论文标题
弹跳和崩溃的宇宙双重到后期的宇宙学模型
Bouncing and collapsing universes dual to late-time cosmological models
论文作者
论文摘要
我们使用Jordan Frame-Einstein框架对应关系来探索与宇宙学演变对比的双重宇宙。我们研究了爱因斯坦和约旦框架之间的映射,其中爱因斯坦框架宇宙描述了物理宇宙的晚期演变,该宇宙是由黑暗能量和非偏见的物质驱动的。 Brans-Dicke的重力理论被认为是约旦框架中的双重标量调整理论。我们表明,以$λ$ CDM模型的宇宙演化的爱因斯坦框架宇宙始终对应于由Brans-Dicke理论支配的弹跳的Jordan框架宇宙。另一方面,具有非相关物质成分的暗能量的典型模型被证明是对带有转弯的Brans-Dicke Jordan框架(即弹跳或倒塌)的双重偶。典型场状态方程的演变决定了转弯是弹跳还是倒塌。所有情况下的Jordan帧转弯点可以通过选择适当的Brans-Dicke参数来调节任何地方。这本质上导致了对物理宇宙的晚期演变的替代描述,这是在约旦框架中弹跳或崩溃的Brans-Dicke宇宙。因此,黑暗能量的效果可以等效地看作是在共同连接的宇宙中空间的崩溃。我们进一步研究了此类保形图对线性扰动的稳定性。当前加速宇宙的有效弹跳和崩溃描述可能对宇宙学背景中的扰动和量子波动的发展具有有趣的含义。
We use the Jordan frame-Einstein frame correspondence to explore dual universes with contrasting cosmological evolutions. We study the mapping between Einstein and Jordan frames where the Einstein frame universe describes the late-time evolution of the physical universe, which is driven by dark energy and non-relativistic matter. The Brans-Dicke theory of gravity is considered to be the dual scalar-tensor theory in the Jordan frame. We show that an Einstein frame universe, with cosmological evolution of the $Λ$CDM model, always corresponds to a bouncing Jordan frame universe governed by a Brans-Dicke theory. On the other hand, quintessence models of dark energy with non-relativistic matter component are shown to be always dual to a Brans-Dicke Jordan frame with a turn-around, i.e., a bounce or a collapse. The evolution of the equation of state of the quintessence field determines whether the turn-around is a bounce or a collapse. The point of the Jordan frame turn-around for all the cases can be tuned anywhere by choosing an appropriate Brans-Dicke parameter. This essentially leads to alternative descriptions of the late-time evolution of the physical universe, in terms of bouncing or collapsing Brans-Dicke universes in the Jordan frame. Therefore,the effect of dark energy can equivalently be seen as collapse of space in a conformally connected universe. We further study the stability of such conformal maps against linear perturbations. The effective bouncing and collapsing descriptions of the current accelerating universe may have interesting implications for the evolutions of perturbations and quantum fluctuations in the cosmological background.