The DOI matches its Crossref record; 44 of the 44 references it cites were found in a registry or an index.
Transients from initial conditions in cosmological simulations
Open accessAbstract
We study the impact of setting initial conditions in numerical simulations using the standard procedure based on the Zel'dovich approximation (ZA).As it is well known from the perturbation theory, ZA initial conditions have incorrect second-and higher-order growth and therefore excite long-lived transients in the evolution of the statistical properties of density and velocity fields.We also study the improvement brought by using more accurate initial conditions based on second-order Lagrangian perturbation theory (2LPT).We show that 2LPT initial conditions reduce transients significantly and thus are much more appropriate for numerical simulations devoted to precision cosmology.Using controlled numerical experiments with ZA and 2LPT initial conditions, we show that simulations started at redshift z i = 49 using the ZA underestimate the power spectrum in the non-linear regime by about 2, 4 and 8 per cent at z = 0, 1, and 3, respectively, whereas the mass function of dark matter haloes is underestimated by 5 per cent at m = 10 15 M h -1 (z = 0) and 10 per cent at m = 2 × 10 14 M h -1 (z = 1).The clustering of haloes is also affected to the few per cent level at z = 0.These systematics effects are typically larger than statistical uncertainties in recent mass function and power spectrum fitting formulae extracted from numerical simulations.At large scales, the measured transients in higher-order correlations can be understood from first principle calculations based on perturbation theory.
Overview
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
Citations
Cites
The cosmological simulation code gadget-2
Springel, V. (2005) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2005.09655.x · Cited by 6,368
Lewis, A., Challinor, A., & Lasenby, A. (2000) · The Astrophysical Journal · doi:10.1086/309179 · Cited by 4,920
The cosmological simulation code GADGET-2
Petkova, M., & Springel, V. (2005) · Cited by 3,918
Large-scale bias and the peak background split
Sheth, R. K., & Tormen, G. (1999) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.1999.02692.x · Cited by 2,783
Stable clustering, the halo model and non-linear cosmological power spectra
Smith, R. E., Peacock, J. A., Jenkins, A., White, S. D. M., Frenk, C. S., Pearce, F. R., Thomas, P. A., Efstathiou, G., & Couchman, H. M. P. (2003) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2003.06503.x · Cited by 2,054
Cosmological Perturbation Theory in the Synchronous and Conformal Newtonian Gauges
Ma, C.-P., & Bertschinger, E. (1995) · The Astrophysical Journal · doi:10.1086/176550 · Cited by 2,040
A Line-of-Sight Integration Approach to Cosmic Microwave Background Anisotropies
Seljak, U., & Zaldarriaga, M. (1996) · The Astrophysical Journal · doi:10.1086/177793 · Cited by 2,019
Large-scale structure of the Universe and cosmological perturbation theory
Bernardeau, F., Colombi, S., Gaztañaga, E., & Scoccimarro, R. (2002) · Physics Reports · doi:10.1016/s0370-1573(02)00135-7 · Cited by 1,922
Self-citationThe mass function of dark matter haloes
Jenkins, A., Frenk, C. S., White, S. D. M., Colberg, J. M., Cole, S., Evrard, A. E., Couchman, H. M. P., & Yoshida, N. (2001) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2001.04029.x · Cited by 1,659
A line of sight integration approach to cosmic microwave background anisotropiesPreprint
Zaldarriaga, M. (1996) · Cited by 1,367
Cited by
THE AVERAGE STAR FORMATION HISTORIES OF GALAXIES IN DARK MATTER HALOS FROM z = 0-8
Behroozi, P. S., Wechsler, R. H., & Conroy, C. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/770/1/57 · Cited by 2,167
THE LARGE-SCALE BIAS OF DARK MATTER HALOS: NUMERICAL CALIBRATION AND MODEL TESTS
Tinker, J. L., Robertson, B. E., Kravtsov, A. V., Klypin, A., Warren, M. S., Yepes, G., & Gottlöber, S. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/724/2/878 · Cited by 989
Multi-scale initial conditions for cosmological simulations
Hahn, O., & Abel, T. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2011.18820.x · Cited by 834
Angulo, R. E., Springel, V., White, S. D. M., Jenkins, A., Baugh, C. M., & Frenk, C. S. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21830.x · Cited by 490
Villaescusa-Navarro, F., Hahn, C., Massara, E., Banerjee, A., Delgado, A. M., Ramanah, D. K., Charnock, T., Giusarma, E., Li, Y., Allys, E., et al. (2020) · The Astrophysical Journal Supplement Series · doi:10.3847/1538-4365/ab9d82 · Cited by 336
Self-citation
Metadata
- Authors
- Crocce, M., Pueblas, S., & Scoccimarro, R.
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2006-11-21
- Volume
- 373
- Issue
- 1
- Pages
- 369-381
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W2029234737
- Cited by
- 657
- References
- 44
- FWCI
- 10.61
- Type
- journal article
- Language
- en
- Open access
- bronze
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review
How to cite
Cite CoChat for the checks on this page, and the paper for its own findings.
- This page
- CoChat. (2026). Citation check: Transients from initial conditions in cosmological simulations. https://app.cochat.ai/papers/10.1111/j.1365-2966.2006.11040.x
- The paper
- Crocce, M., Pueblas, S., & Scoccimarro, R. (2006). Transients from initial conditions in cosmological simulations. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1111/j.1365-2966.2006.11040.x
Data sources
Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.