排序方式: 共有16条查询结果,搜索用时 15 毫秒
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In spherically symmetric systems, in spite of Birkhoff's Theorem, the rates of clocks in vacuum regions on either side of moving mass shells must be continually readjusted to stay in synchrony. This shows up as time-dependence of the metric in terms of the globally meaningful time coordinate. 相似文献
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We study the evolution of radiating and viscous fluid spheres assuming an additional homothetic symmetry on the spherically symmetric space-time. We match a very simple solution to the symmetry equations with the exterior one (Vaidya). We then obtain a system of two ordinary differential equations which rule the dynamics, and find a self-similar collapse which is shear-free and with a barotropic equation of state. Considering a huge set of initial self-similar dynamics states, we work out a model with an acceptable physical behavior. 相似文献
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A. Di Prisco N. Falcón L. Herrera M. Esculpi N. O. Santos 《General Relativity and Gravitation》1997,29(11):1391-1405
The influence of processes occurring before the system relaxes into diffusion, on the evolution of a radiating sphere, is exhibited in a specific example. The luminosity profiles, and consequently the general evolution of the object, are shown to be quite sensitive to the value of relaxation time. 相似文献
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确定硼烷的杂硼烷价成键轨道对称性的拓扑方法 总被引:1,自引:0,他引:1
本文通过对硼烷的分子轨道的定域化分析, 建立了由硼烷或杂硼烷的骨架多面体的几何性质, 确定其价成键轨道对称性的拓扑方法。从以多面体骨架的三角面和缺顶点周围的边为基约化出的不同约表示中, 按建议的能量与节面数的对应规则,选定出分子的价成键轨道所属的不可约表示。 相似文献
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Nikolai V. Mitskievich 《General Relativity and Gravitation》1999,31(5):713-717
We show that combinations of (in general,non-linear) two- and threeform fields, analogous to theMaxwell (one-form) field, completely describe perfectfluids, including the rotating ones. In the non-rotating case, the two-form field is sufficient, and afree three-form field proves to be equivalent toappearance of the cosmological term in Einstein'sequations (the square-root non-linearity correspondingto = 0). The gauge degrees of freedombreak down when a rotation is included, but even whenthey exist, there fails to be realized an equivalence ofthe two-form field and the massless scalar one recently claimed by Weinberg. 相似文献
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We show that a relativistic gas may be at"global" equilibrium in the expanding universe for anyequation of state 0 < p /3, provided thatthe gas particles move under the influence of aself-interacting, efiective one-particle force in between elasticbinary collisions. In the force-free limit we recoverthe equilibrium conditions for ultrarelativistic matterwhich imply the existence of a conformal timelike Killing vector. 相似文献
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η^5-RO~2CC~5H~4(CO)~3MNa与R^1HgCl,R^1=Me, Et, Ph)可发生一种非预期的金属键形成反应, 生成[η^5-RO~2CC~5H~4(CO)~3M]~2Hg(R=Me,Et;M=Cr,Mo,W)。对反应中间物η^5-EtO~2CC~5H~4(CO)~3MoHgPh的研究表明: 反应是按缩合及对称化两步机理进行的。(R=Et,M=Mo)属三斜晶系, 空间群P-1。a=0.6333(1), b=0.7712(1), c=1.4204(4)nm; a=77.31(1),β=74.51(2), γ=68.72(1)^°; V=0.61714nm^3;Z=1;D~x=2.246g/cm^3;R=0.044。 相似文献
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