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<dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:invenio="http://invenio-software.org/elements/1.0" 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:identifier>doi:10.1103/PhysRevD.111.064020</dc:identifier><dc:language>eng</dc:language><dc:creator>Asorey, Manuel</dc:creator><dc:creator>Ezquerro, Fernando</dc:creator><dc:creator>Pardina, Miguel</dc:creator><dc:title>Stability of cosmological singularity-free solutions in quadratic gravity</dc:title><dc:identifier>ART-2025-143445</dc:identifier><dc:description>We introduce a large family of homogeneous and isotropic cosmological solutions in quadratic gravity which are singularity-free at early and late times. This kind of smooth solutions only emerge beyond the nonstandard de Sitter branch 3⁢ &lt;,  and  being the couplings of the 2 and −2 ⁢ terms. We have analyzed the stability of these singularity-free solutions by computing the second-order variation of the action. We show that the expected instability is similar to that of the standard Λ Cold Dark Matter (Λ CDM) scenario. Thus, they provide cosmological background scenarios as legitimate as that of the Standard Model. The complete analysis shows that a singular big bang scenario can emerge from a singularity-free cosmological scenario when the parameters of the theory are slightly modified, which provides a bridge between the two very different cosmological scenarios with similar instabilities.</dc:description><dc:date>2025</dc:date><dc:source>http://zaguan.unizar.es/record/152174</dc:source><dc:doi>10.1103/PhysRevD.111.064020</dc:doi><dc:identifier>http://zaguan.unizar.es/record/152174</dc:identifier><dc:identifier>oai:zaguan.unizar.es:152174</dc:identifier><dc:relation>info:eu-repo/grantAgreement/ES/DGA-FSE/E21-17R</dc:relation><dc:relation>info:eu-repo/grantAgreement/ES/DGIID-DGA/2020-E21-17R</dc:relation><dc:relation>info:eu-repo/grantAgreement/ES/MICINN/PGC2022-126078NB-C21</dc:relation><dc:relation>info:eu-repo/grantAgreement/ES/NextGenerationEU/PRTR</dc:relation><dc:identifier.citation>Physical Review D 111, 6 (2025), 9 pp.</dc:identifier.citation><dc:rights>by</dc:rights><dc:rights>https://creativecommons.org/licenses/by/4.0/deed.es</dc:rights><dc:rights>info:eu-repo/semantics/closedAccess</dc:rights></dc:dc>

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