Journal
PHYSICAL REVIEW D
Volume 85, Issue 12, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.85.123519
Keywords
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Funding
- Spanish Ministerio de Ciencia e Innovacion (MICINN) [AYA2009-13936]
- Consolider-Ingenio [CSD2007- 00060]
- European Commission Marie Curie Initial Training Network CosmoComp [PITN-GA-2009-238356]
- Generalitat de Catalunya [2009-SGR-1398]
- Juan de la Cierva
- NSF [AST-1109432]
- NASA [NNA10A171G]
- National de Cosmologie et Galaxies
- Division Of Astronomical Sciences
- Direct For Mathematical & Physical Scien [1109432] Funding Source: National Science Foundation
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We present a new scheme for the general computation of cosmic propagators that allow to interpolate between standard perturbative results at low k and their expected large-k resummed behavior. This scheme is applicable to any multipoint propagator and allows the matching of perturbative low-k calculations to any number of loops to their large-k behavior, and can potentially be applied in case of nonstandard cosmological scenarios such as those with non-Gaussian initial conditions. The validity of our proposal is checked against previous prescriptions and measurements in numerical simulations showing a remarkably good agreement. Such a generic prescription for multipoint propagators provides the necessary building blocks for the computation of polyspectra in the context of the so-called Gamma expansion introduced by F. Bernardeau, M. Crocce, and R. ScoccimarroPhys. Rev. D 78, 103521 (2008).. As a concrete application we present a consistent calculation of the matter bispectrum at one-loop order.
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