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BAOs (Baryon Acoustic Oscillations)

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RPT, CLA and N-body simulations agree within errorbars in almost the same range ... RPT and CLA have better convergence properties than SPT in the plotted ranges. ... – PowerPoint PPT presentation

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Title: BAOs (Baryon Acoustic Oscillations)


1
Accuracy of Cosmological N-body Simulations
DARK ENERGY
Ludwig-Maximilians-University, Munich
Takahiro Nishimichi (the Univ. of Tokyo)
Introduction
  • BAOs (Baryon Acoustic Oscillations)
  • A promising tool to access dark energy.
  • Demand for more accurate theoretical modeling
  • Nonlinearity of gravitational structure formation
  • Redshift-space distortion
  • Galaxy biasing
  • Methods
  • Perturbation theory
  • Newly developed renormalized perturbation theory
  • N-body simulations
  • 1 error on BAO scale -gt 35 Error on DE e.o.s.
  • Is the currently achieved accuracy enough?

Our simulations
After correction
2LPT
Gadget2
  • SPT standard perturbation theory
  • RPT renormalized perturbation theory
    (CrocceScoccimarro06a,b,08)
  • CLA closure approximation (TaruyaHiramatsu08)
  • LIN linear theory
  • Convergence test is difficult from this figure
    because of large errorbars due to small total
    volume of N-body simulations (4h-3Gpc3).
  • Errorbars largely reduced to sub-percent level!
  • The three nonlinear models and N-body simulations
    agree at largest scales (klt0.05hMpc-1).
  • RPT, CLA and N-body simulations agree within
    errorbars in almost the same range for a given
    redshift.
  • RPT and CLA have better convergence properties
    than SPT in the plotted ranges.

Correction for finiteness of volume
Errorbars
2pt correlation (preliminary)
Recovery of BAOs
Convergence regime
C is a constant to be determined.
Preliminary
  • M08 Matsubara08
  • SK07 SefusattiKomatsu07
  • JK06 JeongKomatsu06
  • We construct smooth reference spectra using
    B-spline fit. (e.g., Percival07, Nishimichi07)
  • The convergence regimes for the extracted BAO
    phases are wider than those for the amplitudes of
    P(k) (vertical arrows).
  • The scale shift parameter a can be constrained
    tightly using the modes within our convergence
    regimes alone.
  • The number of N-body realizations increased to
    30.
  • A good convergence in real space?
  • Monopole and quadrupole moments are reasonably
    converged in redshift space?
  • We determined the 1 and 3 convergence regimes
    where theoretical predictions and N-body
    simulations agree within 1 and 3.
  • Our formula explains the results (symbols) very
    well.

Apendix convergence test of our simulations
Initial condition
SPT w/o cutoff scale
N-body code
Fake agreement of SPT for small boxsize
boxsize
2LPT vs. ZA
RPT w/ cutoff scale
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