Modeling parity-violating spectra in Galactic dust polarization with filaments and its applications to cosmic birefringence searches

The detection of rotation of linearly polarized cosmic microwave background photons, which is called cosmic birefringence, may suggest new parity-violating physics. However, scattering by dust can also mimic this same effect. In this paper, the authors extends a pre-existing dust filament model to compute this effect to make a forecast for future CMB experiments and assess the effect of this dust on present isotropic measurements of cosmic birefringence.

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2025-04-15
DOI
https://doi.org/10.1103/physrevd.111.083532
Citations
8
Primary Topic
Dark Matter and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
14.96

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article

Modeling parity-violating spectra in Galactic dust polarization with filaments and its applications to cosmic birefringence searches

P. Diego-Palazuelos, Susan E. Clark, Carlos Hervías-Caimapo, A. Cukierman et al.
8 citations
Physical review. D/Physical review. D.
Dark Matter and Cosmic Phenomena
14.96
article

Modeling parity-violating spectra in Galactic dust polarization with filaments and its applications to cosmic birefringence searches

P. Diego-Palazuelos, Susan E. Clark, Carlos Hervías-Caimapo, A. Cukierman, K. M. Huffenberger
article en
8 citations

Abstract

The detection of rotation of linearly polarized cosmic microwave background photons, which is called cosmic birefringence, may suggest new parity-violating physics. However, scattering by dust can also mimic this same effect. In this paper, the authors extends a pre-existing dust filament model to compute this effect to make a forecast for future CMB experiments and assess the effect of this dust on present isotropic measurements of cosmic birefringence.

Physical review. D/Physical review. D.Vol. 111(8)
Florida State University (US), California Institute of Technology (US), Pontificia Universidad Católica de Chile (CL), Mitchell Institute (US), Kavli Institute for Particle Astrophysics and Cosmology (US), Max Planck Institute for Astrophysics (DE), Texas A&M University (US), Stanford University (US)
National Science Foundation, U.S. Department of Energy, National Aeronautics and Space Administration, National Energy Research Scientific Computing Center, Centro de Astrofísica y Tecnologías Afines, Agencia Nacional de Investigación y Desarrollo, Fondo Nacional de Desarrollo Científico y Tecnológico
Climate action
Openalex Percentile: Top 1%
Dark Matter and Cosmic Phenomena
14.96
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