Abstract
The antisymmetric part of two-point cross-correlation between intensity maps
of the HI 21 cm line and the CO 2.61 mm line has emerged as a new probe of
cosmic reionization. In this Letter we demonstrate that the slope of the dipole
of HI-CO cross-power spectrum at large scales is linear to the rate of change
of global neutral fraction of hydrogen in a model-independent way, until the
slope levels out near the end of reionization. The HI-CO dipole, therefore, can
be a smoking-gun probe for the speed of reionization, or "standard
speedometer". Observations of this new signal will unveil the global
reionization history from the midpoint to near the completion of reionization.
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