电子束辐射固化环氧树脂的反应过程分析

对双酚A型环氧树脂的电子束辐射固化反应过程进行了分析.考察了引发剂、稀释剂对树脂体系辐射反应的影响,以环氧丙烷作为模型化合物,研究了环氧丙烷-碘盐体系的电子束辐射反应机理,证实了在电子束辐射下,碘盐分解产生质子酸,引发环氧树脂阳离子开环聚合的反应过程.观测环氧树脂辐射固化区域发现,电子束穿过样品时发生强烈的散射,在辐射方向以及周围一定区域内引发固化反应,固化反应从活性中心开始向体系内部层层扩展,整个固化区域由很多的层状结构组成.     

利用微波技术合成4-芳基-5-甲氧羰基-6-甲基3,4-二氢吡啶-2-酮

微波辐射;二氢吡啶酮;芳醛;麦氏酸;利用微波技术合成4-芳基-5-甲氧羰基-6-甲基3;4-二氢吡啶-2-酮     

Radiative Corrections to Casimir Force of Maxwell-Chern-Simons Gauge Field

We discuss the two-loop radiative correction to the Casimir force of Maxwell Chern Simons Abelian gauge field between two parallel ideal conducting wires in terms of Feynman path integral method.     

The dispersive properties of a dielectric-rod loaded waveguide immersed in a magnetized annular plasma

Propagation properties of electromagnetic waves in a dielectric-rod waveguide immersed in a magnetized annular plasma are presented in this paper. The dispersion relations are derived and calculated. The results show that the dielectric-rod loading can make the structure less dispersive and the transmission frequency-band broadened.     

Radiative lifetimes of Rydberg 6pnd J=2 states of Pb I by multichannel quantum defect theory

Energy levels of the odd-parity 6pnd J=2 Rydberg states of Pb I are analysed by the multichannel quantum defect theory (MQDT) in the frame of a five-channel three-limit calculation model. With optimal MQDT parameters, channel admixture coefficients are obtained and used to calculate the theoretical lifetimes of the levels by comparing to the previously measured lifetimes. The predicted lifetimes for higher-lying Rydberg states are given and discussed. These predicted lifetimes are very different from those obtained by the four-channel two-limit model pl:eviously used, which means that introduction of the additional interacting channel is important for studying the 6pnd J=2 Rydberg states of Pb I.     

Hawking radiation of Weyl neutrinos in a rectilinearly non—uniformly accelerating Kinnersley black hole

The quantum thermal effect of Weyl neutrinos in a rectilinearly non-uniformly accelerating Kinnersley black hole is investigated using the generalized tortoise coordinate transformation.The equations that determine the location,the Hawking temperature of the event horizon and the thermal radiation spectrum of neutrinos are derived.Our results show that the location and the temperature of the event horizon depend not only on the time but also on the angle.     

Constructive interference via collision—aided radiative excitation

We have studied theoretically constructive interference via collision-aided radiative excitation in an open four-level system using a density matrix approach. The four-level system consists of a Λ-type three-level quantum-beat configuration driven by one laser field and a fourth level coupled by a vacuum mode. It is shown that through the incoherent process (collision), coherence between widely-separated doublets and subsequent constructive interference can be realized. We analyse the effects of the collision-induced coherent and incoherent decay rates, laser intensity, and energy separation of the doublets on the interference. Meanwhile, the constructive interference between the two transition pathways 3P_1/2-4D and 3P_3/2-4D via equal-frequency hybrid excitation and collision-aided radiative excitation in an Na₂-Na system is experimentally observed. A good agreement between the theoretical and experimental results is obtained.     

CaF2∶Dy的热释光特性研究

经测量与分析得出,CaF2∶Dy受X射线辐照后在25～290K及300～670K范围内有76、84、137、170、349、363、388、414、437、465K等热释光(TL)峰,各峰均含4个窄发光带,其中心波长分别为480、575、675及775nm。由X射线激发导致的辐射致发光(RL)谱中除上述4个窄带外在较短波长处还有宽带出现。由对发光曲线的分析中得出的动力学参数值推测,窄带发光可能是由较为邻近的空穴-Dy2+贯穿势垒复合而形成,而宽带则可能是激子或自俘激子发光。380K以下的TL峰在室温下很不稳定,可见光对上述各TL发光都有衰减作用。     

弯管结构塑性极限分析的数值方法及应用

从塑性极限分析数值计算的角度,分析了多组载荷联合作用下弯管结构的塑性极限承载能力。为了克服塑性极限上限分析中目标函数非线性非光滑所导致的数值困难,提出了一种弯管结构塑性极限上限分析的无搜索优化迭代算法;采用一种改进的弯管单元并利用加载路径的径向射求解方案处理多组载荷系统。通过对典型弯管结构进行塑性极限分析得出了一些有价值的结论。     

γ噪Blazar天体的γ射线和近红外光辐射研究

收集了29个有γ噪的Blazar天体(其中有16个BL Lac天体和13个平谱射电类星体)的近红外流量密度和γ射线流量密度,获得以下主要结果:1)23个天体中的γ射线流量密度和近红外流量密度在低态时存在较强的相关性而在高态时有弱的相关性.2)在29个天体中,有6个天体只有一个观测数据点,将其认为是高态时,γ射线流量密度与近红外光流量密度之间有弱相关性,而认为是低态时有强相关性.3)29个源的γ射线流量密度与X射线流量密度在低态时有相关性,但是γ射线流量与光学流量密度,γ射线流量与射电流量密度均没有相关性.4)在16个BL Lac天体中γ射线流量与近红外光流量不论在高态还是低态都有相关性,而13个平谱射电类星体没有相关性.讨论了γ噪Blazar天体的γ射线辐射机制,认为γ射线的辐射机制主要是同步自康普顿散射.而逆康普顿散射来自绕中心核且温度约为2000K的尘埃,这些尘埃的区域大约有r=3pc,聚束的相对论电子也可能是这种尘埃模型辐射机制的一个重要补充.平谱射电类星体和BL Lac天体的γ辐射机制可能有些不同. 关键词： Blazar天体 星系γ射线观测辐射机制 非热辐射