We review the physics and phenomenology of wave dark matter: a bosonic dark matter
candidate lighter than about 30 eV. Such particles have a de Broglie wavelength exceeding …

Ultra-light dark matter is a class of dark matter models (DM), where DM is composed by
bosons with masses ranging from 10^-24\, eV< m< eV 10-24 eV< m< eV. These models …

We use observations of ultrafaint dwarf (UFD) galaxies to constrain the particle mass of
ultralight dark matter. Potential fluctuations created by wave interference in virialized “fuzzy” …

We look for and place observational constraints on the imprint of ultralight dark matter
(ULDM) soliton cores in rotation-dominated galaxies. Extending previous analyses, we find …

A fuzzy dark matter halo consists of a soliton core close to the center and a Navarro-Frenk-
White–like density profile in the outer region. Previous investigations found that the soliton …

We present a wave generalization of the classic Schwarzschild method for constructing self-
consistent halos—such a halo consists of a suitable superposition of waves instead of …

We show that fuzzy dark matter haloes exhibit spatial differentiation in the coherence of the
field configuration, ranging from completely coherent in the central solitonic core to …

Ultralight dark matter (ULDM) is an axion-like dark matter candidate with an extremely small
particle mass. ULDM halos consist of a spherically symmetric solitonic core and an NFW-like …

Ultralight dark matter (ULDM) is usually taken to be a single scalar field. Here we explore the
possibility that ULDM consists of N light scalar fields with only gravitational interactions. This …

We explore the orbital implications of the binary Supermassive Black Holes (SMBHs)
discovered in UGC4211, for the frequency spectrum of stochastic gravitational wave …