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Wu Zhong Chao 《General Relativity and Gravitation》1999,31(2):223-231
For a spherically symmetric vacuum model with anegative cosmological constant, a complex constrainedinstanton is considered as the seed for the quantum paircreation of Schwarzschild-anti-de Sitter black holes. The relative creation probability isfound to be the exponential of the negative of the blackhole entropy. The black hole entropy is known to be onequarter of the black hole horizon area. In the absence of a general noboundary proposal foropen creation, the constrained instanton approach isused in treating both the open and closed pair creationsof black holes. 相似文献
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U. Kasper 《General Relativity and Gravitation》1997,29(2):221-233
The Hamilton formalism of cosmological models in fourth-order theories of gravity is considered. An approach to constructing the Hamilton function is presented which starts by replacing the second order derivatives of configuration space coordinates by functions depending on these coordinates, its first order derivatives, and additional variables playing the role of configuration space coordinates. This formalism, which does not resort to the Ostrogradski or Dirac formalism, is elucidated and applied to examples. For a special class of Lagrange functions, it is demonstrated that the canonical coordinates of the considered formalism and of the Ostrogradski formalism are related via a canonical transformation. The canonical transformation is a transformation of the configuration space coordinates and a transformation of momentum components induced by the transformation of the configuration space coordinates for a special element of the class of Lagrange functions mentioned. The Wheeler-DeWitt equations belonging to this Lagrange function are related via minisuperspace coordinate transformations. 相似文献
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Quantum Black Hole 总被引:1,自引:0,他引:1
Wu Zhong Chao 《General Relativity and Gravitation》1998,30(1):115-121
Creation of a black hole in quantum cosmology is the third way of black hole formation. In contrast to the gravitational collapse from a massive body in astrophysics or from the quantum fluctuation of matter fields in the very early universe, in the quantum cosmology scenario the black hole is essentially created from nothing. The black hole originates from a constrained gravitational instanton. The probability of creation for all kinds of single black holes in the Kerr-Newman family, at the semiclassical level, is the exponential of the total entropy of the universe, or one quarter of the sum of both the black hole and the cosmological horizon areas. The de Sitter spacetime is the most probable evolution at the Planckian era. 相似文献
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本文采用飞行时间质谱技术测定了在紫外(355nm), 可见(560nm)和近代红外(1064nm)脉冲激光作用下, 氯分子束与Ti表面反应产物的质量分布和速度分布。所得结果表明, 不同波长激光诱导反应的主要产物相同, 有Ti, TiCl, TiCl3和TiCl4。在高能量密度的紫外激光作用下, 首次测得具有很高动能的原生Ti+。各种含Ti氯化物的飞行时间谱, 能满意地用单组分或多组分Maxwell-Boltzmann公式拟合和分析。上述激光诱导气-固表面反应的机理主要由氯分子在Ti表面上的解离吸附,吸附态氯原子在表面上生成TiClx(X=1~4)的连串反应以及激光诱导脱附所组成。近红外激光主要引起热脱附, 而紫外激光的作用还原可能有非热脱附过程。 相似文献
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本文测定了配合物3AgNO3·2BPrTE的晶体结构, 该晶体属三斜晶系, 空间各为PI,晶胞参数: a=0.8945(1), b=1.2355(2), c=1.3572(5)nm; α=98.69(2)°, β=92.74(2)°, γ=90.45(1)°; V=1.480nm^3; Z=2, 分子中三个Ag原子的配位数均为5, 但它们的配位多面体各不相同, Ag(3)为四方锥体, Ag(2)为三角双锥, Ag(1)则介于两者之间, NO3^-以单齿、不等长双齿和等长双齿两种形式配位于Ag原子。配体BPrTE也具有两种构象, 反式构象具有C1对称性, 并以两种形式和Ag原子配位, 偏转式构象不具有C4对称性, 与Ag原子形成五元螯合环, 分子为三维无限长链结构。 相似文献
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本文报道一个新的三核钼原子簇化合物在室温和77K固态和液态的EPR谱,这些谱均呈现出a,b两套谱线的叠加,分析谱线的强度比,线宽和谱参数,认为g值较大的a谱归属于三核钼原子簇化合物,而b谱归属于单核钼杂质。从由X射线晶体结构方法确定的空间结构出发,三核钼原子簇化合物可能有两种分子形式:Mo3(μ3-S)(μ2-S)3Cl[S2P(OEt)2]4 1Mo3(μ3-S)(μ2-S)(μ2-Cl)2Cl[S2P(OEt)2]4 2分别用简单量子化学理论和EHMO法计算出未配对电子所处的分子轨道,求出g1和g1,并与EPR实验值相比较,认为该化合物的分子式应为2,簇骼{Mo3}属七电子体系,在77K温度下,其未配对电子主要局域在三个钼原子所组成的近似等腰三角形簇骼的顶点钼原子周围。 相似文献
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