Cosmic Inflation: From Observations to Particle Models

Contribution List

1. Gravitational Waves

Stavros Katsanevas

18/06/2022, 09:15

2. Gravitational Anomalies, torsion and potential geometric origin of the Universe Dark Sector

Nikolaos Mavromatos (National Tech. U. Athens)

18/06/2022, 10:00

10. de Sitter vacua, moduli stabilisation and hybrid inflation in string theory

George Leontaris

18/06/2022, 10:30

5. Looking for torsional modified gravity signatures in inflationary observables

EMMANOUIL SARIDAKIS (National Technical University of Athens)

18/06/2022, 11:00

4. Quintessential Inflation Latest

Kostas Dimopoulos

18/06/2022, 12:00

9. Cosmic Inflation and Gravity Waves

Qaisar Shafi

18/06/2022, 12:30

16. Models for Freeze-in Baryogenesis

Vasilis Spanos

18/06/2022, 13:00

11. Formulating E- & T-Model Inflation in Supergravity

Constantinos Pallis (AUTH)

18/06/2022, 14:10

12. New inflationary solutions from old ones

Andronikos Paliathanasis (Durban University of Technology)

18/06/2022, 14:30

13. Cosmological Hyperfluids, Torsion and Non-metricity

Damianos Iosifidis

18/06/2022, 14:50

14. Reduced Einstein-Hilbert action: Inflation and the Swampland criteria

Achilles Gitsis (Aristotle University of Thessaloniki)

18/06/2022, 15:10

6. Modified Gravity Effects on Primordial Gravitational Waves

Vasilis Oikonomou

18/06/2022, 15:30

3. CMB polarization B-mode search with QUBIC and CMB-S4

Sotiris Loucatos (Irfu CEA-Saclay and APC Paris)

8. Rescaled Einstein-Hilbert Gravity: Inflation and the Swampland Criteria

Achilles Gitsis (Aristotle University of Thessaloniki)

In this work, a class of f(R, φ) gravity models is studied which during the inflationary era,
which is the large curvature regime, result to an effective inflationary Lagrangian that contains a
rescaled Einstein-Hilbert term αR in the presence of a canonical minimally coupled scalar field. The
dimensionless parameter α is chosen to take values in the range 0 < α < 1 and the main...

15. TBA

Konstantinos Dialektopoulos