Stochastic gravitational wave backgrounds

N Christensen - Reports on Progress in Physics, 2018 - iopscience.iop.org
A stochastic background of gravitational waves could be created by the superposition of a
large number of independent sources. The physical processes occurring at the earliest …

[HTML][HTML] Detection methods for stochastic gravitational-wave backgrounds: a unified treatment

JD Romano, NJ Cornish - Living reviews in relativity, 2017 - Springer
We review detection methods that are currently in use or have been proposed to search for a
stochastic background of gravitational radiation. We consider both Bayesian and frequentist …

Planck 2015 results-XX. Constraints on inflation

PAR Ade, N Aghanim, M Arnaud, F Arroja… - Astronomy & …, 2016 - aanda.org
We present the implications for cosmic inflation of the Planck measurements of the cosmic
microwave background (CMB) anisotropies in both temperature and polarization based on …

Causality constraints on corrections to the graviton three-point coupling

XO Camanho, JD Edelstein, J Maldacena… - Journal of High Energy …, 2016 - Springer
A bstract We consider higher derivative corrections to the graviton three-point coupling
within a weakly coupled theory of gravity. Lorentz invariance allows further structures …

The quest for B modes from inflationary gravitational waves

M Kamionkowski, ED Kovetz - Annual Review of Astronomy and …, 2016 - annualreviews.org
The search for the curl component (B mode) in the cosmic microwave background (CMB)
polarization induced by inflationary gravitational waves is described. The canonical single …

Testing general relativity with present and future astrophysical observations

E Berti, E Barausse, V Cardoso… - … and Quantum Gravity, 2015 - iopscience.iop.org
One century after its formulation, Einstein's general relativity (GR) has made remarkable
predictions and turned out to be compatible with all experimental tests. Most of these tests …

Planck intermediate results-XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes

R Adam, PAR Ade, N Aghanim, M Arnaud… - Astronomy & …, 2016 - aanda.org
The polarized thermal emission from diffuse Galactic dust is the main foreground present in
measurements of the polarization of the cosmic microwave background (CMB) at …

Joint Analysis of BICEP2/Keck Array and Planck Data

PAR Ade, N Aghanim, Z Ahmed, RW Aikin… - Physical review …, 2015 - APS
We report the results of a joint analysis of data from BICEP2/Keck Array and Planck. BICEP2
and Keck Array have observed the same approximately 400 deg 2 patch of sky centered on …

[HTML][HTML] Planck 2015 results-xiii. cosmological parameters

PAR Ade, N Aghanim, M Arnaud, M Ashdown… - Astronomy & …, 2016 - aanda.org
This paper presents cosmological results based on full-mission Planck observations of
temperature and polarization anisotropies of the cosmic microwave background (CMB) …

Planck 2015 results-III. LFI systematic uncertainties

PAR Ade, J Aumont, C Baccigalupi, AJ Banday… - Astronomy & …, 2016 - aanda.org
We present the current accounting of systematic effect uncertainties for the Low Frequency
Instrument (LFI) that are relevant to the 2015 release of the Planck cosmological results …