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Zi-Yu Tang (IBS CTPU-CGA)29/07/2025, 16:50
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Pritha Bari (IBS CTPU-CGA)29/07/2025, 17:15
Primordial gravitational waves (GWs), beyond their direct detection prospects, can induce second-order scalar perturbations. These tensor-induced scalar modes evolve similarly to standard matter perturbations and leave distinct imprints on the large-scale structure (LSS). In this talk, I will present a detailed study of these effects, including analytical results for the evolution of induced...
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Huiyu Zhu (IBS CTPU-CGA)29/07/2025, 17:40
Ultralight bosons, predicted in scenarios beyond the Standard Model and viable dark matter (DM)
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Candidates can form superradiant clouds around spinning black holes, influencing their dynamics.
Using century-long monitored OJ287 supermassive black hole binary, we set the first DM–DM-independent,
dynamical constraints on their masses μ = (8.5−22)×10−22 eV. These dynamical constraints,... -
Hyeonmo Koo (U of Seoul)29/07/2025, 18:05
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Yigon Kim (SNU)31/07/2025, 16:50
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Minseong Kwon (SNU)31/07/2025, 17:15
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Pavel Petrov (IBS CTPU-CGA)31/07/2025, 17:40
We present a minimal setup within the framework of Horndeski gravity that describes a nonpathological Genesis scenario. Our setup allows for a fully stable transition to the kination epoch, during which General Relativity (GR) is restored. This Genesis scenario circumvents the no-go theorem, albeit at the cost of encountering the risk of strong coupling in the past. Interestingly, our scenario...
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Qianhang Ding (IBS CTPU-CGA)31/07/2025, 18:05
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