combining different measurements
DESCRIPTION
Combining Different Measurements. Bob Nichol, ICG Portsmouth Tommaso Giannantonio, H-J Seo, Dan Carson , Hubert Lampeitl *, Josh Frieman, Bruce Bassett, Mat Smith, Will Percival (for SDSS Collaboration). * see poster. BAO with Redshift. Measure ratio of volume averaged distance - PowerPoint PPT PresentationTRANSCRIPT
Combining Different Measurements
Bob Nichol, ICG PortsmouthBob Nichol, ICG PortsmouthTommaso Giannantonio, H-J Seo, Tommaso Giannantonio, H-J Seo, Dan Dan
CarsonCarson, , Hubert LampeitlHubert Lampeitl*, Josh *, Josh Frieman, Bruce Bassett, Mat Smith, Will Frieman, Bruce Bassett, Mat Smith, Will
PercivalPercival
(for SDSS Collaboration)(for SDSS Collaboration)
* see poster
BAO with Redshift
99.74% detection
Percival et al. (2006)
143k + 465k
79kz~0.35
z~0.2
Percival et al. 2007
Measure ratio of volume averaged distance
D0.35 /D0.2 = 1.812 ± 0.060
Flat CDM = 1.67
Systematics (damping, BAO fitting) also ~1Next set of measurements will need to worry about this
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Dv(z) =(1+ z)2czDA(z)2
H (z)
⎡
⎣ ⎢
⎤
⎦ ⎥
1
3
Cosmological Constraints
w=
P/
m
Only D0.35 /D0.2
With CMB
Flatness assumed, constant w
Favors w<-1 at 1.4
W
Cosmological Constraints
1
2
3
W
m
Only D0.35 /D0.2
With CMB
Flatness assumed
W
m
m = 0.249 ± 0.018
w = -1.004 ± 0.089
D0.35 /D0.2 = 1.66 ± 0.01
w=
P/
Discrepancy?
• 2.4 difference between SN & BAO. The BAO want more acceleration at z<0.3 than predicted by z>0.3 SNe
• ~1 possible from details of BAO damping - more complex then we thought
• Assumption of flatness and constant w needs to be revisited
Revisit with SDSS SNeOnly look at measurements at z<0.4
500 Ia’s 102 from 05 LCDM line 2 contours q0 = -0.34 (2)
SDSS BAO points
Cosmological ConstraintsOnly look at measurements at z<0.4
ISW (z<0.4) Peacock et al
SDSS BAO points
W SNe
BAO
Flat wCDM
w= -1 (15% stat & sym)
CurvatureOnly look at measurements at z<0.4
ISW (z<0.4) Peacock et al
Distance DualityReturning to BAO and SN discrepancy?
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DL = (1+ z)2+2α DA
Cosmic ChronometersAge of galaxies constraints age of universe (Jimenez & Loeb 2002)
5500 LRGs
Carson et al. (in prep)
(Using Thomas et al. models, marginalised over alpha-enhancement and metallicity)
Cosmic Chronometers IIAge of galaxies constraints age of universe (Jimenez & Loeb 2002)
raw t(z) HST TSR
ISW WMAP
ALL FLAT
Differential Ages H(z)
We find H(z=0.2) ~ 80 +/- 12 km/s
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H(z) =1
(1+ z)
dz
dt
Same value as Gaztanaga et al. but not yet competitive in error
Conclusions
• Tension remains between BAO and SN (over same redshift range). But ~2 at best
• Cosmic Chronometers provide constraints on age-redshift relation (thus h and m). Also provide constraints on H(z) but not yet competitive
• BOSS could do much better, especially if we can do better on the stellar modeling (Maraston et al.)