Constraints of gravitational baryo/leptogenesis on Cardassian expansion

In this paper, proceeding from the relation between the Cardassian model and the accelerated expansion of the universe, adopting a parametric method which does not depend on a precise mechanism for gravitational baryo/leptogenesis and using the model parameter of CPT-violating interaction, we study the role of the modified Friedmann equation which plays a role in the matter asymmetry of the early epoch and the accelerated expansion of the present universe. Thus the appropriate Cardassian component in the radiation-dominated era or in the matter-dominated universe can be obtained. The results indicate that early CPT-violation is included in the Cardassian term. In the same way, the present Cardassian term that belongs to a quintessence-like model can drive the universe towards a flat, matter-dominated and accelerating expansion.     

重离子熔合反应中的静态核-核势

综述了基于改进的量子分子动力学模型对超重核合成中入射道静态势的研究,重点从静态势垒高及其与质量不对称度的关系说明弹靶组合不对称有利于熔合反应的发生,而接触点驱动势最大所对应的弹靶组合为合成超重元素的最佳选择。