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Large scale primordial magnetic fields from inflation and preheating

By Ola Tornkvist, Anne-Christine Davis, Konstantinos Dimopoulos and Tomislav Prokopec


We consider models in which the (transverse) photon mass is non-zero during inflation and drops to zero non-adiabatically at the end of inflation. Through this process, vacuum fluctuations of the photon field are converted into physical, long-wavelength modes with high amplitude. The resulting spectrum of the field strength is approximately B_l ~ 1/l, where l is the relevant coherence scale. With a reasonable model of field evolution we obtain, on comoving galactic scales, a magnetic field strong enough to seed a dynamo mechanism and generate the observed galactic magnetic fields

Publisher: American Institute of Physics
Year: 2000
OAI identifier:
Provided by: Lancaster E-Prints

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