5–9 Sept 2022
TU Wien
Europe/Vienna timezone

Session

Astronomy, Astrophysics and Cosmology

5 Sept 2022, 09:00
TU Wien

TU Wien

Karlsplatz 13, 1040 Wien

Conveners

Astronomy, Astrophysics and Cosmology

  • gianluca inguglia

Astronomy, Astrophysics and Cosmology

  • gianluca inguglia

Astronomy, Astrophysics and Cosmology

  • Maura Graziani (Universita e INFN, Perugia (IT))

Astronomy, Astrophysics and Cosmology

  • Maura Graziani (Universita e INFN, Perugia (IT))

Presentation materials

There are no materials yet.

  1. Jochen Schieck (Austrian Academy of Sciences (AT))
    05/09/2022, 09:00
  2. Gianluca Inguglia (Austrian Academy of Sciences (AT)), gianluca inguglia
    05/09/2022, 09:10
    Contributed Talk
  3. Andrii Neronov, Andrii Neronov (Universite de Geneve (CH))
    05/09/2022, 09:30
  4. Nicolas Leroy
    05/09/2022, 10:00
  5. Domenico D'Urso (Universita e INFN, Perugia (IT))
    05/09/2022, 11:00
  6. Kamlesh Rajpurohit
    05/09/2022, 11:30
  7. Maura Graziani (Universita e INFN, Perugia (IT))
    05/09/2022, 12:00
  8. Chad Finley
    05/09/2022, 14:00
  9. Jutta Schnabel
    05/09/2022, 14:30
  10. Serguei Vorobiov
    05/09/2022, 15:00
    Contributed Talk

    Ultra-high-energy cosmic rays (UHECRs) are mostly protons and heavier nuclei arriving on Earth from space and producing particle cascades in the atmosphere, ”extensive air showers”. As of today, the most precise and high-statistics data set of the rare (≤ 1 particle per square km per year above 10 EeV) UHECR events is obtained by the Pierre Auger Observatory, a large area (~3000 square km)...

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  11. Michael Florian Wondrak (Radboud University Nijmegen)
    05/09/2022, 15:30
  12. Antonio Racioppi (National Institute of Chemical Physics and Biophysics (EE))
    05/09/2022, 16:30
    Astronomy, Astrophysics and Cosmology
    Contributed Talk

    We study single field slow-roll inflation in the presence of $F(R)$ gravity in the Palatini formulation. In contrast to metric $F(R)$, when rewritten in terms of an auxiliary field and moved to the Einstein frame, Palatini $F(R)$ does not develop a new dynamical degree of freedom. However, it is not possible to solve analytically the constraint equation of the auxiliary field for a general...

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  13. Dr Violetta Sagun (University of Coimbra)
    05/09/2022, 17:00
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