Probing cosmic inflation with the LiteBIRD cosmic microwave background polarization survey

LiteBIRD Collaboration, E Allys, K Arnold… - … of Theoretical and …, 2023 - academic.oup.com
Abstract LiteBIRD, the Lite (Light) satellite for the study of B-mode polarization and Inflation
from cosmic background Radiation Detection, is a space mission for primordial cosmology …

Gold nanomaterials at work in biomedicine

X Yang, M Yang, B Pang, M Vara, Y Xia - Chemical reviews, 2015 - ACS Publications
Gold is a precious metal with a characteristic bright and beautiful hue known as the golden
yellow color.(1) As of 2012, a total of 174,100 tons of Au has been mined in human history …

Planck 2018 results-X. Constraints on inflation

Y Akrami, F Arroja, M Ashdown, J Aumont… - Astronomy & …, 2020 - aanda.org
We report on the implications for cosmic inflation of the 2018 release of the Planck cosmic
microwave background (CMB) anisotropy measurements. The results are fully consistent …

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 …

The astrodust+ PAH model: A unified description of the extinction, emission, and polarization from dust in the diffuse interstellar medium

BS Hensley, BT Draine - The Astrophysical Journal, 2023 - iopscience.iop.org
We present a new model of interstellar dust in which large grains are a single composite
material," astrodust," and nanoparticle-sized grains come in distinct varieties including …

Planck 2015 results-X. Diffuse component separation: Foreground maps

R Adam, PAR Ade, N Aghanim, MIR Alves… - Astronomy & …, 2016 - aanda.org
Planck has mapped the microwave sky in temperature over nine frequency bands between
30 and 857 GHz and in polarization over seven frequency bands between 30 and 353 GHz …

Planck 2018 results-XI. Polarized dust foregrounds

Y Akrami, M Ashdown, J Aumont, C Baccigalupi… - Astronomy & …, 2020 - aanda.org
The study of polarized dust emission has become entwined with the analysis of the cosmic
microwave background (CMB) polarization in the quest for the curl-like B-mode polarization …

[HTML][HTML] A nearby galaxy perspective on dust evolution-Scaling relations and constraints on the dust build-up in galaxies with the DustPedia and DGS samples

F Galliano, A Nersesian, S Bianchi, I De Looze… - Astronomy & …, 2021 - aanda.org
Context. The efficiency of the different processes responsible for the evolution of interstellar
dust on the scale of a galaxy are, to date, very uncertain, spanning several orders of …

PRISM (Polarized Radiation Imaging and Spectroscopy Mission): an extended white paper

P André, C Baccigalupi, A Banday… - … of Cosmology and …, 2014 - iopscience.iop.org
Abstract PRISM (Polarized Radiation Imaging and Spectroscopy Mission) was proposed to
ESA in May 2013 as a large-class mission for investigating within the framework of the ESA …

PICO: Probe of inflation and cosmic origins

S Hanany, M Alvarez, E Artis, P Ashton… - arXiv preprint arXiv …, 2019 - arxiv.org
The Probe of Inflation and Cosmic Origins (PICO) is an imaging polarimeter that will scan the
sky for 5 years in 21 frequency bands spread between 21 and 799 GHz. It will produce full …