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Nonuniform cosmological birefringence and active galactic nuclei

Kamionkowski, Marc (2010) Nonuniform cosmological birefringence and active galactic nuclei. Physical Review D, 82 (4). 047302. ISSN 0556-2821. http://resolver.caltech.edu/CaltechAUTHORS:20100913-095859358

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Abstract

The CMB constrains the cosmological-birefringence rotation angle to be |α|≲1° (1σ) out to redshifts z≃1100 for a rotation that is uniform across the sky. However, the rotation angle α(θ,ϕ) may vary with position (θ,ϕ) on the sky, and if so, then it can be sought in current and future future active galactic nuclei data. An upper limit <a^2>^(1/2)≲3.7° to the scatter in the position-angle–polarization offsets in a sample of only N=9 active galactic nuclei already constrains the rotation spherical-harmonic coefficients to (4π)^(-1/2)α_(lm)≲3.7° and constrains the power spectrum for α in models where it is a stochastic field. Future constraints can be improved with more sources and by analyzing well-mapped sources with a tensor-harmonic decomposition of the polarization.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1103/PhysRevD.82.047302DOIUNSPECIFIED
http://link.aps.org/doi/10.1103/PhysRevD.82.047302PublisherUNSPECIFIED
Additional Information:© 2010 American Physical Society. Received 21 April 2010; revised 28 April 2010; published 25 August 2010. I thank S. di Serego Alighieri, R. Caldwell, V. Gluscevic, and A. Readhead for useful discussions. This work was supported by DOE Grant No. DE-FG03-92-ER40701, NASA Grant No. NNX10AD04G.
Group:TAPIR
Funders:
Funding AgencyGrant Number
Department of Energy (DOE)DE-FG03-92-ER40701
NASANNX10AD04G
Classification Code: PACS: 98.80.Es, 98.54.Cm
Record Number:CaltechAUTHORS:20100913-095859358
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20100913-095859358
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:19893
Collection:CaltechAUTHORS
Deposited By: Jason Perez
Deposited On:15 Sep 2010 18:31
Last Modified:26 Dec 2012 12:24

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