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
PAR Ade, RW Aikin, D Barkats, SJ Benton… - Physical Review Letters, 2014 - APS
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 …
[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 …
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 …
BICEP2 I: detection of B-mode polarization at degree angular scales
PA Ade, RW Aikin, D Barkats, SJ Benton… - arXiv preprint arXiv …, 2014 - arxiv.org
(abridged for arXiv) We report results from the BICEP2 experiment, a cosmic microwave
background (CMB) polarimeter specifically designed to search for the signal of inflationary …
background (CMB) polarimeter specifically designed to search for the signal of inflationary …
The Atacama cosmology telescope: CMB polarization at 200< ℓ< 9000
We report on measurements of the cosmic microwave background (CMB) and celestial
polarization at 146 GHz made with the Atacama Cosmology Telescope Polarimeter …
polarization at 146 GHz made with the Atacama Cosmology Telescope Polarimeter …
CLASS: the cosmology large angular scale surveyor
The Cosmology Large Angular Scale Surveyor (CLASS) is an experiment to measure the
signature of a gravitationalwave background from inflation in the polarization of the cosmic …
signature of a gravitationalwave background from inflation in the polarization of the cosmic …
ACTPol: a polarization-sensitive receiver for the Atacama Cosmology Telescope
MD Niemack, PAR Ade, J Aguirre… - … , and Far-Infrared …, 2010 - spiedigitallibrary.org
The six-meter Atacama Cosmology Telescope (ACT) in Chile was built to measure the
cosmic microwave background (CMB) at arcminute angular scales. We are building a new …
cosmic microwave background (CMB) at arcminute angular scales. We are building a new …
Five-year wilkinson microwave anisotropy probe* observations: Angular power spectra
We present the temperature and polarization angular power spectra of the cosmic
microwave background derived from the first five years of Wilkinson Microwave Anisotropy …
microwave background derived from the first five years of Wilkinson Microwave Anisotropy …