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The Dark Age… before the stars, beyond the galaxies…

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Presentation on theme: "The Dark Age… before the stars, beyond the galaxies…"— Presentation transcript:

1 The Dark Age… before the stars, beyond the galaxies…

2 Overview of history of Universe …

3 The Dark Age … How do you study neutral hydrogen?

4 ??? How do you find H clouds ??? ??? How do you find HI clouds ???

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7 Dutch Westerbork Telescope

8 Comparison: Hubble, Radio, very deep optical from ground

9 Energy Levels in Hydrogen E = 0 Ground State Energy Lyman Balmer Paschen

10 Emission Lines: from Photoionization Lyman alpha

11 Energy Levels in Hydrogen E = 0 Ground State Energy free electron Photo- ionization Recombination radiative decay

12 Energy Levels in Hydrogen E = 0 Ground State Energy To excite optical & UV lines …need at least 10.2 eV Hot Stars Quasars

13 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

14 Comparison: Hubble, Radio, very deep optical from ground

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25 Blue galaxies => young, massive stars

26 Red galaxies… What makes them RED ??? red stars redshift “reddening” (dust)

27 The `microwave sky’ (all sky picture from WMAP map.gfsc.nasa.gov)

28 WMAP:

29 The `microwave sky’ (all sky picture)

30 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

31 The CMB

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33 Gnedin’s simulation of Reionization: log(Neutral fraction) log(density) log T log(mean intensity of ionizing flux) http://casa.colorado.edu/~gnedin/GALLERY/

34 Energy Levels in Hydrogen E = 0 Ground State Energy free electron Photo- ionization Recombination radiative decay

35 High Z SDSS Quasar (Fan et al 2002) Gunn-Peterson Trough

36 Lyman Alpha Moderate Z Quasar Highest Z Quasar

37 Cut off from view of optical wavelengths !!! n HI n HI +n HII  10 -3 If neutral fraction >

38 Square Kilometre Array

39 ARRAY Simple antenna “elements” “Station” “Array”

40 D Sensivity depends on collecting area Angular resolution ~ /D

41 D Sensivity depends on collecting area Angular resolution ~ /D

42 VLA ALMA ESO VLTI

43 ARRAY Simple antenna “elements” “Station” “Array”

44 SKA Design “Magic Carpet”

45 Eggs on Legs

46 LOFAR = Low Frequency Array

47 on map of the Netherlands

48 10 arcmin LOFAR and SKA … Quasar distributed star formation

49 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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