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 …

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 …

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 …

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 …

Precision results on cosmic-ray electrons are presented in the energy range from 0.5 GeV to
1.4 TeV based on 28.1× 10 6 electrons collected by the Alpha Magnetic Spectrometer on the …

We consider a classically scale invariant version of the Standard Model, extended by an
extra dark SU (2) X gauge group. Apart from the dark gauge bosons and a dark scalar …

The next generation magnetic spectrometer in space, AMS-100, is designed to have a
geometrical acceptance of 100 m 2 sr and to be operated for at least ten years at the Sun …

We present the precision measurements of 11 years of daily cosmic positron fluxes in the
rigidity range from 1.00 to 41.9 GV based on 3.4× 10 6 positrons collected with the Alpha …

In this work we study a classically scale-invariant extension of the Standard Model in which
the dark matter and electroweak scales are generated through the Coleman-Weinberg …