Search Publications

Post-Planck dark energy constraints
DOI: 10.1103/PhysRevD.91.083005 Bibcode: 2015PhRvD..91h3005H

Hazra, Dhiraj Kumar; Pal, Supratik; Sen, Anjan A. +2 more

We constrain plausible dark energy models using the recently published cosmic microwave background (CMB) temperature anisotropy data from Planck together with WMAP9 low-ℓ polarization data and the data from low redshift surveys. To circumvent the limitations of any particular equation of state toward describing all existing dark energy models, we …

2015 Physical Review D
Planck 34
Searching for features of a string-inspired inflationary model with cosmological observations
DOI: 10.1103/PhysRevD.92.121303 Bibcode: 2015PhRvD..92l1303C

Hu, Bin; Cai, Yi-Fu; Ferreira, Elisa G. M. +1 more

The latest Planck results show a power deficit in the temperature anisotropies near ℓ≈20 in the cosmic microwave background (CMB). This observation can hardly be explained within the standard inflationary Λ -cold-dark-matter (Λ CDM ) scenario. In this paper we consider a string theory inspired inflationary model (axion monodromy inflation) with a …

2015 Physical Review D
Planck 31
Robustness of cosmological axion mass limits
DOI: 10.1103/PhysRevD.91.123505 Bibcode: 2015PhRvD..91l3505D

Di Valentino, Eleonora; Mena, Olga; Gariazzo, Stefano +1 more

We present the cosmological bounds on the thermal axion mass in an extended cosmological scenario in which the primordial power spectrum of scalar perturbations differs from the usual power-law shape predicted by the simplest inflationary models. The power spectrum is instead modeled by means of a "piecewise cubic Hermite interpolating polynomial"…

2015 Physical Review D
Planck 31
Searching for primordial localized features with CMB and LSS spectra
DOI: 10.1103/PhysRevD.91.064039 Bibcode: 2015PhRvD..91f4039H

Hu, Bin; Torrado, Jesús

Inspired by the study of mild transient reductions in the speed of sound of the adiabatic mode during inflation, we search for a primordial localized feature imprinted in cosmic microwave background and large-scale structure formation observables. We find some common oscillatory patterns both in the Planck CMB temperature-temperature power spectru…

2015 Physical Review D
Planck 30
CMB power spectrum of Nambu-Goto cosmic strings
DOI: 10.1103/PhysRevD.91.083519 Bibcode: 2015PhRvD..91h3519L

Shellard, E. P. S.; Landriau, Martin; Lazanu, Andrei

We improve predictions of the cosmic microwave background (CMB) power spectrum induced by cosmic strings by using source terms obtained from Nambu-Goto network simulations in an expanding universe. We use three high-resolution cosmic string simulations that cover the entire period from recombination until late-time Λ domination to calculate unequa…

2015 Physical Review D
Planck 28
Constraints on the early and late integrated Sachs-Wolfe effects from the Planck 2015 cosmic microwave background anisotropies in the angular power spectra
DOI: 10.1103/PhysRevD.92.063534 Bibcode: 2015PhRvD..92f3534C

Melchiorri, Alessandro; Cabass, Giovanni; Gerbino, Martina +3 more

The integrated Sachs-Wolfe (ISW) effect predicts additional anisotropies in the cosmic microwave background (CMB) due to time variation of the gravitational potential when the expansion of the Universe is not matter dominated. The ISW effect is therefore expected in the early Universe, due to the presence of relativistic particles at recombination…

2015 Physical Review D
Planck 27
Sound speed of scalar field dark energy: Weak effects and large uncertainties
DOI: 10.1103/PhysRevD.91.083007 Bibcode: 2015PhRvD..91h3007S

Sergijenko, Olga; Novosyadlyj, Bohdan

The possibility of a reconstruction of the Lagrangian for the scalar field dark energy with constant effective sound speed cs is analyzed. It is found that such a reconstruction can be made with accuracy up to an arbitrary constant. The value of cs is estimated together with other dark energy parameters (Ωd e , w

2015 Physical Review D
Planck 27
Cosmological tests of modified gravity: Constraints on F (R ) theories from the galaxy clustering ratio
DOI: 10.1103/PhysRevD.91.103503 Bibcode: 2015PhRvD..91j3503B

Brax, Philippe; Marinoni, Christian; Bel, Julien +1 more

The clustering ratio η , a large-scale structure observable originally designed to constrain the shape of the power spectrum of matter density fluctuations, is shown to provide a sensitive probe of the nature of gravity in the cosmological regime. We apply this analysis to F (R ) theories of gravity using the luminous red galaxy sample extracted f…

2015 Physical Review D
Planck 26
Constraints on the exponential f (R ) model from latest Hubble parameter measurements
DOI: 10.1103/PhysRevD.91.044019 Bibcode: 2015PhRvD..91d4019C

Geng, Chao-Qiang; Lee, Chung-Chi; Chen, Yun +2 more

We investigate the viable exponential f (R ) gravity in the metric formalism with f (R )=-β Rs(1 -e-R /Rs). The latest sample of the Hubble parameter measurements with 23 data points is used to place bounds on this f (R ) model. A joint analysis is also performed with the luminosity distances of type Ia supernovae …

2015 Physical Review D
Planck 23
Generation of large-scale magnetic fields, non-Gaussianity, and primordial gravitational waves in inflationary cosmology
DOI: 10.1103/PhysRevD.91.043509 Bibcode: 2015PhRvD..91d3509B

Bamba, Kazuharu

The generation of large-scale magnetic fields in inflationary cosmology is explored, in particular, in a kind of moduli inflation motivated by racetrack inflation in the context of the type IIB string theory. In this model, the conformal invariance of the hypercharge electromagnetic fields is broken thanks to the coupling of both the scalar and ps…

2015 Physical Review D
Planck 22