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    <subfield code="a">10.1103/PhysRevD.111.064020</subfield>
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    <subfield code="a">Asorey, Manuel</subfield>
    <subfield code="u">Universidad de Zaragoza</subfield>
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    <subfield code="a">Stability of cosmological singularity-free solutions in quadratic gravity</subfield>
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    <subfield code="a">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.</subfield>
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    <subfield code="a">Ezquerro, Fernando</subfield>
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    <subfield code="a">Pardina, Miguel</subfield>
    <subfield code="u">Universidad de Zaragoza</subfield>
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    <subfield code="1">2004</subfield>
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    <subfield code="a">Universidad de Zaragoza</subfield>
    <subfield code="b">Dpto. Física Teórica</subfield>
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    <subfield code="g">111, 6 (2025), 9 pp.</subfield>
    <subfield code="p">Phys. rev. D</subfield>
    <subfield code="t">Physical Review D</subfield>
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