五维几何真空诱导的具有衰减宇宙函数$Λ(t)$的幻影宇宙学
Phantom cosmology with a decaying cosmological function $Λ(t)$ induced from five-dimensional (5D) geometrical vacuum
摘要:
从5维Riemann平坦度规出发,以几何方式引入一个可变的宇宙学函数$Λ(t)$,研究了对于每一个能够产生幻影宇宙学的4维动力学超曲面,是否有一个几何准则来选择一个合适的宇宙学函数$Λ(t)$.
英文摘要:
Introducing a variable cosmological function $Λ(t)$ in a geometrical manner from a 5D Riemann-flat metric, we investigate the possibility of having a geometrical criterion to choose a suitable cosmological function $Λ(t)$ for every 4D dynamical hypersurface capable of generate phantom cosmologies.
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