28 July 2025 to 1 August 2025
Jeonju, Best Western Hotel
Asia/Seoul timezone

Contribution List

32 out of 32 displayed
  1. Prof. Piljin Yi (KIAS)
    29/07/2025, 10:00
  2. Taeyeon Kim (SNU/KIAS)
    29/07/2025, 10:35
  3. Prof. David Parkinson (KASI)
    29/07/2025, 11:30
  4. Chandra Shekhar Saraf (KASI)
    29/07/2025, 12:05
  5. Junggi Yoon (Kyunghee U)
    29/07/2025, 14:30
  6. Vinay Malvimat (Kyunghee U)
    29/07/2025, 15:05
  7. Anthony Scott Carr (KASI)
    29/07/2025, 15:30

    The structure of galaxies we see in the sky today was seeded in the very early universe. The evolution from initial tiny density perturbations to the cosmic web of voids, clusters and filaments of galaxies tells us about what the universe is made of. There are many ways to utilise this large scale structure to probe cosmology, but measuring the growth rate itself in the nearby universe is...

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  8. Fumiya Sano (IBS CTPU-CGA)
    29/07/2025, 15:55

    We compute a holographic entanglement entropy via Ryu-Takayanagi prescription in the three-dimensional Friedmann-Lemaître-Robertson-Walker universe. We consider two types of holographic scenarios analogous to the static patch holography and the half de Sitter holography, in which the holographic boundary is timelike and placed in the bulk. We find in general that the strong subadditivity can...

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  9. Zi-Yu Tang (IBS CTPU-CGA)
    29/07/2025, 16:50
    100
  10. Pritha Bari (IBS CTPU-CGA)
    29/07/2025, 17:15
    100

    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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  11. Huiyu Zhu (IBS CTPU-CGA)
    29/07/2025, 17:40
    100

    Ultralight bosons, predicted in scenarios beyond the Standard Model and viable dark matter (DM)
    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,...

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  12. Hyeonmo Koo (U of Seoul)
    29/07/2025, 18:05
    100
  13. Prof. Keun-Young Kim (GIST)
    30/07/2025, 10:00
  14. Shaun D. Hampton (KIAS)
    30/07/2025, 10:35
  15. Prof. Ho Seong Hwang (SNU)
    30/07/2025, 11:30
  16. Michiru Uwabo-Niibo
    30/07/2025, 12:05
  17. Prof. Sangmin Lee (SNU)
    31/07/2025, 10:00
  18. Hojin Lee (SNU)
    31/07/2025, 10:35
  19. Prof. Atsuhisa Ota (Chongqing U)
    31/07/2025, 11:30

    We study stimulated emission and absorption of gravitons in a squeezed vacuum
    state immersed in a thermal radiation bath. Employing one-loop
    interaction-picture perturbation theory, we track the time evolution of the
    graviton number operator and its expectation value in the squeezed vacuum,
    which characterizes the inflationary graviton state. In a Minkowski background
    with a thermal bath...

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  20. Rinku Maji (IBS CTPU-CGA)
    31/07/2025, 12:05
  21. Ji-Hoon Kim (SNU)
    31/07/2025, 14:30
  22. Siyao Li (IBS CTPU-CGA)
    31/07/2025, 15:05

    Oscillons are long-lived, spherically symmetric solitons that can arise in real scalar field theories with potentials shallower than quadratic ones. They are considered to form via parametric resonance during the preheating stage after inflation and have extended lifetimes. However, the estimation of their lifespan becomes complicated when taking into account the interactions between the...

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  23. Dongkok Kim (SNU)
    31/07/2025, 15:30
  24. Tomotaka Kuroda (IBS CTPU-CGA)
    31/07/2025, 15:55
  25. Yigon Kim (SNU)
    31/07/2025, 16:50
    100
  26. Minseong Kwon (SNU)
    31/07/2025, 17:15
    100
  27. Pavel Petrov (IBS CTPU-CGA)
    31/07/2025, 17:40
    100

    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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  28. Qianhang Ding (IBS CTPU-CGA)
    31/07/2025, 18:05
    100
  29. Hyun Seok Yang (GIST)
    01/08/2025, 10:00
  30. Nils Albin Nilsson (IBS CTPU-CGA)
    01/08/2025, 10:35
  31. Prof. Sebastian Bahamonde (IPMU/CTPU-CGA)
    01/08/2025, 11:30
  32. Yuhang Zhu (IBS CTPU-CGA)
    01/08/2025, 12:05