LHAASO源脉冲星风云的伽马射线辐射物理分析

LHAASO在0.1-1000TeV波段有极高的灵敏度，将发现许多发射TeV伽马射线辐射的天体。本项目将对LHAASO观测到的伽马射线天体，结合多波段观测结果，基于多波段非热辐射含时演化模型系统研究脉冲星风云的多波段辐射性质，特别是伽马射线起源问题，获得脉冲星风云中高能粒子分布的一般特征及其与脉冲星参数之间的关系。

LHAASO will detect many celestial objects emitting TeV gamma-rays due to its high sensitivity in the band 0.1-1000 TeV. Pulsar wind nebulae are important sources of TeV gamma-rays in the Galaxy. Using the time-dependent model of multiband nonthermal emission from pulsar wind nebulae, we will study the multiband radiative properties, especially the origin of the gamma-rays, and the distribution of high-energy particles in the pulsar wind nebulae and the relations of the distribution with the parameters of the pulsars can be derived.