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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.

Zheng , Yi 郑逸 Shanghai Astronomical Observatory P . Zhang, J. Pan, and Y. Zheng , 1207.2722

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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. Outline . - PowerPoint PPT Presentation

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Page 1: Zheng , Yi   郑逸 Shanghai Astronomical Observatory P . Zhang, J. Pan, and Y.  Zheng , 1207.2722

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: Zheng , Yi   郑逸 Shanghai Astronomical Observatory P . Zhang, J. Pan, and Y.  Zheng , 1207.2722

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: Zheng , Yi   郑逸 Shanghai Astronomical Observatory P . Zhang, J. Pan, and Y.  Zheng , 1207.2722

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: Zheng , Yi   郑逸 Shanghai Astronomical Observatory P . Zhang, J. Pan, and Y.  Zheng , 1207.2722

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: Zheng , Yi   郑逸 Shanghai Astronomical Observatory P . Zhang, J. Pan, and Y.  Zheng , 1207.2722

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: Zheng , Yi   郑逸 Shanghai Astronomical Observatory P . Zhang, J. Pan, and Y.  Zheng , 1207.2722

Velocity power spectrum

Definition:

𝑽 𝛿

𝑽 𝑆

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

𝑽 𝐵

Page 7: Zheng , Yi   郑逸 Shanghai Astronomical Observatory P . Zhang, J. Pan, and Y.  Zheng , 1207.2722

Velocity correlation function

Definition:

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

Page 8: Zheng , Yi   郑逸 Shanghai Astronomical Observatory P . Zhang, J. Pan, and Y.  Zheng , 1207.2722

𝑽 𝛿 𝑽 𝑆 𝑽 𝐵

2.Determined by W(k)!

A new RSD formulae 1.Underestimation of by

3. Physical FOG:CL, dispersion, NG

Page 9: Zheng , Yi   郑逸 Shanghai Astronomical Observatory P . Zhang, J. Pan, and Y.  Zheng , 1207.2722

Window function I

𝜃= 𝑓 𝛿

underestimation

Page 10: Zheng , Yi   郑逸 Shanghai Astronomical Observatory P . Zhang, J. Pan, and Y.  Zheng , 1207.2722

~𝑊 (𝑘 )=𝑃𝛿𝜃

𝑓 𝑃𝛿𝛿= 1

1+𝛼 𝑓 𝛽 Δ𝛿𝛿2 (𝑘)

𝛼=0.48 , 𝛽=0.5125% 𝑎𝑡 𝑘≳ 0.7h/𝑀𝑝𝑐

Window function II

Do fitting using region Δ 𝛿𝛿2 =𝑘3 Δ𝛿𝛿

2 /2𝜋

Page 11: Zheng , Yi   郑逸 Shanghai Astronomical Observatory P . Zhang, J. Pan, and Y.  Zheng , 1207.2722

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: Zheng , Yi   郑逸 Shanghai Astronomical Observatory P . Zhang, J. Pan, and Y.  Zheng , 1207.2722

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.