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Cited by 274

The DOI matches its Crossref record; 104 of the 104 references it cites were found in a registry or an index.

Enhanced non-Gaussianity from excited initial states

Open access
Holman, R, Tolley, Andrew J·2008·Journal of Cosmology and Astroparticle Physics

Abstract

We use the techniques of effective field theory in an expanding universe to examine the effect of choosing an excited inflationary initial state built over the Bunch–Davies state on the CMB bi-spectrum. We find that, even for Hadamard states, there are unexpected enhancements in the bi-spectrum for certain configurations in momentum space due to interactions of modes in the early stages of inflation. These enhancements can be parametrically larger than the standard ones and are potentially observable in future data. These initial state effects have a characteristic signature in l -space which distinguishes them from the usual contributions, with the enhancement being most pronounced for configurations corresponding to flattened triangles for which two momenta are collinear.

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Crossref · 10.1088/1475-7516/2008/05/001

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Metadata

Authors
Holman, R., & Tolley, A. J.
Venue
Journal of Cosmology and Astroparticle Physics
Published
2008-05-06
Volume
2008
Issue
05
Pages
001
ISSN
  • 1475-7508 (ISSN-L)
  • 1475-7516
OpenAlex
W1978365844
Cited by
274
References
104
FWCI
13.36
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Enhanced non-Gaussianity from excited initial states. https://app.cochat.ai/papers/10.1088/1475-7516/2008/05/001
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Holman, R., & Tolley, A. J. (2008). Enhanced non-Gaussianity from excited initial states. Journal of Cosmology and Astroparticle Physics. https://doi.org/10.1088/1475-7516/2008/05/001

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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.