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Non-Gaussianities in DBI inflation with angular motion
DOI: 10.1103/PhysRevD.90.023515 Bibcode: 2014PhRvD..90b3515K

Kidani, Taichi; Koyama, Kazuya

We study DBI spinflation models with angular potentials that are derived in string theory. We analyze the background dynamics with different parameter sets and study the impact of changing each parameter on inflationary dynamics. It is known that the conversion of the entropy perturbation into the curvature perturbation gives multifield Dirac-Born…

2014 Physical Review D
Planck 5
Updated constraints on large field hybrid inflation
DOI: 10.1103/PhysRevD.90.083527 Bibcode: 2014PhRvD..90h3527C

Clesse, Sébastien; Rekier, Jérémy

We revisit the status of hybrid inflation in the light of Planck and recent BICEP2 results, taking care of possible transient violations of the slow-roll conditions as the field passes from the large field to the vacuum dominated phase. The usual regime where observable scales exit the Hubble radius in the vacuum dominated phase predicts a blue sc…

2014 Physical Review D
Planck 5
Planck constraints on neutrino isocurvature density perturbations
DOI: 10.1103/PhysRevD.90.083531 Bibcode: 2014PhRvD..90h3531D

Di Valentino, Eleonora; Melchiorri, Alessandro

The recent cosmic microwave background data from the Planck satellite experiment, when combined with Hubble Space Telescope determinations of the Hubble constant, are compatible with a larger, nonstandard number of relativistic degrees of freedom at recombination, parametrized by the neutrino effective number Neff . In the curvaton scen…

2014 Physical Review D
Planck 5
Observational effects of the early episodically dominating dark energy
DOI: 10.1103/PhysRevD.90.083526 Bibcode: 2014PhRvD..90h3526P

Park, Chan-Gyung; Lee, Jae-heon; Hwang, Jai-chan +1 more

We investigate the observational consequences of the early episodically dominating dark energy on the evolution of cosmological structures. For this aim, we introduce the minimally coupled scalar-field dark energy model with the Albrecht-Skordis potential, which allows a sudden ephemeral domination of a dark energy component during the radiation o…

2014 Physical Review D
Planck 2
Is Planck data consistent with primordial deuterium measurements?
DOI: 10.1103/PhysRevD.90.103514 Bibcode: 2014PhRvD..90j3514S

Melchiorri, Alessandro; Salvati, Laura; Said, Najla

The recent measurements of the cosmic microwave background anisotropies provided by the Planck satellite experiment have significantly improved the constraints on several cosmological parameters. In this brief paper we point out a small but interesting tension present between recent values of the primordial deuterium measured from quasar absorptio…

2014 Physical Review D
Planck 1
Test for the zero mean hypothesis in cosmology
DOI: 10.1103/PhysRevD.90.123008 Bibcode: 2014PhRvD..90l3008I

Ichiki, Kiyotomo

One working hypothesis on which analyses of cosmological data are based is the zero ensemble mean hypothesis, which is related to the statistical homogeneity of cosmological perturbations. This hypothesis, however, should be tested by observational data in the current era of precision cosmology. Herein, we test the hypothesis by analyzing recent, …

2014 Physical Review D
Planck 1
Higher order nonlinear parameters with Planck constraints
DOI: 10.1103/PhysRevD.89.023516 Bibcode: 2014PhRvD..89b3516G

Takahashi, Tomo; Gong, Jinn-Ouk

We investigate how higher-order nonlinear parameters affect lower-order ones through loop effects. We calculate the loop corrections up to two loops and explicitly show that the tree contribution is stable against loop terms in most cases. We argue that, nevertheless, observational constraints on nonlinear parameters such as fNL and τ

2014 Physical Review D
Planck 1