宇宙学

The Big Bang theory is the most widely accepted cosmological explanation for the origin of the universe.
大爆炸理论是关于宇宙起源最被广泛接受的宇宙学解释。
Cosmologists study the large-scale structure of the universe and its evolution over time.
宇宙学家研究宇宙的大尺度结构及其随时间的演化。
Dark matter and dark energy are key components in contemporary cosmology, shaping the universe's structure.
暗物质和暗能量是当代宇宙学中的关键组成部分，塑造着宇宙的结构。
The cosmic microwave background radiation is a remnant from the early universe, providing crucial evidence for the Big Bang model.
宇宙微波背景辐射是早期宇宙的遗迹，为大爆炸模型提供了关键证据。
The expansion of the universe, as demonstrated by Hubble's law, is a fundamental concept in cosmology.
哈勃定律所展示的宇宙膨胀是宇宙学中的一个基本概念。
String theory offers a potential unification of quantum mechanics and cosmology, but it remains highly speculative.
弦理论提供了量子力学与宇宙学可能统一的途径，但仍然高度推测性。
The multiverse hypothesis suggests that our observable universe is just one of many within an infinite cosmos.
多重宇宙假说认为我们可观测的宇宙只是无限宇宙中众多宇宙之一。
Cosmic inflation, a rapid expansion shortly after the Big Bang, helps explain the universe's uniformity on a large scale.
宇宙膨胀是指大爆炸后迅速的扩张，它有助于解释宇宙在大尺度上的均匀性。
Black holes, despite their local gravitational intensity, play a role in shaping galaxies, a subject of interest in cosmology.
尽管黑洞具有强大的局部引力，它们在塑造星系的过程中扮演着角色，这是宇宙学研究的一个兴趣点。
Gravitational waves, detected by LIGO, provide a new way to observe and understand the cosmos, especially events like merging black holes.
通过LIGO探测到的引力波为观察和理解宇宙提供了新途径，特别是像黑洞合并这样的事件。