On SuperPotentials in the Theory of Newtonian Gravitation.
Abstract
The character of the gravitational equilibrium of bodies in rotation and with prevalent magnetic fields depends on the tensor potential, 4=G})P(x') ( ')( ) dx', lxx'13 and the associated tensors, ii= $ iidx and pq;ij= fvPXp% $dX This paper is devoted to a consideration of these fundamental tensors It is shown, in particular, that the tensor potential can be expressed in the form ii= where is the gravitational potential as usually defined and x is a superpotential determined by the equation V2x= 2 .
 Publication:

The Astrophysical Journal
 Pub Date:
 January 1962
 DOI:
 10.1086/147261
 Bibcode:
 1962ApJ...135..238C