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Swiss-cheese model of the cosmos full of holes

机译:充满孔洞的宇宙的瑞士奶酪模型

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A Universe riddled with holes would do away with the need for dark energy. Unfortunately that idea itself now seems to have a few holes. In 1998, astronomers found that distant supernovae were dimmer, and thus farther away, than expected. According to the standard model of cosmology, which assumes that the universe is homogenous on large scales, this suggested that the expansion of the universe was speeding up. That acceleration was attributed to a mysterious "dark energy" inherent in the fabric of space-time. Then, last year, Edward Kolb of the Fermi National Accelerator Laboratory in Batavia, Illinois, and colleagues re-examined the supernovae data in the context of the "Swiss-cheese" model, which assumes the universe is full of holes or voids with less matter than other regions. It was inspired by the accidental discovery of a giant void about 1 billion light years across. The astronomers who discovered the supernovae anomaly in the late 1990s had assumed that matter was distributed more or less evenly. But in the Swiss-cheese model, less dense regions would act as a concave lens, bending part of the light from a distant object away from us. Therefore supernova light that travelled through a series of such voids would appear dimmer than expected without the need to invoke dark energy.
机译:一个充满孔洞的宇宙将消除对暗能量的需求。不幸的是,这个想法本身现在似乎有一些漏洞。 1998年,天文学家发现遥远的超新星比预期的要暗,因此距离更远。根据宇宙学的标准模型,该模型假定宇宙在很大程度上是同质的,这表明宇宙的膨胀正在加速。这种加速归因于时空结构中固有的神秘“暗能量”。然后,去年,伊利诺伊州巴达维亚费米国家加速器实验室的爱德华·科尔布及其同事在“瑞士奶酪”模型的背景下重新检查了超新星数据,该模型假定宇宙充满了较少的孔洞或空隙比其他地区重要。它的灵感来自偶然发现的大约10亿光年的巨大空洞。在1990年代后期发现超新星异常的天文学家已经假设物质或多或少是均匀分布的。但是在瑞士奶酪模型中,密度较小的区域将充当凹面透镜,将来自遥远物体的一部分光弯曲到远离我们的位置。因此,穿过一系列此类空洞的超新星光将显得比预期的更暗,而无需调用暗能量。

著录项

  • 来源
    《New scientist》 |2008年第2678期|11|共1页
  • 作者

    Anil Ananthaswamy;

  • 作者单位
  • 收录信息 美国《科学引文索引》(SCI);美国《化学文摘》(CA);
  • 原文格式 PDF
  • 正文语种 eng
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  • 关键词

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