17–22 Aug 2025
Utop Marina Hotel & Resort, Yeosu, Korea
Asia/Seoul timezone

Session

Parallel session 1

19 Aug 2025, 14:00
Utop Marina Hotel & Resort, Yeosu, Korea

Utop Marina Hotel & Resort, Yeosu, Korea

Conveners

Parallel session 1

  • Kwang Sik Jeong (Pusan National University)

Presentation materials

There are no materials yet.

  1. Dhong Yeon Cheong (Yonsei University)
    19/08/2025, 14:00
    Parallel talk

    In this talk, I will outline a fundamentally quantum description of bosonic dark matter. Following a quantum optics-inspired approach, I will show the density matrix of dark matter, which takes a mixed Gaussian form over a coherent state basis. This formalism also allows a precise description of quantities related to dark matter coherence. I will further give a continuous description of dark...

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  2. SangHwan Kim (Department of Physics, Yonsei University)
    19/08/2025, 14:20
    Parallel talk

    Dark matter (DM) plays an important role in modern high-energy physics and indirect signals can provide evidence of DM interactions with Standard model (SM) particles. Among various of SM channels, gamma-rays are one of the most prominent channel because they head directly to the Earth unlike other charged cosmic-ray particles. Using gamma-ray data of Fermi-LAT, a space telescope that is cable...

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  3. Wakutaka Nakano (YITP)
    19/08/2025, 14:40
    Parallel talk

    A detection scheme is explored for light dark matter, such as axion dark matter or
    dark photon dark matter, using a Paul ion trap system. We first demonstrate that
    a qubit, constructed from the ground and first excited states of vibrational modes
    of ions in a Paul trap, can serve as an effective sensor for weak electric fields due
    to its resonant excitation. As a consequence, a Paul ion...

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  4. Sarif Khan (Chung-Ang University, Seoul)
    19/08/2025, 15:00
    Parallel talk

    In this work, we have explored the conversion-driven freeze-out scenario, where the next-to-lightest stable particle (NLSP) sets the dark matter (DM) abundance through
    the process ``NLSP SM $\leftrightarrow$ DM SM". Although DM is produced via
    freeze-out mechanism, its interaction strength with the visible sector can
    range from weak-scale to feeble-scale couplings. This leads to a vast,...

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  5. Seongsik KIm (Chung-Ang University)
    19/08/2025, 15:20
    Parallel talk

    We consider the extension of the Standard Model with an inert scalar doublet, three right-handed neutrinos, and singlet scalar fields, φ and S. In this model, neutrino masses are zero in the limit of the unbroken Z4 discrete symmetry. We show that when the singlet scalar field φ gets a VEV, the Z4 symmetry is broken to Z2, and neutrino masses are generated at one-loops due to the mixings...

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  6. Vicky Thounaojam (Indian Institute of Technology Hyderabad)
    Parallel talk

    Light dark matter (DM) with mass around the GeV scale faces weaker bounds from direct detection experiments. If DM couples strongly to a light mediator, it is possible to have observable direct detection rate. However, this also leads to a thermally under-abundant DM relic due to efficient annihilation into light mediators. We propose a novel scenario
    where a first-order phase transition...

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