28 research outputs found

    Cosmic histories of star formation and reionization: An analysis with a power-law approximation

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    With a simple power-law approximation of high-redshift (≳3.5\gtrsim3.5) star formation history, i.e., ρ˙∗(z)∝[(1+z)/4.5]−α\dot{\rho}_*(z)\propto [(1+z)/4.5]^{-\alpha}, we investigate the reionization of intergalactic medium (IGM) and the consequent Thomson scattering optical depth for cosmic microwave background (CMB) photons. A constraint on the evolution index α\alpha is derived from the CMB optical depth measured by the {\it Wilkinson Microwave Anisotropy Probe} (WMAP) experiment, which reads α≈2.18lg⁥Nγ−3.89\alpha\approx2.18\lg{\mathscr{N}_{\gamma}}-3.89, where the free parameter NÎł\mathscr{N}_\gamma is the number of the escaped ionizing ultraviolet photons per baryon. Moreover, the redshift for full reionization, zfz_f, can also be expressed as a function of α\alpha as well as NÎł\mathscr{N}_{\gamma}. By further taking into account the implication of the Gunn-Peterson trough observations to quasars for the full reionization redshift, i.e., 6â‰Čzfâ‰Č76\lesssim z_f \lesssim7, we obtain 0.3â‰Čαâ‰Č1.30.3\lesssim\alpha\lesssim1.3 and 80â‰ČNÎłâ‰Č23080\lesssim\mathscr{N}_{\gamma}\lesssim230. For a typical number of ∌4000\sim4000 of ionizing photons released per baryon of normal stars, the fraction of these photons escaping from the stars, fescf_{\rm esc}, can be constrained to within the range of (2.0−5.8)(2.0-5.8)%.Comment: 10 pages, 4 figures, accepted for publication in JCA

    Baryons: What, When and Where?

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    We review the current state of empirical knowledge of the total budget of baryonic matter in the Universe as observed since the epoch of reionization. Our summary examines on three milestone redshifts since the reionization of H in the IGM, z = 3, 1, and 0, with emphasis on the endpoints. We review the observational techniques used to discover and characterize the phases of baryons. In the spirit of the meeting, the level is aimed at a diverse and non-expert audience and additional attention is given to describe how space missions expected to launch within the next decade will impact this scientific field.Comment: Proceedings Review for "Astrophysics in the Next Decade: JWST and Concurrent Facilities", ed. X. Tielens, 38 pages, 10 color figures. Revised to address comments from the communit
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