2–8 Feb 2025
Brisbane, Australia
Australia/Brisbane timezone

Session

Session 13

7 Feb 2025, 11:00
Tamborine Mountain Glades (Brisbane, Australia)

Tamborine Mountain Glades

Brisbane, Australia

Tamborine Mountain Rd, Cedar Creek Falls Rd, Tamborine Mountain QLD 4272

Conveners

Session 13: Friday

  • Agne Semenaite (Swinburne University of Technology)

Presentation materials

There are no materials yet.

  1. Ryan Camilleri (The University of Queensland)
    07/02/2025, 11:00

    Type Ia Supernovae act as standard candles which provide a fundamental way to probe the expansion history of the Universe. While the standard cosmological model fits current data well, uncertainty remains. This uncertainty has led to a wealth of exotic cosmological models being proposed. In my work, I constrain a variety non-standard models using the DES 5-year sample - the largest single...

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  2. Giulia Degni
    07/02/2025, 11:20

    Cosmic voids, large under-dense regions in the Universe, serve as promising laboratories for extracting cosmological information. They offer opportunities to explore deviations from $\Lambda$CDM and provide insights into dark energy and modification of gravity. Upcoming surveys will enable detailed void analyses, allowing access to a huge number of voids. Voids' significance lies in their...

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  3. Geraint Lewis
    07/02/2025, 11:40

    I will present our recent results exploring the integrity of the cosmological principle, the idea that, on sufficient scales, the universe is homogeneous and isotropic. Recent tensions have arisen between the dipole of cosmological sources and its interpretation from the CMB as a kinematic departure from the local Hubble Flow, bringing the cosmological principle into doubt. With a...

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  4. Dr Fei Qin (CPPM)
    07/02/2025, 12:00

    The large-scale structure of the Universe and its evolution over time contains an abundance of cosmological information.One way to unlock this is by measuring the density and momentum power spectrum from the positions and peculiar velocities of galaxies, and fitting the cosmological parameters from these power spectrum.In this work, we will explore the cross power spectrum between the ...

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  5. Anthony Carr (Korea Astronomy and Space Science Institute)
    07/02/2025, 12:20

    At low redshift, peculiar velocities are particularly well-suited to studying the nature of dark energy through the growth rate of structure. Supernovae Ia are precise distance indicators, and we can estimate peculiar velocities from their Hubble residuals at low-redshift, i.e., roughly their departure from motion caused purely by expansion. The Pantheon+ supernova sample is currently the most...

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