The interaction between dark matter and dark energy can be incorporated into field theory
models of dark energy that have proved successful in alleviating the coincidence problem …

The strong discrepancy between local and early-time (inverse distance ladder) estimates of
the Hubble constant H 0 could be pointing towards new physics beyond the concordance Λ …

The question of whether cosmic microwave background (CMB) temperature and polarization
data from Planck favor a spatially closed universe with curvature parameter Ω K< 0 has been …

We present here up-to-date neutrino mass limits exploiting the most recent cosmological
data sets. By making use of the cosmic microwave background temperature fluctuation and …

We explore cosmological constraints on the sum of the three active neutrino masses M ν in
the context of dynamical dark energy (DDE) models with equation of state (EoS) …

Blázquez-Salcedo et al.[Phys. Rev. Lett. 126, 101102 (2021) PRLTAO 0031-9007
10.1103/PhysRevLett. 126.101102] obtained asymptotically flat traversable wormhole …

We revisit cosmological constraints on the sum of the neutrino masses Σ m ν from a
combination of full-shape BOSS galaxy clustering [P (k)] data and measurements of the …

In this work we update the bounds on∑ m ν from latest publicly available cosmological data
and likelihoods using Bayesian analysis, while explicitly considering particular neutrino …

We have updated the constraints on flavour universal neutrino self-interactions mediated by
a heavy scalar, in the effective 4-fermion interaction limit. We use the relaxation time …

We present an updated data-analysis comparison of the most recent observations of the
cosmic microwave background temperature anisotropies and polarization angular power …