共查询到20条相似文献,搜索用时 0 毫秒
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Research over the past 25 years has led to the view that the rich tapestry of present-day cosmic structure arose during the first instants of creation, where weak ripples were imposed on the otherwise uniform and rapidly expanding primordial soup. Over 14 billion years of evolution, these ripples have been amplified to enormous proportions by gravitational forces, producing ever-growing concentrations of dark matter in which ordinary gases cool, condense and fragment to make galaxies. This process can be faithfully mimicked in large computer simulations, and tested by observations that probe the history of the Universe starting from just 400,000 years after the Big Bang. 相似文献
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在王锡阐(1628—1682年)有关天体运行的3篇文献《历说.五》、《日月左右旋问答》和《五星行度解》的基础上,分析了王锡阐改上三星本天之行为左旋的原因,揭示了《晓庵新法》中以地心为心的五星运动模型和《五星行度解》中的类第谷体系之间的关系,探讨了王锡阐对第谷模型进行修正的原因。 相似文献
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贫金属星对于我们了解元素起源和宇宙的化学演化具有关键意义。本文将描述这些稀有天体的发现历史,分析它们的光谱确定其表面化学丰度的方法,以及如何利用它们的丰度模式来阐释其起源与演化。 相似文献
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根据爱因斯坦广义相对论,时空弯曲,宇宙是有限的。现在已被主流物理学家普遍接受的是标准宇宙论,按标准宇宙论经过严格的数学推导,演算得到了宇宙的年龄、宇宙物质密度。作者根据广大天体物理工作者认可的观察数据和结论,通过初等数学的计算,得到的结果大相径庭。根本没天体物工作者寻找的暗物质。 相似文献
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梁英贤 《重庆邮电学院学报(自然科学版)》1999,11(1):41-43
宇宙中存在各类天体,它们都在一定条件下处于平衡状态,才使得宇宙具有一定的结构。星体主要是受引力,电力,热压力,简并压力等4种因素的支配平衡。 相似文献
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本文将虚数引入太极宇宙模型并建立起太极宇宙模型的数学模式,利用现代宇宙学研究成果验证可见宇宙在太极宇宙模型中的适用性,同时应用哲学语言论证太极宇宙模型所表述的哲学宇宙精神. 相似文献
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在广义相对论的基础上,可以研究宇宙的时空演化。宇宙的极早期会有一个暴胀时期,在这个时期内会产生影响宇宙大尺度结构的密度扰动。本论文讨论彩虹引力下的暴胀模型,导出了度规场和标量场的扰动方程,分析了密度扰动随时间变化的性质。通过求解功率谱,发现彩虹宇宙里功率谱的标度不变性依然保持。谱指数与标准暴胀型中一致,但是其功率谱的幅值缺与探测粒子的能量有关。 相似文献
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Supernova explosions in the Universe 总被引:1,自引:0,他引:1
During the lifetime of our Milky Way galaxy, there have been something like 100 million supernova explosions, which have enriched the Galaxy with the oxygen we breathe, the iron in our cars, the calcium in our bones and the silicon in the rocks beneath our feet. These exploding stars also influence the birth of new stars and are the source of the energetic cosmic rays that irradiate us on the Earth. The prodigious amount of energy (approximately 10(51), or approximately 2.5 x 10(28) megatonnes of TNT equivalent) and momentum associated with each supernova may even have helped to shape galaxies as they formed in the early Universe. Supernovae are now being used to measure the geometry of the Universe, and have recently been implicated in the decades-old mystery of the origin of the gamma-ray bursts. Together with major conceptual advances in our theoretical understanding of supernovae, these developments have made supernovae the centre of attention in astrophysics. 相似文献