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Sébastien Renaux-Petel (IAP-CNRS)17/05/2021 14:00
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Chiara Caprini17/05/2021 14:10
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Lorenzo Sorbo17/05/2021 14:40
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Mauro Pieroni17/05/2021 15:10
In this talk I will discuss Stochastic Gravitational Wave Backgrounds (SGWB) characterization with LISA. After a general introduction on SGWB detection, I will explain the peculiar features of LISA with a focus on the response function and on the noise spectrum. The core of my talk will be the presentation of two different methods for model independent SGWB frequency reconstruction:
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- The... -
17/05/2021 15:40
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Azadeh Maleknejad17/05/2021 16:30
Modern cosmology inevitably involves particle physics beyond the Standard Model to explain long-standing puzzles: the origin of matter asymmetry, nature of dark matter and cosmic inflation. In this talk, I will explain that gauge fields in inflation can possibly solve and relate these seemingly unrelated mysteries of modern cosmology. As a smoking gun, this setup has robust observable...
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Matteo Fasiello17/05/2021 17:00
Some of our best ideas on early universe physics are about to be put to the test by an unprecedented array of cosmological probes. The data these will collect span a vast range of scales, from the CMB to large scale structure, from pulsar timing arrays all the way to laser interferometers. This combined wealth of new information holds the potential to transform not just our understanding of...
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Ema Dimastrogiovanni17/05/2021 17:30
Inflation predicts a stochastic background of gravitational waves. In this talk I will discuss how anisotropies in the gravitational wave energy density can be a powerful tool in characterizing the inflationary GW background and potentially distinguishing it from backgrounds due to other sources.
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17/05/2021 18:00
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Subodh Patil18/05/2021 13:30
CMB anisotropies probe primordial gravitational wave backgrounds of frequencies between 10^{-18} and 10^{-15} Hz. Pulsar timing arrays begin to be sensitive to backgrounds starting in the nano-hertz regime, seemingly leaving an approximately six decade gap in frequency coverage. This talk will discuss how spectral distortions of the CMB covers this gap in a meaningful way, and discuss various...
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Matteo Braglia18/05/2021 14:00
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Lukas Witkowski18/05/2021 14:30
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Spyros Sypsas18/05/2021 15:00
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18/05/2021 15:30
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Gianmassimo Tasinato18/05/2021 16:30
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Caner Ünal18/05/2021 17:00
I will talk about the imprints of small, mild and large primordial local NG in density perturbations on the induced GW spectrum.
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Guillem Domènech18/05/2021 17:30
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18/05/2021 18:00
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Shi Pi19/05/2021 14:00
I will briefly review the properties of SGWB induced by the scalar perturbation, as well as its connection to the primordial black holes (PBHs). NANOGrav reported the discovery of a common-spectrum process of the time residuals in their 12.5-yr data set of pulsar timing array, which might be the first detection of nano-hertz SGWB. Based on the recent developments on the spectral shape of SGWB,...
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Antonio Riotto19/05/2021 14:30
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Sebastien Clesse19/05/2021 15:00
The detection of gravitational-waves from binary black hole mergers has rekindled the idea that primordial black holes may have formed in the early Universe. I will review some recent developments in the field of primordial black holes: formation mechanisms, mass function, astrophysical limits, possible contribution to the Dark Matter and links to the Baryogenesis. I will particularly focus...
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19/05/2021 15:30
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Jinno Ryusuke19/05/2021 16:30
In recent years, the possibility of having large density perturbations at high wavenumbers has been actively studied, especially in the study of primordial black holes (PBHs). In this presentation, we point out that such density perturbations affect any pre-existing gravitational wave (GW) spectrum through CMB-like effects. Since GWs produced in the early universe propagate through the density...
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Daniel Figueroa19/05/2021 17:00
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19/05/2021 17:30
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