the dark age… before the stars, beyond the galaxies…

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

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

The Dark Age…

before the stars, beyond the galaxies…

Page 2: The Dark Age… before the stars, beyond the galaxies…

Overview of history of Universe …

Page 3: The Dark Age… before the stars, beyond the galaxies…

The Dark Age … How do you study neutral hydrogen?

Page 4: The Dark Age… before the stars, beyond the galaxies…

??? How do you find H clouds ???

??? How do you find HI clouds ???

Page 5: The Dark Age… before the stars, beyond the galaxies…
Page 6: The Dark Age… before the stars, beyond the galaxies…
Page 7: The Dark Age… before the stars, beyond the galaxies…

Dutch Westerbork Telescope

Page 8: The Dark Age… before the stars, beyond the galaxies…

Comparison: Hubble, Radio, very deep optical from ground

Page 9: The Dark Age… before the stars, beyond the galaxies…

Energy Levels in Hydrogen

E = 0

Ground State

En

erg

y

Lyman

BalmerPaschen

Page 10: The Dark Age… before the stars, beyond the galaxies…

Emission Lines: from Photoionization

Lymanalpha

Page 11: The Dark Age… before the stars, beyond the galaxies…

Energy Levels in Hydrogen

E = 0

Ground State

En

erg

yfree electron

Photo-ionization

Recombination

radiative decay

Page 12: The Dark Age… before the stars, beyond the galaxies…

Energy Levels in Hydrogen

E = 0

Ground State

En

erg

y To excite optical & UV lines …need at least 10.2 eV

• Hot Stars• Quasars

Page 13: The Dark Age… before the stars, beyond the galaxies…

Energy Levels in Hydrogen

E = 0

Ground State

En

erg

y

Hyperfine splitting of H ground state

21 cm line

E = 6 x 10 eV-6

thermally excited by collisions in cold gas

Page 14: The Dark Age… before the stars, beyond the galaxies…

Comparison: Hubble, Radio, very deep optical from ground

Page 15: The Dark Age… before the stars, beyond the galaxies…
Page 16: The Dark Age… before the stars, beyond the galaxies…
Page 17: The Dark Age… before the stars, beyond the galaxies…
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Blue galaxies=> young, massive stars

Page 26: The Dark Age… before the stars, beyond the galaxies…

Red galaxies…

What makes them RED ???

• red stars• redshift• “reddening” (dust)

Page 27: The Dark Age… before the stars, beyond the galaxies…

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

Page 28: The Dark Age… before the stars, beyond the galaxies…

WMAP:

Page 29: The Dark Age… before the stars, beyond the galaxies…

The `microwave sky’ (all sky picture)

Page 30: The Dark Age… before the stars, beyond the galaxies…

from Jordi Miralda-Escude 2003, Science, 300, 1904

1 10 100 10001 + Z1 + Z

Age of Universe [years] 1010 109 108 107 106

Page 31: The Dark Age… before the stars, beyond the galaxies…

The CMB

Page 32: The Dark Age… before the stars, beyond the galaxies…
Page 33: The Dark Age… before the stars, beyond the galaxies…

Gnedin’s simulation of Reionization:

log(Neutral fraction)

log(density)log T

log(mean intensity of ionizing flux)

http://casa.colorado.edu/~gnedin/GALLERY/

Page 34: The Dark Age… before the stars, beyond the galaxies…

Energy Levels in Hydrogen

E = 0

Ground State

En

erg

yfree electron

Photo-ionization

Recombination

radiative decay

Page 35: The Dark Age… before the stars, beyond the galaxies…

High Z SDSS Quasar (Fan et al 2002)

Gunn-Peterson Trough

Page 36: The Dark Age… before the stars, beyond the galaxies…

Lyman AlphaModerate Z Quasar

Highest Z Quasar

Page 37: The Dark Age… before the stars, beyond the galaxies…

Cut off fromview of opticalwavelengths !!!

nHI

nHI +nHII 10-3

If neutral fraction

>

Page 38: The Dark Age… before the stars, beyond the galaxies…

SquareKilometreArray

Page 39: The Dark Age… before the stars, beyond the galaxies…

ARRAY

Simple antenna“elements”

“Station” “Array”

Page 40: The Dark Age… before the stars, beyond the galaxies…

D

Sensivity depends on collecting area

Angular resolution

~ /D

Page 41: The Dark Age… before the stars, beyond the galaxies…

D

Sensivity depends on collecting area

Angular resolution

~ /D

Page 42: The Dark Age… before the stars, beyond the galaxies…

VLA

ALMAESO VLTI

Page 43: The Dark Age… before the stars, beyond the galaxies…

ARRAY

Simple antenna“elements”

“Station” “Array”

Page 44: The Dark Age… before the stars, beyond the galaxies…

SKA Design“Magic Carpet”

Page 45: The Dark Age… before the stars, beyond the galaxies…

Eggs on Legs

Page 46: The Dark Age… before the stars, beyond the galaxies…

LOFAR = Low Frequency Array

Page 47: The Dark Age… before the stars, beyond the galaxies…

on map of theNetherlands

Page 48: The Dark Age… before the stars, beyond the galaxies…

10 arcmin

LOFAR and SKA …

QuasarQuasardistributeddistributedstar formationstar formation

Page 49: The Dark Age… before the stars, beyond the galaxies…

LOFAR and SKA …

Z = 13.5 12.8 12.0

11.3 10.6 9.9

9.3 8.7 8.1

log(

neutr

al fr

act

ion

)

Ciardi & Madau 2003