Isospin Effect of Charged Particle Multiplicity in Intermediate Energy Heavy Ion Collisions

The dependences of He and intermediate mass fragments (IMF) production rates in the reactions 55 MeV/u ^40Ar ^58,64 Ni on the isospin, impact parameter and primary excitation energy of the reaction nuclear system were studied by using the 4π charged particle multi-detector array system (MUDAL). For the mentioned two reaction systems, the measured He particle contribution in the total charged particle multiplicity increases with increasing the total charged particle multiplicity but for the contribution of IMFs in the total charged particle multiplicity increases with increasing the total charged particle multiplicity at lower total charged particle multiplicities, and latter on it drops down with further increasing of the total charged particle multiplicities (see Fig.l). The experimental results of these two reaction systems with the same nuclear charge indicate that the contribution of He and IMFs in the total charged particle multiplicities are obviously isospin dependent.     

The production of slow particles in 16O－Em interactions at 4.5 A GeV/c

A sample of 1233 events is used to study the general characteristics of {}^{16}O－Em interactions at 4.5 A GeV/c. Multiplicity and angular distributions of slow particles and correlations among them are discussed. The present data are compared with the corresponding results from the interactions of other projectiles at the same energy and also the same projectile at different energies. The results indicate that black particle production is independent of the energy and mass of the projectile, but for grey particles it is dependent on the mass of projectile.     

Δ—scaling and Information Entropy in Ultra—Relativistic Nucleus—Nucleus Collisions

The Δ-scaling method has been applied to ultra-relativistic p p,C C and Pb Pb collision data simulated using a high-energy Monte Carlo package,LUCIAE 3.0.The Δ-scaling is found to be valid for some physical variables,such as charged particle multiplicity,strange particle multiplicity and number of binary nucleon-nucleon-nucleon collisions from these simulated nucleus-nucleus collisions over an extended energy ranging from E1ab=20 to 200A GeV.In addition we derive the information entropy from the multiplicity distribution as a function of beam energy for these collisions.     

Dependence of Isospin Fractionation on Beam Energy in Heavy Ion Collisions at Intermediate Energies

We investigated the dependence of isospin fractionation degree (N/Z)n/ (N/Z)Nfrag on the beam energy by using the isospin dependent quantum molecular dynamics model (IQMD). The (N/Z)n and (N/Z)Nfrag are the neutron proton ratio of nucleon emission (gas phase) and that of fragment emission (liquid phase) respectively. The calculated results show that (N/Z)n / (N/Z)Nfrag enhances with increasing the beam energy due to the increase of excitation energy of colliding system. But above properties is only occurred in the definiteenergy region.     

Investigation of the mean free path of projectile fragments produced in 16O－Em collision at 60 A GeV

Results are presented for an investigation of the mean free path of projectile fragments with charge 3≤Z≤8, produced by 60 A GeV {}^{16}O in nuclear emulsion. No dependence of mean free path on the distance from the point of the fragment emission is observed and our result is consistent with the nonexistence of anomalons.     

HI—V族化合物半导体的高能重离子辐照缺陷研究·

用正电子湮没寿命谱技术研究了2.4×1O15/cm2、2.2×1016/cm2注量的85MeV19F离子辐照N型GaP和1.6×1016/cm 2注量的85MeV19F离子辐照P型InP所产生的辐照缺陷.结果表明:两种注量辐照在GaP中均产生较高浓度的单空位.其浓度随着辐照注量的增大而增加;辐照也在InP中产生较高浓度的单空位.     

能量回收型直线加速器

 能量回收型直线加速器(EnergyRecoveringLinacs,简称ERL),是一种新型的、发展中的加速器,它具有直线加速器的优质束流性能,具有接近环型加速器的高效率。已在自由电子激光等方面投入应用,并具有多方面的发展和应用前景。一、由来和优势我们知道,高频电子直线加速器是用高频电场加速沿直线轨道运动的电子束的装置。通常,电子束只通过直线加速结构一次,在达到要求的能量后,即离开直线加速器,或直接用于科学实验、医学放疗、材料辐照、自由电子激光驱动等;或注入到环型加速器中继续加速和积累,用于同步辐射光源或高能物理实验等。     

破解太阳中微子失踪之谜

 2001至2003这3年时间里,太阳中微子的研究进入了一个黄金时期。在这个时期中,一个困扰了物理学家40年的难题被漂亮地解决了。这个难题的解决对于物理学和天文学来说都非常重要。本文将简要回顾3年来关于太阳中微子研究的惊人进展。太阳中微子的产生20世纪上半叶,物理学家们普遍相信太阳发光图1太阳内部的典型核聚变反应是由于其内部不断发生从氢到氦的核聚变反应。根据这一理论,在太阳内部每4个氢核(即质子)转化成1个氦核(4He)、2个正电子(e+)和2个神秘的中微子(νe),见图1所示。     

量子输运理论与非平衡手征凝聚

讨论量子输运理论以及反常手征凝聚 (DCC)的产生和演化 .建立了手征Nambu Jona Lasinio模型的量子输运方程和约束方程 .发现非平衡的夸克自旋分布是产生DCC的主要物理起因 ,而量子离壳效应可能导致长寿命的DCC .