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相关论文: WMAPping inflationary physics

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We extract parameters relevant for distinguishing among single-field inflation models from the Wilkinson Microwave Anisotropy Probe (WMAP) three-year data set, and also from WMAP in combination with the Sloan Digital Sky Survey (SDSS)…

天体物理学 · 物理学 2008-11-26 William H. Kinney , Edward W. Kolb , Alessandro Melchiorri , Antonio Riotto

We assay how inflationary models whose properties are dominated by the dynamics of a single scalar field are constrained by cosmic microwave background (CMB) data from the Wilkinson Microwave Anisotropy Probe (WMAP). We classify…

高能物理 - 唯象学 · 物理学 2009-09-15 V. Barger , Hye-Sung Lee , Danny Marfatia

We confront predictions of inflationary scenarios with the WMAP data, in combination with complementary small-scale CMB measurements and large-scale structure data. The WMAP detection of a large-angle anti-correlation in the…

The implications of the WMAP (Wilkinson Microwave Anisotropy Probe) third year data for inflation are investigated using both the slow-roll approximation and an exact numerical integration of the inflationary power spectra including a…

天体物理学 · 物理学 2009-11-11 Jerome Martin , Christophe Ringeval

We clarify inflaton models by considering them as effective field theories in the Ginzburg-Landau spirit.In this new approach, the precise form of the inflationary potential is constructed from the present WMAP data, and a useful scheme is…

天体物理学 · 物理学 2009-11-10 D. Cirigliano , H. J. de Vega , N. G. Sanchez

We confront the predicted effects of hybrid inflationary models on the Cosmic Microwave Background (CMB) with three years of Wilkinson Microwave Anisotropy Probe (WMAP) observations. Using model selection, we compare the ability of a simple…

天体物理学 · 物理学 2010-10-27 Aurélien A. Fraisse

The first year WMAP measurement of the CMB temperature anisotropy is intriguingly consistent with a larger running of the inflationary scalar spectral index than would be expected for single-field inflation. We revisit the issue of a large…

天体物理学 · 物理学 2009-11-11 James M. Cline , Loison Hoi

We use cosmic microwave background (CMB) data from the 9-year WMAP release to derive constraints on monodromy inflation, which is characterized by a linear inflaton potential with a periodic modulation. We identify two possible periodic…

宇宙学与河外天体物理 · 物理学 2013-10-01 Hiranya Peiris , Richard Easther , Raphael Flauger

Observations of the temperature anisotropies in the Cosmic Microwave Background (CMB) radiation show that the models of inflation with the monomial potentials are inconsistent with the allowed $n_s-r$ bounds. However certain monomial…

宇宙学与河外天体物理 · 物理学 2022-03-17 Richa Arya , Raghavan Rangarajan

In addition to density perturbations, inflationary models of the early universe generally predict a stochastic background of gravitational waves or tensor fluctuations. By making use of the inflationary flow approach for single field models…

天体物理学 · 物理学 2008-11-26 Brett C. Friedman , Asantha Cooray , Alessandro Melchiorri

We present constraints on canonical single-field inflation derived from WMAP five year, ACBAR, QUAD, BICEP data combined with the halo power spectrum from SDSS LRG7. Models with a non-scale-invariant spectrum and a red tilt n_s < 1 are now…

宇宙学与河外天体物理 · 物理学 2010-04-30 Fabio Finelli , Jan Hamann , Samuel M. Leach , Julien Lesgourgues

Measurements of CMB temperature fluctuations by the Wilkinson Microwave Anisotropy Probe (WMAP) indicate that the fluctuation amplitude in one half of the sky differs from the amplitude in the other half. We show that such an asymmetry…

天体物理学 · 物理学 2008-12-30 Adrienne L. Erickcek , Marc Kamionkowski , Sean M. Carroll

Since this is a meeting on inflation the title of this talk should probably have been ``The cosmos as a lab for inflation''. I will illustrate how, by combining WMAP observations of the cosmic microwave background (CMB) with smaller scales…

天体物理学 · 物理学 2007-05-23 Licia verde

We constrain models of single field inflation with the pre-\textit{Planck} CMB data. The data used here is the 9-year Wilkinson Microwave Anisotropy Probe (\textit{WMAP}) data, South Pole Telescope (SPT) data and Atacama Cosmology Telescope…

宇宙学与河外天体物理 · 物理学 2015-06-15 Cheng Cheng , Qing-Guo Huang , Yin-Zhe Ma

The CMB power spectra are studied for different families of single field new and chaotic inflation models in the effective field theory approach to inflation. We implement a systematic expansion in 1/N_e where N_e ~ 50 is the number of…

天体物理学 · 物理学 2008-11-26 D. Boyanovsky , H. J. de Vega , C. M. Ho , N. G. Sanchez

We study the single field slow-roll inflation models that better fit the available CMB and LSS data including the three years WMAP data: new inflation and hybrid inflation. We study them as effective field theories in the Ginsburg-Landau…

天体物理学 · 物理学 2009-11-11 H. J. de Vega , N. G. Sanchez

The Wilkinson Microwave Anisotropy Probe (WMAP) three year results are used to constraint non-minimal inflation models. Two different non-minimally coupled scalar field potentials are considered to calculate corresponding slow-roll…

天体物理学 · 物理学 2008-12-25 Kourosh Nozari , S. Davood Sadatian

Recent fits of cosmological parameters by the Wilkinson Microwave Anisotropy Probe (WMAP) measurement favor a primordial scalar spectrum with varying index. This result, if stands, could severely constrain inflation model buildings. Most…

天体物理学 · 物理学 2008-11-26 Bo Feng , Mingzhe Li , Ren-Jie Zhang , Xinmin Zhang

Inflation in a five-dimensional brane world model with two boundary branes is studied. We make use of the moduli space approximation whereby the low energy theory reduces to a four-dimensional biscalar-tensor gravity plus a minimally…

天体物理学 · 物理学 2009-11-13 Christophe Ringeval , Philippe Brax , Carsten van de Bruck , Anne-Christine Davis

In this paper we will analyse the constraints on a sub-Planckian excursion of a single inflaton field, which would yield a large tensor to scalar ratio, while explaining the temperature anisotropy of the cosmic microwave background (CMB)…

高能物理 - 理论 · 物理学 2014-04-01 Sayantan Choudhury , Anupam Mazumdar
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