30 November 2025 to 5 December 2025
Building 40, Room 153
Australia/Sydney timezone
AIP Summer Meeting 2025 - University of Wollongong

Session

Astroparticle Physics

5 Dec 2025, 10:40
Hope Theatre (Building 40, Room 153)

Hope Theatre

Building 40, Room 153

University of Wollongong Northfields Avenue Wollongong NSW 2522

Conveners

Astroparticle Physics: Astroparticle Physics - sponsored by OzGrav

  • Martin White

Presentation materials

There are no materials yet.

  1. Csaba Balazs (Monash University)
    05/12/2025, 10:40
    Astroparticle Physics
    Invited/Keynote talk

    Predicting the gravitational wave spectrum from symmetry breaking in the early universe during first-order phase transitions is key to understanding these symmetries. In this talk I present our recent advancements in developing a self-consistent framework for predicting such gravitational wave spectra. Our approach enhances existing calculations by providing a more comprehensive treatment of...

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  2. Sharry Kapoor (The University of Sydney)
    05/12/2025, 11:10
    Astroparticle Physics
    Contributed Oral

    Photomultiplier Tubes (PMTs) are central to the SABRE South experiment’s
    ability to detect rare, low-energy events, such as potential dark matter interac-
    tions in ultra-pure NaI(Tl) crystals. To correctly interpret what the detector
    sees, we need simulations that faithfully reproduce how our PMTs respond to
    real signals. This work presents the comparison of the simulated PMT wave-
    forms...

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  3. Raj Aryan Singh (Swinburne University of Technology)
    05/12/2025, 11:25
    Astroparticle Physics
    Contributed Oral

    The QCD axion is a well-motivated hypothetical particle that offers simultaneous solutions to two major open questions in physics: the Strong CP problem and the nature of dark matter. If axions make up the dark matter halo of our galaxy, they may be detected through their resonant conversion into microwave photons in the presence of a strong magnetic field—a technique used in the axion...

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  4. Neil Lu (Australian National University)
    05/12/2025, 11:40
    Astroparticle Physics
    Contributed Oral

    The post-merger stage of a binary black hole coalescence is known as "ringdown", when the remnant settles into a stable state through the emission of quasi-normal modes. Analyzing ringdown signals from gravitational-wave events offers a powerful test of general relativity in the strong-field regime and provides an independent consistency check on the full waveform analysis. In this talk, I...

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  5. Igor Samsonov (UNSW)
    05/12/2025, 11:55
    Astroparticle Physics
    Invited/Keynote talk

    Light scalar and pseudoscalar fields—such as axion- and dilaton-like particles—are well-motivated dark-matter candidates. Their couplings to Standard-Model fields can induce tiny, stochastic modulations of atomic transition frequencies. A statistical framework for clock-based searches is developed, showing that higher-order statistical moments of the measured fluctuations (e.g., skewness,...

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Building timetable...