Particle physics today faces the challenge of explaining the mystery of dark matter, the origin
of matter over anti-matter in the Universe, the origin of the neutrino masses, the apparent …

We obtain a reliable cosmological bound on the axion mass ma by (1) deriving the
production rate directly from pion-pion scattering data, which overcomes the breakdown of …

The cosmic neutrino background (CNB) is a definite prediction of the standard cosmological
model and its direct discovery would represent a milestone in cosmology and neutrino …

The recent DESI Baryon Acoustic Oscillation measurements have led to tight upper limits on
the neutrino mass sum, potentially in tension with oscillation constraints requiring $\sum m …

We propose a new probe of cosmic relic neutrinos (CνB) using their resonant scattering
against cosmogenic neutrinos. Depending on the lightest neutrino mass and the energy …

The existence of a cosmic neutrino background has been inferred indirectly from
cosmological surveys through its effect on the linear-theory evolution of primordial density …

Cosmological neutrino mass bounds are becoming increasingly stringent. The latest limit
within $\Lambda $ CDM from Planck 2018+ ACT lensing+ DESI is $\sum m_\nu< 0.072\,{\rm …

We present robust, model-marginalized limits on both the total neutrino mass (∑ m ν) and
abundances (N eff) to minimize the role of parametrizations, priors and models when …

Gravitational potentials of the Milky Way and extragalactic structures can influence the
propagation of the cosmic neutrino background (CNB). Of particular interest to future CNB …

A bstract Cosmological constraints on the sum of the neutrino masses can be relaxed if the
number density of active neutrinos is reduced compared to the standard scenario, while at …