Abstract The standard Λ Cold Dark Matter (ΛCDM) cosmological model provides a good
description of a wide range of astrophysical and cosmological data. However, there are a …

WDs and neutron stars are far-reaching and multi-faceted laboratories in the hunt for dark
matter. We review detection prospects of wave-like, particulate, macroscopic and black hole …

Matter evolved under the influence of gravity from minuscule density fluctuations.
Nonperturbative structure formed hierarchically over all scales and developed non …

Abstract The Nancy Grace Roman Space Telescope will conduct a High Latitude
Spectroscopic Survey (HLSS) over a large volume at high redshift, using the near-IR grism …

We present exoplanets as new targets to discover dark matter (DM). Throughout the Milky
Way, DM can scatter, become captured, deposit annihilation energy, and increase the heat …

Optimal analyses of many signals in the cosmic microwave background (CMB) require map-
level extraction of individual components in the microwave sky, rather than measurements at …

We perform for the first time a joint analysis of the monopole and quadrupoles for power
spectrum, bispectrum and integrated trispectrum (i-trispectrum) from the redshift space …

Gravitational microlensing finds planets through their gravitational influence on the light
coming from a more distant background star. The presence of the planet is then inferred from …

We explore the potential of precision cosmological data to study non-minimal dark sectors
by updating the cosmological constraint on the mirror twin Higgs model (MTH). The MTH …

We analyse the clustering of matter on large scales in an extension of the concordance
model that allows for spatial curvature. We develop a consistent approach to curvature and …