103 citations · 186 across the 10 of their papers we have counts for
10 papers
Gamma-Ray Burst observations by the high-energy charged particle detector on board the CSES-01 satellite between 2019 and 2021
Francesco Palma, Matteo Martucci, Coralie Neubüser +68
In this paper we report the detection of five strong Gamma-Ray Bursts (GRBs) by the High-Energy Particle Detector (HEPD-01) mounted on board the China Seismo-Electromagnetic Satell…
Cosmic-ray Antinuclei as Messengers of New Physics: Status and Outlook for the New Decade
P. von Doetinchem, K. Perez, T. Aramaki +59
The precise measurement of cosmic-ray antinuclei serves as an important means for identifying the nature of dark matter and other new astrophysical phenomena, and could be used wit…
Production of cosmic-ray antinuclei in the Galaxy and background for dark matter searches
Nicola Tomassetti, Alberto Oliva
Antimatter nuclei in cosmic rays (CR) represent a promising discovery channel for the indirect search of dark matter. We present astrophysical background calculations of CR antideu…
Fresh Insights on Cosmic-ray Propagation from the New AMS Data
Nicola Tomassetti, Jie Feng, Alberto Oliva
The Alpha Magnetic Spectrometer (AMS) experiment has released new measurements of primary and secondary nuclei in cosmic rays at the TeV energy scale. Using these data, we present…
Secondary antinuclei from supernova remnants and background for dark matter searches
Nicola Tomassetti, Alberto Oliva
We compute the spectra of cosmic-ray (CR) nuclei and antinuclei under a scenario where hadronic interaction processes inside supernova remnants (SNRs) can produce a diffusively-sho…
Production of antimatter nuclei in Galactic cosmic rays
Alberto Oliva, Nicola Tomassetti, Jie Feng
Antimatter nuclei in cosmic rays (CRs) are a promising tool for the indirect detection of dark-matter annihilation signatures. However, the search of new-physics signals in CRs rel…
Production and acceleration of antinuclei in supernova shockwaves
Nicola Tomassetti, Alberto Oliva
We compute the energy spectra of antideuterons and antihelium in cosmic rays (CRs) in a scenario where hadronic interactions inside supernova remnants (SNRs) can produce a diffusiv…
Bayesian analysis of cosmic-ray propagation parameters: secondary antiparticles from spatial-dependent diffusion models
Jie Feng, Nicola Tomassetti, Alberto Oliva
The antiparticle energy spectra of Galactic cosmic rays (CRs) have several exciting features such as the unexpected positron excess at 10-200\,GeV and the remarkably hard an…
Bayesian analysis of spatial-dependent cosmic-ray propagation: astrophysical background of antiprotons and positrons
Jie Feng, Nicola Tomassetti, Alberto Oliva
The AMS-02 experiment has reported a new measurement of the antiproton/proton ratio in Galactic cosmic rays (CRs). In the energy range 60-450 GeV, this ratio is found to b…
Identification of Light Cosmic-Ray Nuclei with AMS-02
Nicola Tomassetti, Alberto Oliva
AMS-02 is a wide acceptance (0.5 m2 sr) and long duration (up to 20 years) magnetic spectrometer operating onboard the International Space Station since May 2011. Its main scientif…