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The Dark Age… before the stars, beyond the galaxies…
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Overview of history of Universe …
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The Dark Age … How do you study neutral hydrogen?
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??? How do you find H clouds ??? ??? How do you find HI clouds ???
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Dutch Westerbork Telescope
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Comparison: Hubble, Radio, very deep optical from ground
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Energy Levels in Hydrogen E = 0 Ground State Energy Lyman Balmer Paschen
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Emission Lines: from Photoionization Lyman alpha
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Energy Levels in Hydrogen E = 0 Ground State Energy free electron Photo- ionization Recombination radiative decay
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Energy Levels in Hydrogen E = 0 Ground State Energy To excite optical & UV lines …need at least 10.2 eV Hot Stars Quasars
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Energy Levels in Hydrogen E = 0 Ground State Energy Hyperfine splitting of H ground state 21 cm line E = 6 x 10 eV -6-6 thermally excited by collisions in cold gas
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Comparison: Hubble, Radio, very deep optical from ground
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Blue galaxies => young, massive stars
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Red galaxies… What makes them RED ??? red stars redshift “reddening” (dust)
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The `microwave sky’ (all sky picture from WMAP map.gfsc.nasa.gov)
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WMAP:
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The `microwave sky’ (all sky picture)
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from Jordi Miralda-Escude 2003, Science, 300, 1904 1 10 100 1000 1 + Z Age of Universe [years] 10 10 10 9 10 8 10 7 10 6
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The CMB
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Gnedin’s simulation of Reionization: log(Neutral fraction) log(density) log T log(mean intensity of ionizing flux) http://casa.colorado.edu/~gnedin/GALLERY/
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Energy Levels in Hydrogen E = 0 Ground State Energy free electron Photo- ionization Recombination radiative decay
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High Z SDSS Quasar (Fan et al 2002) Gunn-Peterson Trough
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Lyman Alpha Moderate Z Quasar Highest Z Quasar
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Cut off from view of optical wavelengths !!! n HI n HI +n HII 10 -3 If neutral fraction >
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Square Kilometre Array
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ARRAY Simple antenna “elements” “Station” “Array”
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D Sensivity depends on collecting area Angular resolution ~ /D
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D Sensivity depends on collecting area Angular resolution ~ /D
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VLA ALMA ESO VLTI
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ARRAY Simple antenna “elements” “Station” “Array”
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SKA Design “Magic Carpet”
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Eggs on Legs
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LOFAR = Low Frequency Array
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on map of the Netherlands
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10 arcmin LOFAR and SKA … Quasar distributed star formation
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LOFAR and SKA … Z = 13.5 12.8 12.0 11.3 10.6 9.9 9.3 8.7 8.1 log( neutral fraction ) Ciardi & Madau 2003
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