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
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. |
Material: |