Photon mass new limits from strong photon-torsion coupling generation of primordial magnetic fields
Garcia de Andrade

TL;DR
This paper establishes new upper limits on photon mass and photon-torsion coupling by analyzing primordial magnetic fields, suggesting that stronger couplings could generate seed fields for galactic dynamos, but are constrained by observational limits.
Contribution
It introduces tighter bounds on photon mass and photon-torsion coupling, linking them to primordial magnetic field generation and galactic dynamo seed conditions.
Findings
Photon mass limit of ~10^{-24} eV consistent with previous literature.
Strong photon-torsion coupling can generate primordial magnetic fields sufficient for galactic seeds.
Weaker couplings produce magnetic fields without dynamo amplification.
Abstract
Recently Adelberger et al [Phys Rev Lett 98: 010402, (2007)] have placed a limit to photon mass by investigating the primordial magnetic fields. Earlier Bertolami et al [Phys Lett \textbf{B} 455, 96(1999)] showed that massive photons in a spontaneous Lorentz breaking may generate primordial magnetic fields consistent with galactic dynamo seeds. Torsion coupling constant of order , much higher than the previously obtained by de Sabbata and Sivaram of , leads to strong amplification of magnetic field able to seed galactic dynamo at recombination era contrary to what happens in general relativistic dynamos. This results in where is the massive photon-torsion coupling. Thus in order to obtain the observed galaxy field of one should have a coupling , never observed in the universe. Thus we may…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Geomagnetism and Paleomagnetism Studies · Geophysics and Gravity Measurements
