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arxiv: 0709.3672 · v2 · submitted 2007-09-23 · 🌌 astro-ph

Baryon Acoustic Oscillation Intensity Mapping as a Test of Dark Energy

classification 🌌 astro-ph
keywords darkenergyacousticmappingbaryonintensityoscillationtest
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The expansion of the universe appears to be accelerating, and the mysterious anti-gravity agent of this acceleration has been called ``dark energy''. To measure the dynamics of dark energy, Baryon Acoustic Oscillations (BAO) can be used. Previous discussions of the BAO dark energy test have focused on direct measurements of redshifts of as many as $10^9$ individual galaxies, by observing the 21cm line or by detecting optical emission. Here we show how the study of acoustic oscillation in the 21 cm brightness can be accomplished by economical three dimensional intensity mapping. If our estimates gain acceptance they may be the starting point for a new class of dark energy experiments dedicated to large angular scale mapping of the radio sky, shedding light on dark energy.

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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Mapping Cosmological Signal Scales to Beam Calibration Requirements in 21cm Experiments and Implications for Near-Field Measurement

    astro-ph.IM 2026-05 unverdicted novelty 6.0

    New method maps 21cm cosmological structures to ~100m reflection scales for HERA-like and EDGES-like instruments, showing near-field beam calibration is required.