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White Noise from Dark Matter: 21 cm Observations of Early Baryon Collapse | Kathryn M. Zurek
; Craig J. Hogan
; | Date: |
26 Mar 2007 | Abstract: | In concordance cosmology, dark matter density perturbations generated by inflation lead to nonlinear, virialized minihalos, into which baryons collapse at redshift $z sim 20$. We survey here novel baryon evolution produced by a modification of the power spectrum from white noise density perturbations at scales below $k sim 10 h {Mpc}^{-1}$ (the smallest scales currently measured with the Lyman-$alpha$ forest). Exotic dark matter dynamics, such as would arise from scalar dark matter with a late phase transition (similar to an axion, but with lower mass), create such an amplification of small scale power. The dark matter produced in such a phase transition collapses into minihalos, with a size given by the dark matter mass within the horizon at the phase transition. If the mass of the initial minihalos is larger than $sim 10^{-3} M_odot$, the modified power spectrum is found to cause widespread baryon collapse earlier than standard $Lambda$CDM, leading to earlier gas heating. It also results in higher spin temperature of the baryons in the 21 cm line relative to $Lambda$CDM at redshifts $z > 20$ if the mass of the minihalo is larger than $1 M_odot$. It is estimated that experiments probing 21 cm radiation at high redshift will contribute a significant constraint on dark matter models of this type for initial minihalos larger than $sim 10 M_odot$. Early experiments reaching to $zapprox 15$ will constrain minihalos down to $sim 10^3 M_odot$. | Source: | arXiv, astro-ph/0703624 | Services: | Forum | Review | PDF | Favorites |
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