State of the Universe

Evolution of Helical Magnetic Fields Up To Recombination

by Mr. Sayan Mandal (Carnegie Mellon University)

Thursday, February 22, 2018 from to (Asia/Kolkata)
at A304
Description
We study the evolution of magnetic fields generated in the early universe with different spectra, strengths and helicity due to MHD processes till the epoch of recombination. We compare our results with the bounds from observations of TeV Blazar Spectra.
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