Polarization Signals of the 21 cm Background from the Era of Reionization

Details Polarization Signals of the 21 cm Background from the Era of Reionization Polarization Signals of the 21 cm Background from the Era of Reionization

2004-08-17

arxiv.org/abs/astro-ph/0408314v1

Mon.Not.Roy.Astron.Soc. 359 (2005) L47-L52

Astronomy and Astrophysics

Astrophysics

6 pages, 2 figures, submitted to MNRAS

Scientific paper

10.1111/j.1745-3933.2005.00035.x

While emission and absorption lines of the 21 cm spin-flip transition of neutral Hydrogen are intrinsically unpolarized, a magnetic field creates left- and right-handed polarized components through the Zeeman effect. Here we consider the resulting polarization of the redshifted 21 cm background from the intergalactic medium before reionization. The polarization is detectable in regions with a strong gradient in the mean brightness temperature. In principle, this can open a new window on the evolution of intergalactic magnetic fields. One possible approach is an extended integration of an individual target during this era, such as the Mpc-scale HII regions inferred to surround quasars at z ~ 6.5. The differential intensity between the two polarization states can be used as a probe of the magnetic field at the edge of the HII region. We estimate that the SKA could (ignoring systematics) detect B \~ 200 (10) \muG coherent over several kiloparsecs with an observational bandwidth of 100 (2) kHz. Beyond individual sources, the statistical properties of wide-field 21 cm polarization maps, such as the angular power spectrum, can be used to constrain the large-scale magnetic field. In this case, the SKA can detect $B \sim 100 \mu$G fields coherent over many megaparsecs. The magnetic field can be measured in any epoch over which the 21 cm background changes rapidly (for example because the ionized fraction or spin temperature change). Although the resulting constraints with SKA are relatively weak compared to theoretical expectations, they nevertheless offer a unique direct probe of magnetic fields in the high-redshift universe.

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