title: Radiative transfer dynamo effect.
abstract: Magnetic fields in rotating and radiating astrophysical plasma can be produced due to a radiative interaction between plasma layers moving relative to each other. The efficiency of current drive, and with it the associated dynamo effect, is considered in a number of limits. It is shown here, however, that predictions for these generated magnetic fields can be significantly higher when kinetic effects, previously neglected, are taken into account.
authors.affiliation: Princeton Plasma Physics Laboratory, Princeton University, Princeton, New Jersey 08543, USA and Department of Astrophysical Sciences, Princeton University, Princeton, New Jersey 08540, USA.
authors.forename: Vadim R
authors.initials: VR
authors.lastname: Munirov
authors.affiliation: Princeton Plasma Physics Laboratory, Princeton University, Princeton, New Jersey 08543, USA and Department of Astrophysical Sciences, Princeton University, Princeton, New Jersey 08540, USA.
authors.forename: Nathaniel J
authors.initials: NJ
authors.lastname: Fisch