首页> 外文期刊>International journal of modern physics, D. Gravitation, astrophysics, cosmology >The existence of an old quasar at z=3.91 and its implications for Lambda(t) deflationary cosmologies
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The existence of an old quasar at z=3.91 and its implications for Lambda(t) deflationary cosmologies

机译:z = 3.91的旧类星体的存在及其对Lambda(t)通缩宇宙学的影响

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摘要

We investigate some observational constraints on decaying vacuum cosmologies based on the recently discovered old high redshift quasar APM 08279+5255. This object is located at z = 3.91 and has an estimated age of 2-3 Cyr. The class of Lambda(t) cosmologies is characterized by a positive beta parameter smaller than unity which quantifies the ratio between the vacuum and the total energy density. Assuming the lower limit age (2 Gyr) and that the cold dark matter contributes with Omega(M) = 0.2 we show that beta is constrained to be greater than or equal to 0.07 while for an age of 3 Cyr and Omega(M) = 0.4 the beta parameter must be greater than 0.32. Our analysis includes closed, flat and hyperbolic scenarios, and it strongly suggests that there is no age crisis for this kind of A(t) cosmologies. Lower limits to the redshift quasar formation are also briefly discussed to the flat case. For Omega(M) = 0.4 we found that the redshift formation is constrained by z(f) greater than or equal to 8.0.
机译:我们基于最近发现的旧的高红移类星体APM 08279 + 5255,研究了对衰变真空宇宙学的一些观测约束。该对象位于z = 3.91,估计年龄为2-3 Cyr。 Lambda(t)宇宙论的特征是小于β的正β参数,该参数量化了真空与总能量密度之间的比率。假设下限年龄为(2 Gyr),并且寒冷的暗物质的贡献为Omega(M)= 0.2,则表明在3 Cyr和Omega(M)的年龄中,β被约束为大于或等于0.07。 0.4 beta参数必须大于0.32。我们的分析包括封闭的,平坦的和双曲线的情况,并且强烈暗示这种A(t)宇宙没有年龄危机。红移类星体形成的下限也针对平坦情况进行了简短讨论。对于Omega(M)= 0.4,我们发现红移形成受到z(f)大于或等于8.0的约束。

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