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<dc:title>Modification of the mean free path of very high-energy photons due to a relativistic deformed kinematics</dc:title>
<dc:creator>Carmona Martínez, José Manuel</dc:creator>
<dc:creator>Cortés Azcoiti, José Luis</dc:creator>
<dc:creator>Relancio Martínez, José Javier</dc:creator>
<dc:creator>Reyes Hung, Maykoll Anthonny</dc:creator>
<dc:creator>Vincueria, Alicia</dc:creator>
<dc:subject>Matemáticas</dc:subject>
<dc:subject>Física</dc:subject>
<dc:subject>Mathematics</dc:subject>
<dc:subject>Physics</dc:subject>
<dc:description>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.</dc:description>
<dc:description>This work is supported by Spanish Grants PGC2018-095328-B-I00 (FEDER/AEI), and DGIID-DGA No. 2015-E24/2. JJR acknowledges support from the INFN Iniziativa Specifica GeoSymQFT and Unión Europea-NextGenerationEU (“Ayudas Margarita Salas para la formación de jóvenes doctores”). The work of MAR was supported by MICIU/AEI/FSE (FPI Grant PRE2019-089024). This work has been partially supported by Agencia Estatal de Investigación (Spain) under Grant PID2019-106802GB-I00/AEI/10.13039/501100011033. The authors would like to acknowledge the contribution of the COST Action CA18108 “Quantum gravity phenomenology in the multi-messenger approach”.</dc:description>
<dc:date>2023-02-06T11:42:57Z</dc:date>
<dc:date>2023-02-06T11:42:57Z</dc:date>
<dc:date>2022-07</dc:date>
<dc:type>info:eu-repo/semantics/article</dc:type>
<dc:type>info:eu-repo/semantics/publishedVersion</dc:type>
<dc:identifier>http://hdl.handle.net/10259/7399</dc:identifier>
<dc:identifier>10.1140/epjp/s13360-022-02920-3</dc:identifier>
<dc:identifier>2190-5444</dc:identifier>
<dc:language>eng</dc:language>
<dc:relation>The European Physical Journal Plus. 2022, V. 137, n. 7, 768</dc:relation>
<dc:relation>https://doi.org/10.1140/epjp/s13360-022-02920-3</dc:relation>
<dc:relation>info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PGC2018-095328-B-I00/ES/MAS ALLA DE LOS MODELOS ESTANDAR: SIMETRIA, GRAVEDAD Y MATERIA OSCURA/</dc:relation>
<dc:relation>info:eu-repo/grantAgreement/Gobierno de Aragón//2015-E24%2F2/</dc:relation>
<dc:relation>info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PRE2019-089024/</dc:relation>
<dc:relation>info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PID2019-106802GB-I00/ES/GRUPO CUANTICOS, GRUPOS DE POISSON-LIE, ESPACIOS HOMOGENEOS Y APLICACIONES/</dc:relation>
<dc:relation>info:eu-repo/grantAgreement/COST//CA18108/EU/Quantum gravity phenomenology in the multi-messenger approach/QG-MM/</dc:relation>
<dc:rights>Atribución 4.0 Internacional</dc:rights>
<dc:rights>http://creativecommons.org/licenses/by/4.0/</dc:rights>
<dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
<dc:format>application/pdf</dc:format>
<dc:publisher>Springer Nature</dc:publisher>
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