collaborators

16 papers

hep-th2026

Evidence for renormalized instantons in real-time simulations of vacuum decay

Emilie Hertig, Alexander C. Jenkins, Hiranya V. Peiris +2

While vacuum decay is traditionally described by Euclidean instanton methods, lattice simulations enable real-time modeling of dynamical observables relevant to cosmology and upcom…

astro-ph.GA2026

pop-cosmos: Disentangling galaxy properties from observables using data-driven approaches

Benedict Van den Bussche, Sinan Deger, Hiranya V. Peiris +6

The physical processes that shape a galaxy's spectrum are strongly degenerate in observations, obscuring which processes act independently. Leveraging the pop-cosmos generative gal…

astro-ph.GA2026

pop-cosmos: Galaxy size evolution across structural and star-formation classifications in COSMOS-Web

Madalina N. Tudorache, Hiranya V. Peiris, Stephen Thorp +7

Galaxy sizes are correlated with stellar mass and redshift, as characterised by size scaling relations. The inferred forms of these scaling relations are sensitive to how galaxies…

astro-ph.CO2026

Thermostats, Not Engines: A New Picture of Halo Gas Regulation

Hiranya V. Peiris, Andrew Pontzen, Madalina N. Tudorache +5

We propose that black hole feedback regulates gas in massive halos by establishing an entropy ceiling; the resulting buoyant gas migrates to the virial radius with no additional en…

stat.ML2026

StAD: Stein Amortized Divergence for Fast Likelihoods with Diffusion and Flow

Gurjeet Jagwani, Stephen Thorp, Sinan Deger +1

Diffusion and flow-based models are ubiquitously used for generative modelling and density estimation. They admit a deterministic probability flow ordinary differential equation (P…

astro-ph.GA2026

The limits of feedback from active galactic nuclei

Andrew Pontzen, Hiranya V. Peiris, Joop Schaye +1

We use FLAMINGO to investigate why feedback from active galactic nuclei (AGN) significantly depletes gas in galaxy groups but is ineffective in clusters. We delineate three radial…