A new probe of primordial magnetic fields at high redshift
APA
Gluscevic, V. (2016). A new probe of primordial magnetic fields at high redshift. Perimeter Institute. https://pirsa.org/16060011
MLA
Gluscevic, Vera. A new probe of primordial magnetic fields at high redshift. Perimeter Institute, Jun. 14, 2016, https://pirsa.org/16060011
BibTex
@misc{ pirsa_PIRSA:16060011, doi = {10.48660/16060011}, url = {https://pirsa.org/16060011}, author = {Gluscevic, Vera}, keywords = {Cosmology}, language = {en}, title = {A new probe of primordial magnetic fields at high redshift}, publisher = {Perimeter Institute}, year = {2016}, month = {jun}, note = {PIRSA:16060011 see, \url{https://pirsa.org}} }
University of Southern California
Talk Type
Subject
Abstract
I will present a novel method for probing extremely weak large-scale magnetic fields in the intergalactic medium prior to the epoch of reionization. This method relies on the effect of spin alignment of hydrogen atoms in a cosmological setting, and on the effect of magnetic precession of the atoms on the statistics of the 21–cm brightness–temperature fluctuations. It is intrinsically sensitive to magnetic fields weaker than 10^{-19} Gauss in physical units, and thus has a potential to reach many orders of magnitude below the current constraints on primordial magnetic fields. I will discuss the physical mechanism, lay out the estimator formalism that enables searches with future 21-cm tomographic surveys, and present forecasts for detecting magnetic fields in the high-redshift universe using this method.