25–29 Apr 2026
Kechuang Building
Asia/Shanghai timezone

Searching for VHE Pulsars with LHAASO

27 Apr 2026, 17:10
5m
A102 (Kechuang Building)

A102

Kechuang Building

NO.1520 Taihu Blvd, Suzhou, Jiangsu, China
Poster report(print size: 0.6m Wide*0.9m High) Pulsar Wind Nebulae & Haloes & Pulsars session

Speaker

建立 张 (NAOC)

Description

Gamma-ray observations have established energetic isolated pulsars as outstanding particle accelerators and antimatter factories. However, many questions are still open regarding the acceleration and radiation processes involved, as well as the locations where they occur. The radiation spectra of all gamma-ray pulsars observed to date show strong break above energies of a few GeV. LHAASO may reveal the highest pulsation component from pulsars. Furthermore, they pave the way for investigating pulsars through their TeV emission, thereby imposing additional constraints on the acceleration and emission processes in their extreme energy limit.

Primary authors

Dr Hui Zhu 建立 张 (NAOC)

Presentation materials

There are no materials yet.