We review several current aspects of dark matter theory and experiment. We overview the
present experimental status, which includes current bounds and recent claims and hints of a …

We present an overview of scenarios where the observed Dark Matter (DM) abundance
consists of Feebly Interacting Massive Particles (FIMPs), produced nonthermally by the so …

The region around the Galactic Center (GC) is now well established to be brighter at
energies of a few GeV than what is expected from conventional models of diffuse gamma …

One of the simplest viable models for dark matter is an additional neutral scalar, stabilised
by a Z _2 Z 2 symmetry. Using the GAMBIT package and combining results from four …

The Galactic center excess (GCE) remains one of the most intriguing discoveries from the
Fermi Large Area Telescope (LAT) observations. We revisit the characteristics of the GCE by …

An anomalous gamma-ray excess emission has been found in the Fermi Large Area
Telescope data covering the centre of the Galaxy,. Several theories have been proposed for …

Cosmic rays are an important tool to study dark matter (DM) annihilation in our Galaxy.
Recently, a possible hint for dark matter annihilation was found in the antiproton spectrum …

The dark matter (DM) searches falling under the umbrella of indirect detection seek to
identify possible visible products of DM interactions, originating from the DM already present …

Cosmic rays (CRs) with energies≪ TeV comprise a significant component of the interstellar
medium (ISM). Major uncertainties in CR behaviour on observable scales (much larger than …

The Fermi-LAT data accumulated over 7 years of γ-ray observations, together with the high
resolution gas (CO & HI) and the dust opacity maps, are used to study the emissivity of γ …