کد مقاله کد نشریه سال انتشار مقاله انگلیسی نسخه تمام متن
1770479 1523349 2016 11 صفحه PDF دانلود رایگان
عنوان انگلیسی مقاله ISI
Primordial magnetogenesis before recombination
ترجمه فارسی عنوان
مغناطیسی اولیه قبل از نوترکیب
موضوعات مرتبط
مهندسی و علوم پایه فیزیک و نجوم نجوم و فیزیک نجومی
چکیده انگلیسی

The origin of large magnetic fields in the Universe remains currently unknown. We investigate here a mechanism before recombination based on known physics. The source of the vorticity is due to the changes in the photon distribution function caused by the fluctuations in the background photons. We show that the magnetic field generated in the MHD limit, due to the Coulomb scattering, is of the order 10−4910−49 G on a coherence scale of 10 kpc. We explicitly show that the magnetic fields generated from this process are sustainable and are not erased by resistive diffusion. We compare the results with current observations and discuss the implications. Our seed magnetic fields are generated on small scales whereas the main mechanisms studied in the literature are on scale bigger than 1 Mpc. However, compared to more exotic theories generating seed magnetic fields on similar scales, the strength of our fields are generally smaller.

ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Astroparticle Physics - Volume 77, April 2016, Pages 44–54
نویسندگان
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