <mods:dateIssued encoding="iso8601">2019-08-12</mods:dateIssued>
   </mods:originInfo>
   <mods:identifier type="issn">2469-9985</mods:identifier>
   <mods:identifier type="doi">10.1103/PhysRevC.100.024315</mods:identifier>
   <mods:identifier type="uri">https://hdl.handle.net/20.500.14352/88349</mods:identifier>
   <mods:identifier type="essn">2469-9993</mods:identifier>
   <mods:identifier type="officialurl">https://journals.aps.org/prc/abstract/10.1103/PhysRevC.100.024315</mods:identifier>
   <mods:abstract>A new approach to observe the radiative decay of the ^229 Th nuclear isomer, and to determine its energy and radiative lifetime, is presented. Situated at a uniquely low excitation energy, this nuclear state might be a key ingredient for the development of a nuclear clock or a nuclear laser and, the search for time variations of fundamental constants like the fine structure constant. The isomer's gamma decay towards the ground state will be studied with a high-resolution vacuum ultraviolet (VUV) spectrometer after its production by the beta decay of ^Ac 229. The novel production method presents a number of advantages asserting its competitive nature with respect to the commonly used ^U 233 alpha-decay recoil source. In this paper, a feasibility analysis of this new concept, and an experimental investigation of its key ingredients, using a pure ^Ac 229 ion beam produced at the ISOLDE radioactive beam facility, is reported.</mods:abstract>
   <mods:language>
      <mods:languageTerm>eng</mods:languageTerm>
   </mods:language>
   <mods:accessCondition type="useAndReproduction">open access</mods:accessCondition>
   <mods:titleInfo>
      <mods:title>Alternative approach to populate and study the ^229 Th nuclear clock isomer</mods:title>
   </mods:titleInfo>
   <mods:genre>journal article</mods:genre>
</mods:mods></metadata></record></GetRecord></OAI-PMH>