Conveners
Early Universe Cosmology: Plenary 1-2
- Maria Mylova
Early Universe Cosmology: Plenary 22-24
- Maria Mylova
Early Universe Cosmology: Parallel G
- Maria Mylova
Early Universe Cosmology: Parallel N
- Maria Mylova
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Ana Achucarro (Leiden University)28/10/2024, 09:00Early Universe Cosmology
Inflation remains the favoured explanation for the origin of the primordial density fluctuations that seeded all large-scale structures in the universe. A precise connection between inflation and particle physics (and quantum gravity) would give a unique observational window into physics at the highest energies. After a general introduction to multifield scenarios, I will discuss recent...
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Gonzalo Palma (Universidad de Chile)28/10/2024, 09:30Early Universe Cosmology
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Oksana Iarygina (Nordic Institute for Theoretical Physics, Stockholm University)31/10/2024, 10:30Early Universe Cosmology
Currently, the search for primordial gravitational waves is largely focused on detecting the parity-odd polarization pattern in the Cosmic Microwave Background—the B-modes. Accurately interpreting B-mode measurements depends heavily on understanding their production mechanisms. A particularly compelling scenario involves gravitational wave generation through the interaction of axion with gauge...
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Xi Tong (DAMTP, University of Cambridge)31/10/2024, 11:00Early Universe Cosmology
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Scott Melville (Queen Mary University of London)31/10/2024, 11:30Early Universe Cosmology
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Dibya Chakraborty (Indian Institute of Technology Madras)31/10/2024, 14:00Early Universe Cosmology
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Maximilian Berbig (IFIC & University of Valencia)31/10/2024, 14:15Early Universe Cosmology
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Mattia Cielo (University of Naples & INFN & IFT - UAM, Madrid)31/10/2024, 14:30Early Universe Cosmology
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Rudnei Ramos (Rio de Janeiro State University)31/10/2024, 14:45Early Universe Cosmology
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Chon Man Sou (Tsinghua University)01/11/2024, 10:30Early Universe Cosmology
We revisit the decoherence of primordial scalar curvature and tensor perturbations in minimal single-field inflation, by considering the slow-roll unsuppressed non-Gaussian phase in their wave functional. The phase can be seen either from boundary (total time-derivative) terms in the action, produced by the usual integration-by-parts procedure, or the WKB approximation of the Wheeler-DeWitt...
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Luca Marchetti (University of New Brunswick)01/11/2024, 10:45Early Universe Cosmology
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Paul Martens (Chinese University of Hong Kong (CUHK))01/11/2024, 11:00Early Universe Cosmology
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Shouvik Roy Choudhury (Academia Sinica Institute of Astronomy and Astrophysics)01/11/2024, 11:15Early Universe Cosmology