2018/05/31 by F. Vazza, M. Brüggen, P. M. Hinz +6 · 1 citation
Physics and Astronomy · #Astronomy #Astrophysics #Cosmology and Gravitation Theories #Faraday cage #Faraday effect #Galaxy #Line-of-sight #Magnetic field #Measure (data warehouse) #Physics #Pulsars and Gravitational Waves Research #Quantum mechanics #Radio Astronomy Observations and Technology #Redshift #Rotation (mathematics) #Sky #astro-ph.CO #astro-ph.IM
paper · pdf · doi:10.1093/mnras/sty1968
8 pages, 10 figures, MNRAS accepted, in press. A color-blind friendly version can be downloaded here https://storage.googleapis.com/wzukusers/user-14759165/documents/5b5586d8d71601wxVuGn/frb-magnetic-fields-6.pdf
arxiv created 2018/07/23 · openalex publication_date 2018/07/23 · arxiv updated 2018/07/24 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
The joint analysis of the Dispersion and Faraday Rotation Measure (RM) from distant, polarized Fast Radio Bursts (FRBs) may be used to put constraints on the origin and distribution of extragalactic magnetic fields on cosmological scales. While the combination of Dispersion and Faraday RM can in principle give the average magnetic fields along the line-of-sight, in practice this method must be used with care because it strongly depends on the assumed magnetization model on large cosmological scales. Our simulations show that the observation of RMs with |≥ 1-10 \rm rad m-2| in ∼102–103 FRBs will likely be able to discriminate between extreme scenarios for the origin of cosmic magnetic fields, independent of the exact distribution of sources with redshift. This represents a strong case for incoming (e.g. ALERT, CHIME) and future (e.g. with the Square Kilometer Array) radio polarization surveys of the sky.