Evolution of Helical Magnetic Fields Up To Recombination

by Mr Sayan Mandal (Carnegie Mellon University)

Thursday 22 Feb 2018, 16:30 → 17:30 Asia/Kolkata

A304

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.

Poster sou_sayan.pdf