31 May 2023 to 2 June 2023
CERN
Europe/Zurich timezone

Session

Early Universe

1 Jun 2023, 09:30
500/1-001 - Main Auditorium (CERN)

500/1-001 - Main Auditorium

CERN

400
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Conveners

Early Universe

  • Silvia Pascoli

Early Universe

  • Silvia Pascoli

Presentation materials

There are no materials yet.

  1. Mehrdad Mirbabayi
    01/06/2023, 09:30
  2. Julia Harz
    01/06/2023, 10:00
  3. Ville Vaskonen
    01/06/2023, 11:15
  4. Guillermo Franco Abellán
    01/06/2023, 11:45
    early universe cosmology

    Although the CMB and galaxy surveys provide precise measurements of the primordial power spectrum at large scales, the small-scale power spectrum remains largely unconstrained. An enhancement in the small-scale primordial spectrum can lead to the formation of Ultra-Compact-Mini-Halos (UCMH) much earlier than standard halo can form. As a result, the DM annihilation signal receives a boost than...

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  5. Basabendu Barman
    01/06/2023, 11:52
    early universe cosmology

    We show that a minimal scenario, utilizing only the graviton as an intermediate messenger between the inflaton, the dark sector and the Standard Model (SM), is able to generate simultaneously the observed relic density of dark matter (DM), the baryon asymmetry through leptogenesis, as well as a sufficiently hot thermal bath after inflation. The possibility of reheating via minimal...

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  6. Denis Werth
    01/06/2023, 11:59
    early universe cosmology

    Correlation functions of primordial density fluctuations provide an exciting probe of the physics governing the earliest moments of our Universe. However, the standard approach to compute them is technically challenging. Theoretical predictions are therefore available only in restricted classes of theories, which can completely bias the interpretation of data.

    In this talk, I will present...

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  7. Anna Kormu
    01/06/2023, 12:06
    early universe cosmology

    In the Standard Model the electroweak phase transition is a crossover, but in many beyond the Standard Model theories the transition is of first order. Strong first order phase transitions could produce gravitational waves that might be detectable by the Laser Interferometer Space Antenna (LISA). Perturbation theory is commonly used to estimate the parameters that enter the calculation of...

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  8. Alejandro Perez Rodriguez (Universidad Autonoma de Madrid)
    01/06/2023, 12:13
    early universe cosmology

    Introducing an energy transfer between the inflaton field and a thermal bath modifies the primordial power spectrum $\mathcal{P}_\mathcal{R}$ due to the thermal fluctuations acting as a stochastic source for the curvature perturbations. We propose a fast and accurate method to compute $\mathcal{P}_\mathcal{R}$ in this context based on the Fokker-Planck equation, and verify its consistency...

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  9. Helena Kolesova (Institute for Theoretical Physics, University of Bern)
    01/06/2023, 12:20
    early universe cosmology

    As the nature of dark matter remains unresolved, existence of a whole dark sector is an intriguing possibility. It is also natural to assume that such dark sector couples to inflationary dynamics. As an example, we consider the case of warm axion inflation coupled to a non-Abelian dark sector, both in weakly and strongly coupled regime. We show that this simple setup provides rich...

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  10. Denis WERTH
  11. Alejandro PEREZ RODRIGUEZ
  12. Guillermo FRANCO ABELLÁN
  13. Anna KORMU
  14. Helena KOLESOVA
  15. BARMAN BASABENDU
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