constraining dark energy from large scale structures
DESCRIPTION
Constraining dark energy from large scale structures. Yipeng Jing Shanghai Astronomical Observatory. The “Hubble diagram” of Type Ia supernovae tells us that matter is not enough…. log( Distance d L ). a(t). Perlmutter et al. 1999, Riess et al. 1998. Redshift of spectral lines. - PowerPoint PPT PresentationTRANSCRIPT
Constraining Constraining dark energydark energy from from large scale structureslarge scale structures
Yipeng Jing
Shanghai Astronomical Observatory
Perlmutter et al. 1999, Riess et al. 1998
The “Hubble diagram” of Type Ia supernovae tells us that matter is not enough…
log(
Dis
tanc
e d L
)lo
g(D
ista
nce
d L)
dL (1 z)c dz'
H(z',m , )0
z
Redshift of spectral lines Redshift of spectral lines
H Ý a
a
a(t)
Luigi Guzzo
Cosmic ConcordanceCosmic Concordance
Large-Scale Structure/Clusters
•m =0.25-0.3
Cosmic Microwave Background
• Flat geometry (TOT=1)
• m ~0.25 > 0
Supernovae
Accelerating expansion
• ~ 1
Altogether (any two of them)
• m ~0.25 ~0.75
1990 Dec Nature, 348,20
Matter (m)
Dark energy (
Today
Size=2 Size=4Size=1/2Size=1/4
If w=-1 and the cosmological constant corresponds to some sort of “quantum zero-point”, then its value today is a factor ~10120 too small, plus it is suspiciously fine-tuned: anthropic argument?
time
Fine-tuning and Cosmic Fine-tuning and Cosmic CoincidenceCoincidence
Fine-tuning and Cosmic Fine-tuning and Cosmic CoincidenceCoincidence
Thus could we have w = w(z) ? --> e.g. quintessence, a cosmic scalar field slowly rolling to the minimum of its potential (e.g. Wetterich 1988), inducing an evolving -1 < w(z) < -1/3. Or more complex interactions between DM and DE (e.g. Amendola 2000; Liddle et al. 2008; He et al.) ?
redshift
z=3 z=1
Observational Probes
• Supernovae M(z)
• Baryonic Acoustic Oscillations (BAO)
• Abundance of rich clusters
• Weak Lensing
• Redshift distortion
SNe Future experiments: JDEM, DES,
PanSTARRS,LSST
BAO: SDSS/2dF, WiggleZ, FMOS, BOSS,Bigboss HETDEX, WFMOS,
PAU
Luminous Red Galaxies , LRG) two-point CF
. J. Eisenstein et al., Astrophys. J. 619, 178 (2005).
But we need to look at both sides of the But we need to look at both sides of the story…story…
R 1
2g R
8G
c2 T
Add dark energyModify gravity theory [e.g. R f(R) ]
R 1
2g R
8G
c2 T g
“…the Force be with you”
So, the equation of state is not the end of the So, the equation of state is not the end of the story…story…
Cosmic acceleration can also be explained by modifying the theory of gravity [as e.g. in f(R) theories, Capozziello et al. 2005, or in multi-dimensional “braneworld” models, Dvali et al. (DGP) 2000].
The growth equation (and thus the growth rate) depends not only on the expansion history H(t) (and thus on w) but also on the gravitation theory (e.g. Lue et al. 2004)
which has a growing solution:
(x , t) ˆ (x )D(t)
Ý Ý 2H (t) Ý 4G
f d lnD
d lnafrom which we define a growth rate
How to distinguish between these two options, observationally?Growth of linear density fluctuations in the expanding Universe (in GR):
Observational Probes
• Supernovae M(z)
• Baryonic Acoustic Oscillations (BAO)
• Abundance of rich clusters
• Weak Lensing
• Redshift distortion
Clusters:SZA, SPT, DES, ACT, 400d, eROSITA
Weak Lensing: LSST, EUCLID, DES, PanSTARRS
1.1o1.1o simulated shear field by Hamana
()
(+)
Redshift distortion: Bigboss, Vipers, Euclid etc
4 个引力模型 : GR ,f(R) , DGP , TeVeS
张鹏杰等提出在宇宙学尺度上检验广义相对论与其
他引力论的新方法
通过通过 EEGG 方法,广义相对论方法,广义相对论在一亿光年尺度上得到了确认在一亿光年尺度上得到了确认
Reyes et al. (Nature,464, 256-258,11 March 2010) 应用我们的 EG 方法分析了 SDSS 星系巡天的数据。
右图即为其主要结果。测量到的一亿光年尺度上的 EG 与广义相对论的预言相符。
该结果基本排除了 TeVeS 修改引力,并有力限制对 f(R) 引力
We also consider the dependence on the information used: the full galaxy power spectrum P(k), P(k) marginalized over its shape, or just the Baryon Acoustic Oscillations (BAO). We find that the inclusion of growth rate information (extracted using redshift space distortion and galaxy clustering amplitude measurements) leads to a factor of 3 improvement in the FoM, assuming general relativity is not modified. This inclusion partially compensates for the loss of information when only the BAO are used to give geometrical constraints, rather than using the full P(k) as a standard ruler. We
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通过改造美国国家天文台的 4m 望远镜到直径 3度的视场 , 在焦面上放置 5000 根光纤开展光谱巡天 , 光谱覆盖范围从近红外到光学,分辨率为 5000 ;已经获准;
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