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Peculiar velocity decomposition, redshift distortion and velocity reconstruction in redshift surveys Zheng, Yi 郑郑 Shanghai Astronomical Observatory P. Zhang, J. Pan, and Y. Zheng, 1207.2722. Y. Zheng, P. Zhang et al. (2012), in preparation.

Peculiar velocity decomposition, redshift distortion and velocity reconstruction in redshift surveys Zheng, Yi 郑逸 Shanghai Astronomical Observatory P

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Page 1: Peculiar velocity decomposition, redshift distortion and velocity reconstruction in redshift surveys Zheng, Yi 郑逸 Shanghai Astronomical Observatory P

Peculiar velocity decomposition, redshift distortion and velocity reconstruction in redshift

surveys

Zheng, Yi 郑逸Shanghai Astronomical Observatory

P. Zhang, J. Pan, and Y. Zheng, 1207.2722.Y. Zheng, P. Zhang et al. (2012), in preparation.

Page 2: Peculiar velocity decomposition, redshift distortion and velocity reconstruction in redshift surveys Zheng, Yi 郑逸 Shanghai Astronomical Observatory P

Outline

• I. Introduction. (Why RSD interesting?) • II. Velocity decomposition. (What do

decomposed velocity components look like?)• III. RSD modeling and velocity reconstruction. • IV. Discussions and conclusions

Page 3: Peculiar velocity decomposition, redshift distortion and velocity reconstruction in redshift surveys Zheng, Yi 郑逸 Shanghai Astronomical Observatory P

Introduction

A. J. S. Hamilton, astro-ph/9708102

Observationally:

Euclid, BigBOSS et all:

O(1%)

5-10%

Theoretically:1. Nonlinear mapping 2. Nonlinear evolution 3. Bias modelling

Torre & Guzzo, 1202.5559

The redshift position s:

𝒔=𝒙+𝑣 𝑧/ (𝑎𝐻) �̂�

Reid et al. 2012

Page 4: Peculiar velocity decomposition, redshift distortion and velocity reconstruction in redshift surveys Zheng, Yi 郑逸 Shanghai Astronomical Observatory P

RSD modeling I

The redshift position s: 𝒔=𝒙+𝑣 𝑧/ (𝑎𝐻) �̂�

From mass conservation: (1+𝛿𝑠 (𝒔 ) )𝑑3 𝑠=(1+𝛿(𝒙 ))𝑑3 𝑥

The redshift space power spectrum:

Dark matter and LCDM cosmology

Page 5: Peculiar velocity decomposition, redshift distortion and velocity reconstruction in redshift surveys Zheng, Yi 郑逸 Shanghai Astronomical Observatory P

Velocity decomposition

Background from Wang et al. 2012

𝑽 (𝒙)rotational component

𝑽 𝑩=𝑽 (𝒌 )−𝑽 𝑬

irrotational component

𝑽 𝑬=[𝑽 (𝒌 ) ∙ �̂�]�̂�

𝜃 (𝒌 )=𝑖𝒌∙𝑽 𝑬 (𝒌)/𝑎𝐻

correlated with

𝜃𝛿(𝑘)=𝛿 (𝑘 )𝑊 (𝑘)

uncorrelated with

𝜃𝑆 (𝑘 )=𝜃 (𝑘 )−𝜃𝛿

Page 6: Peculiar velocity decomposition, redshift distortion and velocity reconstruction in redshift surveys Zheng, Yi 郑逸 Shanghai Astronomical Observatory P

Velocity power spectrum

Definition:

𝑽 𝛿

𝑽 𝑆

Simulation: 1200 Mpc/h & 100 Mpc/h, 1024^3Nearest Particle method

𝑽 𝐵

Page 7: Peculiar velocity decomposition, redshift distortion and velocity reconstruction in redshift surveys Zheng, Yi 郑逸 Shanghai Astronomical Observatory P

Velocity correlation function

Definition:

O(1 Mpc/h) O(10 Mpc/h)

Page 8: Peculiar velocity decomposition, redshift distortion and velocity reconstruction in redshift surveys Zheng, Yi 郑逸 Shanghai Astronomical Observatory P

𝑽 𝛿 𝑽 𝑆𝑽 𝐵

2.Determined by W(k)!

A new RSD formulae 1.Underestimation of by

3. Physical FOG:CL, dispersion, NG

Page 9: Peculiar velocity decomposition, redshift distortion and velocity reconstruction in redshift surveys Zheng, Yi 郑逸 Shanghai Astronomical Observatory P

Window function I

𝜃= 𝑓 𝛿

underestimation

Page 10: Peculiar velocity decomposition, redshift distortion and velocity reconstruction in redshift surveys Zheng, Yi 郑逸 Shanghai Astronomical Observatory P

~𝑊 (𝑘 )=𝑃𝛿𝜃

𝑓 𝑃𝛿𝛿

= 11+𝛼 𝑓 𝛽 Δ𝛿𝛿

2 (𝑘)

𝛼=0.48 , 𝛽=0.5125% 𝑎𝑡 𝑘≳ 0.7h/𝑀𝑝𝑐

Window function II

Do fitting using region Δ𝛿𝛿2 =𝑘3 Δ𝛿𝛿

2 /2𝜋

Page 11: Peculiar velocity decomposition, redshift distortion and velocity reconstruction in redshift surveys Zheng, Yi 郑逸 Shanghai Astronomical Observatory P

3D velocity reconstruction

1. The 1st Method:

2. The 2nd Method:

By tuning such that is isotropic at large scales, we could obtain the correct and hence the correct field.

k-SZ effect

Application example: k-SZ tomography (Ho et al. 0903.2845, Shao et al. 1004.1301)

Velocity field Momentum field

CMBMissing baryons

Page 12: Peculiar velocity decomposition, redshift distortion and velocity reconstruction in redshift surveys Zheng, Yi 郑逸 Shanghai Astronomical Observatory P

Conclusions and discussions

• Conclusions:– a velocity decomposition method a new RSD model lower systematic error.

– a simple fitting formula for – 2 new methods for 3D velocity reconstruction in light of

RSD information.

• Future work:– More simulation calculations to impove RSD model and

test its accuracy, halo, galaxy....– Velocity reconstruction methods need more theoretical and

numerical considerations.