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 …

Although dark matter is a central element of modern cosmology, the history of how it became
accepted as part of the dominant paradigm is often ignored or condensed into an anecdotal …

We test Milgromian dynamics (MOND) using wide binary stars (WBs) with separations of 2–
30 kAU. Locally, the WB orbital velocity in MOND should exceed the Newtonian prediction …

This report presents a comprehensive collection of searches for new physics performed by
the ATLAS Collaboration during the Run 2 period of data taking at the Large Hadron …

We propose a relativistic gravitational theory leading to modified Newtonian dynamics, a
paradigm that explains the observed universal galactic acceleration scale and related …

ABSTRACT We introduce SPARC (Spitzer Photometry and Accurate Rotation Curves): a
sample of 175 nearby galaxies with new surface photometry at 3.6 μm and high-quality …

Astronomical observations reveal a major deficiency in our understanding of physics—the
detectable mass is insufficient to explain the observed motions in a huge variety of systems …

A wealth of astronomical data indicate the presence of mass discrepancies in the Universe.
The motions observed in a variety of classes of extragalactic systems exceed what can be …

We present high-resolution rotation curves and mass models of 26 dwarf galaxies from"
Local Irregulars That Trace Luminosity Extremes, The H i Nearby Galaxy Survey"(LITTLE …

We provide ingredients and recipes for computing signals of TeV-scale Dark Matter
annihilations and decays in the Galaxy and beyond. For each DM channel, we present the …