new approaches to modeling nonlinear structure formation
DESCRIPTION
New Approaches to Modeling Nonlinear Structure Formation. Nuala McCullagh Johns Hopkins University Cosmology on the Beach Cabo San Lucas, Mexico January 13, 2014 In collaboration with: Alex Szalay and Mark Neyrinck. Outline. Introduction Modeling the correlation function - PowerPoint PPT PresentationTRANSCRIPT
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New Approaches to Modeling Nonlinear Structure Formation
Nuala McCullaghJohns Hopkins University
Cosmology on the BeachCabo San Lucas, Mexico
January 13, 2014
In collaboration with:Alex Szalay and Mark Neyrinck
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Outline
• Introduction• Modeling the correlation function• Beyond Gaussianity: log transform• Conclusions
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z=0
z=1100
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Modeling 2-point statistics: Linear Theory
Linear Theory:
Correlation Function:
Power Spectrum:
Overdensity:
Linear power spectrum
Linear correlation function
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Modeling 2-point statistics: Systematics
π [M
pc/h
]
σ [Mpc/h]0 20-20
020
-20
Hawkins et al. (2002), astro-ph/02123752dFGRS: β=0.49±0.09
Nonlinearity
Redshift-space distortions
Galaxy bias
Image: Max Tegmark
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Modeling 2-point statistics: SPTStandard Perturbation Theory: perturbative solution to the fluid equations in Fourier space:
Figure: Carlson, White, Padmanabhan, arXiv:0905.0497 (2009)
Linear2nd order3rd order
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Modeling 2-point statistics: New Approach
• Structure of the Fourier space kernels suggests that in configuration space, the result may be simpler
• Terms beyond 2nd order may be simplified in configuration space compared to Fourier space
• Configuration space can be more easily extended to redshift space
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Modeling 2-point statistics: New Approach
1st order Lagrangian perturbation theory (Zel’dovich approximation):
1LPT:
Poisson:
Expansion of the density in terms of linear quantities:
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Modeling 2-point statistics: New Approach
Nonlinear correlation function:
McCullagh & Szalay. ApJ, 752, 21 (2012)
First nonlinear contribution to the correlation function in terms of initial quantities:
Where:
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77 Indra simulationsT. Budavári, S. Cole, D. Crankshaw, L. Dobos, B. Falck, A. Jenkins, G. Lemson, M. Neyrinck, A. Szalay, and J. Wang
z=1.08 z=0.41
z=0.06 z=0.00
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Line
of si
ght
Linear Nonlinear, z=0
Modeling 2-point statistics: New Approach
Zel’dovich model extended to redshift space:
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Beyond Gaussianity: Log transform
A=log(1+δ(x))
McCullagh, Neyrinck, Szapudi, & Szalay. ApJL, 763, L14 (2013)
δ
log(1+δ)
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Beyond Gaussianity: Log transformLinear Theory: 106.4 Mpc/hZel’dovich density: 105.8 Mpc/h -0.6 Mpc/hZel’dovich log-density: 106.1 Mpc/h -0.3 Mpc/h
McCullagh, Neyrinck, Szapudi, & Szalay. ApJL, 763, L14 (2013)
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Conclusions & Future Directions• Extracting cosmological information from large-scale
structure requires accurate modeling of systematics• Modeling statistics in configuration space simplifies
higher-order corrections and extension to redshift space– Our approach should be extended to higher orders in LPT for
greater accuracy• Log-transform restores information to the 2-point
statistics– Possible improvements to BAO, redshift-space distortions, and
small-scale power spectrum– Must be demonstrated in real data in presence of discreteness
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Thank you!