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  <title>RIUNACH Comunidad :</title>
  <link rel="alternate" href="http://https://repositorio.unach.mx:80/jspui/handle/123456789/4087" />
  <subtitle />
  <id>http://https://repositorio.unach.mx:80/jspui/handle/123456789/4087</id>
  <updated>2026-05-12T21:56:09Z</updated>
  <dc:date>2026-05-12T21:56:09Z</dc:date>
  <entry>
    <title>Constraining the nature of dark matter and cosmic inflation using CMB spectral distortions</title>
    <link rel="alternate" href="http://https://repositorio.unach.mx:80/jspui/handle/123456789/4089" />
    <author>
      <name>RAÚL ANTONIO HENRÍQUEZ ORTIZ</name>
    </author>
    <id>http://https://repositorio.unach.mx:80/jspui/handle/123456789/4089</id>
    <updated>2023-10-05T18:39:43Z</updated>
    <published>2023-02-01T00:00:00Z</published>
    <summary type="text">Título : Constraining the nature of dark matter and cosmic inflation using CMB spectral distortions
Autor: RAÚL ANTONIO HENRÍQUEZ ORTIZ
Descripción : With the advent of new missions to probe spectral distortions of the cosmic microwave back-ground with unprecedented precision, the study of theoretical predictions of these signals be-comes a promising avenue to test our description of the early Universe  To explore new constraints on dark matter and inflation based on alternative models beyond o cosmological standard model, we compute the spectral distortions of two models, reveal-ing interesting features that maybe compatible with Planck data and future missions like the&#xD;
Primordial Inflation Explorer (PIXIE). First, for the dark matter model we used a QCD dark matter scenario that is a model characterized by a phase transition in the early universe. Sec-ond, for the inflation model we used the axion monodromy, whose main feature is a potential with oscillations.</summary>
    <dc:date>2023-02-01T00:00:00Z</dc:date>
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