<?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>2026-06-27T12:24:06Z</responseDate><request verb="GetRecord" identifier="oai:docta.ucm.es:20.500.14352/44523" metadataPrefix="mods">https://docta.ucm.es/rest/oai/request</request><GetRecord><record><header><identifier>oai:docta.ucm.es:20.500.14352/44523</identifier><datestamp>2025-08-06T17:01:46Z</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>Barbado, L. C.</mods:namePart>
   </mods:name>
   <mods:name>
      <mods:namePart>Barceló, C.</mods:namePart>
   </mods:name>
   <mods:name>
      <mods:namePart>Garay Elizondo, Luis Javier</mods:namePart>
   </mods:name>
   <mods:name>
      <mods:namePart>Jannes, Gil</mods:namePart>
   </mods:name>
   <mods:extension>
      <mods:dateAvailable encoding="iso8601">2023-06-20T03:50:00Z</mods:dateAvailable>
   </mods:extension>
   <mods:extension>
      <mods:dateAccessioned encoding="iso8601">2023-06-20T03:50:00Z</mods:dateAccessioned>
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   <mods:originInfo>
      <mods:dateIssued encoding="iso8601">2011</mods:dateIssued>
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   <mods:identifier type="citation">Barbado, L. C., C. Barceló, L. J. Garay, y G. Jannes. «The Trans-Planckian Problem as a Guiding Principle». Journal of High Energy Physics 2011, n.o 11 (23 de noviembre de 2011): 112. https://doi.org/10.1007/JHEP11(2011)112.</mods:identifier>
   <mods:identifier type="issn">1126-6708</mods:identifier>
   <mods:identifier type="doi">10.1007/JHEP11(2011)112</mods:identifier>
   <mods:identifier type="uri">https://hdl.handle.net/20.500.14352/44523</mods:identifier>
   <mods:identifier type="officialurl">http://dx.doi.org/10.1007/JHEP11(2011)112</mods:identifier>
   <mods:identifier type="relatedurl">http://link.springer.com/</mods:identifier>
   <mods:abstract>We use the avoidance of the trans-Planckian problem of Hawking radiation as a guiding principle in searching for a compelling scenario for the evaporation of black holes or black-hole-like objects. We argue that there exist only three possible scenarios, depending on whether the classical notion of long-lived horizon is preserved by high-energy physics and on whether the dark and compact astrophysical objects that we observe have long-lived horizons in the first place. Along the way, we find that i) a theory with high-energy superluminal signalling and a long-lived trapping horizon would be extremely unstable in astrophysical terms and that i i) stellar pulsations of objects hovering right outside but extremely close to their gravitational radius can result in a mechanism for Hawking-like emission.</mods:abstract>
   <mods:language>
      <mods:languageTerm>spa</mods:languageTerm>
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   <mods:accessCondition type="useAndReproduction">open access</mods:accessCondition>
   <mods:titleInfo>
      <mods:title>The trans-Planckian problem as a guiding principle</mods:title>
   </mods:titleInfo>
   <mods:genre>journal article</mods:genre>
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