Cited by 270Cosmology and Gravitation TheoriesNoncommutative and Quantum Gravity TheoriesBlack Holes and Theoretical Physics

On non-Gaussianities in single-field inflation

Open access
Creminelli, Paolo·2003·Journal of Cosmology and Astroparticle Physics

Abstract

We study the impact of higher dimension operators in the inflaton Lagrangian on the non-Gaussianity of the scalar spectrum. These terms can strongly enhance the effect without spoiling slow-roll, though it is difficult to exceed f NL ~1, because the scale which suppresses the operators cannot be too low, if we want the effective field theory description to make sense. In particular we explicitly calculate the three-point function given by an higher derivative interaction of the form (∇ϕ) 4 , which is expected to give the most important contribution. The angular dependence of the result turns out to be quite different from the minimal case without higher dimension operators.

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.

A few free checks a day · papers already verified open instantly · results are public

Integrity signals

Registry

Crossref · 10.1088/1475-7516/2003/10/003

Cites

Statistics

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.

A few free checks a day · papers already verified open instantly · results are public

Claims other papers make about this one

Each is checked against this paper’s own text: does it say what the citing paper says it does?

  • Inflationary models with higher derivative operators, such as ghost inflation or inflation based on the Dirac-Born-Infeld action, can produce higher non-Gaussianity, possibly detectable.

    “On the other hand, inflationary models with higher derivative operators, such as ghost inflation or inflation based on the Dirac-Born-Infeld action, can produce higher non-Gaussianity [6, 7, 8, 9], possibly detectable.”

    From Non-Gaussianities in two-field inflation (2006) · cites this paper as [9]

    The Abstract says higher-dimension operators, including a higher-derivative interaction, can strongly enhance non-Gaussianity. The Conclusions say the predicted effect is near the threshold of detectability. Our copy does not identify ghost inflation or Dirac–Born–Infeld inflation as examples, so those specifics are not supported by this source. (LLM, conf=0.86)

    Experimental — accuracy not yet measured

Self-check

Percentages, sums and reported differences re-computed from the paper’s own numbers.

The self-check needs the paper’s full text.

Cites

No references could be resolved yet.

Research works printed but not linked: 21

  1. The literature about this so-called 'trans-Planckian' problem is quite broad. See e.g. Brandenberger R H and Martin J, On signatures of short distance physics in the cosmic microwave background, 2002 Int. J. Mod. Phys. A 17 3663 [SPIRES] [hep-th/0202142] · arXiv
  2. Kaloper N, Kleban M, Lawrence A, Shenker S and Susskind L, Initial conditions for inflation, 2002 J. High Energy Phys. JHEP11(2002)037 [SPIRES] [hep-th/0209231] and references therein Journal of Cosmology and Astroparticle Physics 10 (2003) 003 (stacks.iop.org/JCAP/2003/i=10/a=003) JCAP 10(2003)003 · arXiv
  3. Kaloper N, Kleban M, Lawrence A E and Shenker S, Signatures of short distance physics in the cosmic microwave background, 2002 Phys. Rev. D 66 123510 [SPIRES] [hep-th/0201158] · arXiv
  4. Shiu G and Wasserman I, On the signature of short distance scale in the cosmic microwave background, 2002 Phys. Lett. B 536 1 [SPIRES] [hep-th/0203113] · arXiv
  5. Knox L, Future probes of the primordial scalar and tensor perturbation spectra: prospects from the CMB, cosmic shear and high-volume redshift surveys, 2003 Preprint astro-ph/0304370 · arXiv
  6. Maldacena J, Non-Gaussian features of primordial fluctuations in single field inflationary models, 2003 J. High Energy Phys. JHEP05(2003)013 [SPIRES] [astro-ph/0210603] · arXiv
  7. Acquaviva V, Bartolo N, Matarrese S and Riotto A, Second-order cosmological perturbations from inflation, 2002 Preprint astro-ph/0209156 · arXiv
  8. For recent experimental limits on non-Gaussianity in the CMBR see Komatsu E et al, First year Wilkinson Microwave Anisotropy Probe (WMAP) observations: tests of Gaussianity, 2003 Preprint astro-ph/0302223 and references therein · arXiv
  9. Bartolo N, Matarrese S and Riotto A, Non-Gaussianity from inflation, 2002 Phys. Rev. D 65 103505 [SPIRES] [hep-ph/0112261] · arXiv
  10. Bernardeau F and Uzan J P, Non-Gaussianity in multi-field inflation, 2002 Phys. Rev. D 66 103506 [SPIRES] [hep-ph/0207295] · arXiv
  11. Lyth D H, Ungarelli C and Wands D, The primordial density perturbation in the curvaton scenario, 2003 Phys. Rev. D 67 023503 [SPIRES] [astro-ph/0208055] · arXiv
  12. Dvali G, Gruzinov A and Zaldarriaga M, A new mechanism for generating density perturbations from inflation, 2003 Preprint astro-ph/0303591 · arXiv
  13. Zaldarriaga M, Non-Gaussianities in models with a varying inflaton decay rate, 2003 Preprint astro-ph/0306006 · arXiv
  14. Arkani-Hamed N, Cheng H C, Creminelli P and Randall L, Extranatural inflation, 2003 Preprint hep-th/0301218 · arXiv
  15. Arkani-Hamed N, Cheng H C, Creminelli P and Randall L, Pseudonatural inflation, 2003 Preprint hep-th/0302034 · arXiv
  16. Kaplan D E and Weiner N J, Little inflatons and gauge inflation, 2003 Preprint hep-ph/0302014 · arXiv
  17. Armendariz-Picon C, Damour T and Mukhanov V, k-inflation, 1999 Phys. Lett. B 458 209 [SPIRES] [hep-th/9904075] · arXiv
  18. Komatsu E, The pursuit of non-Gaussian fluctuations in the Cosmic Microwave Background, 2002 Preprint astro-ph/0206039 · arXiv
  19. Verde L, Wang L M, Heavens A and Kamionkowski M, Large-scale structure, the cosmic microwave background, and primordial non-Gaussianity, 2000 Mon. Not. R. Astron. Soc. 313 L141 [astro-ph/9906301] · arXiv
  20. Verde L, Jimenez R, Kamionkowski M and Matarrese S, Tests for primordial non-Gaussianity, 2001 Mon. Not. R. Astron. Soc. 325 412 [astro-ph/0011180] · arXiv
  21. Gaztanaga E and Wagg J, three-point temperature anisotropies in WMAP: Limits on CMB non-Gaussianities and non-linearities, 2003 Preprint astro-ph/0305327 · arXiv

Cited by

Sorted by citations

Authors
Creminelli, P.
Affiliations
Harvard University (US)
Corresponding author
Creminelli, Paolo
Venue
Journal of Cosmology and Astroparticle Physics
Published
2003-10-03
Volume
2003
Issue
10
Pages
003-003
ISSN
  • 1475-7508 (ISSN-L)
  • 1475-7516
OpenAlex
W2104264206
Cited by
270
References
0
Citations by year
2026: 3 · 2025: 8 · 2024: 11 · 2023: 10 · 2022: 13 · 2021: 5 · 2020: 7 · 2019: 9 · 2018: 8 · 2017: 7 · 2016: 10 · 2015: 8 · 2014: 9 · 2013: 9 · 2012: 21
FWCI
7.52
Type
journal article
Language
en
Open access
Locations
  • Journal of Cosmology and Astroparticle Physics (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
  • arXiv (Cornell University)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
  • Physical Sciences › Physics and Astronomy › Statistical and Nonlinear Physics › Noncommutative and Quantum Gravity Theories
  • Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Black Holes and Theoretical Physics
Keywords
non-Gaussianity, single-field inflation, higher-dimensional operators, slow-roll inflation, three-point functions, bispectrum, angular dependence, effective field theory, primordial scalar perturbations

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