Evidence for Strong Intracluster Magnetic Fields in the Early Universe
نویسندگان
چکیده
The origin of magnetic fields in clusters galaxies is still a matter debate. Observations for intracluster over wide range redshifts are crucial to constrain possible scenarios the and evolution fields. (Differences Faraday rotation measures (RMs) an embedded double radio sources, i.e. pair lobes mostly Fanaroff--Riley type II galaxies, free from contributions interstellar medium inside Milky Way intergalactic between us, hence provide novel way estimate average field within galaxy clusters.) We have obtained sample 627 pairs whose RMs available most updated RM catalogues redshift databases. differences derived. statistically large $z>0.9$ indicate that as strong about 4~$\mu$G. Such at half age Universe, comparable strength nearby clusters, pose challenge on theories cosmic
منابع مشابه
Magnetic Fields in the Early Universe
We discuss some old and new results on mangetic fields
متن کاملMagnetic Fields in the Early Universe
The observed galactic magnetic fields may have a primordial origin. I briefly review the observations, their interpretation in terms of the dynamo theory, and the current limits on cosmological magnetic fields. Several possible mechanisms for generating a primordial magnetic field are then discussed. Turbulence and the evolution of the microscopic fields to macroscopic fields is described in te...
متن کاملOn the evolution of magnetic fields in the early universe
We address the question of the existence of magnetic domains in a recent scenario for the creation of primordial magnetic fields. We write down the magnetohydrodynamic equation in an expanding universe in the infinite conductivity limit and discuss its solution. No domains are found. [email protected]; [email protected] We have recently presented a scenario for the creation of a primord...
متن کاملDecay of Magnetic Fields in the Early Universe∗
We study the evolution of a stochastic helical magnetic field generated in the early Universe after the electroweak phase transition, using standard magnetohydrodynamics (MHD). We find how the coherence length ξ, magnetic energy EM and magnetic helicity H evolve with time. We show that the self-similarity of the magnetic power spectrum alone implies that ξ ∼ t1/2. This in turn implies that magn...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: The Astrophysical Journal
سال: 2022
ISSN: ['2041-8213', '2041-8205']
DOI: https://doi.org/10.3847/1538-4357/ac4095