Perturbation theory reloaded: analytical calculation of non-linearity in baryonic oscillations in the real space matter power spectrum - INSPIRE

DataBETA

Perturbation theory reloaded: analytical calculation of non-linearity in baryonic oscillations in the real space matter power spectrum

Apr, 2006

5 pages

Published in:

Astrophys.J. 651 (2006) 619-626

e-Print:

astro-ph/0604075 [astro-ph]

DOI:

10.1086/507781

View in:

ADS Abstract Service

reference search184 citations

Citations per year

Abstract: (arXiv)

We compare the non-linear matter power spectrum in real space calculated analytically from 3rd-order perturbation theory with N-body simulations at 11, the shape of oscillations is distorted from the linear theory prediction. Nevertheless, our results suggest that one can correct the distortion caused by non-linearity almost exactly. We also find that perturbation theory, which does not contain any free parameters, provides a significantly better fit to the simulations than the conventional approaches based on empirical fitting functions to simulations. The future work would include perturbation theory calculations of non-linearity in redshift space distortion and halo biasing in the weakly non-linear regime.

cosmology: theory
large-scale structure of universe

References(40)

Figures(0)

First year Wilkinson Microwave Anisotropy Probe (WMAP) observations: Preliminary maps and basic results

WMAP

Collaboration

•

C.L. Bennett

et al.

- Astrophys.J.Suppl. 148 (2003) 1-27
•
e-Print:
- astro-ph/0302207
•
DOI:
- 10.1086/377253

Large scale structure of the universe and cosmological perturbation theory

F. Bernardeau
(
- Saclay
)
,
S. Colombi
(
- Paris, Inst. Astrophys.
)
,
E. Gaztanaga
(
- CSIC, Catalunya and
- INAOE, Puebla
)
,
R. Scoccimarro
(
- Princeton, Inst. Advanced Study and
- New York U.
)

- Phys.Rept. 367 (2002) 1-248
•
e-Print:
- astro-ph/0112551
•
DOI:
- 10.1016/S0370-1573(02)00135-7

Probing dark energy using baryonic oscillations in the galaxy power spectrum as a cosmological ruler

Chris Blake
(
- New South Wales U.
)
,
Karl Glazebrook
(
- Johns Hopkins U.
)

- Astrophys.J. 594 (2003) 665-673
•
e-Print:
- astro-ph/0301632
•
DOI:
- 10.1086/376983

The 2dF Galaxy Redshift Survey: Power-spectrum analysis of the final dataset and cosmological implications

2dFGRS

Collaboration

•

Shaun Cole

et al.

- Mon.Not.Roy.Astron.Soc. 362 (2005) 505-534
•
e-Print:
- astro-ph/0501174
•
DOI:
- 10.1111/j.1365-2966.2005.09318.x

Transients from Initial Conditions in Cosmological Simulations

- Mon.Not.Roy.Astron.Soc. 373 (2006) 369-381
•
e-Print:
- astro-ph/0606505
•
DOI:
- 10.1111/j.1365-2966.2006.11040.x

Baryonic features in the matter transfer function

- Astrophys.J. 496 (1998) 605
•
e-Print:
- astro-ph/9709112
•
DOI:
- 10.1086/305424

The Galaxy correlation hierarchy in perturbation theory

James N. Fry
(
- Chicago U., Astron. Astrophys. Ctr.
)

- Astrophys.J. 279 (1984) 499-510
•
DOI:
- 10.1086/161913

Biasing and hierarchical statistics in large scale structure

James N. Fry
(
- Fermilab
)
,
Enrique Gaztanaga
(
- Fermilab
)

- Astrophys.J. 413 (1993) 447-452
•
e-Print:
- astro-ph/9302009
•
DOI:
- 10.1086/173015

Coupling of Modes of Cosmological Mass Density Fluctuations

- Astrophys.J. 311 (1986) 6-14
•
DOI:
- 10.1086/164749

Dark energy and cosmic sound: w(z) surveys with the Gemini/Subaru wide-field multi-object spectrograph

Karl Glazebrook
(
- Johns Hopkins U.
)
,
Daniel Eisenstein
(
- Arizona U., Astron. Dept. - Steward Observ.
)
,
Arjun Dey
(
- NOAO, Tucson
)
,
Bob Nichol
(
- Portsmouth U.
)

e-Print:
- astro-ph/0507457

Reconstructing the primordial spectrum of fluctuations of the universe from the observed nonlinear clustering of galaxies

- Astrophys.J.Lett. 374 (1991) L1
•
DOI:
- 10.1086/186057

The Nonlinear redshift-space power spectrum of galaxies

A.F. Heavens
(
- Royal Observ., Edinburgh
)
,
S. Matarrese
(
- Padua U.
)
,
Licia Verde
(
- Royal Observ., Edinburgh
)

- Mon.Not.Roy.Astron.Soc. 301 (1998) 797-808
•
e-Print:
- astro-ph/9808016
•
DOI:
- 10.1046/j.1365-8711.1998.02052.x

The Hobby‐Eberly Telescope Dark Energy Experiment

- AIP Conf.Proc. 743 (2004) 1, 224
•
DOI:
- 10.1063/1.1848329

Redshifting rings of power

Wayne Hu
(
)
,
Zoltan Haiman
(
- Columbia U., Astron. Astrophys.
)

- Phys.Rev.D 68 (2003) 063004
•
e-Print:
- astro-ph/0306053
•
DOI:
- 10.1103/PhysRevD.68.063004

Second order power spectrum and nonlinear evolution at high redshift

Bhuvnesh Jain
(
- MIT, LNS
)
,
Edmund Bertschinger
(
- MIT, LNS and
- Princeton, Inst. Advanced Study
)

- Astrophys.J. 431 (1994) 495
•
e-Print:
- astro-ph/9311070
•
DOI:
- 10.1086/174502

Large scale bias in the universe: Bispectrum method

S. Matarrese
(
- Padua U.
)
,
Licia Verde
(
- Padua U. and
- Royal Observ., Edinburgh
)
,
A.F. Heavens
(
- Royal Observ., Edinburgh
)

- Mon.Not.Roy.Astron.Soc. 290 (1997) 651-662
•
e-Print:
- astro-ph/9706059
•
DOI:
- 10.1093/mnras/290.4.651

Baryonic signatures in large scale structure

- Mon.Not.Roy.Astron.Soc. 304 (1999) 851-864
•
e-Print:
- astro-ph/9812214
•
DOI:
- 10.1046/j.1365-8711.1999.02369.x

- Phys.Rev.D 46 2

On second order perturbation theories of gravitational instability in Friedmann-Lemaitre models

Takahiko Matsubara
(
- Tokyo U.
)

- Prog.Theor.Phys. 94 (1995) 1151-1156
•
e-Print:
- astro-ph/9510137
•
DOI:
- 10.1143/PTP.94.1151

Apparent clustering of intermediate-redshift galaxies as a probe of dark energy

Takahiko Matsubara
(
- Nagoya U.
)
,
Alexander S. Szalay
(
- Johns Hopkins U.
)

- Phys.Rev.Lett. 90 (2003) 021302
•
e-Print:
- astro-ph/0208087
•
DOI:
- 10.1103/PhysRevLett.90.021302

Nonlinear evolution of cosmological power spectra

- Mon.Not.Roy.Astron.Soc. 280 (1996) L19
•
e-Print:
- astro-ph/9603031
•
DOI:
- 10.1093/mnras/280.3.L19

A Cosmological hydrodynamic code based on the total variation diminishing scheme

Dong-su Ryu
(
- Princeton U. Observ.
)
,
Jeremiah P. Ostriker
(
- Princeton U. Observ.
)
,
Hye-sung Kang
(
- Princeton U. Observ.
)
,
Ren-yue Cen
(
- Princeton U. Observ.
)

- Astrophys.J. 414 (1993) 1
•
DOI:
- 10.1086/173051

- Astrophys.J. 381 349

Redshift-space distortions, pairwise velocities and nonlinearities

Roman Scoccimarro
(
- New York U., CCPP
)

- Phys.Rev.D 70 (2004) 083007
•
e-Print:
- astro-ph/0407214
•
DOI:
- 10.1103/PhysRevD.70.083007

1-25 of 40
1
2
25 / page