<?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>2026-07-30T21:32:31Z</responseDate><request verb="GetRecord" identifier="oai:riubu.ubu.es:10259/7399" metadataPrefix="mods">https://riubu.ubu.es/oai/request</request><GetRecord><record><header><identifier>oai:riubu.ubu.es:10259/7399</identifier><datestamp>2023-03-24T13:04:55Z</datestamp><setSpec>com_10259.4_2557</setSpec><setSpec>com_10259_5086</setSpec><setSpec>com_10259_2604</setSpec><setSpec>col_10259.4_2558</setSpec></header><metadata><mods:mods xmlns:mods="http://www.loc.gov/mods/v3" xmlns:doc="http://www.lyncode.com/xoai" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.loc.gov/mods/v3 http://www.loc.gov/standards/mods/v3/mods-3-1.xsd">
<mods:name>
<mods:namePart>Carmona Martínez, José Manuel</mods:namePart>
</mods:name>
<mods:name>
<mods:namePart>Cortés Azcoiti, José Luis</mods:namePart>
</mods:name>
<mods:name>
<mods:namePart>Relancio Martínez, José Javier</mods:namePart>
</mods:name>
<mods:name>
<mods:namePart>Reyes Hung, Maykoll Anthonny</mods:namePart>
</mods:name>
<mods:name>
<mods:namePart>Vincueria, Alicia</mods:namePart>
</mods:name>
<mods:extension>
<mods:dateAvailable encoding="iso8601">2023-02-06T11:42:57Z</mods:dateAvailable>
</mods:extension>
<mods:extension>
<mods:dateAccessioned encoding="iso8601">2023-02-06T11:42:57Z</mods:dateAccessioned>
</mods:extension>
<mods:originInfo>
<mods:dateIssued encoding="iso8601">2022-07</mods:dateIssued>
</mods:originInfo>
<mods:identifier type="uri">http://hdl.handle.net/10259/7399</mods:identifier>
<mods:identifier type="doi">10.1140/epjp/s13360-022-02920-3</mods:identifier>
<mods:identifier type="essn">2190-5444</mods:identifier>
<mods:abstract>Ultra-high-energy physics is about to enter a new era thanks to the impressive results of experiments such as the Large&#xd;
High Altitude Air Shower Observatory, detecting photons of up to 1.4 × 1015 eV (PeV scale). These new results could be used to&#xd;
test deviations with respect to special relativity. While this has been already explored within the approach of Lorentz Invariance&#xd;
Violation theories, in this work we consider, for the first time, modifications due to a relativistic deformed kinematics (which appear&#xd;
in Doubly Special Relativity, or DSR, theories). In particular, we study the mean free path of very high-energy photons due to&#xd;
electron-positron pair creation when interacting with low-energy photons of the cosmic microwave background. Depending on the&#xd;
energy scale of the relativistic deformed kinematics, present (or near future) experiments can be sensitive enough to be able to&#xd;
identify deviations from special relativity.</mods:abstract>
<mods:language>
<mods:languageTerm>eng</mods:languageTerm>
</mods:language>
<mods:accessCondition type="useAndReproduction">http://creativecommons.org/licenses/by/4.0/</mods:accessCondition>
<mods:accessCondition type="useAndReproduction">info:eu-repo/semantics/openAccess</mods:accessCondition>
<mods:accessCondition type="useAndReproduction">Atribución 4.0 Internacional</mods:accessCondition>
<mods:titleInfo>
<mods:title>Modification of the mean free path of very high-energy photons due to a relativistic deformed kinematics</mods:title>
</mods:titleInfo>
<mods:genre>info:eu-repo/semantics/article</mods:genre>
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