Primordial non-Gaussianity in multi-scalar slow-roll inflation
Open accessAbstract
We analyse the non-Gaussianity for primordial curvature perturbations generated in a multi-scalar slow-roll inflation model including the model with non-separable potential by making use of δ N formalism. Many authors have investigated the possibility of large non-Gaussianity for the models with separable potential, and they have found that the non-linear parameter, f NL , is suppressed by the slow-roll parameters. We show that for the non-separable models f NL is given by the product of a factor which is suppressed by the slow-roll parameters and a possible enhancement factor which is given by exponentials of quantities of O(1).
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The condition to neglect quantum fluctuations is |χ̇|π/H^2 > √3/2.
“In order that we can neglect the effect of the quantum fluctuations, the condition we require on the background trajectory is | ˙ χ | π/H 2 > √ 3 / 2 [40].”
From Conditions for large non-Gaussianity in two-field slow-roll inflation (2008) · cites this paper as [40]
The background-equations section (p. 3) discusses neglecting the non-Gaussian contribution of initial field perturbations, not a condition for neglecting quantum fluctuations along a background trajectory. Searches for quantum fluctuations, χ̇, and √3/2 found no passage stating the claimed inequality; equations in our copy are not decoded. (LLM, conf=0.72)
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Cites
Non-Gaussianities in two-field inflation
Vernizzi, F., & Wands, D. (2006) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2006/05/019 · Cited by 274 · see citing works
Spectral running and non-Gaussianity from slow-roll inflation in generalized two-field models
Choi, K.-Y., Hall, L. M. H., & Bruck, C. V. D. (2007) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2007/02/029 · Cited by 98 · see citing works
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Research works printed but not linked: 13
- [16]T. Moroi and T. Takahashi, Phys. Lett. B 522 , 215 (2001) [Erratum-ibid. B 539 , 303 (2002)] [arXiv:hep-ph/0110096]. · arXiv
- [17]D. H. Lyth and D. Wands, Phys. Lett. B 524 , 5 (2002) [arXiv:hep-ph/0110002]. · arXiv
- [18]D. H. Lyth, C. Ungarelli and D. Wands, Phys. Rev. D 67 , 023503 (2003) [arXiv:astro-ph/0208055]. · arXiv
- [19]N. Bartolo, S. Matarrese and A. Riotto, Phys. Rev. D 69 , 043503 (2004) [arXiv:hep-ph/0309033]. · arXiv
- [20]K. A. Malik and D. H. Lyth, JCAP 0609 , 008 (2006) [arXiv:astro-ph/0604387]. · arXiv
- [21]M. Sasaki, J. Valiviita and D. Wands, Phys. Rev. D 74 , 103003 (2006) [arXiv:astro-ph/0607627]. J. Valiviita, M. Sasaki and D. Wands, arXiv:astro-ph/0610001. · arXiv
- [22]G. I. Rigopoulos, E. P. S. Shellard and B. W. van Tent, Phys. Rev. D 73 , 083521 (2006) [arXiv:astro-ph/0504508]. G. I. Rigopoulos, E. P. S. Shellard and B. W. van Tent, Phys. Rev. D 73 , 083522 (2006) [arXiv:astro-ph/0506704]. · arXiv
- [23]S. A. Kim and A. R. Liddle, Phys. Rev. D 74 , 063522 (2006) [arXiv:astro-ph/0608186]. · arXiv
- [24]F. Vernizzi and D. Wands, JCAP 0605 , 019 (2006) [arXiv:astro-ph/0603799]. · arXiv
- [25]T. Battefeld and R. Easther, JCAP 0703 , 020 (2007) [arXiv:astro-ph/0610296]. · arXiv
- [27]K. Y. Choi, L. M. H. Hall and C. van de Bruck, JCAP 0702 , 029 (2007) [arXiv:astro-ph/0701247]. · arXiv
- [28]M. Sasaki and E. D. Stewart, Prog. Theor. Phys. 95 , 71 (1996) [arXiv:astro-ph/9507001]. · arXiv
- [29]M. Sasaki and T. Tanaka, Prog. Theor. Phys. 99 , 763 (1998) [arXiv:gr-qc/9801017]. · arXiv
Cited by
Sorted by citations
Conditions for large non-Gaussianity in two-field slow-roll inflation
Byrnes, C. T., Choi, K.-Y., & Hall, L. M. H. (2008) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2008/10/008 · Cited by 143 · see citing works
- Authors
- Yokoyama, S., Suyama, T., & Tanaka, T.
- Affiliations
- Kyoto University (JP)
- Institute for Cosmic Ray Research (JP)
- Venue
- Journal of Cosmology and Astroparticle Physics
- Publisher
- IOP Publishing
- Published
- 2007-07-17
- Volume
- 2007
- Issue
- 07
- Pages
- 013-013
- ISSN
- 1475-7508 (ISSN-L)
- 1475-7516
- OpenAlex
- W2118496247
- Cited by
- 103
- References
- 2
- Citations by year
- 2026: 2 · 2025: 2 · 2024: 2 · 2022: 2 · 2021: 2 · 2020: 2 · 2018: 6 · 2017: 2 · 2016: 9 · 2015: 4 · 2014: 7 · 2013: 11 · 2012: 14
- FWCI
- 5.59
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Locations
- Journal of Cosmology and Astroparticle Physics (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- arXiv (Cornell University)
- Funders
- Japan Society for the Promotion of Science
- 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 › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Keywords
- primordial non-Gaussianity, slow-roll inflation, curvature perturbations, delta N formalism, inflationary perturbations
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