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Neutrino mass tension or suppressed growth rate of matter perturbations?

William Giarè ^1,*, Olga Mena^2,†, Enrico Specogna ^1,‡, and Eleonora Di Valentino ^1,§

¹School of Mathematical and Physical Sciences, University of Sheffield, Hounsfield Road, Sheffield S3 7RH, United Kingdom
²Instituto de Física Corpuscular (IFIC), University of Valencia-CSIC, Parc Científic UV, c/ Catedrático José Beltrán 2, E-46980 Paterna, Spain

^*Contact author: w.giare@sheffield.ac.uk
^†Contact author: omena@ific.uv.es
^‡Contact author: especogna1@sheffield.ac.uk
^§Contact author: e.divalentino@sheffield.ac.uk

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Articles Citing

Neutrino mass tension or suppressed growth rate of matter perturbations?

Creation of viscous dark energy by the Hubble flow: Comparison with SNe Ia Master sample binned data

Cosmological preference for a positive neutrino mass at 2.7σ: A joint analysis of DESI DR2, DESY5, and DESY1 data

Gravitational wave standard sirens from GWTC-3 combined with DESI DR2 and DESY5: A late-universe probe of the Hubble constant and dark energy

Dark Energy in the DESI Era: A Brief Review of Evidence, Beyond-ΛCDM Interpretations, and Tensions

Joint curvature and growth rate measurements with supernova peculiar velocities and the CMB

Late-time background constraints on linear and non-linear interacting dark energy after DESI DR2

Revisiting CPL with sign-switching density: To cross or not to cross the NECB

Measuring neutrino mass in light of ACT DR6 and DESI DR2

Is dark energy dynamical in the DESI era? A critical review

Dissecting the Hubble tension: Insights from a diverse set of sound-horizon-free H0 measurements

When one-parameter dark energy makes neutrinos physical again

Three-band dark-siren cosmology with intermediate mass black hole binaries: Synergy of Taiji, LGWA, and the Einstein Telescope

Minimal dark SU(2) origin of a massless Dirac neutrino

Joint constraints on neutrinos and dynamical dark energy in minimally modified gravity

Slow rolling down the curvature: A reassessment of the Planck constraints on ϕ2 inflation in a closed universe

Neutrino decays as a natural explanation of the neutrino mass tension

Intertwined constraints in extended cosmologies: Dark energy, curvature, neutrinos, and inflation

Universal Seesaw leptogenesis

Neutrino mass limits and decaying dark matter: background evolution versus perturbations

Connecting cosmologically decaying dark matter to neutrino physics

Probing Physics beyond the Standard Model through Combined Analyses of Next-generation Type Ia Supernova, Cosmic Microwave Background, and Baryon Acoustic Oscillation Surveys

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