Scale-dependent local primordial non-Gaussianity as a solution to the tension

C Stahl, B Famaey, R Ibata, O Hahn, N Martinet… - Physical Review D, 2024 - APS
For the last decade, several probes have pointed to a cosmological tension between the
amplitude of density fluctuations extrapolated from the cosmic microwave background within …

The FLAMINGO project: the coupling between baryonic feedback and cosmology in light of the S8 tension

W Elbers, CS Frenk, A Jenkins, B Li… - Monthly Notices of …, 2025 - academic.oup.com
Large-scale structure surveys have reported measurements of the density of matter, Ωm, and
the amplitude of clustering, σ8, that are in tension with the values inferred from observations …

Investigating Late-Time Dark Energy and Massive Neutrinos in Light of DESI Y1 BAO

J Rebouças, DHF de Souza, K Zhong… - arXiv preprint arXiv …, 2024 - arxiv.org
Baryonic Acoustic Oscillation (BAO) data from the Dark Energy Spectroscopic Instrument
(DESI), in combination with Cosmic Microwave Background (CMB) data and Type Ia …

Impact of baryonic feedback on HSC-Y1 weak lensing non-Gaussian statistics

D Grandón, GA Marques, L Thiele, S Cheng… - Physical Review D, 2024 - APS
Baryonic feedback is a major systematic in weak lensing cosmology. Its most studied effect
is the suppression of the lensing power spectrum, a second-order statistic, on small scales …

The FLAMINGO project: baryonic impact on weak gravitational lensing convergence peak counts

JC Broxterman, M Schaller, J Schaye… - Monthly Notices of …, 2024 - academic.oup.com
Weak gravitational lensing convergence peaks, the local maxima in weak lensing
convergence maps, have been shown to contain valuable cosmological information …

Validating the clustering predictions of empirical models with the FLAMINGO simulations

S Contreras, RE Angulo, J Chaves-Montero… - Astronomy & …, 2024 - aanda.org
Context. Mock galaxy catalogues are essential for correctly interpreting current and future
generations of galaxy surveys. Despite their significance in galaxy formation and cosmology …

Everything hot everywhere all at once: Neutrinos and hot dark matter as a single effective species

A Upadhye, MR Mosbech, G Pierobon… - Journal of Cosmology …, 2025 - iopscience.iop.org
Observational cosmology is rapidly closing in on a measurement of the sum M ν of neutrino
masses, at least in the simplest cosmologies, while opening the door to probes of non …

FLAMINGO: combining kinetic SZ effect and galaxy-galaxy lensing measurements to gauge the impact of feedback on large-scale structure

IG McCarthy, A Amon, J Schaye, E Schaan… - arXiv preprint arXiv …, 2024 - arxiv.org
Energetic feedback processes associated with accreting supermassive black holes can
expel gas from massive haloes and significantly alter various measures of clustering on …

Implications of feedback solutions to the tension for the baryon fractions of galaxy groups and clusters

J Salcido, IG McCarthy - arXiv preprint arXiv:2409.05716, 2024 - arxiv.org
Recent large-scale structure (LSS) surveys have revealed a persistent tension in the value
of $ S_8 $ compared to predictions from the standard cosmological model. This tension may …

Asimulation: Domain formation and impact on observables in resolved cosmological simulations of the (a) symmetron

Ø Christiansen, F Hassani, DF Mota - Astronomy & Astrophysics, 2024 - aanda.org
The symmetron is a dark energy and dark matter candidate that forms topological defects in
the late-time universe and holds the promise of resolving some of the cosmological tensions …