activity
20242026
collaborators

5 papers

astro-ph.CO2026

Non-parametric exploration of minimally coupled gravity with phantom crossing

Matteo Cataneo, Kazuya Koyama

Recent measurements of the baryon acoustic oscillations by the Dark Energy Spectroscopic Instrument (DESI), especially when combined with cosmic microwave background (CMB) and supe…

astro-ph.CO2025

A field-level reaction for screened modified gravity

Daniela Saadeh, Kazuya Koyama, Xan Morice-Atkinson

We present a field-level reaction framework to emulate the nonlinear effects of screened modified gravity on the cosmic web. This approach is designed to enable field-level inferen…

astro-ph.GA2025

Using a minimally parametrised SHAM to constrain the link between dark matter and galaxies

F. L. Davidson, D. Bacon, A. Amara +6

Models of the galaxy-halo connection are needed to understand both galaxy clusters and large scale structure. To make said models, we need a robust method that assigns galaxies to…

astro-ph.CO2024

A field-level emulator for modified gravity

Daniela Saadeh, Kazuya Koyama, Xan Morice-Atkinson

Stage IV surveys like LSST and Euclid present a unique opportunity to shed light on the nature of dark energy. However, their full constraining power cannot be unlocked unless accu…

astro-ph.CO2024

Extending MGCAMB tests of gravity to nonlinear scales

Zhuangfei Wang, Daniela Saadeh, Kazuya Koyama +4

Modified Growth with {\tt CAMB} ({\tt MGCAMB}) is a patch for the Einstein-Boltzmann solver {\tt CAMB} for cosmological tests of gravity. Until now, {\tt MGCAMB} was limited to sca…