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Prof. Yann Mambrini (CNRS, IJCLab, Université Paris-Saclay)14/09/2026 09:45
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Ed Copeland14/09/2026 10:00
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Juri Smirnov (University of Liverpool)14/09/2026 10:45
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Oleg Lebedev (University of Helsinki)14/09/2026 12:00
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Rocky Kolb (The University of Chicago)14/09/2026 14:00
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William Kinney (Univ. at Buffalo, SUNY)14/09/2026 14:45
The well-known Borde-Guth-Vilenkin Theorem shows that inflationary
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spacetimes are generically geodesically past-incomplete, necessitating
the existence of a pre-inflationary boundary of some sort, possibly
singular. In this talk, I discuss the generalization of the BGV theorem
to spactimes beyond inflation, including inhomogeneous and cyclic
models. I argue that the cyclic model proposed... -
Prof. Mikhail Shaposhnikov (EPFL)14/09/2026 16:00
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Julien Froustey (IFIC, CSIC-UV)14/09/2026 16:45
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15/09/2026 09:50
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Kamila Kowalska (National Centre for Nuclear Research)15/09/2026 10:00
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Marek Lewicki (University of Warsaw & AstroCeNT)15/09/2026 10:30
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Mathieu Gross (IJCLab)15/09/2026 11:30
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Juri Smirnov (University of Liverpool), Pedro Schwaller (Mainz University)15/09/2026 12:00
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Zurab Berezhiani (University of Aquila)15/09/2026 14:00
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Yann GOUTTENOIRE (IAP)15/09/2026 14:30
I will present the 13 channels of gravitational wave production which are at play when the universe is reheated from the evaporation of a population of primordial black holes dominating the energy density of the universe
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Stephen King15/09/2026 15:00
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Kyohei Mukaida15/09/2026 16:00
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Enrico Maria Sessolo (National Centre for Nuclear Research, Warsaw)15/09/2026 16:30
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Matteo Braglia (CERN)16/09/2026 10:00
eviations from slow-roll can leave characteristic oscillatory imprints in the spectrum of primordial perturbations, known as primordial features. If detected, such signals could reveal new energy scales during inflation or provide evidence for additional massive degrees of freedom. In this talk, I will review what we can learn from primordial features, discuss the hints currently present in...
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Marco Peloso (University of Padua and INFN, Sezione di Padova)16/09/2026 10:30
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Emilian Dudas (CPTHE (Ecole polytechnique))16/09/2026 11:30
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Matthew Mccullough (CERN)16/09/2026 12:00
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Thomas Colas (DAMTP - University of Cambridge)16/09/2026 14:00
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Pasquale SERPICO (LAPTh)16/09/2026 14:30
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David Stefanyszyn (University of Nottingham)16/09/2026 15:00
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Bogumiła Świeżewska (University of Warsaw)16/09/2026 16:00
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Pedro Schwaller (Mainz University)16/09/2026 16:30
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16/09/2026 19:45
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Marco Drewes (UCLouvain)17/09/2026 10:00
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Fotis Koutroulis (IHEP, Beijing)17/09/2026 10:30
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Prof. Ruth Durrer (Université de Genève, DPT)17/09/2026 11:30
Gravitational waves (GWs) have a very weak absorption cross section. This makes them difficult to observe on the one hand, but it is also for this reason they carry pristine information from their generation mechanism. Their observation may allow glimpses back to the highest redshifts and energies in the Universe.
After a brief introduction to the significance of the observation of a...
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Chiara Caprini (CERN and University of Geneva)17/09/2026 12:00
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Sébastien RENAUX-PETEL (IAP - CNRS)17/09/2026 14:00
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David Wands (University of Portsmouth)17/09/2026 14:30
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Lucas PINOL (CNRS, LPENS)17/09/2026 15:00
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Nicolás Bernal (New York University Abu Dhabi)17/09/2026 16:00
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Ayuki Kamada (University of Warsaw)17/09/2026 16:30
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Alejandro Ibarra (Technical University of Munich)17/09/2026 17:00
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Marta Losada (NYU Abu Dhabi)18/09/2026 09:30
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Marek Olechowski (University of Warsaw)18/09/2026 10:00
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Kazuki Sakurai (University of Warsaw)18/09/2026 10:30
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JOE Silk (IAP/JHU)18/09/2026 11:30
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Xi Tong (DAMTP, University of Cambridge)18/09/2026 12:00
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Guillermo Ballesteros (University of Madrid)18/09/2026 12:30
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