AAWSAP DIRD, Negative Mass Propulsion, January 2011

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UNCLASSIFIED//fOR. 8FFI61.t..k W&i QJsll,¥
or
2
~
V
<l> = - ­
2
(93)
~ A= -cv
Apart from the factor m/e, this is same as (84).
For weak gravitational fields produced by slowly moving matter, Einstein's linearized
gravitational field equations permit the gauge condition (replacing the Lorentz gauge)
4 8<l>
~
--+divA =0
C 8t
With the gauge transformation for <l> and A
<I>' = <I>
A' =A+gradf
(94)
where f has to satisfy the potential equation
(95)
For a stationary gravitational field the vector potential changes phase of the
Schrodinger wave function according to
1
f// = f// exp [lm
he j'] ,
(96)
leading to phase shift on a closed path
,r\
IJ<p = - -
'
" ds
C
A
26
UNCLASSIFIED//POllt: OPPIEIICL tf!H!!! or~LY