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首页> 外文期刊>Physical review letters >Predictions for the Sky-Averaged Depth of the 21 cm Absorption Signal at High Redshift in Cosmologies with and without Nonbaryonic Cold Dark Matter
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Predictions for the Sky-Averaged Depth of the 21 cm Absorption Signal at High Redshift in Cosmologies with and without Nonbaryonic Cold Dark Matter

机译:在有和没有非重子冷暗物质的宇宙学中,高红移时21 cm吸收信号的天空平均深度的预测

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摘要

We consider the 21 cm absorption signal expected at high redshift in cosmologies with and without nonbaryonic cold dark matter. The expansion of the early Universe decelerates strongly with dark matter, but approximately coasts without it. This results in a different path length across the epochs when absorption is expected, with the consequence that the absorption is predicted to be a factor of similar to 2 greater without dark matter than with it. Observation of such a signal would motivate consideration of extended theories of gravity in lieu of dark matter.
机译:我们考虑在有和没有非重子冷暗物质的宇宙学中预期在高红移下的21 cm吸收信号。早期宇宙的膨胀在暗物质的作用下急剧减速,但在没有暗物质的情况下大约会滑行。当期望吸收时,这导致跨历元的路径长度不同,结果是,与暗物质相比,暗物质的吸收被预测为大两倍。观察这种信号将促使人们考虑扩展引力理论来代替暗物质。

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  • 来源
    《Physical review letters》 |2018年第8期|081305.1-081305.7|共7页
  • 作者

    McGaugh Stacy S.;

  • 作者单位

    Case Western Reserve Univ, Dept Astron, 10900 Euclid Ave, Cleveland, OH 44106 USA;

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  • 正文语种 eng
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