AAWSAP DIRD, Advanced Space Propulsion Based on Vacuum (Spacetime Metric) Engineering, March 2010
DOW-UAP-D132 · page 8 of 17
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UNCLASSIFIED/ /FOR 8Ffl@IAL tl.!I!! er•t a TIMEINTERVAL, FREQUENCY, ENERGY Begin by considering the case where ~ < 1, typical for an altered spacetime metric in the vicinity of, say, a stellar mass, as expressed by the leading term in Equation (4). Local measurements with physical clocks within the altered spacetime yield a time interval ..[i";;dt < dt; thus an interval of time dt between two events in an undistorted spacetime remote1 from the mass-say, 10 seconds-would be judged by local (proper) measurement from within the altered spacetime to occur in a lesser time interval, .[i";;;dt <dt-say, 5 seconds. From this one can rightly infer that, relatively speaking, clocks (atomic processes and so forth) within the altered spacetime run slower. Given this result, a physical process (for example, interval between clock ticks, atomic emissions) that takes a time !:::.t in unaltered spacetime slows to !).t ➔ M/.ji;, when occurring within the altered spacetime. Conversely, under conditions (for example, metric engineering) for which Ji;; > 1, processes within the spacetime-altered region are sped up. Thus the first entry for a table of physical effects (see Table 1) is made. Given that frequency measurements are the reciprocal of time duration measurements, the associated expression for frequency w is given by m➔ m.Jg;; , our second entry in Table 1. This accounts, for example, for the redshifting of atomic emissions from dense masses where ..[i";; < 1. Conversely, under conditions for which Ji;; > 1, blueshifting of emissions would occur. In addition, given that quanta of energy are given by E = hm, energy scales with Jg;; , as does frequency, E ➔ E.jg;,, our third entry in the table. Depending on the value of .Ji: in the spacetime-altered region, energy states may be raised or lowered relative to an unaltered spacetime region. 1 An observer at "infinity." UNCLASSIFIED/ j POI\ OPPIEIICL tl.!I!! BHLY 3