发表机构
University College London（伦敦大学学院）
机构由 AI 辅助整理，请以论文原文为准。AI 中文总结
本文评估了近期宇宙学观测对恒定宇宙学常数与动力学暗能量的证据强度，并展望了宇宙及其最神秘成分的未来理解。
AI 中文摘要
宇宙学常数 $\Lambda$ 及其推广形式暗能量，构成了当前宇宙约 70% 的能量密度，并且超过四分之一个世纪以来一直是占主导地位的 $\Lambda$CDM 宇宙学范式的一部分。然而，近期对星系成团性、Ia 型超新星以及宇宙微波背景的测量已将其置于审判之下。在本展望中，我们评估了近期发展背景下，支持恒定 $\Lambda$ 与动力学暗能量（DDE）的证据强度。我们还评估了未来对我们的宇宙以及我们对这一最神秘组成部分的理解而言将会带来什么。
英文摘要
The cosmological constant $Λ$, and its generalization as Dark Energy, makes up roughly 70% of the present-epoch universe and has been part of the dominant $Λ$CDM cosmological paradigm for more than a quarter of a century. It has been put on trial by recent measurements of galaxy clustering, Type Ia supernovae, and the cosmic microwave background. In this Perspective we evaluate the strength of the evidence for a constant $Λ$, versus Dynamical Dark Energy (DDE) in the light of recent developments. We also assess what the future holds both for our Universe and our understanding of its most mysterious component.
Comments15 pages, 1 Table, 1 Figure; a Perspective article accepted for publication by Nature Astronomy and to appear in the October 2026 issue
