宇宙学常数

探讨了有效宇宙学常数A（或总有效真空能密度ρv）的演化规律及它的存在与演化对宇宙演化不同阶段中各种参数的影响。

In this paper , we present a law of variation for the effective cosmological constant and discuss its affections to some cosmological parameters in different time-dependent phases of the cosmos .

我们证明了在诱导引力理论中Baby-Parent宇宙相互作用是非定域的，并论证了在低能极限下诱导的宇宙学常数为零。

We prove that the interactions between the baby-parent universes are non-local , and argue that the induced low-energy cosmological constant is zero .

应用Bulk时空流形对宇宙学常数的研究

The Research on Cosmological Constant Frome Bulk Spacetime Manifold

宇宙学常数与高红移星系观测

Cosmological constant and high redshift Galaxy observation

具有可变宇宙学常数的宇宙

The Cosmos With the Variable Cosmological Constant

本文用超空间方法对其有宇宙学常数的二维诱生引力进行量子化。

The two dimensional theory of induced gravity with cosmological constant is quantized in the superspace approach .

宇宙学常数疑难

The cosmological constant problem

宇宙学常数的物理学起源问题被视为现代物理中最重大的疑难之一。

The physical origin of the cosmological constant is considered to be one of the most difficult and important problems in modern physics .

然而现有物理学理论还无法给出合理的解释，因此宇宙学常数问题成为物理学和天文学上最重大的疑难之一。

However , the small cosmological constant and cosmic coincidence problem cannot be resolved within the known laws of physics , which is the famous cosmological constant problem in physics and astronomy .

对于当前宇宙学所面临的宇宙学常数问题，提出了一种新的解释。

We present the new explanation of the cosmological constant problem .