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arXiv 0807.3614astro-ph
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用射电干涉仪重建HI功率谱研究暗能量

Reconstruction of HI power spectra with radio-interferometers to study dark energy

R. Ansari, J. -M. Le Goff, Ch. Magneville, M. Moniez, N. Palanque-Delabrouille, J. Rich, V. Ruhlmann-Kleider, Ch. Yèche

摘要:

在研究推动宇宙膨胀的暗能量的工具中,重子声学振荡(BAO)及其对物质功率谱的影响尤其引人注目。最近有人提出通过在红移范围$0.5<z<3$中绘制中性氢的21 cm发射来研究这些振荡。我们在这里讨论的精度,这种测量使用无线电干涉仪阵列的碟形或南北方向的圆柱。然后,我们讨论了由此产生的不确定性的BAO尺度和灵敏度的暗能量状态方程的参数。

英文摘要:

Among the tools available for the study of the dark energy driving the expansion of the Universe, Baryon Acoustic Oscillations (BAO) and their effects on the matter power spectrum are particularly attractive. It was recently proposed to study these oscillations by mapping the 21cm emission of the neutral hydrogen in the redshift range $0.5<z<3$. We discuss here the precision of such measurements using radio-interferometers consisting of arrays of dishes or north-south oriented cylinders. We then discuss the resulting uncertainties on the BAO scales and the sensitivity to the parameters of the Dark Energy equation of state.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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