Abstract
The Lorentz term raises the linear matter power on small scale which leads to interesting signatures in the 21 cm signal. Numerical simulations of the resulting nonlinear density field, the distribution of ionized hydrogen and the 21 cm signal at different values of redshift are presented for magnetic fields with field strength B=5 nG, and spectral indices nB=−2.9, −2.2 and −1.5 together with the adiabatic mode for the best fit data of Planck13+WP. Prospects of constraining the magnetic field parameters with SKA1-LOW of the Square Kilometre Array (SKA) as well as the Hydrogen Epoch of Reionization Array (HERA) are discussed.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
