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From the 1 of 22 linked papers with an AI index.

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22 papers

hep-ph2026

Defect-Mediated Conversion: Dark Matter from Cosmological Domain-Wall Scattering

João Paulo Pinheiro, Mohamed Younes Sassi

We propose a new mechanism for dark matter genesis, \emph{Defect-Mediated Conversion} (DMC). Cosmological domain walls can host a scalar condensate in their core acting as a mixing…

astro-ph.GA2026

Stellar photoionisation modelling in SYNTHESIZER

Aswin P. Vijayan, Stephen M. Wilkins, Sophie L. Newman +5

The paper introduces photoionised gas emission modeling into the SYNTHESIZER code, allowing realistic stellar and nebular spectra to be generated for galaxy formation studies.

astro-ph.GA2026

Cloudy-Maraston: Integrating nebular continuum and line emission with the Maraston stellar population synthesis models

Sophie L. Newman, Christopher C. Lovell, Claudia Maraston +5

The James Webb Space Telescope has ushered in an era of abundant high-redshift observations of young stellar populations characterized by strong emission lines, motivating us to in…

astro-ph.GA2026

First Light and Reionization Epoch Simulations (FLARES) XXII: UV-dust spatial offsets at the Epoch of Reionisation

Paurush Punyasheel, Aswin P. Vijayan, William J. Roper +8

Recent observations have revealed intriguing offsets between the UV and FIR emission in high redshift galaxies. In this study, we use the First Light And Reionisation Epoch Simulat…

astro-ph.GA2026

First Light And Reionization Epoch Simulations (FLARES) XXI: The UV Indices of Galaxies in the Early Universe

Connor Sant Fournier, Stephen M. Wilkins, Joseph Caruana +5

UV absorption line indices trace chemical enrichment and star formation histories in high-redshift galaxies, yet their reliability as quantitative stellar metallicity, Z*, diagnost…

astro-ph.GA2026

The LISA Astrophysics MBHcatalogues Project: A comparison of predictions of simulated massive black hole binaries

David Izquierdo-Villalba, Melanie Habouzit, Matteo Bonetti +67

In the hierarchical paradigm of galaxy formation, central massive black holes (MBHs) are expected to coalesce after the merger of their host galaxies. One of the main goals of the…