核天体反应直接测量中的γ加和谱解析方法

带电粒子辐射俘获反应是核天体物理的主要研究内容之一,对了解恒星核合成过程具有重要意义．由于恒星温度（伽莫夫窗口）下这些反应的截面极小,γ射线产额非常低,实验需要结合高效率的γ加和探测技术进行测量．本文基于贝叶斯理论和相关分析程序,发展了一种对加和型γ探测阵列能谱的解析方法,并利用该方法对锦屏深地核天体物理实验项目测量的实验数据进行分析,验证了该解析方法的有效性,并显著减小了γ加和峰探测效率的误差,进一步提高了γ加和探测技术的测量精度．      

Possible light neutral boson and particle mass quantization

Qualities of nucleons, such as the fundamental parameter mass, might be modified in extreme conditions relative to those of isolated nucleons. We show the ratio of the EMC-effect tagged nucleon mass to that of the free one(m*/m);these values are derived from the nuclear structure function ratio between heavy nuclei and deuterium measured in the electron Deep Inelastic Scattering(DIS) reaction in 0.3≤x≤0.7. The increase in m*/mwith A-1/3 is phenomenologically interpreted via the release of a color-singlet cluster formed by sea quarks and gluons in bound nucleons holding high momentum in the nucleus, from which the mass and fraction of non-nucleonic components in nuclei can be deduced. The mass of color-singlet clusters released per short range correlated(SRC) proton in the high momentum region(k > 2 fm-1) is extracted to be 16.890 ±0.016 MeV/c2, which evidences the possibility of a light neutral boson and quantized mass of matter.