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相关论文: A Probe of Primordial Gravity Waves and Vorticity

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The investigation of polarized light of protoplanetary disks is key for constraining the dust properties, disk morphology and embedded magnetic fields. However, different polarization mechanisms and the diversity of dust grain shapes and…

太阳与恒星天体物理 · 物理学 2019-07-17 Robert Brunngräber , Sebastian Wolf

An observable stochastic background of gravitational waves is generated whenever primordial black holes are created in the early universe thanks to a small-scale enhancement of the curvature perturbation. We calculate the anisotropies and…

宇宙学与河外天体物理 · 物理学 2020-03-10 N. Bartolo , D. Bertacca , V. De Luca , G. Franciolini , S. Matarrese , M. Peloso , A. Ricciardone , A. Riotto , G. Tasinato

We study the polarization-polarization and polarization-temperature correlations in standard adiabatic scenarios for structure formation. Temperature anisotropies due to gravitational potential wells and oscillations in the…

天体物理学 · 物理学 2009-10-22 David Coulson , Robert G. Crittenden , Neil Turok

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

The physical properties of electromagnetic waves in the presence of a gravitational plane wave are analyzed. Formulas for the Stokes parameters describing the polarization of light are obtained in closed form. The particular case of a…

广义相对论与量子宇宙学 · 物理学 2013-05-21 Shahen Hacyan

We calculate the large scale polarization of the cosmic microwave background induced by the anisotropy of the spatial geometry of our universe. Assuming an eccentricity at decoupling of about $0.64 10^{-2}$, we find $\Delta T_{pol}/ T_0…

天体物理学 · 物理学 2007-10-24 Paolo Cea

The next generation of instruments designed to measure the polarization of the cosmic microwave background (CMB) will provide a historic opportunity to open the gravitational wave window to the primordial Universe. Through high sensitivity…

Some results are presented of the Earth's microseismic background. It is assumed that background peaks should correspond to the resonance gravity-wave exchange in the system of two gravity-connected bodies. The microseismic spectrum is…

天体物理学 · 物理学 2007-05-23 V. A. Dubrovskiy

We demonstrate that the multipoles associated with the density matrix are truly observable quantities that can be unambiguously determined from intensity moments. Given their correct transformation properties, these multipoles are the…

We derive in this an expression for the rotation of plane of polarization, of an electromagnetic wave, induced by the field of a gravitational wave propagating along the same direction $\approx \f{G\mu d^2\Omega^4}{3\o}$, $\o$ and $\Omega$…

天体物理学 · 物理学 2010-12-17 A. R. Prasanna , S. Mohanty

The polarized component of the diffuse radio synchrotron emission of our Galaxy shows structure, which is apparently unrelated to the structure in total intensity, on many scales. The structure in the polarized emission can be due to…

天体物理学 · 物理学 2009-11-10 M. Haverkorn , P. Katgert , A. G. de Bruyn

Our local Hubble volume might be contained within a bubble that nucleated in a false vacuum with only two large spatial dimensions. We study bubble collisions in this scenario and find that they generate gravity waves, which are made…

高能物理 - 理论 · 物理学 2015-06-11 Michael P. Salem , Prashant Saraswat , Edgar Shaghoulian

Polarized dust emission outside of disks reveal the magnetic field morphology of molecular clouds. Within disks, however, polarized dust emission can arise from very different mechanisms (e.g., self-scattering), and each of them are useful…

We present a brief review of the polarization properties of the cosmic microwave background in dark matter models for structure formation. Quite independently of the model parameters, the polarization level is expected to be $\sim 10%$ of…

天体物理学 · 物理学 2016-08-30 Alessandro Melchiorri , Nicola Vittorio

The power spectrum of a homogeneous and isotropic stochastic variable, characterized by a finite correlation length, does in general not vanish on scales larger than the correlation scale. If the variable is a divergence free vector field,…

天体物理学 · 物理学 2008-11-26 Chiara Caprini , Ruth Durrer

In the weak field regime, gravitational waves can be considered as being made up of collisionless, relativistic tensor modes that travel along null geodesics of the perturbed background metric. We work in this geometric optics picture to…

宇宙学与河外天体物理 · 物理学 2017-05-17 Carlo R. Contaldi

A large peculiar velocity of the intergalactic medium produces a Doppler shift of the cosmic microwave background with a frequency-dependent quadrupole term. This quadrupole will act as a source for polarization of the cosmic microwave…

宇宙学与河外天体物理 · 物理学 2014-02-20 Elinore Roebber , Gilbert Holder

There is an extremely simple relationship between the spectrum of the gravitational wave background produced by a cosmological distribution of discrete gravitational wave sources, the total time-integrated energy spectrum of an individual…

天体物理学 · 物理学 2007-05-23 E. S. Phinney

A generic consequence of supersymmetry is formation of a scalar condensate along the flat directions of the potential at the end of cosmological inflation. This condensate is usually unstable, and it can fragment into non-topological…

天体物理学 · 物理学 2008-12-18 Alexander Kusenko , Anupam Mazumdar

Primordial gravitational waves are expected to create a stochastic background encoding information about the early Universe that may not be accessible by other means. However, the primordial background is obscured by an astrophysical…

高能天体物理现象 · 物理学 2020-12-11 Sylvia Biscoveanu , Colm Talbot , Eric Thrane , Rory Smith