Fuzzy dark matter (FDM) is a dark matter candidate consisting of ultralight scalar particles
with masses around, a regime where cold bosonic matter behaves as a collective wave …

Measuring the magnetic field in cosmic filaments reveals how the Universe is magnetized
and the process that magnetized it. Using the Rotation Measures (RM) at 144 MHz from the …

For decades, the boundary of cosmic filaments has been a subject of debate. In this work,
we determine the physically motivated radii of filaments by constructing stacked galaxy …

Context. A significant fraction of the predicted baryons remain undetected in the local
Universe. We adopted the common assumption that a large fraction of the missing baryons …

Filaments are elongated structures that connect groups and clusters of galaxies and are
visually the striking feature in cosmological maps. In the literature, typically filaments are …

Galaxy cluster outskirts are described by complex velocity fields induced by diffuse material
collapsing towards filaments, gas, and galaxies falling into clusters, and gas shock …

Faraday rotation studies of distant radio sources can constrain the evolution and the origin of
cosmic magnetism. We use data from the LOFAR Two-Metre Sky Survey: Data Release 2 …

We present the study of gas phases around cosmic-web filaments detected in the TNG300-1
hydro-dynamical simulation at redshift z= 0. We separate the gas into five different phases …

Context. About 30%–40% of the baryons in the local Universe remain unobserved. Many of
these" missing" baryons are expected to reside in the warm-hot intergalactic medium …

Matter distribution around clusters is highly anisotropic because clusters are the nodes of
the cosmic web. The shape of the clusters and the number of filaments to which they are …