核电荷半径的同位旋相关性及其微观诠释

原子核电荷半径R_c所有的实验数据都表明, R_c系统偏离A^1/3律, 即随A增大R_c/A^1/3系统地递减, 而R_c/Z^1/3则比较接近于一个常量. 原子核巨单极共振能量E_x ∝ R^－1的大量实验数据也支持这一结论. 根本原因在于A^1/3律与同位旋无关, 而Z^1/3律已部分反映了同位旋的影响. 基于壳模型, 给出了Z^1/3律的微观诠释. 壳模型中质子和中子谐振子势强度参数ω_p和ω_n的差异, 可以用Z^1/3律说明. 基于与Wigner的原子核同位旋多重态质量公式(IMME)相似的理论考虑, 提出了核电荷半径改进的Z^1/3律.     

巨单极共振和对称能

基于带有混合同位旋标量-矢量非线性耦合的有效拉格朗日量, 在完全自洽的相对论无规位相近似的框架内, 通过单极压缩模式讨论了核物质的不可压缩性. 比较核²⁰⁸Pb,¹⁴⁴Sm,¹¹⁶Sn和⁹⁰Zr实验和计算的巨单极共振能量, 给出了核物质不可压缩系数的取值范围. 新的同位旋标量-矢量非线性耦合软化核物质的对称能, 但无损于基态性质与实验的一致性. 讨论了对称能的软化对巨单极共振的影响.     

Hawking radiation from the with a global monopole via Schwarzschild black hole gravitational anomaly

This paper derives the Hawking flux from the Schwarzschild black hole with a global monopole by using Robinson and Wilczek＇s method. Adopting a dimensional reduction technique, it can describe the effective quantum field in the （3 ＋ 1）-dimensional global monopole background by an infinite collection of the （1 ＋ 1）-dimensional massless fields if neglecting the ingoing modes near the horizon, where the gravitational anomaly can be cancelled by the （1 ＋ 1）- dimensional black body radiation at the Hawking temperature.     

杨-密耳斯理论的单极机制

对于未加规范条件的杨-密耳斯理论,提出了SU(2)规范场一种新的离壳分解.在一定的规范条件下,该分解可以导出类似于Skyrme-Faddeev形式的Wilson作用量并在经典层次上肯定了色单位矢量场的高阶导数的存在.进一步独立地证明了’tHooft关于低能杨-密耳斯理论的单极动力学是投射无关的猜想.     

Search for GUT magnetic monopoles and nuclearites with the MACRO experiment

We present the final results obtained by the MACRO experiment in the search for GUT magnetic monopoles and nuclearites. Several searches were performed with different subdetectors, i.e. scintillation counters, limited streamer tubes and nuclear track detectors. No magnetic monopole or nuclearite candidates were found. The MACRO upper limit to the local flux of GUT magnetic monopoles is at the level of 1.4×10⁻¹⁶ cm⁻² s⁻¹ sr⁻¹.     

The monopole equations and -holomorphic curves on weakly convex almost Kähler 4-manifolds

We prove that a weakly convex almost Kähler 4-manifold contains a compact, non-constant -holomorphic curve if the corresponding monopole invariant is not zero and if the corresponding line bundle is non-trivial.

     

Hawking Radiation from Horizons of Reissner-Nordström de Sitter Black Hole with a Global Monopole via Anomalies

Hawking radiation from cosmological horizon and event horizon of the Reissner-Nordström de Sitter black hole with a global monopole is studied via a new method that was propounded by Robinson and Wilzek and elaborated by Banerjee and Kulkarni. The results show that the gauge current and energy-momentum tensor fluxes, which required keeping gauge covariance and general coordinate invariance at the quantum level in the effective field theory, are exactly equivalent to those of Hawking radiation from the event horizon and the cosmological horizon, respectively.     

THERMODYNAMICS OF GLOBAL MONOPOLE ANTI-DE-SITTER BLACK HOLE IN GRAND CANONICAL ENSEMBLE

In this paper, we investigate the thermodynamics of the global monopole anti-de-Sitter black hole in the grand canonical ensemble following the York's formalism. The black hole is enclosed in a cavity with a finite radius where the temperature and potential are fixed. We have studied some thermodynamical properties, i.e. the reduced action, thermal energy and entropy. By investigating the stability of the solutions, we find stable solutions and instantons.     

F-theory inspired GUTs with extra charged matter

We consider GUT models inspired by recent local F-theory constructions. We show that after switching on vevs to scalars the extra matter becomes messengers. We discuss conditions on these vevs under which the models do not lead to unacceptable baryon/lepton number violating processes.