When a charged insulating spherical shell is uniformly accelerated, an oppo
sitely directed electric field is produced inside. Outside the field is the
Born field of a uniformly accelerated charge, modified by a dipole. Radiat
ion is produced. When the acceleration is annulled by the nearly uniform gr
avity field of an external shell with a 1 + beta cos theta surface distribu
tion of mass, the differently viewed Born field is static and joins a stati
c field outside the external shell; no radiation is produced. We discuss gr
avitational analogues of these phenomena. When a massive spherical shell is
accelerated, an untouched test mass inside experiences a uniform gravity f
ield and accelerates parallelly to the surrounding shell. In the strong gra
vity regime we illustrate these effects using exact conformastatic solution
s of the Einstein-Maxwell equations with charged dust. We consider a massiv
e charged shell on which the forces due to nearly uniform electrical and gr
avitational fields balance. Both fields are reduced inside by the ratio of
the g(00) inside the shell to that away from it. The acceleration of a free
test particle, relative to a static observer, is reduced correspondingly.
We give physical explanations of these effects. (C) 1999 Academic Press.