Physics of the Early Universe

Name: Physics of the Early Universe
Start: 2022-06-13T09:00:00+02:00
End: 2022-06-17T18:00:00+02:00
Location: No location set

13–17 Jun 2022

Europe/Zurich timezone

Contact

early-universe@epfl.ch

Contribution List

9. Starting the Universe from strong gravity regime

Valery Rubakov (Institute for Nuclear Research of RAS)

13/06/2022, 10:20

10. A de-Sitter no-hair theorem for spacetimes with isometry group forming two-dimensional orbits

Leonardo Senatore

13/06/2022, 11:00

50. New boundary conditions for cosmology

Neil Turok

13/06/2022, 11:40

20. From Wormholes and Baby Universes to Inflation and the Measure Problem

Arthur Hebecker

13/06/2022, 14:00

21. Gravity and Axion

Gia Dvali

13/06/2022, 14:40

11. Quantum gravity from the beginning to the present Universe

Christof Wetterich

13/06/2022, 15:20

23. Gravitational wave production in non-local Starobinsky model

Anna Tokareva

13/06/2022, 16:30

24. Path integrals in some 2D and 4D quadratic gravity models

Vladimir Belokurov

13/06/2022, 17:10

12. Field redefinitions, perturbative unitarity, and Higgs inflation

Georgios Karananas

14/06/2022, 10:20

13. Higgs inflation as a door to gravity

Syksy Räsänen

14/06/2022, 11:00

14. Scale symmetry, the Higgs and the Nature of Gravity

Javier Rubio

14/06/2022, 11:40

15. IR effects in de Sitter and in Inflation

Victor Gorbenko

14/06/2022, 14:00

16. Bootstrapping large graviton non-Gaussianities

Enrico Pajer

14/06/2022, 14:40

Gravitational interferometers and cosmological observations of the cosmic microwave background offer us the prospect to probe the laws of gravity in the primordial universe. To study and interpret these datasets we need to know the possible graviton non-Gaussianities. To this end, we derive the most general tree-level three-point functions (bispectra) for a massless graviton to all orders in...

17. Fundamental Physics from Galaxy Surveys

Mikhail Ivanov

14/06/2022, 15:20

The distribution of galaxies on large scales is a sensitive probe of cosmological physics. In particular, the structure of this distribution depends on properties of dark matter and the dynamics of the early universe. Understanding this dependence, however, is a challenging task because the observed galaxy distribution is modulated by a variety of non-linear effects. I will present theoretical...

18. Generation of peaks in primordial perturbation spectra due to variable number of slow-roll inflatons

Alexei Starobinsky

14/06/2022, 16:30

19. Cosmological attractors after Planck/BICEP/Keck

Andrei Linde

14/06/2022, 17:10

25. Aspects of High Scale Leptogenesis with Low Energy CP Violation

Serguey Petcov

15/06/2022, 10:20

26. Resonant Leptogenesis

Björn Garbrecht

15/06/2022, 11:00