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Alejandro Ibarra (Technical University of Munich)09/02/2026, 09:30
We summarize the status of dark matter indirect searches using neutrinos as messengers, and we point out that dark matter spikes around supermassive black holes can enhance significantly the neutrino flux from nearby galaxies, possibly even at the reach of neutrino telescopes. In particular, we propose that the measured neutrino flux from NGC1068 could be attributed to dark matter...
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Dr Takashi Toma (Kanazawa University)09/02/2026, 10:00
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Prof. Kimiko Yamashita (Ibaraki University)09/02/2026, 11:00
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Jong-Hyun Yoon09/02/2026, 11:30
I begin with a pedagogical introduction to cosmological particle production during and after inflation, reviewing the theoretical framework of inflaton dynamics, gravitational particle production, and numerical techniques. I discuss various production scenarios studied in different cosmological contexts, with emphasis on computational methods and challenges. I then present our recent work on...
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Adriana Menkara09/02/2026, 12:00
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Dr Adil Jueid (Institute for Basic Science)09/02/2026, 14:30
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Tatsuya Banno09/02/2026, 15:00
We present a comprehensive study of Higgs boson production associated with a neutrino pair at e+e− colliders (e+e−→hνν¯) at the next-to-leading-order accuracy in both the Standard Model and the two-Higgs-doublet model. We show that new physics effects from the extended Higgs sector can be probed through electroweak corrections, which lead to several percent deviations from the Standard Model...
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Kiyoto Ogawa (Nagoya.Univ)09/02/2026, 15:15
There has been remarkable progress in recent years in the electric dipole moment (EDM) measurements of electron using paramagnetic atom or molecule. In a previous study, we calculated the contribution to the electron EDM induced by the CP-violating Yukawa interaction of electroweak multiplets at the three-loop level in effective field theory. We found that this contribution might reach the...
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Ms ROJALIN PADHAN (Institute of Physics, Bhubaneswar)09/02/2026, 16:00
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Shota Saito (Kavli IPMU)09/02/2026, 16:30
We classify 4D N=1 truly confining supersymmetric gauge theories, in which no center charges can be screened. This property guarantees that Wilson loops in the fundamental representation exhibit an area law. We systematically identify all such theories for simple Lie groups and determine the allowed matter content. In each theory, we find condensing magnetic operators, which are expected to...
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Hyeonmo Koo09/02/2026, 16:45
We investigate the impact of repulsive self-interaction in ultralight dark matter (ULDM) on dynamical friction in circular orbits in ULDM halos and its implications for the Fornax dwarf spheroidal (dSph) galaxy's globular clusters. Using the Gross-Pitaevskii-Poisson equations, we derive the dynamical friction force considering soliton density profiles for both non-interacting and strongly...
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Eung Jin Chun (Korea Institute for Advanced Study)10/02/2026, 09:30
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Bin Xu10/02/2026, 10:00
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Dr Sang Hui Im (IBS CTPU)10/02/2026, 11:00
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Shohei Okawa (APCTP)10/02/2026, 11:30
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Jong-Wan Lee (Institute for Basic Science (IBS))10/02/2026, 12:00
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Chui-Fan Kong10/02/2026, 15:00
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Lucca Radicce Justino10/02/2026, 15:30
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Junghoon Joh (SungKyunKwan University)10/02/2026, 15:45
We study a mechanism to make dark matter stable based on the Pauli blocking in the fermion background. In the background where fermions occupy the states, the decay of dark matter to those final states is not allowed, as a result, DM becomes stable. We derive the evolution equations of the distribution function in the quantum field theory and compare it with the Boltzmann equation. We apply...
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Yongsoo Jho10/02/2026, 16:30
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Seongsik Kim (Chung-Ang University)10/02/2026, 17:00
We consider the extension of the SM with an inert scalar doublet,
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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 between the... -
Katsuki Aoki (YITP, Kyoto University)11/02/2026, 09:30
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Dr Minxi He11/02/2026, 10:00
Astrophysical probes are powerful tools to search for Beyond the Standard Model (BSM) particles, complementary to terrestrial detectors. As commonly exist throughout the Universe, black holes (BH) are intriguing astrophysical objects due to their strong gravity that can help to study BSM particles. In this talk, I will show that BSM particles can interact and form structures around BHs, here...
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Shuntaro AOKI11/02/2026, 11:00
Modular symmetry arises in various extensions of the Standard Model and plays an important role in particle phenomenology, particularly as a framework for flavor symmetries. In this talk, I will explore the cosmological implications of modular symmetry, with a special focus on inflationary physics. I will discuss how specific couplings between moduli and the Standard Model sector can influence...
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Sarif Khan (Goettingen University)11/02/2026, 11:30
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Junho Song11/02/2026, 12:00
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Jeonghak Han11/02/2026, 12:15
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Dr Jongkuk Kim (Chung-Ang University)11/02/2026, 14:30
The Belle II Collaboration recently announced the first observation of the 𝐵 → 𝐾 + 𝜈 𝜈 decay process. This decay channel provides a particularly clean signal and allows for high theoretical precision. However, their measurement shows a 2.7𝜎 deviation from the Standard Model prediction. To address this excess, we study a scalar dark matter model. Assuming a dark 𝑈 (1)𝑋≡𝑈(1)𝐿𝜇−𝐿𝜏 symmetry, this...
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Arghyajit Datta11/02/2026, 15:00
We present a type-I seesaw scenario within the supersymmetric $U(1)_{B-L}$
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extension of the Standard Model that simultaneously explains the large electron–neutrino asymmetry suggested by EMPRESS and the observed tiny baryon asymmetry. Both asymmetries originate from the decay of the $B−L$ Higgs condensate dominating the early Universe. It`s early rare decays into heavy right-handed... -
Yechan Kim (KAIST)11/02/2026, 15:30
The oscillating wave dark matter can act as a periodic driver, producing distinct modulation signatures not only in particle physics (e.g., neutrinos), but also in solid-state physics (e.g., superconductors). This talk is based on our recent papers PRD 108, 095028 (2023); JHEP 07 (2025) 269; arXiv: 2509.22892.
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Dong Woo Kang (KIAS)11/02/2026, 16:15
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Alberto Navarro (Seoultech)11/02/2026, 16:45
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Joern Kersten (University of Bergen)12/02/2026, 09:30
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Wenyuan Ai12/02/2026, 10:00
First-order phase transitions in the early Universe are a well-motivated source of gravitational
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waves (GWs). In this talk, I will discuss a previously overlooked GW production mechanism:
gravitational transition radiation, arising from graviton emission by particles whose mass changes
as they pass through expanding bubble walls. The resulting spectrum features a distinctive shape with a... -
Carlo Branchina (Università della Calabria)12/02/2026, 11:00
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Kyohei Mukaida (DESY)12/02/2026, 11:30
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Sung Hak Lim (Rutgers University)12/02/2026, 12:00
Mapping the Milky Way’s dark matter requires moving beyond traditional, rigid dynamical models. In this talk, generative models—specifically Normalizing Flows— are used to learn the stellar phase space distribution directly from Gaia data. This approach enables a flexible, model-independent reconstruction of the Galactic gravitational potential and local dark matter density. These data-driven...
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Jeonghyeon Song
We present a systematic study of large CP violation in the Complex Two-Higgs-Doublet Model with softly broken $Z_2$ symmetry, based on global scans of Type-I and Type-II realizations including theoretical consistency, collider data, and the stringent electron EDM constraint. We identify two qualitatively different CP-violating regimes: in Type-I, sizable gauge-sector CP violation is possible...
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