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astro-ph.COMar 18, 2015
authors
  • Rohoollah Mohammadi
  • Moslem Zarei
arXiv abstractPDF
paper

Generation of CMB B-mode Polarization from Circular Polarization

arXiv:1503.05356

Abstract

In this work we consider non-zero circular polarization for the CMB radiation as a result of new interactions. We then rewrite the Boltzmann equations for the Stokes parameters Q, U and V and show that the circular polarization can generate the B-mode polarization even if no tensor perturbations are present.

References in corpus (16)

  • BICEP2 I: Detection Of B-mode Polarization at Degree Angular Scales
  • An All-Sky Analysis of Polarization in the Microwave Background
  • Statistics of Cosmic Microwave Background Polarization
  • CMB Anisotropies: Total Angular Momentum Method
  • CBR Anisotropy and the Running of the Scalar Spectral Index
  • Cosmic Microwave Background Polarization
  • Generation of circular polarization of the CMB
  • Did BICEP2 see vector modes? First B-mode constraints on cosmic defects
  • Can topological defects mimic the BICEP2 B-mode signal?
  • Can primordial magnetic fields be the origin of the BICEP2 data?
  • Generation of Circular Polarization of the Cosmic Microwave Background
  • Circular Polarization of the CMB: A probe of the First stars
  • Photon-neutrino scattering and the B-mode spectrum of CMB photons
  • Last scattering, relic gravitons and the circular polarization of the CMB
  • Planck 2015 results. XX. Constraints on inflation
  • Photon-photon interactions can be a source of CMB circular polarization
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