detecting the first light
DESCRIPTION
Detecting the first light. Han Jiaxin USTC,2007. http://2dark.org. Reionization. last scattering and CMB (300kyr,z~1100) Dark age reionisation(1Gyr,z~6) from first stars structure formation and expansion till present. Expanding and cooling…. Reionization Phases. UV reionization - PowerPoint PPT PresentationTRANSCRIPT
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Detecting the first light
Han Jiaxin
USTC,2007
http://2dark.org
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Reionization
last scattering and CMB (300kyr,z~1100)
Dark age reionisation(1Gyr,z~6) f
rom first stars structure formation and
expansion till present
Expanding and cooling…
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Reionization Phases
UV reionization StrÖmgren sphere Percolation / overlap Etching away
Open questions: Single epoch vs. Multiepoch (galaxy feedback,SF efficiency
…) Inside-out vs. Outside-in Reionization sources:X-ray,decaying particle…
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Methods of Observation
Lyα absorption Cosmic StrÖmgren Spheres Metal lines GRB CMB polarization and anisotropy 21cm line
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Lyα absorption
Lyα resonance absorption(1215.67A) UV
Continuous absorption at different z: Gun-Peterson trough
(Gun-Peterson 1965)
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Z<5: Lyman alpha forest (fluctuating GP effect)
Zem= 3.62 QSO1422C23 (V = 16.5) (Keck)
Z>5: overlap of lines, strong evolution
Z>6: complete trough, τ>>1,
Fallback: saturation
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Gun-Peterson Test
z~6: Dramatic decreas
e in transmitted flux
Increase in optical depth
Lya+Lyb+Lyr : phase transition
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Comparison with Simulations: overlap-postoverlap
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CMB Probes
Rescattering at Reionization Sensitive to Ionized fraction Testing Observables:
Large scale Polarization Small scale anisotropy
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CMB Probe:Polarization
τ-A degeneracy
Polarization: Low-l EE peak (larger horizon than recombination)
Not contaminated by ISW Future Observertions: Perce
nt level constraints on partial reionization
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CMB Probe:Polarization
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CMB Probe: B-mode pol
New low-l BB peak Gravitational lensing: E-->B More Stringent constraints on GW
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CMB Probe: Anisotropy
Patchy Reionization Secondary effects:
Ostriker-Vishniac effect:
Baryon Inhomogeneity Electron Inhomogeneity Kinetic SZ
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CMB Probe: kSZ
PGM Bulk velocitykSZ
Silk dampingtSZ domination at <4’
tSZ null(217GHz)
Te=10keV,y=10-4,Vpec=500km/s
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CMB Probe:Anisotropy
Small scales (<0.1deg,l>2000) Amplitude: duration of patchy phase No detection yet
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21cm
Direct measurement, 3D image No saturation
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21cm:Basics
Frequency:1420.4MHz,(200~9)MHz after redshift
Brightness Temperature
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21cm: Interplay with CMB
Z>200: Thompson scattering, collision TCMB=Tk=Ts, TB=0
Z:30~200 Tk~1/(1+z)2,TCMB~1/(1+z) TCMB>Tk=Ts, TB<0
Z:20~30 Local coupling by Lya, Local IGM warming by X-ray TB<0, TB=0, TB>0 regions
Z:6~20 Global IGM warming by first galaxy, BH Likely TCMB<Tk, TB>0
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21cm:Observation
Z=12 Z=9 Z=7
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21cm:Observation
Solid: density domination
Dotted: with reionization
Blue: SKA sensitivity
Red: LOFAR sensitivity
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21cm:Observational Challenges Foregrounds Ionosphere Interference
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Summary