Recent LHAASO Results on Cosmic-Ray Energy Spectra and Mass Composition

16 Jul 2026, 11:18
15m
江门厅 (2号楼三楼)

江门厅

2号楼三楼

Speaker

利苹 王 (IHEP)

Description

Abstract: LHAASO has achieved high-precision cosmic-ray measurements with excellent angular resolution, (10%)–(15%) energy resolution, nearly composition-independent energy reconstruction, and strong particle-identification capability. Benefiting from its large acceptance and high statistics, LHAASO has enabled a series of breakthrough results in astroparticle physics. In cosmic-ray studies, LHAASO has measured the energy spectra of individual species, especially protons and helium nuclei, with high-purity samples and a precision comparable to that of direct space-borne experiments. These measurements extend the continuous coverage of the cosmic-ray spectrum from (10,\mathrm{GeV}) to (10,\mathrm{PeV}) and reveal unexpected spectral structures, including proton hardening around (0.1,\mathrm{PeV}), a proton knee at (3.3,\mathrm{PeV}), continuous helium softening above (0.1,\mathrm{PeV}), and a weak hardening before the helium knee near (7,\mathrm{PeV}). Furthermore, LHAASO’s precise all-particle spectrum measurement, with well-controlled systematic uncertainties, reveals intrinsic spectral features and the correlation between mass composition and spectral structures. These results provide a global picture of Galactic cosmic rays over six orders of magnitude, offering important clues to their origin and acceleration mechanisms.

请选择分会 中微子物理、粒子天体物理与宇宙学

Primary authors

Shoushan Zhang (Institute of High Energy Physics) lingling Malingling_马玲玲_羊八井 (ihep) 利苹 王 (IHEP)

Presentation materials

There are no materials yet.