Brans-Dicke理论中静态球对称引力场的de Broglie-Bohm量子化

将量子力学的deBroglieBohm(dBB)解释引入BransDicke(BD)理论中.在小超空间近似下,求出了Brans类型1量子黑洞的波函数.利用dBB解释求得Brans类型1的量子轨迹和量子势.在量子黑洞背景几何上,研究了径向光的行为.发现Brans类型1量子化后的黑洞“温度”是奇异的.另外,由于BD引力理论在BD参数ω趋于无穷大时应与广义相对论等价,因而Schwarzschild黑洞在dBB量子化后“温度”也是奇异的.这似乎意味着dBB量子化不能应用于黑洞. 关键词： deBroglie-Bohm解释 Brans-Dicke引力理论 量子轨迹 小超空间近似     

Plane Symmetric Vacuum Bianchi Type-III Cosmological Model in Brans-Dicke Theory

We have obtained an exact solution of the vacuum Brans-Dicke (Phys. Rev. 124:925, 1961) field equations for the metric tensor of a spatially homogeneous and anisotropic model. Some physical properties of the model are also studied.     

充满物质的Friedmann-Robertson-Walker宇宙的稳定性

研究了在含有宇宙(学)常数的Friedmann-Robertson-Walker宇宙模型中,充满、满足p=(γ-1)ρ物质宇宙的稳定性.通过计算引力波的扰动,以及dp/dp=γ-1的扰动,得到对于ε=-1,Λ<0,满足Einstein场方程的宇宙只要γ≥0是不稳定的. 关键词： 充满物质的Friedmann-Robertson-Walker宇宙 虫洞 时空稳定性     

Hypersurface Homogeneous Space Time with Anisotropic Dark Energy in Brans Dicke Theory of Gravitation

The main purpose of the present paper is to explore hypersurface homogenous space time in Brans Dicke theory of gravitation in terms of the dark energy source. To obtain solution of the field equation, we have taken into account the relation between and the average scale factor a. The volumetric expansions are considered to get deterministic solutions. Physical properties of the models are also discussed in detail.     

Non-equilibrium Dynamics of an Optomechanical Dicke Model

Motivated by the experimental realization of Dicke model in optical cavities, we model an optomechanical system consisting of two-level BEC atoms with transverse pumping. We investigate the transition from normal and inverted state to the superradiant phase through a detailed study of the phase portraits of the system. The rich phase portraits generated by analytical arguments display two types of superradiant phases, regions of coexistence and some portion determining the persistent oscillations. We study the time evolution of the system from any phase and discuss the role of mirror frequency in reaching their attractors. Further, we add an external mechanical pump to the mirror which is capable of changing the mirror frequency through radiation pressure and study the impact of the pump on the phase portraits and the dynamics of the system. We find the external mirror frequency changing the phase portraits and even shifting the critical transition point, thereby predicting a system with controllable phase transition.     

Periodic Distribution of Galaxies in Generalized Scalar Tensor Theory

With the help of Nordtvedt's scalar tensor theory an exact analytic model of a non–minimally coupled scalar field cosmology in which the gravitational coupling G and the Hubble factor H oscillate during the radiation era is presented. A key feature is that the oscillations are confined to the early stages of the radiation dominated era with G approaching its present constant value while H becoming a monotonically decreasing function of time. The Brans Dicke parameter is chosen to be a function of Brans Dicke scalar field so that no conflict with observational constraints regarding its present value arises.     

单离子阱中基本量子逻辑单元的实现

建议了一种利用单个囚禁冷却离子实现基本量子逻辑门操作(单比特门和两比特受控旋转门)的理论方法,通过数值计算给出了各种相关实验参量的合理设置要求.在这一方案中,量子逻辑门的操作既不要求离子辅助能级的参与,也不限定只在弱耦合的LambDicke区内进行,因而将更容易地为实验所实现 关键词： 量子计算机 受控量子逻辑门操作 LambDicke耦合参数     

A theoretical construction of thin shell wormhole from tidal charged black hole

Recently, Dadhich et al. (Phys. Lett. B 487, 1, 2000) have discovered a black hole solution localized on a three brane in five dimensional gravity in the Randall–Sundrum scenario. In this article, we develop a new class of thin shell wormhole by surgically grafting above two black hole spacetimes. Various aspects of this thin wormhole are also analyzed.     

The Momentum Four-Vector in Brans–Dicke Wormholes

In this work, in order to compute energy and momentum distributions (due to matter plus fields including gravitation) associated with the Brans–Dicke wormhole solutions we consider Møller’s energy-momentum complexes both in general relativity and the teleparallel gravity, and the Einstein energy-momentum formulation in general relativity. We find exactly the same energy and momentum in three of the formulations. The results obtained in teleparallel gravity is also independent of the teleparallel dimensionless coupling parameter, which means that it is valid not only in the teleparallel equivalent of general relativity, but also in any teleparallel model. Furthermore, our results also sustains (a) the importance of the energy-momentum definitions in the evaluation of the energy distribution of a given spacetime and (b) the viewpoint of Lessner that the Møller energy-momentum complex is a powerful concept of energy and momentum. (c) The results calculated supports the hypothesis by Cooperstock that the energy is confined to the region of non-vanishing energy-momentum tensor of matter and all non-gravitational fields.     

Non-equilibrium dynamical phases of the two-atom Dicke model

In this paper, we investigate the non-equilibrium dynamical phases of the two-atom Dicke model, which can be realized in a two species Bose–Einstein condensate interacting with a single light mode in an optical cavity. Apart from the usual non-equilibrium normal and inverted phases, a non-equilibrium mixed phase is possible which is a combination of normal and inverted phase. A new kind of dynamical phase transition is predicted from non-superradiant mixed phase to the superradiant phase which can be achieved by tuning the two different atom–photon couplings. We also show that a dynamical phase transition from the non-superradiant mixed phase to the superradiant phase is forbidden for certain values of the two atom–photon coupling strengths.