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相关论文: Tensor B mode and stochastic Faraday mixing

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We present a covariant and gauge invariant formalism suited to the study of second-order effects associated with higher order tensor perturbations. The analytical method we have developed enables us to characterize pure second-order tensor…

广义相对论与量子宇宙学 · 物理学 2017-04-04 Bob Osano

Standard models describing the radiation transfer of the cosmic microwave background (CMB) through Compton scattering predict that cosmological scalar perturbations at linear order are not able to source V and B polarization modes. In this…

高能物理 - 唯象学 · 物理学 2019-08-13 Nicola Bartolo , Ahmad Hoseinpour , Sabino Matarrese , Giorgio Orlando , Moslem Zarei

We estimate the B-polarisation induced in the Cosmic Microwave Background by the non-linear evolution of density perturbations. Using the second-order Boltzmann code SONG, our analysis incorporates, for the first time, all physical effects…

宇宙学与河外天体物理 · 物理学 2014-09-08 Christian Fidler , Guido W. Pettinari , Martin Beneke , Robert Crittenden , Kazuya Koyama , David Wands

The ongoing and future experiments will measure the B-mode from different sky coverage and frequency bands, with the potential to reveal non-trivial features in polarization map. In this work we study the TT, TB, EB and BB correlations…

宇宙学与河外天体物理 · 物理学 2014-08-15 Xingang Chen , Razieh Emami , Hassan Firouzjahi , Yi Wang

Recently, BICEP2 measurements of the cosmic microwave background (CMB) $B$-mode polarization has indicated the presence of primordial gravitational waves at degree angular scales, inferring the tensor-to-scalar ratio of $r=0.2$ and a…

宇宙学与河外天体物理 · 物理学 2018-06-11 Seokcheon Lee , Guo-Chin Liu , Kin-Wang Ng

The influences of triaxial dynamics on the anomalous $E2$ transitional behaviors in the interacting boson model (IBM) have been comprehensively examined without symmetry restrictions. Specifically, different triaxial schemes in the IBM have…

核理论 · 物理学 2025-08-22 Yu Zhang , Wei Teng

New phenomenon of temporal oscillations of nonlinear Faraday rotation in a driven four-level system is predicted. We show that in this system with one upper level, under the conditions of electromagnetically induced transparency created by…

量子物理 · 物理学 2007-05-23 Malakyan Yu. P

We discuss the production of circular polarization in compact radio sources both by the intrinsic mechanism and by Faraday conversion. We pay particular attention to the magnetic field structure, considering partially ordered fiel ds and…

天体物理学 · 物理学 2009-11-07 John F. C. Wardle , Daniel C. Homan

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-field slow-roll model of inflation is presented, and we explain…

宇宙学与河外天体物理 · 物理学 2016-10-05 Marc Kamionkowski , Ely D. Kovetz

We study the angular power spectra of the polarized component of the Galactic synchrotron emission in the 28-deg^2 Test Region of the Southern Galactic Plane Survey at 1.4 GHz. These data were obtained by the Australia Telescope Compact…

We study the magnetic fields in galaxy clusters through Faraday rotation measurements crossing systems in different dynamical states. We confirm that magnetic fields are present in those systems and analyze the difference between relaxed…

宇宙学与河外天体物理 · 物理学 2019-05-27 Federico A. Stasyszyn , Martín de los Rios

We describe singularities in the distribution of polarized intensity as a function of Faraday depth (i.e. the Faraday spectrum) caused by line-of-sight (LOS) magnetic field reversals. We call these features Faraday caustics because of their…

星系天体物理 · 物理学 2015-05-28 M. R. Bell , H. Junklewitz , T. A. Enßlin

The complete calculation of the CMB polarization observables (i.e. E- and B-modes) is reported within the conventional $\Lambda$CDM paradigm supplemented by a stochastic magnetic field. Intriguing perspectives for present and forthcoming…

天体物理学 · 物理学 2008-04-15 Massimo Giovannini , Kerstin E. Kunze

We investigate the properties of the Galactic ISM by applying Faraday tomography to a radio polarization data set in the direction of the Galactic anti-centre. We address the problem of missing large-scale structure in our data, and show…

天体物理学 · 物理学 2015-05-13 D. H. F. M. Schnitzeler , P. Katgert , A. G. de Bruyn

We show that the Faraday effect can be derived from a simple two-state model. This approach uses a quantized electromagnetic field and does not make reference to differences in refractive indices of left- and right-circularly polarized…

量子物理 · 物理学 2024-10-04 Benjamin W. Butler

Probing primordial curvature perturbations on small scales, beyond those accessible using cosmic microwave background (CMB) primary anisotropies and Lyman-$\alpha$ forest data, remains a major open challenge. Current constraints on the…

高能物理 - 唯象学 · 物理学 2025-09-03 Aurora Ireland , Kuver Sinha , Tao Xu

We present a polarization and Faraday rotation study of the hybrid morphology radio galaxy NGC 612 (PKS 0131-36), using Australian Telescope Compact Array observations from 1 to 3 GHz. In general, the results are consistent with an external…

高能天体物理现象 · 物理学 2018-11-16 J. K. Banfield , S. P. O'Sullivan , M. H. Wieringa , B. H. C. Emonts

Faraday rotation has been seen at millimeter wavelengths in several low luminosity active galactic nuclei, including Event Horizon Telescope (EHT) targets M87* and Sgr A*. The observed rotation measure (RM) probes the density, magnetic…

高能天体物理现象 · 物理学 2020-10-07 Angelo Ricarte , Ben S. Prather , George N. Wong , Ramesh Narayan , Charles Gammie , Michael Johnson

Polarization observations at 21cm and 18cm towards the local Taurus molecular cloud complex were made with the Effelsberg 100-m telescope. Highly structured, frequency-dependent polarized emission features were detected. We discuss…

天体物理学 · 物理学 2009-11-10 M. Wolleben , W. Reich

At linear order the only expected source of a curl-like, B mode, polarization pattern in the cosmic microwave background (CMB) is primordial gravitational waves. At second-order B modes are also produced from purely scalar, density, initial…

宇宙学与河外天体物理 · 物理学 2021-12-01 William R. Coulton
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