25–27 Jun 2025
NYCU
Asia/Taipei timezone

Session

Gravitational aspects of particle physics

25 Jun 2025, 11:00
Science Building III/SC353 (NYCU)

Science Building III/SC353

NYCU

Science Building III, No 1001, University Rd., Hsinchu 300, Taiwan

Conveners

Gravitational aspects of particle physics

  • Jan Tristram Acuña (Department of Physics, National Tsing Hua University)

Gravitational aspects of particle physics

  • Priyanka Sarmah (NTHU)

Presentation materials

There are no materials yet.

  1. TC Yuan (IOP, Academia Sinica)
    25/06/2025, 11:00
    Regular talk

    We investigate the possibility of a strong first-order electroweak phase transition (FOEWPT) during the early universe within the framework of the gauged two-Higgs doublet model (G2HDM) and explore its detectability through stochastic gravitational wave signals. The results indicate that forthcoming detectors such as BBO, LISA, DECIGO, TianQin and Taiji could potentially detect the...

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  2. Dr Van Que Tran (NCTS, National Taiwan University)
    25/06/2025, 11:30
    Regular talk

    Employing effective field theory techniques, we advance computations of thermal parameters that enter predictions for the gravitational wave spectra from first-order electroweak phase transitions. Working with the real-singlet-extended Standard Model, we utilize recent lattice simulations to confirm the existence of first-order phase transitions across the free parameter space. For the first...

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  3. Karan Fernandes (NTNU)
    26/06/2025, 16:00
    Regular talk

    In recent years, classical limits of scattering amplitudes have emerged as a powerful tool for deriving state-of-the-art results for gravitational wave observables from interacting binary compact objects. In this talk, I will explore gravitational dressing operators from the worldline formalism and discuss their significance for late time radiative observables. We will first consider how...

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  4. Hsiang-Chieh Hsu (Institute of Physics, Academia Sinica)
    26/06/2025, 16:30
    Regular talk

    We discuss the prospects for discovering macroscopic Dark Matter (DM) using large-scale ground-based gravitational wave (GW) detectors. Here, as an example, we consider a DM candidate with long-range Yukawa-like interactions in the kg- to tonne-scale mass range, where the analysis can potentially be further generalised for other DM models. The DM in this mass range will produce a signal that...

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