Features and new physical scales in primordial observables: theory and observation
All cosmological observations to date are consistent with adiabatic, Gaussian and nearly
scale invariant initial conditions. These findings provide strong evidence for a particular …
scale invariant initial conditions. These findings provide strong evidence for a particular …
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 …
[图书][B] Inflation and string theory
D Baumann, L McAllister - 2015 - books.google.com
The past two decades have seen transformative advances in cosmology and string theory.
Observations of the cosmic microwave background have revealed strong evidence for …
Observations of the cosmic microwave background have revealed strong evidence for …
Gravitational waves from inflation
MC Guzzetti, N Bartolo, M Liguori… - La Rivista del Nuovo …, 2016 - Springer
The production of a stochastic background of gravitational waves is a fundamental
prediction of any cosmological inflationary model. The features of such a signal encode …
prediction of any cosmological inflationary model. The features of such a signal encode …
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 …
Primordial gravitational waves from axion-gauge fields dynamics
E Dimastrogiovanni, M Fasiello… - Journal of Cosmology and …, 2017 - iopscience.iop.org
Inspired by the chromo-natural inflation model of Adshead&Wyman, we reshape its scalar
content to relax the tension with current observational bounds. Besides an inflaton, the setup …
content to relax the tension with current observational bounds. Besides an inflaton, the setup …
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 …
CMB-S4 technology book
CMB-S4 is a proposed experiment to map the polarization of the Cosmic Microwave
Background (CMB) to nearly the cosmic variance limit for angular scales that are accessible …
Background (CMB) to nearly the cosmic variance limit for angular scales that are accessible …
Four-year Cosmology Large Angular Scale Surveyor (CLASS) observations: on-sky receiver performance at 40, 90, 150, and 220 GHz frequency bands
Abstract The Cosmology Large Angular Scale Surveyor (CLASS) observes the polarized
cosmic microwave background (CMB) over the angular scales of 1≲ θ≤ 90 with the aim of …
cosmic microwave background (CMB) over the angular scales of 1≲ θ≤ 90 with the aim of …
Second season QUIET observations: Measurements of the cosmic microwave background polarization power spectrum at 95 GHz
D Araujo, C Bischoff, A Brizius, I Buder… - The Astrophysical …, 2012 - iopscience.iop.org
ABSTRACT The Q/U Imaging ExperimenT (QUIET) has observed the cosmic microwave
background (CMB) at 43 and 95 GHz. The 43 GHz results have been published in a …
background (CMB) at 43 and 95 GHz. The 43 GHz results have been published in a …