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CUBES 2026

24–26 Apr 2026
The-K Jirisan Family Hotel, Sandong, Gurye
Asia/Seoul timezone

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Session

Young Researchers Session

25 Apr 2026, 17:05
Cheonwangbong Hall (The-K Jirisan Family Hotel, Sandong, Gurye)

Cheonwangbong Hall

The-K Jirisan Family Hotel, Sandong, Gurye

Jeollanam-do, Republic of Korea

Conveners

Young Researchers Session

  • Ki-Young Choi (Sungkyunkwan University)

Presentation materials

There are no materials yet.

  1. 16. Localized Overdensities from Inflationary Particle Production and Their Signatures in Cosmic Structure Formation
    Junseung Pi (Chungbuk National University)
    25/04/2026, 17:05
  2. 17. Pioneering Sub-GeV Dark Matter Limits with COSINE-100
    Wonkyung Kim (IBS CUP / UST)
    25/04/2026, 17:20

    We report new constraints on the spin-dependent (SD) WIMP-proton cross section using the COSINE-100 experiment at the Yangyang Underground Laboratory. This analysis achieves a pioneering detection threshold of 3 and 4 pulse clusters corresponding to the measured photoelectrons. This allows us to access the unstudied few-photoelectron regime, significantly below the previous 8-photoelectron...

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  3. 18. Probing Neutrinoless Double Electron Capture in Calcium-40 with AMoRE
    Bijaya Sharma (IBS CUP)
    25/04/2026, 17:35

    The search for neutrinoless double electron capture (0ν2EC) is a powerful probe for lepton-number violation and the Majorana nature of neutrinos. We report on a search for the 0ν2EC decay of 40Ca using the AMoRE-I cryogenic detector array, which utilizes metallic magnetic calorimeters (MMCs) and 48depl.Ca100MoO4 crystals. Analyzing a total...

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  4. 19. Galactic Center Excess from the 17.5 Years of Fermi-LAT Data
    Haebarg Kang (Jeonbuk National University)
    25/04/2026, 17:50
  5. 20. Photon Axion Enhancement around PBH
    Junghoon Joh (Sungkyunkwan University)
    25/04/2026, 18:05

    Dark matter (DM) can be gravitationally captured around a massive compact object, forming a dense halo. If primordial black holes (PBHs) exist, surrounding dark matter particles can be accreted through gravitational attraction, leading to the formation of a DM halo with a steep spike profile near the PBH.

    If the dark matter consists of axions or axion-like particles (ALPs), the high number...

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