Physics
Scientific paper
Nov 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009phrvl.103t1803r&link_type=abstract
Physical Review Letters, vol. 103, Issue 20, id. 201803
Physics
1
Photons, Classical Electromagnetism, Maxwell Equations, Experimental Tests, Interplanetary Magnetic Fields
Scientific paper
The effect of the Proca photon mass mph and cosmic vector potential AC on the dynamics of solar wind is considered. For large-enough values of the parameter ACmph2, the solar wind structure at a distance of ˜40AU from the Sun should change significantly with respect to the actual observed flow. The absence of such deviations gives an upper bound on the parameter ACmph2 9 orders of magnitude less than in laboratory experiments measuring torque on a toroidal magnet.
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