The DOI matches its Crossref record; 19 of the 19 references it cites were found in a registry or an index.
The IR-resummed Effective Field Theory of Large Scale Structures
Open accessAbstract
We present a new method to resum the effect of large scale motions in the Effective Field Theory of Large Scale Structures. Because the linear power spectrum in ΛCDM is not scale free the effects of the large scale flows are enhanced. Although previous EFT calculations of the equal-time density power spectrum at one and two loops showed a remarkable agreement with numerical results, they also showed a 2% residual which appeared related to the BAO oscillations. We show that this was indeed the case, explain the physical origin and show how a Lagrangian based calculation removes this differences. We propose a simple method to upgrade existing Eulerian calculations to effectively make them Lagrangian and compare the new results with existing fits to numerical simulations. Our new two-loop results agrees with numerical results up to k ∼ 0.6 h Mpc −1 to within 1% with no oscillatory residuals. We also compute power spectra involving momentum which is significantly more affected by the large scale flows. We show how keeping track of these velocities significantly enhances the UV reach of the momentum power spectrum in addition to removing the BAO related residuals. We compute predictions for the real space correlation function around the BAO scale and investigate its sensitivity to the EFT parameters and the details of the resummation technique.
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
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
Cosmological non-linearities as an effective fluid
Baumann, D., Nicolis, A., Senatore, L., & Zaldarriaga, M. (2012) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2012/07/051 · Cited by 642
Self-citationThe effective field theory of cosmological large scale structures
Carrasco, J. J. M., Hertzberg, M. P., & Senatore, L. (2012) · Journal of High Energy Physics · doi:10.1007/jhep09(2012)082 · Cited by 641
Self-citationRenormalized cosmological perturbation theory
Crocce, M., & Scoccimarro, R. (2006) · Physical Review D · doi:10.1103/physrevd.73.063519 · Cited by 534
Improving Cosmological Distance Measurements by Reconstruction of the Baryon Acoustic Peak
Eisenstein, D. J., Seo, H., Sirko, E., & Spergel, D. N. (2007) · The Astrophysical Journal · doi:10.1086/518712 · Cited by 514
Nonlinear evolution of baryon acoustic oscillations
Crocce, M., & Scoccimarro, R. (2008) · Physical Review D · doi:10.1103/physrevd.77.023533 · Cited by 464
THE COYOTE UNIVERSE. I. PRECISION DETERMINATION OF THE NONLINEAR MATTER POWER SPECTRUM
Heitmann, K., White, M., Wagner, C., Habib, S., & Higdon, D. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/715/1/104 · Cited by 321
Uncorrelated modes of the non-linear power spectrum
Hamilton, A. J. S. (2000) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2000.03071.x · Cited by 307
Heitmann, K., Higdon, D., White, M., Habib, S., Williams, B. J., Lawrence, E., & Wagner, C. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/705/1/156 · Cited by 242
THE COYOTE UNIVERSE EXTENDED: PRECISION EMULATION OF THE MATTER POWER SPECTRUM
Heitmann, K., Lawrence, E., Kwan, J., Habib, S., & Higdon, D. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/780/1/111 · Cited by 240
Cited by
Desjacques, V., Jeong, D., & Schmidt, F. (2018) · Physics Reports · doi:10.1016/j.physrep.2017.12.002 · Cited by 817
d'Amico, G., Gleyzes, J., Kokron, N., Markovic, K., Senatore, L., Zhang, P., Beutler, F., & Gil-Marín, H. (2020) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2020/05/005 · Cited by 448
Self-citationCosmological parameters from the BOSS galaxy power spectrum
Ivanov, M. M., Simonović, M., & Zaldarriaga, M. (2020) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2020/05/042 · Cited by 441
Self-citationDi Valentino, E., Said, J. L., Riess, A., Pollo, A., Poulin, V., Gómez-Valent, A., Weltman, A., Palmese, A., Huang, C. D., Bruck, C. V. D., et al. (2025) · Physics of the Dark Universe · doi:10.1016/j.dark.2025.101965 · Cited by 319
Full-shape galaxy power spectra and the curvature tension
Glanville, A., Howlett, C., & Davis, T. (2022) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stac2891 · Cited by 69
Metadata
- Authors
- Senatore, L., & Zaldarriaga, M.
- Venue
- Journal of Cosmology and Astroparticle Physics
- Publisher
- IOP Publishing
- Published
- 2015-02-10
- Volume
- 2015
- Issue
- 02
- Pages
- 013-013
- ISSN
- 1475-7508 (ISSN-L)
- 1475-7516
- OpenAlex
- W1977223600
- Cited by
- 260
- References
- 19
- FWCI
- 9.84
- 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: The IR-resummed Effective Field Theory of Large Scale Structures. https://app.cochat.ai/papers/10.1088/1475-7516/2015/02/013
- The paper
- Senatore, L., & Zaldarriaga, M. (2015). The IR-resummed Effective Field Theory of Large Scale Structures. Journal of Cosmology and Astroparticle Physics. https://doi.org/10.1088/1475-7516/2015/02/013
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.