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相关论文: The Quest for B Modes from Inflationary Gravitatio…

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We review current observational constraints on the polarization of the Cosmic Microwave Background (CMB), with a particular emphasis on detecting the signature of primordial gravitational waves. We present an analytic solution to the…

天体物理学 · 物理学 2009-11-11 Brian G. Keating , Alexander G. Polnarev , Nathan J. Miller , Deepak Baskaran

The curl-modes of Cosmic Microwave Background (CMB) polarization probe horizon-scale primordial gravitational waves related to inflation. A significant source of confusion is expected from a lensing conversion of polarization related to…

天体物理学 · 物理学 2009-11-10 Asantha Cooray

These lectures introduce some of the basic theory of cosmic microwave background (CMB) polarization with the primary aim of developing the theory of CMB polarization from inflationary gravitational waves, as well as some of the related…

天体物理学 · 物理学 2007-05-23 Paolo Cabella , Marc Kamionkowski

We consider a novel contribution to the polarization of the Cosmic Microwave Background induced by vector and tensor modes generated by the non-linear evolution of primordial scalar perturbations. Our calculation is based on relativistic…

天体物理学 · 物理学 2009-11-10 Silvia Mollerach , Diego Harari , Sabino Matarrese

A stochastic background of primordial gravitational waves could be detected soon in the polarization of the CMB and/or with laser interferometers. There are at least three GWB coming from inflation: those produced during inflation and…

宇宙学与河外天体物理 · 物理学 2010-05-11 Juan Garcia-Bellido

The BICEP2 collaboration reported recently a B-mode polarization of the cosmic microwave background (CMB) radiation inconsistent with the null hypothesis at a significance of > 5 {\sigma}. This result has been often interpreted as a…

综合物理 · 物理学 2014-08-28 Luis Gonzalez-Mestres

Detecting the parity-odd, or B-mode, polarization pattern in the cosmic microwave background radiation due to primordial gravity waves is considered to be the final observational key to confirming the inflationary paradigm. The search for…

天体物理学 · 物理学 2009-06-23 Levon Pogosian , Mark Wyman

The inflationary $B$-mode signals encode invaluable information about the origin of our Universe and searching for potential signatures of primordial gravitational waves (PGWs) is one of the major science goals for future precision…

宇宙学与河外天体物理 · 物理学 2025-12-09 Sen Li , Chang Feng , Filipe B. Abdalla

We introduce the real space correlation function of $B$-mode polarization of the cosmic microwave background (CMB) as a probe of superhorizon tensor perturbations created by inflation. By causality, any non-inflationary mechanism for…

宇宙学与河外天体物理 · 物理学 2010-01-15 Daniel Baumann , Matias Zaldarriaga

Primordial gravitational waves leave a characteristic imprint on the cosmic microwave background (CMB) in the form of $B$-mode polarization. Photons are also deflected by large scale gravitational waves which intervene between the source…

宇宙学与河外天体物理 · 物理学 2017-09-20 Connor Sheere , Alexander van Engelen , P. Daniel Meerburg , Joel Meyers

The curl (B) modes of cosmic microwave background (CMB) polarization anisotropies are a unique probe of the primordial background of inflationary gravitational waves (IGWs). Unfortunately, the B-mode polarization anisotropies generated by…

天体物理学 · 物理学 2007-05-23 Kris Sigurdson , Asantha Cooray

The B-mode polarization of the cosmic microwave background (CMB) provides a unique window into tensor perturbations from inflationary gravitational waves. Survey effects complicate the estimation and description of the power spectrum on the…

宇宙学与河外天体物理 · 物理学 2016-09-28 Eric R. Switzer , Duncan J. Watts

One of the most promising ways of detecting primordial gravitational waves generated during inflation is to observe B-modes of polarization, generated by Thomson scattering after reionization, in the cosmic microwave background (CMB). Large…

宇宙学与河外天体物理 · 物理学 2014-11-20 Scott Dodelson

A B-mode polarization signal in the cosmic microwave background (CMB) is widely regarded as smoking gun evidence for gravitational waves produced during inflation. Here, we demonstrate that tensor perturbations sourced during…

宇宙学与河外天体物理 · 物理学 2026-04-22 Kylar Greene , Aurora Ireland , Gordan Krnjaic , Yuhsin Tsai

Weak gravitational lensing by foreground density perturbations generates a gradient mode in the shear of background images. In contrast, cosmological tensor perturbations induce a non-zero curl mode associated with image rotations. In this…

天体物理学 · 物理学 2008-11-26 Devdeep Sarkar , Paolo Serra , Asantha Cooray , Kiyotomo Ichiki , Daniel Baumann

Inflationary gravitational waves (GW) contribute to the curl component in the polarization of the CMB. Cosmic shear--gravitational lensing of the CMB-- converts a fraction of the dominant gradient polarization to the curl component.…

天体物理学 · 物理学 2009-11-07 Michael Kesden , Asantha Cooray , Marc Kamionkowski

Gravitational waves from inflation induce polarization patterns in the cosmic microwave background (CMB). It is known that there are only two types of non-Gaussianities of the gravitaional waves in the most general scalar field theories…

宇宙学与河外天体物理 · 物理学 2018-08-01 Hiroaki W. H. Tahara , Jun'ichi Yokoyama

[Abridged] The polarization of the CMB is widely recognized as a potential source of information about primordial gravitational waves. The gravitational wave contribution can be separated from the dominant CMB polarization created by…

天体物理学 · 物理学 2009-11-10 Christopher M. Hirata , Abraham Loeb , Niayesh Afshordi

The primordial B-modes component of the cosmic microwave background (CMB) polarization is a promising experimental dataset to probe the inflationary paradigm. B-modes are indeed a direct consequence of the presence of gravitational waves in…

宇宙学与河外天体物理 · 物理学 2018-02-28 Alessandro Manzotti

The anisotropy study cosmic microwave background (CMB) is one of the main observational tools for modern cosmology. However, alongside the study of the thermal fluctuations of the CMB are other equally important information, which is known…

宇宙学与河外天体物理 · 物理学 2016-01-18 Alexander Bonilla Rivera
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