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991.
A comparison between spatial burning in the semiclassical theory of laser and the intensity contours of the fringes due to multiple reflections in a Fabry-Perot cavity is presented. The concept of spatial hole burning is also used in a quantum well system.  相似文献   
992.
涂层性能超声无损评价   总被引:1,自引:0,他引:1  
本研究旨在建立热喷涂涂层超声无损评价的方法.热喷涂涂层中的超声声速根据超声脉冲在被测介质中的传播时间来计算,用TT-260型磁性测厚仪测得涂层厚度,用试纸法测得涂层孔隙率,用显微硬度计测得涂层的显微硬度,并对超声声速与热喷涂涂层特性(孔隙率、显微硬度)之间的关系作了探讨.实验结果表明,涂层中的超声声速与孔隙率之间的关系是,随着孔隙率的增大,超声声速减小.涂层中的超声声速与显微硬度的关系是,随着显微硬度的增大,超声声速也增大.  相似文献   
993.
黑洞球对称吸积存在稳恒态的亚声速-跨声速解,该解对应最大可能吸积率的稳恒态吸积流.在本文中,我们应用计算流体动力学方法成功得到了跨声速吸积流的整体解.该方法的优点在于,吸积流体从初态沿着时间方向不断推进到稳恒态的过程是物理的、真实的演化过程.另外,计算流体力学方法发展得比较成熟,为我们求解跨声速吸积流提供了非常强大的工具.除了球对称吸积过程,计算流体力学的方法也应该同样适用于求解辐射无效吸积流以及超Eddington吸积流的整体动力学结构.  相似文献   
994.
Since the discovery of Hawking radiation, its consistency with quantum theory has been widely questioned. In the widely described picture, irrespective of what initial state a black hole starts with before collapsing, it eventually evolves into a thermal state of Hawking radiations after the black hole is exhausted. This scenario violates the principle of unitarity as required for quantum mechanics and leads to the acclaimed ‘‘information loss paradox'. This paradox has become an obstacle or a reversed touchstone for any possible theory to unify the gravity and quantum mechanics. Based on the results from Hawking radiation as tunneling, we recently show that Hawking radiations can carry off all information about the collapsed matter in a black hole. After discovering the existence of information-carrying correlation, we show in great detail that entropy is conserved for Hawking radiation based on standard probability theory and statistics. We claim that information previously considered lost remains hidden inside Hawking radiation. More specifically, it is encoded into correlations between Hawking radiations. Our study thus establishes harmony between Hawking radiation and the unitarity of quantum mechanics, which establishes the basis for a significant milestone toward resolving the long-standing information loss paradox. The paper provides a brief review of the exciting development on Hawking radiation. In addition to summarize our own work on this subject, we compare and address other related studies.  相似文献   
995.
Three areas in which Coulomb interactions are of obvious importance are considered in turn, namely liquid alkali metals, electron–hole droplets, and lithium halides. The focus in the first two areas is dominantly on critical point properties, whereas in the third area the solid–liquid transition is the predominant interest.  相似文献   
996.
The dynamic behavior of photoinduced optical anisotropy of amorphous PMMA/Sudan Red III thin films has been investigated using the pump-probe method. The results showed that the anisotropy increased rapidly in an exponential fashion in the first seconds of pumping, so that a photostationary state was reached as a result of the photoisomerization process cycles. The anisotropy relaxation phase decreased exponentially in a slow manner, which means the anisotropy did not disappear instantaneously when the irradiation was switched off. Evidence of the existence of the Angular Hole Burning (AHB) and the Angular Redistribution (AR) effects in the Sudan Red III molecules in the PMMA polymeric host is presented. The relative photoinduced optical anisotropy was calculated. The results showed that, at room temperature, the thermal isotropic relaxation of the photoisomer was negligible compared to the anisotropic reverse photoisomerization that occurred as soon as the pump beam was cut-off.  相似文献   
997.
998.
In this article, we explored the noncovalent bonding interactions between O?C?S, S?C?S, F2C?S, Cl2C?S, and singlet carbene. Six chalcogen‐bonded complexes were obtained. It is found that all the vibrational frequencies of C?S bond presented a red shift character. Interaction energy, topology property of the electron density and its Laplacian, and the donor–acceptor interaction have been investigated. All these results show that there exists a weak nonbonded interaction between the chalcogen bond donor and CH2. An energy decomposition analysis was performed to disclose that the electrostatic interaction is the main stabilized factor in these nonbonded complexes. © 2010 Wiley Periodicals, Inc. Int J Quantum Chem, 2011  相似文献   
999.
We explore the quadratic form of the f(R)=R+bR2 gravitational theory to derive rotating N-dimensions black hole solutions with ai,i1 rotation parameters. Here, R is the Ricci scalar and b is the dimensional parameter. We assumed that the N-dimensional spacetime is static and it has flat horizons with a zero curvature boundary. We investigated the physics of black holes by calculating the relations of physical quantities such as the horizon radius and mass. We also demonstrate that, in the four-dimensional case, the higher-order curvature does not contribute to the black hole, i.e., black hole does not depend on the dimensional parameter b, whereas, in the case of N>4, it depends on parameter b, owing to the contribution of the correction R2 term. We analyze the conserved quantities, energy, and angular-momentum, of black hole solutions by applying the relocalization method. Additionally, we calculate the thermodynamic quantities, such as temperature and entropy, and examine the stability of black hole solutions locally and show that they have thermodynamic stability. Moreover, the calculations of entropy put a constraint on the parameter b to be b<116Λ to obtain a positive entropy.  相似文献   
1000.
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