Limit on primordial small-scale magnetic fields from cosmic microwave background distortions
Spatially varying primordial magnetic fields may be efficiently dissipated prior to the epoch of recombination due to the large viscosity of the baryon-photon fluid. We show that this dissipation may result in observable chemical potential &mgr; and Compton y distortions in the cosmic microwave background spectrum. Current upper limits on &mgr; and y from FIRAS constrain magnetic fields to have strength B0<3x10(-8) G (scaled to the present) between comoving coherence length approximately 400 pc and approximately 0.6 Mpc. These represent the strongest upper limits on small-scale primordial magnetic fields to date.
Jedamzik
K
Max-Planck-Institut fur Astrophysik, 85748 Garching bei Munchen, Germany.
Katalinic
V
Olinto
AV