Cited by 49Cosmology and Gravitation TheoriesNoncommutative and Quantum Gravity TheoriesDark Matter and Cosmic Phenomena

Non-Gaussianity for a two component hybrid model of inflation

Open access
Alabidi, Laila·2006·Journal of Cosmology and Astroparticle Physics

Abstract

We consider a hybrid model of inflation, in which two fields drive inflation. Our results show that, if the parameters are finely tuned, this model may generate an observable non-Gaussian contribution to the curvature spectrum, within the limits allowed by the recent WMAP year three data. We show that if one field has a mass η ϕ <0 and an initial value ϕ * <0.025 M pl , while the other field has a mass η σ >0 and an initial field value 0.45 M pl <σ≤ M pl , then the non-Gaussianity is observable with , but that f NL becomes much less than the observable limit should we take both masses to have the same sign, or if we loosened the constraints on the initial field values.

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 · 10.1088/1475-7516/2006/10/015

Cites

1 of 1 references verified0 citation errors · 0 not checkable

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?

  • Our formula for f_NL^(4) is consistent with the calculation of [5].

    “Our formula for f (4) NL is also consistent with the calculation of [5] but our analysis of the parameter space is more extensive and in particular it allows for very small initial field values.”
  • We find a region with much larger non-Gaussianity than was found in [5].

    “We therefore find a region with much larger non-Gaussianity than was found in [5].”
  • Our analysis of the parameter space is more extensive than [5] and allows for very small initial field values.

    “Our formula for f (4) NL is also consistent with the calculation of [5] but our analysis of the parameter space is more extensive and in particular it allows for very small initial field values.”

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

Flagged first, then by citations

Research works printed but not linked: 14

  1. Lyth D H and Rodriguez Y, The inflationary prediction for primordial non-gaussianity, 2005 Phys. Rev. Lett. 95 121302 [SPIRES] [astro-ph/0504045] · DOI · Paper page
  2. Zaballa I, Rodriguez Y and Lyth D H, Higher order contributions to the primordial non-gaussianity, 2006 J. Cosmol. Astropart. Phys. JCAP06(2006)013 [SPIRES] [astro-ph/0603534] · DOI
  3. Malik K A and Wands D, Evolution of second order cosmological perturbations, 2004 Class. Quantum Grav. 21 L65 [SPIRES] [astro-ph/0307055] · DOI
  4. Sasaki M and Stewart E D, A general analytic formula for the spectral index of the density perturbations produced during inflation, 1996 Prog. Theor. Phys. 95 71 [SPIRES] [astro-ph/9507001] · DOI · Paper page
  5. Lyth D H, Generating the curvature perturbation at the end of inflation, 2005 J. Cosmol. Astropart. Phys. JCAP11(2005)006 [SPIRES] [astro-ph/0510443] · DOI
  6. Salem M P, On the generation of density perturbations at the end of inflation, 2005 Phys. Rev. D 72 123516 [SPIRES] [astro-ph/0511146] · DOI
  7. Alabidi L and Lyth D, Curvature perturbation from symmetry breaking the end of inflation, 2006 Preprint astro-ph/0604569 · arXiv
  8. Boubekeur L and Lyth D H, Detecting a small perturbation through its non-gaussianity, 2006 Phys. Rev. D 73 021301 [SPIRES] [astro-ph/0504046] · DOI
  9. Lyth D H and Zaballa I, A bound concerning primordial non-gaussianity, 2005 J. Cosmol. Astropart. Phys. JCAP10(2005)005 [SPIRES] [astro-ph/0507608] · DOI
  10. Komatsu E and Spergel D N, Acoustic signatures in the primary microwave background bispectrum, 2001 Phys. Rev. D 63 063002 [SPIRES] [astro-ph/0005036] · DOI
  11. Bartolo N, Komatsu E, Matarrese S and Riotto A, Non-gaussianity from inflation: theory and observations, 2004 Phys. Rep. 402 103 [SPIRES] [astro-ph/0406398] · DOI
  12. Liddle A R and Lyth D H, 2000 Cosmological Inflation and Large-scale Structure (Cambridge: University Press) p 400
  13. Spergel D N et al , Wilkinson Microwave Anisotropy Probe (WMAP) three year results: Implications for cosmology, 2006 Preprint astro-ph/0603449 · arXiv
  14. Alabidi L and Lyth D H, Inflation models and observation, 2006 J. Cosmol. Astropart. Phys. JCAP05(2006)016 [SPIRES] [astro-ph/0510441] Journal of Cosmology and Astroparticle Physics 10 (2006) 015 (stacks.iop.org/JCAP/2006/i=10/a=015) · DOI

Cited by

Sorted by citations

Authors
Alabidi, L.
Affiliations
Lancaster University (GB)
Corresponding author
Alabidi, Laila
Venue
Journal of Cosmology and Astroparticle Physics
Published
2006-10-20
Volume
2006
Issue
10
Pages
015-015
ISSN
  • 1475-7508 (ISSN-L)
  • 1475-7516
OpenAlex
W2055902244
Cited by
49
References
1
Citations by year
2026: 1 · 2021: 1 · 2018: 1 · 2017: 1 · 2016: 1 · 2014: 2 · 2013: 3 · 2012: 3
FWCI
3.64
Type
journal article
Language
en
Open access
Locations
  • Journal of Cosmology and Astroparticle Physics (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • arXiv (Cornell University)
Funders
Dowager Countess Eleanor Peel Trust
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 › Dark Matter and Cosmic Phenomena
Keywords
hybrid inflation, non-Gaussianity, two-field inflation, curvature perturbations, f_NL, scalar field mass, primordial power spectrum

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