7–11 Jun 2026
Chung-Ang University
Asia/Seoul timezone

Session

Inflation & GW

Not scheduled
Chung-Ang University

Chung-Ang University

Graduate school 302-502, Chung-Ang University, Seoul 06974, Republic of Korea

Presentation materials

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  1. Masahide Yamaguchi (Tokyo Institute of Technology)
  2. Prof. Marcos A. Garcia Garcia (Instituto de Fisica, UNAM)
  3. Yann Mambrini
  4. Arghyajit Datta
  5. Shuntaro AOKI

    The cosmological collider program, which aims to extract direct information about heavy particles during inflation via primordial non-Gaussianity, has attracted attention as it offers a window into high-energy physics beyond the reach of terrestrial experiments. However, analyses based on concrete particle physics models remain limited, and it is still unclear under what conditions a large...

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  6. Jong-Hyun Yoon

    In physics, while analytical calculations remain appealing, there are situations where the use of computers becomes indispensable. A straightforward example is the three-body problem, where even the interactions of just three bodies are challenging to solve analytically. This necessity is similarly evident in studies of the early universe. Understanding the dynamics of the inflaton requires...

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  7. Dr Yong Tang (University of Chinese Academy of Sciences)
  8. Jinn-Ouk Gong
  9. Prof. Seong Chan Park (Yonsei University)
  10. SATYABRATA MAHAPATRA (Sungkyunkwan University)

    In this talk I will introduce a novel particle physics framework addressing multiple cosmological tensions, including discrepancies in the Hubble parameter, S8, and Lyman-\alpha forest data. This model, SIDR+z_t (Self-Interacting Dark Radiation with transition redshift), features an inelastic dark matter (IDM) scenario coupled with dark radiation under a dark gauge symmetry. The model...

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  11. Dr Kuldeep Deka (New York University Abu Dhabi)

    The dynamics of cosmic reheating, that is, on how the energy stored in the inflaton is transferred to the standard model (SM) thermal bath, is largely unknown. In this work, we show that the phenomenology of the nonbaryonic dark matter (DM) ultraviolet freeze-in production strongly depends on the dynamics of the cosmic-reheating era. Using a general parametrization for the Hubble expansion...

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