cosmological reionization

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Cosmological Cosmological Reionization Reionization Nick Gnedin

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Cosmological Reionization. Nick Gnedin. Outline. The brief history of time What we know about reionization Reionization: ABC Data vs theory Conclusions. End of inflation: z=10 27 t=10 -36 s. Recombination: z=1089 t=379 kyr. Today: z=0 t=13.7 Gyr. neutral. ionized. ionized. - PowerPoint PPT Presentation

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Page 1: Cosmological Reionization

Cosmological ReionizationCosmological Reionization

Nick Gnedin

Page 2: Cosmological Reionization

OutlineOutline

•The brief history of time•What we know about reionization•Reionization: ABC•Data vs theory•Conclusions

Page 3: Cosmological Reionization

The Brief History of TimeThe Brief History of Time

Today:z=0

t=13.7 Gyr

End of inflation:z=1027

t=10-36s

Recombination:z=1089

t=379 kyrionized neutral ionized

RE-IONIZATIONRE-IONIZATION

Page 4: Cosmological Reionization

What We Know About What We Know About ReionizationReionization

Ly- Ly-

Page 5: Cosmological Reionization

What We Know About What We Know About Reionization: A or B?Reionization: A or B?

Sloanquasars

Frac

tion

of fl

uxtr

ansm

itted

“…the universe is approaching the reionization epoch at z~6”

(Becker et al. 2001)

Page 6: Cosmological Reionization

SimulationsSimulations

• dark matter dynamics• gas dynamics• star formation• metal cooling• exact physics of primeval plasma• fine print (secondary electrons, Ly- pumping, …)• radiative transfer

That’s the key!

the only phenomenology!

Note: non-existing things are not included

Page 7: Cosmological Reionization

Cosmological Parameters Cosmological Parameters 20032003

Baryons: 4%Dark matter: 23%Dark energy: 73%

Page 8: Cosmological Reionization

How It All Happens… How It All Happens…

GalaxiesHII regions

Neutral hydrogen

4 chimps

Page 9: Cosmological Reionization

How It All Happens… How It All Happens…

Page 10: Cosmological Reionization

How It All Happens: ABCHow It All Happens: ABCPre-overlap: HII regions

expand in the low density gas.

Overlap: HII regions merge – the moment of reionization.

Post-overlap: High density regions are being ionized from the outsize.

Page 11: Cosmological Reionization

Redshift of OverlapRedshift of OverlapPre-overlap

Overlap Post-overlap“A redshift of reionization”

Page 12: Cosmological Reionization

Redshift of OverlapRedshift of Overlap

zREI = 6.1 + 0.3 (2)

Page 13: Cosmological Reionization

WMAP modelWMAP model• Individual spectra of bright quasars are very similar to that of SLOAN quasars.• Large galaxies at z~4 have colors identical to observed Lyman Break Galaxies.• Star formation rate is consistent with observational measurements at z~4.• Smallest galaxies formed in the simulation look like dwarf spheroidals in all their properties, including abundance (no satellite problem).• Lyman-alpha forest (including metal absorption systems) is consistent with observations.• but …

Page 14: Cosmological Reionization

SLOAN quasarsSLOAN quasars

Page 15: Cosmological Reionization

Lyman-Break Galaxies Lyman-Break Galaxies Observed LB galaxies Simulated galaxies

L

Obs

erva

tions

Sim

ulat

ions

Page 16: Cosmological Reionization

Dwarf GalaxiesDwarf Galaxies

Real dwarfs

Virtual dwarfs

Page 17: Cosmological Reionization

Star FormationStar Formation

Page 18: Cosmological Reionization

MetallicityMetallicity

Page 19: Cosmological Reionization

KinematicsKinematics

Page 20: Cosmological Reionization

But But

= 0.17 = 0.06 = 0.17

Page 21: Cosmological Reionization

Conclusions IConclusions I• Reionization proceeds in 3 stages:• In the pre-overlap stage more-or-less isolated HII regions expand into the neutral IGM (bubbles of ionized gas in the sea of neutral gas). Measurement of high indicates that new physics was present in this stage. • During the overlap isolated HII regions merge together (looks like a mess). It happened at zREI = 6.1 + 0.3.

• In the post-overlap stage the remains of the neutral gas are being ionized from the outside – most of them become

Lyman-limit systems (bubbles of neutral gas in the sea of ionized gas).

Page 22: Cosmological Reionization

Conclusions IIConclusions II

• Our theoretical models reach the stage when we are able to make a quantitative comparison between theory and all existing observational data.• Future observations will be matched by the adequate progress in our abilities to model formation of early galaxies and supermassive black holes.• If this decade is a decade of CMB in astronomy, the next one will be a decade of reionization.

Page 23: Cosmological Reionization

The EndThe End

Page 24: Cosmological Reionization

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