B-mode CMB polarization from patchy screening during reionization
- 1. Kavli Institute for Cosmological Physics and Enrico Fermi Institute, University of Chicago, Chicago, Illinois 60637 (United States)
- 2. Department of Physics, University of Chicago, Chicago, Illinois 60637 (United States)
- 3. Department of Astronomy and Astrophysics, University of Chicago, Chicago, Illinois 60637 (United States)
- 4. Institute of Astronomy, University of Cambridge, Cambridge CB3 0HA (United Kingdom)
Description
B modes in CMB polarization from patchy reionization arise from two effects: generation of polarization from scattering of quadrupole moments by reionization bubbles and fluctuations in the screening of E modes from recombination. The scattering contribution has been studied previously, but the screening contribution has not yet been calculated. We show that on scales smaller than the acoustic scale (l > or approx. 300), the B-mode power from screening is larger than the B-mode power from scattering. The ratio approaches a constant ∼2.5 below the damping scale (l > or approx. 2000). On degree scales relevant for gravitational waves (l < or approx. 100), screening B modes have a white noise tail and are subdominant to the scattering effect. These results are robust to uncertainties in the modeling of patchy reionization.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.79.107302;
- arXiv
- arXiv:0902.4413v2;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 79
- Journal Issue
- 10
- Journal Page Range
- p. 107302-107302.4
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41042704
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- FLUCTUATIONS; GRAVITATIONAL WAVES; NOISE; POLARIZATION; QUADRUPOLE MOMENTS; RECOMBINATION; RELICT RADIATION; SCATTERING; SCREENING; SIMULATION
- Descriptors DEC
- ELECTROMAGNETIC RADIATION; MICROWAVE RADIATION; RADIATIONS; VARIATIONS
Optional Information
- Notes
- (c) 2009 The American Physical Society