Finding Evidence for Inflation and the Origin of Galactic Magnetic Fields with CMB Surveys
Sayan Mandal, Neelima Sehgal, Toshiya Namikawa

TL;DR
This paper explores how future CMB surveys can detect or constrain primordial magnetic fields generated during inflation, which could confirm the inflationary origin of galactic magnetic fields.
Contribution
It demonstrates that upcoming CMB measurements can significantly improve constraints on inflationary magnetic fields, potentially providing evidence for inflation.
Findings
CMB-HD could lower the upper bound to 0.072 nG at 95% CL.
Future surveys can improve sensitivity to Mpc-scale inflationary PMFs by an order of magnitude.
Detection of inflationary PMFs at 3σ significance or higher is possible with CMB-HD.
Abstract
The origin of the G magnetic fields observed in galaxies is unknown. One promising scenario is that magnetic fields generated during inflation, larger than 0.1 nG on Mpc scales, were adiabatically compressed to G strengths in galaxies during structure formation. Thus, detecting a scale-invariant primordial magnetic field (PMF) above 0.1 nG on Mpc scales just after recombination would indicate an inflationary origin of galactic magnetic fields. This would also provide compelling evidence that inflation occurred since only an inflationary mechanism could generate such a strong, scale-invariant magnetic field on Mpc scales. In contrast, constraining the scale-invariant PMF strength to be below 0.1 nG would imply an inflationary scenario is not the primary origin, since such weak PMFs cannot be amplified enough via adiabatic compression to produce the strength of the galactic…
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Taxonomy
TopicsCosmology and Gravitation Theories · Solar and Space Plasma Dynamics · Space Technology and Applications
