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Improved Constraints on Primordial Gravitational Waves using Planck, WMAP, and BICEP/Keck Observations through the 2018 Observing Season
We present results from an analysis of all data taken by the BICEP2, Keck Array, and
BICEP3 CMB polarization experiments up to and including the 2018 observing season. We …
BICEP3 CMB polarization experiments up to and including the 2018 observing season. We …
Primordial backgrounds of relic gravitons
M Giovannini - Progress in Particle and Nuclear Physics, 2020 - Elsevier
The diffuse backgrounds of relic gravitons with frequencies ranging between the aHz band
and the GHz region encode the ultimate information on the primeval evolution of the plasma …
and the GHz region encode the ultimate information on the primeval evolution of the plasma …
Detection of -Mode Polarization at Degree Angular Scales by BICEP2
We report results from the BICEP2 experiment, a cosmic microwave background (CMB)
polarimeter specifically designed to search for the signal of inflationary gravitational waves …
polarimeter specifically designed to search for the signal of inflationary gravitational waves …
Five-year wilkinson microwave anisotropy probe* observations: cosmological interpretation
ABSTRACT The Wilkinson Microwave Anisotropy Probe (WMAP) 5-year data provide
stringent limits on deviations from the minimal, six-parameter Λ cold dark matter model. We …
stringent limits on deviations from the minimal, six-parameter Λ cold dark matter model. We …
MultiNest: an efficient and robust Bayesian inference tool for cosmology and particle physics
We present further development and the first public release of our multimodal nested
sampling algorithm, called MultiNest. This Bayesian inference tool calculates the evidence …
sampling algorithm, called MultiNest. This Bayesian inference tool calculates the evidence …
Three-year Wilkinson Microwave Anisotropy Probe (WMAP) observations: implications for cosmology
A simple cosmological model with only six parameters (matter density, Ω mh 2, baryon
density, Ω bh 2, Hubble constant, H 0, amplitude of fluctuations, σ 8, optical depth, τ, and a …
density, Ω bh 2, Hubble constant, H 0, amplitude of fluctuations, σ 8, optical depth, τ, and a …
[HTML][HTML] Review of particle physics
K Nakamura - Journal of Physics G: Nuclear and …, 2010 - bibliotecadigital.exactas.uba.ar
This biennial Review summarizes much of particle physics. Using data from previous
editions, plus 2158 new measurements from 551 papers, we list, evaluate, and average …
editions, plus 2158 new measurements from 551 papers, we list, evaluate, and average …
A measurement of the cosmic microwave background B-mode polarization power spectrum at sub-degree scales with POLARBEAR
PAR Ade, Y Akiba, AE Anthony, K Arnold… - The Astrophysical …, 2014 - iopscience.iop.org
We report a measurement of the B-mode polarization power spectrum in the cosmic
microwave background (CMB) using the Polarbear experiment in Chile. The faint B-mode …
microwave background (CMB) using the Polarbear experiment in Chile. The faint B-mode …
Bayes in the sky: Bayesian inference and model selection in cosmology
R Trotta - Contemporary Physics, 2008 - Taylor & Francis
The application of Bayesian methods in cosmology and astrophysics has flourished over the
past decade, spurred by data sets of increasing size and complexity. In many respects …
past decade, spurred by data sets of increasing size and complexity. In many respects …
Five-year wilkinson microwave anisotropy probe* observations: likelihoods and parameters from the Wmap data
This paper focuses on cosmological constraints derived from analysis of WMAP data alone.
A simple ΛCDM cosmological model fits the five-year WMAP temperature and polarization …
A simple ΛCDM cosmological model fits the five-year WMAP temperature and polarization …