Abstract The Alpha Magnetic Spectrometer (AMS) is a precision particle physics detector on
the International Space Station (ISS) conducting a unique, long-duration mission of …

Understanding the physical mechanisms that control galaxy formation is a fundamental
challenge in contemporary astrophysics. Recent advances in the field of astrophysical …

The Review summarizes much of particle physics and cosmology. Using data from previous
editions, plus 2,143 new measurements from 709 papers, we list, evaluate, and average …

The measurement of the energy spectrum of cosmic ray helium nuclei from 70 GeV to 80
TeV using 4.5 years of data recorded by the Dark Matter Particle Explorer (DAMPE) is …

We examine the theoretical motivations for long-lived particle (LLP) signals at the LHC in a
comprehensive survey of standard model (SM) extensions. LLPs are a common prediction of …

The diffuse Galactic γ-ray emission, mainly produced via interactions between cosmic rays
and the interstellar medium and/or radiation field, is a very important probe of the …

Precision measurements of cosmic ray positrons are presented up to 1 TeV based on 1.9
million positrons collected by the Alpha Magnetic Spectrometer on the International Space …

A precision measurement by AMS of the antiproton flux and the antiproton-to-proton flux
ratio in primary cosmic rays in the absolute rigidity range from 1 to 450 GV is presented …

Knowledge of the rigidity dependence of the boron to carbon flux ratio (B/C) is important in
understanding the propagation of cosmic rays. The precise measurement of the B/C ratio …

The precise measurement of the spectrum of protons, the most abundant component of the
cosmic radiation, is necessary to understand the source and acceleration of cosmic rays in …