首页> 外文会议>International Meeting "The Sun, the Stars, the Universe, and General Relativity" >Stepanov Institute of physics of NAS of Belarus, Minsk, Belarus220072, Nezalezhnastsi Av., 68 Energy
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Stepanov Institute of physics of NAS of Belarus, Minsk, Belarus220072, Nezalezhnastsi Av., 68 Energy

机译:白俄罗斯州纳斯州NAS的Stepanov物理研究所,白俄罗斯220072,Nezalezhnastsi AV。,68个能量

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摘要

It is demonstrated that entropy and its density play a significant role in solving the problem of the vacuum energy density (cosmological constant) in the Universe and hence the dark energy problem. Taking this in mind, two most popular models for dark energy - Holographic Dark Energy Model and Agegraphic Dark Energy Model - are analyzed. It is shown that the fundamental quantities in the first of these models may be expressed in terms of a new small parameter. Besides, the results obtained on the uncertainty relation of the pair "cosmological constant - volume of space-time", where the cosmological constant is a dynamic quantity, are reconsidered and generalized up to the Generalized Uncertainty Relation (GUP).
机译:证明熵及其密度在解决宇宙中的真空能量密度(宇宙常数)的问题并因此发挥了重要作用。考虑到这一点,分析了两个最受欢迎的深度全息暗能模型和Edgraphic暗能模型的最受欢迎的模型。结果表明,这些模型中的基本量可以以新的小参数表示。此外,在对宇宙学常数为动态量的对“宇宙常数”的不确定关系中获得的结果被重新考虑并推广到广义不确定性关系(GUP)。

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