论文标题

观察者引起的边界条件引起的宇宙常数

Cosmological constant caused by observer-induced boundary condition

论文作者

Stenflo, Jan O.

论文摘要

量子力学中波函数的演变是确定性的,例如经典波的。只有当我们引入观察者时,根本上不同的量子现实才会出现。同样,观察者的引入改变了时空的性质,从而导致过去和未来之间的分歧,这些概念在无观察者的世界中没有很好地定义。诱导的时间边界导致欧几里得时间中度量的振荡真空溶液的共振条件。它对应于实时的指数de Sitter进化,可以用宇宙常数$λ=2π^2/r_u^2 $表示,其中$ r_U $是观察者存在时粒子范围的半径。对于当前时期,我们获得了$λ$的值,该值与观测错误的$2σ$内的观察值一致。这种解释解决了宇宙的巧合问题。我们在宇宙历史上的时代并没有预示着由黑暗能量驱动的通货膨胀阶段的开始。我们表明,由于观察者诱导的边界而不能代表固有进化,从红移推导的观察到的加速膨胀是“边缘效应”。新理论满足了BBN(大爆炸核合成)和CMB(宇宙微波背景)观测约束与标准宇宙学的一致性模型一样好。暗能量与暗物质问题之间没有联系。先前的结论是,暗物质主要是非巴里元的。

The evolution of the wave function in quantum mechanics is deterministic like that of classical waves. Only when we bring in observers the fundamentally different quantum reality emerges. Similarly the introduction of observers changes the nature of spacetime by causing a split between past and future, concepts that are not well defined in the observer-free world. The induced temporal boundary leads to a resonance condition for the oscillatory vacuum solutions of the metric in Euclidean time. It corresponds to an exponential de Sitter evolution in real time, which can be represented by a cosmological constant $Λ=2π^2/r_u^2$, where $r_u$ is the radius of the particle horizon at the epoch when the observer exists. For the present epoch we get a value of $Λ$ that agrees with the observed value within $2σ$ of the observational errors. This explanation resolves the cosmic coincidence problem. Our epoch in cosmic history does not herald the onset of an inflationary phase driven by some dark energy. We show that the observed accelerated expansion that is deduced from the redshifts is an "edge effect" due to the observer-induced boundary and not representative of the intrinsic evolution. The new theory satisfies the BBN (Big Bang nucleosynthesis) and CMB (cosmic microwave background) observational constraints equally well as the concordance model of standard cosmology. There is no link between the dark energy and dark matter problems. Previous conclusions that dark matter is mainly non-baryonic are not affected.

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